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  <front>
    <journal-meta><journal-id journal-id-type="publisher">AMT</journal-id><journal-title-group>
    <journal-title>Atmospheric Measurement Techniques</journal-title>
    <abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1867-8548</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/amt-14-869-2021</article-id><title-group><article-title>What millimeter-wavelength radar reflectivity reveals about snowfall:  an information-centric analysis</article-title><alt-title>What millimeter-wavelength radar reflectivity reveals about snowfall</alt-title>
      </title-group><?xmltex \runningtitle{What millimeter-wavelength radar reflectivity reveals about snowfall}?><?xmltex \runningauthor{N. B. Wood and T. S. L'Ecuyer}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Wood</surname><given-names>Norman B.</given-names></name>
          <email>norman.wood@ssec.wisc.edu</email>
        <ext-link>https://orcid.org/0000-0001-8228-3910</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>L'Ecuyer</surname><given-names>Tristan S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7584-4836</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Space Science and Engineering Center, University of Wisconsin – Madison, Madison, WI, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Atmospheric and Oceanic Sciences, University of Wisconsin – Madison, Madison, WI, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Norman B. Wood (norman.wood@ssec.wisc.edu)</corresp></author-notes><pub-date><day>4</day><month>February</month><year>2021</year></pub-date>
      
      <volume>14</volume>
      <issue>2</issue>
      <fpage>869</fpage><lpage>888</lpage>
      <history>
        <date date-type="received"><day>4</day><month>June</month><year>2020</year></date>
           <date date-type="rev-request"><day>29</day><month>June</month><year>2020</year></date>
           <date date-type="rev-recd"><day>22</day><month>October</month><year>2020</year></date>
           <date date-type="accepted"><day>24</day><month>November</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Norman B. Wood</copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021.html">This article is available from https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021.html</self-uri><self-uri xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e95">The ability of single-frequency, millimeter-wavelength radar reflectivity
observations to provide useful constraints for retrieval of snow particle
size distribution (PSD) parameters, snowfall rates, and snowfall accumulations
is examined. An optimal estimation snowfall retrieval that allows
analyses of retrieval uncertainties and information content is applied
to observations of near-surface W-band reflectivities from multiple
snowfall events during the 2006–2007 winter season in southern Ontario.
Retrieved instantaneous snowfall rates generally have uncertainties
greater than 100 %, but single-event and seasonal snow accumulations
from the retrieval results match well with collocated
measurements of accumulations. Absolute fractional differences are
mainly below 30 % for individual events that have more substantial
accumulations and, for the season, 12.6 %. Uncertainties in retrieved
snowfall rates are driven mainly by uncertainties in the retrieved
PSD parameters, followed by uncertainties in particle model parameters
and, to a lesser extent, the uncertainties in the fall-speed model. Uncertainties attributable to assuming an exponential distribution
are negligible. The results indicate that improvements to PSD and
particle model a priori constraints provide the most impactful path
forward for reducing uncertainties in retrieved snowfall rates. Information
content analyses reveal that PSD slope is well-constrained by the
retrieval. Given the sensitivity of PSD slope to microphysical transformations,
the results show that such retrievals, when applied to radar reflectivity
profiles, could provide information about microphysical transformations
in the snowing column. The PSD intercept is less well-constrained by the retrieval. While applied to near-surface radar observations
in this study, the retrieval is applicable as well to radar observations
aloft, such as those provided by profiling ground-based, airborne,
and satellite-borne radars under lighter snowfall conditions when
attenuation and multiple scattering can be neglected.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e107">Radar observations focused on snowfall from platforms outside the
established weather surveillance radar networks have become ubiquitous
over the last 2 decades, largely due to increased interest in the role of snowfall in mid- and high-latitude microphysics, hydrology,
and climate. This research accelerated with the advent of satellite-borne
radars flown by missions to quantify global hydrometeor and precipitation
properties. These satellite-borne radars (specifically the CloudSat
mission's Cloud Profiling Radar (CPR) <xref ref-type="bibr" rid="bib1.bibx59" id="paren.1"/> and
the Global Precipitation Measurement (GPM) mission's Dual-frequency
Precipitation Radar (DPR) <xref ref-type="bibr" rid="bib1.bibx61" id="paren.2"/>, with two others
anticipated to launch in the coming decade) are capable solely of
measuring vertical profiles of radar reflectivity factor (hereafter,
reflectivity) along with path-integrated attenuation under certain conditions. To understand the capabilities of these satellite-borne
radars for quantifying snowfall, we must know how well radar reflectivity
observations constrain snowfall properties.</p>
      <?pagebreak page870?><p id="d1e116">To these ends, CloudSat and GPM have contributed to multiple field experiments
involving ground-based radars and designed to provide, in part, ground validation data for the radar remote sensing of snowfall: the Canadian CloudSat-CALIPSO Validation Project (C3VP) <xref ref-type="bibr" rid="bib1.bibx19" id="paren.3"/>, the Global
Precipitation Measurement (GPM) Cold-season Precipitation Experiment (GCPEx)
<xref ref-type="bibr" rid="bib1.bibx57" id="paren.4"/>, the Light Precipitation Validation
Experiment (LPVEx) <xref ref-type="bibr" rid="bib1.bibx49" id="paren.5"/>, the International Collaborative
Experiment during the PyeongChang 2018 Olympics and Paralympics (ICE-POP)
<xref ref-type="bibr" rid="bib1.bibx5" id="paren.6"/>, and the Olympic Mountains Experiment (OLYMPEx)
<xref ref-type="bibr" rid="bib1.bibx18" id="paren.7"/>.  These and a number of smaller, more focused field
campaigns <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx55" id="paren.8"/> have made extensive use
of small K-band profiling radars, e.g., METEK's  Micro Rain Radar <xref ref-type="bibr" rid="bib1.bibx26" id="paren.9"><named-content content-type="pre">MRR,</named-content></xref>, but several experiments, including C3VP, GCPEx, and ICE-POP, have deployed ground-based, W-band scanning, or profiling radars.
Although these ground-based radars may provide advanced capabilities such as
Doppler velocity measurement, their reflectivity measurements in snowfall are a
valuable resource for examining the capabilities of the satellite-borne radars
<xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx40" id="paren.10"/>.</p>
      <p id="d1e146">The ability of radar reflectivity to constrain snowfall properties,
however, has not been well-evaluated. Snowfall exhibits a wide range of microphysical characteristics that influence radar reflectivity
and snowfall rate. Most notable to casual observers are variations
in particle habits: pristine dendrites, needles, columns, plates, and bullets; aggregates of the same; pellets and graupel for example.
Underlying these differences in habit are variations in mass, and,
given a particular mass, variations in how mass is distributed within
the particle. Unlike longer-wavelength radars for which radar backscattering
properties of snow particles are sensitive primarily to particle mass,
at millimeter wavelengths those properties are additionally sensitive
to particle shape. Investigations of particle mass and area (an aspect
of shape) <xref ref-type="bibr" rid="bib1.bibx23 bib1.bibx24 bib1.bibx25 bib1.bibx69 bib1.bibx70 bib1.bibx13 bib1.bibx33 bib1.bibx44 bib1.bibx42 bib1.bibx14" id="paren.11"/>
have painstakingly determined the broad extent of these variations.
Along with differences in single-particle properties, populations
of falling snow particles vary substantially in their concentrations
with size (i.e., the spectral particle size distribution, PSD) based
on measurements from the ground <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx21 bib1.bibx11 bib1.bibx53 bib1.bibx4" id="paren.12"><named-content content-type="pre">e.g.,</named-content></xref> and, more recently, with the advent of imaging particle probes, from aircraft <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx9 bib1.bibx10 bib1.bibx3 bib1.bibx68 bib1.bibx15" id="paren.13"><named-content content-type="pre">e.g.,</named-content><named-content content-type="post">and references therein</named-content></xref>. The observed particle concentrations vary over several orders of magnitude.</p>
      <p id="d1e164">In radar-based remote sensing scenarios when these properties are
not known, these variations produce uncertainty in the relationship
between radar reflectivity factor (hereafter, reflectivity) and associated
water content and snowfall rate. A common approach to estimating this
uncertainty has been to evaluate modeled reflectivities, water contents, and snowfall rates using a range of assumed particle models and PSDs.
The results are often expressed using relationships between reflectivity
and snowfall rate (“<inline-formula><mml:math id="M1" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M2" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>” relationships) <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx27 bib1.bibx40 bib1.bibx41" id="paren.14"/>.
This approach allows the uncertainty in a retrieved snowfall rate
to be estimated, but the existing studies have not provided insight
into the dominant sources of uncertainty nor into the ability of observed
radar reflectivity to constrain various properties controlling the
snowfall rate. <xref ref-type="bibr" rid="bib1.bibx51" id="text.15"/>  examined uncertainties
and information content for radar observations of mixed- and ice-phase
regions of a convective storm but targeted radar systems with more advanced capabilities. <xref ref-type="bibr" rid="bib1.bibx36" id="text.16"/> used CloudSat and
aircraft observations to assess how uncertainties in the ice particle
mass-dimension relationship contribute to radar reflectivity forward
model uncertainties but used known, observed particle size distributions and did not examine the influence of the mass-dimension uncertainties
on snowfall retrieval performance.</p>
      <p id="d1e191">In this work, we provide uncertainty and information content analyses for
retrieving snowfall from observations of radar reflectivity at millimeter
wavelengths, focusing on W-band (94 GHz). The results are representative of the
general problem of estimating snowfall from such remote radar reflectivity
observations without supplementary collocated observations of snow particle
mass-dimension relationships, fall speeds, and particle size distributions. The results apply particularly to observations by the CPR <xref ref-type="bibr" rid="bib1.bibx59" id="paren.17"/>
and by the DPR's Ka-band radar, but also to reflectivity measurements from
ground-based radars such as the MRR <xref ref-type="bibr" rid="bib1.bibx26" id="paren.18"/> and the
Department of Energy Atmospheric Radiation Measurement (ARM) program's
Millimeter Wavelength Cloud Radar <xref ref-type="bibr" rid="bib1.bibx45" id="paren.19"/> and Ka-band ARM
Zenith Radar (KAZR) <xref ref-type="bibr" rid="bib1.bibx1" id="paren.20"/>.  The retrieval method used
here is the foundation for the retrieval used for CloudSat's 2C-SNOW-PROFILE
product; that application is the subject of a future companion paper.  Our
objectives here are to identify the snowfall properties that are best
constrained by such observations and the most significant sources of
uncertainty in the radar retrieval of snowfall. The results establish a
performance baseline for reflectivity-only observations of snowfall, indicate
where uncertainty reduction efforts should be focused, and suggest what
improvements to radar-observing systems could be most beneficial.</p>
      <p id="d1e206">The analyses use the optimal estimation (OE) retrieval technique <xref ref-type="bibr" rid="bib1.bibx52" id="paren.21"/>,
which inherently diagnoses information content and uncertainties in
retrieved quantities subject to specified uncertainties in measurements,
forward models, and a priori knowledge of the quantities to be retrieved
<xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx6" id="paren.22"/>. The retrieval produces
best estimates of snow size distribution parameters by using the radar reflectivity observations to refine a priori estimates of those parameters
(Sect. <xref ref-type="sec" rid="Ch1.S2"/>). The information content metrics
provided by OE require all sources of uncertainties in the retrieval
process to be specified. These are discussed in Sect. <xref ref-type="sec" rid="Ch1.S3"/>.
Ground-based radar and<?pagebreak page871?> precipitation observations allow the retrieval
to be tested, showing that size distribution width is best constrained
by the retrieval and that uncertainties in retrieved size distribution
parameters (but not uncertainties due to the assumed exponential form
of the PSD itself) are the strongest contributors to uncertainties
in estimated snowfall rates (Sect. <xref ref-type="sec" rid="Ch1.S4"/>).
The results suggest that the retrieved size distribution widths could
be useful for diagnosing changes in PSD resulting from microphysical
processes <xref ref-type="bibr" rid="bib1.bibx31" id="paren.23"/> and that improved observational
constraints on size distribution parameters, as might be provided
by dual-wavelength radar observations <xref ref-type="bibr" rid="bib1.bibx37" id="paren.24"/>, would
likely enhance snowfall retrieval performance (Sect. <xref ref-type="sec" rid="Ch1.S5"/>).</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Retrieval method</title>
      <p id="d1e238">The retrieval uses measurements of reflectivity to estimate snow microphysical
properties and to quantify water content and snowfall rate. At the
wavelengths characteristic of cloud radars such as CloudSat and shorter-wavelength
precipitation radars, scattering by precipitation-sized particles
does not follow the Rayleigh approximation, and both attenuation and
multiple scattering may affect the radar signal. At these wavelengths,
snow particle scattering and extinction properties depend not only
on mass, but on shape as well. With even simple parameterized expressions
for particle mass, shape, and size distribution, single-frequency observations of radar reflectivity alone are insufficient to reasonably
constrain the resulting set of parameters.</p>
      <p id="d1e241">To address this insufficiency, retrievals must incorporate a priori
information about particle microphysical and scattering properties.
This is accomplished here using OE <xref ref-type="bibr" rid="bib1.bibx52" id="paren.25"/>, a Bayesian
technique that allows a priori information to be included explicitly.
The input for this retrieval is the <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> observed by the radar
for a range gate identified as containing snow. For notational consistency
with other work, we show this as a vector:
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M4" display="block"><mml:mrow><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:msubsup><mml:mi>Z</mml:mi><mml:mrow><mml:mi>e</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">obs</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        A forward model <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> relates <inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="bold-italic">y</mml:mi></mml:math></inline-formula>
to <inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula>, a state vector of unknown properties to be retrieved,
as
          <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M8" display="block"><mml:mrow><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="bold-italic">ϵ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M9" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover></mml:math></inline-formula> are parameters not being retrieved but which
influence the forward model results. The forward model approximates
the true physical relation between <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="bold-italic">y</mml:mi></mml:math></inline-formula>, and
there are uncertainties associated with both the observations <inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="bold-italic">y</mml:mi></mml:math></inline-formula>
and the forward model parameters <inline-formula><mml:math id="M13" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula>. <inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="bold-italic">ϵ</mml:mi></mml:math></inline-formula>
represents the total uncertainty due to all sources. OE attempts to
find <inline-formula><mml:math id="M15" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula>, an estimate of the state which maximizes the
posterior conditional probability density function (PDF) <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>|</mml:mo><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
subject also to prior knowledge about the values of <inline-formula><mml:math id="M17" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula>. This
prior knowledge is described by expected values <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
and their covariances <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Assuming Gaussian statistics
for the model-measurement errors and the a priori state, minimizing
the cost function
          <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M20" display="block"><mml:mtable class="split" rowspacing="0.2ex" columnspacing="1em" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        with respect to <inline-formula><mml:math id="M21" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula> gives this PDF, where <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
is the covariance matrix representing the uncertainties <inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="bold-italic">ϵ</mml:mi></mml:math></inline-formula>.
The Gaussian assumption is reasonable if the expected values and covariance
matrices are known for the model-measurement uncertainties and the
a priori state, but other details are lacking. In that case, the Gaussian
form maximizes the entropy of a PDF <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx52" id="paren.26"/>.
Assuming an alternate form would introduce constraints on the retrieval
that are not justified based on the limited knowledge of the PDF.</p>
      <p id="d1e614">Provided the forward model is not excessively nonlinear, Newtonian
iteration
          <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M24" display="block"><mml:mtable columnspacing="1em" rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">K</mml:mi><mml:mi>i</mml:mi><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msubsup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced open="[" close="]"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">K</mml:mi><mml:mi>i</mml:mi><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msubsup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="bold-italic">F</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>i</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>-</mml:mo><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        leads to <inline-formula><mml:math id="M25" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula>, where <inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="bold">K</mml:mi></mml:math></inline-formula> is the Jacobian of the
forward model with respect to <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="bold">K</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.
Iteration continues until the squared difference in successive <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> normalized by the
current estimate of the a posteriori covariance <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold">S</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is much smaller than
the number of state vector elements <xref ref-type="bibr" rid="bib1.bibx52" id="paren.27"/>. At convergence, this covariance of <inline-formula><mml:math id="M31" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula> is obtained
as
          <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M32" display="block"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold">S</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mi mathvariant="bold">K</mml:mi><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. As a diagnostic
test of the results, a <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">χ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> statistic is calculated using the
retrieved state vector in Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). A value near
the number of observations suggests correct convergence <xref ref-type="bibr" rid="bib1.bibx35" id="paren.28"/>. Several metrics,
determined from the retrieved state and based on information theory, provide insight into the retrieval performance; these metrics are
presented in Sect. <xref ref-type="sec" rid="Ch1.S4"/>.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>The forward model</title>
      <?pagebreak page872?><p id="d1e980">To assess the information provided purely by reflectivity observations,
whether from ground-, aircraft-, or space-based radars, the retrieval
ignores attenuation and multiple scattering. This treatment would
be appropriate for cases with little intervening scattering and extinction
between the radar and observed snowfall, such as when the radar bin
containing the snowfall of interest is near the radar or under light
snowfall conditions. For such a case, the singly-scattered reflectivity
<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msubsup><mml:mi>Z</mml:mi><mml:mi>e</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> as a function of range <inline-formula><mml:math id="M36" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> from the radar is given
by
            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M37" display="block"><mml:mrow><mml:msubsup><mml:mi>Z</mml:mi><mml:mi>e</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Λ</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msup><mml:mfenced close="∥" open="∥"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">min</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:mrow></mml:munderover><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>D</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the backscatter cross section for particle size <inline-formula><mml:math id="M39" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> at range <inline-formula><mml:math id="M40" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the PSD at range <inline-formula><mml:math id="M42" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="normal">Λ</mml:mi></mml:math></inline-formula> is the radar wavelength, and <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
is the dielectric factor for water.</p>
<sec id="Ch1.S2.SS1.SSS1">
  <label>2.1.1</label><title>Forward model parameters: snow particle model</title>
      <p id="d1e1183">Backscattering and extinction cross sections depend intimately on particle mass, shape, and orientation relative to the radar beam. These properties are highly variable for snow particles, and the approach
used here is to specify their PDFs a priori using best estimates and
treat their variability as a source of uncertainty in the retrieval.
We adopt the common model <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx42" id="paren.29"><named-content content-type="pre">e.g.,</named-content></xref>
in which mass and horizontally projected area are described using power laws,

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M45" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>m</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:msubsup><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi><mml:mi mathvariant="italic">β</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:msubsup><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi><mml:mi mathvariant="italic">σ</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              on particle maximum dimension, <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and use the particle properties
and shape “B8pr-30” <xref ref-type="bibr" rid="bib1.bibx67" id="paren.30"/>, an idealized branched
spatial particle that was found to minimize bias in simulated reflectivities versus coincident W-band radar observations. That work used in situ measurements
and remotely sensed X-band reflectivity observations of snow from C3VP <xref ref-type="bibr" rid="bib1.bibx19" id="paren.31"/> along with previously reported single-particle measurements to develop
best estimates and covariances for the power-law parameters <inline-formula><mml:math id="M47" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M48" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M49" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>. These results then constrained
discrete dipole approximation calculations using DDSCAT <xref ref-type="bibr" rid="bib1.bibx7" id="paren.32"/>
to obtain best estimates of snow particle single-scattering properties
and their uncertainties at the desired wavelengths. These a priori
descriptions of size-resolved particle mass, <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and their uncertainties constitute the particle model used in the retrieval and are summarized in Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>The retrieved state</title>
      <p id="d1e1353">The relationship described by Eq. (<xref ref-type="disp-formula" rid="Ch1.E6"/>) requires
information about particle size distributions and single-scattering
properties. With scattering properties and their uncertainties specified
a priori as described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS1.SSS1"/>,
this leaves the snow PSD parameters and their PDFs to be determined
by the retrieval.</p>
      <p id="d1e1360">Snow PSDs are frequently characterized as exponential:
            <disp-formula id="Ch1.E9" content-type="numbered"><label>9</label><mml:math id="M54" display="block"><mml:mrow><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mi>D</mml:mi></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M55" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> is the slope of the distribution and <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> its
intercept. <xref ref-type="bibr" rid="bib1.bibx53" id="text.33"/> used photographs of snowflakes to
develop estimates of snow size distributions based on actual dimensions
and found snow size distributions to be exponential. <xref ref-type="bibr" rid="bib1.bibx4" id="text.34"/>
evaluated both exponential and gamma forms, which have the ability
to represent sub- or super-exponential behavior, for snow size distributions
observed by a 2D video disdrometer over the course of several winter
seasons. Although about 22 % of the observed snow distributions exhibited
super-exponential features, more commonly the fitted gamma distributions
were nearly equivalent to exponential distributions. Several aircraft-based
studies using in situ observations under a wide range of atmospheric
conditions have confirmed exponential behavior, especially at larger
particle sizes <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx17 bib1.bibx31 bib1.bibx9 bib1.bibx3 bib1.bibx68" id="paren.35"/>.
While other studies of aircraft observations have noted departures
from exponential behavior <xref ref-type="bibr" rid="bib1.bibx12" id="paren.36"><named-content content-type="pre">e.g., “super-” or “sub-exponential”,</named-content></xref>,
<xref ref-type="bibr" rid="bib1.bibx15" id="text.37"/> examined the suitability of exponential
distributions for snow. They found that fitted exponential distributions,
when used to simulate IWC and Ze, could provide generally good agreement
with IWC and Ze calculated directly from the observed discrete size
distributions. These studies support the adequacy of exponential distributions
for retrieving snowfall. <inline-formula><mml:math id="M57" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> may be an actual dimension of the snow
particle, the diameter of an equivalent mass ice sphere, or the melted
drop diameter. The choice is significant because <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M59" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>
depend on the choice of <inline-formula><mml:math id="M60" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula>. For this work, we use the maximum particle
dimension, <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, because <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is closely related to the particle
dimensions measured by imagers such as video disdrometers <xref ref-type="bibr" rid="bib1.bibx65" id="paren.38"/>
and aircraft particle probes, making comparisons with other datasets
more straightforward.</p>
      <p id="d1e1490">The exponential size distribution parameters <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M64" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>
are the desired state variables. Values for <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> may range over
several orders of magnitude, so <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is retrieved
instead. The variability of <inline-formula><mml:math id="M67" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> is significantly smaller than
that of <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; however, examination of fitted exponential distributions
from C3VP snow events indicated that the distribution of values for
<inline-formula><mml:math id="M69" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> was strongly non-Gaussian. The log-transformed values are
much less skewed (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a), and accordingly,
<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is retrieved instead. The corresponding state vector
to be retrieved is then
            <disp-formula id="Ch1.E10" content-type="numbered"><label>10</label><mml:math id="M71" display="block"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mfenced close="]" open="["><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          and the associated covariance matrix obtained from the retrieval is
of the form
            <disp-formula id="Ch1.E11" content-type="numbered"><label>11</label><mml:math id="M72" display="block"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold">S</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced open="[" close="]"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mtable class="array" columnalign="center"><mml:mtr><mml:mtd><mml:mrow><mml:mi>s</mml:mi><mml:mfenced close="" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mfenced open="" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mtable class="array" columnalign="center"><mml:mtr><mml:mtd><mml:mrow><mml:mi>s</mml:mi><mml:mfenced close="" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mfenced open="" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mtd><mml:mtd><mml:mrow><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1732"><bold>(a)</bold> Histograms of <inline-formula><mml:math id="M73" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> fitted to C3VP SVI observations. <bold>(b)</bold> Estimates of
<inline-formula><mml:math id="M75" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> determined from fits to size distributions
from C3VP observations, with values provided from several earlier
studies for comparison.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Prior estimates of the state</title>
      <?pagebreak page873?><p id="d1e1793">For each profile, the a priori state consists of a vector of expected
values <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the corresponding covariance matrix <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>,
having the same sizes as the state vector <inline-formula><mml:math id="M79" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula> (Eq. <xref ref-type="disp-formula" rid="Ch1.E10"/>)
and its covariance matrix <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Eq. <xref ref-type="disp-formula" rid="Ch1.E11"/>).
A priori estimates of <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>
are determined using temperature-based parameterizations derived using
snow PSDs observed during C3VP and other field experiments. Exponential
size distributions were fit to the observed size spectra from both
ground-based Snowflake Video Imager, or SVI <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx65" id="paren.39"/>,
and from 2D particle probes carried aboard the National Research Council
Canada's Convair-580 during three C3VP research flights (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b).
Results from a number of earlier studies are shown as well for comparison,
including ground-based observations taken in and near the Rocky Mountain
Front Range <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx4" id="paren.40"/>; and aircraft observations over the central Sierra Nevada <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx10" id="paren.41"/>, in lake effect snow over Lake Michigan <xref ref-type="bibr" rid="bib1.bibx3" id="paren.42"/>, in synoptic
snowfall over central Illinois <xref ref-type="bibr" rid="bib1.bibx48" id="paren.43"/>, and in orographic
and frontal wintertime precipitation in the Pacific Northwest <xref ref-type="bibr" rid="bib1.bibx68" id="paren.44"/>.
Also shown are similar fits performed on 2D probe observations from
a Wakasa Bay research flight on 27 January 2003 <xref ref-type="bibr" rid="bib1.bibx32" id="paren.45"/>.
The results suggest that the C3VP observations adequately represent
snowfall from a number of different regimes, although the number concentrations
from several studies are at the margins of the C3VP observations.</p>
      <p id="d1e1891"><?xmltex \hack{\newpage}?>Both <inline-formula><mml:math id="M83" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> have been observed to vary log-linearly
with temperature (e.g., <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx68" id="altparen.46"/>;
and works reviewed in <xref ref-type="bibr" rid="bib1.bibx54" id="altparen.47"/>). Fits were therefore constructed
for both parameters using the combined C3VP aircraft and SVI data
and uncertainties estimated using residual standard deviations (RSDs)
calculated for data binned into 2 K intervals (Fig. <xref ref-type="fig" rid="Ch1.F2"/>).
The narrow temperature ranges for the Wakasa Bay and <xref ref-type="bibr" rid="bib1.bibx4" id="text.48"/>
observations make comparisons against the C3VP temperature dependence
uninformative. For <inline-formula><mml:math id="M85" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>, the <xref ref-type="bibr" rid="bib1.bibx53" id="text.49"/> observations
are largely outside the bounds of the RSDs but are generally consistent with the C3VP histogram for warmer temperatures. The aircraft observations
other than Wakasa Bay follow a temperature trend similar to the C3VP
observations. For <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, several of the comparison datasets lie
mostly above the RSD bounds but would be well within a <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> RSD bound.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1958">Dependence of <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> on temperature. Central red lines show
the best-fit relationships, while the upper and lower blue lines show
bounds given by <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> residual standard deviation. The shaded gray
shows the 2D histogram of values for the C3VP surface and aircraft
observations (<bold>a</bold> and <bold>c</bold>). Symbols (<bold>b</bold> and <bold>d</bold>) match those
from Fig. <xref ref-type="fig" rid="Ch1.F1"/> except that, in lieu
of symbols for <xref ref-type="bibr" rid="bib1.bibx68" id="text.50"/>, the dashed black line shows
a linear best fit reported by the authors.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f02.png"/>

        </fig>

      <p id="d1e2022">Based on the similarity of C3VP to results from other experiments, the a priori states derived from these observations can be expected
to represent a broad range of snowfall regimes and were adopted for
the retrieval. A priori values for <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> were estimated from the linear fits as
            <disp-formula id="Ch1.E12" content-type="numbered"><label>12</label><mml:math id="M93" display="block"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">ap</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.03053</mml:mn><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">273</mml:mn><mml:mo>.</mml:mo><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.08258</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">ap</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.07193</mml:mn><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">273</mml:mn><mml:mo>.</mml:mo><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2.665</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          with <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> in <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M102" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> in <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>. The RSDs show little variation
with temperature except in the vicinity of 240 K, where they increase
substantially. These large RSDs are in response to a few outlying
samples with small <inline-formula><mml:math id="M104" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> values. Accordingly, variances
were treated as constant and were estimated as the squared RSDs averaged
over all temperatures. The uncertainty model also includes the covariance
between <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>.
Correlation coefficients were evaluated for each of the temperature-binned
data subsets, giving a mean coefficient of 0.72 with a standard deviation of 0.12. The a priori covariance was modeled as <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.72</mml:mn><mml:mo>⋅</mml:mo><mml:mi>s</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">ap</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>⋅</mml:mo><mml:mi>s</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi>a</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>:</mml:mo></mml:mrow></mml:math></inline-formula>
            <disp-formula id="Ch1.E13" content-type="numbered"><label>13</label><mml:math id="M109" display="block"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">ap</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.133</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">ap</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.95</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>s</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">ap</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi>a</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.26</mml:mn><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Implementation and uncertainty sources</title>
      <?pagebreak page874?><p id="d1e2428">Applying the exponential distribution in Eq. (<xref ref-type="disp-formula" rid="Ch1.E6"/>),
the singly-scattered non-attenuated reflectivity <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:msubsup><mml:mi/><mml:mi>e</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is
          <disp-formula id="Ch1.E14" content-type="numbered"><label>14</label><mml:math id="M111" display="block"><mml:mtable class="split" columnspacing="1em" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>Z</mml:mi><mml:msubsup><mml:mi/><mml:mi>e</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup><mml:mfenced open="(" close=")"><mml:mi>R</mml:mi></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Λ</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msup><mml:mfenced open="∥" close="∥"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi mathvariant="normal">M</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi mathvariant="normal">M</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">max</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:munderover><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        The backscatter cross section <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has been written to show its dependence on a vector of parameters <inline-formula><mml:math id="M113" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula> as well
as on <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The vector <inline-formula><mml:math id="M115" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover></mml:math></inline-formula> includes the parameters
for the mass- and area-dimension relations <inline-formula><mml:math id="M116" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M117" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M118" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>,
and <inline-formula><mml:math id="M119" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> which were used to construct the particle models from
which the scattering properties were calculated. The tilde indicates
that these parameters are approximations of the true values and a
source of uncertainty.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Model-measurement uncertainties</title>
      <p id="d1e2652">The error covariance matrix <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is
            <disp-formula id="Ch1.E15" content-type="numbered"><label>15</label><mml:math id="M121" display="block"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>F</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>B</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>F</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
          where <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the covariance matrix for the measurement
uncertainties and <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>F</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is that for the singly-scattered
reflectivities given in Eq. (<xref ref-type="disp-formula" rid="Ch1.E14"/>).
The forward-model uncertainties may be further decomposed as the sum
of two terms: <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>B</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, which is a covariance matrix describing
uncertainties due to the forward model parameters <inline-formula><mml:math id="M125" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula>,
and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>F</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, which is a covariance matrix describing
uncertainties due to other assumptions in the calculation of <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msubsup><mml:mi>Z</mml:mi><mml:mi>e</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>
<sec id="Ch1.S3.SS1.SSS1">
  <label>3.1.1</label><title>Uncertainties for measured reflectivities</title>
      <p id="d1e2808">The sources of reflectivity measurement error include errors in the absolute
radiometric calibration and measurement noise.  For this work, we assume the
radar is well-calibrated, leaving noise as the uncertainty source.  To
estimate <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, we model the noise using the well-characterized
CloudSat CPR <xref ref-type="bibr" rid="bib1.bibx59" id="paren.51"/>. For reflectivities above
<inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> dBZ, 1 standard deviation of noise as a fraction of the mean signal is about <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">16</mml:mn></mml:mrow></mml:math></inline-formula> dB, while for reflectivities below <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> dBZ, noise
is an increasing fraction of the signal, reaching 0 dB at the minimum
detectable signal of <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> dBZ (Richard T. Austin, personal communication, 4 November 2008). The resulting uncertainties range from 3 dBZ for
a reflectivity of <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> dBZ to about 0.1 dBZ for reflectivities above
<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2896">Estimated measurement
uncertainty, based on 1 standard deviation of noise for the CloudSat CPR.</p></caption>
            <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f03.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <label>3.1.2</label><title>Forward model uncertainties</title>
      <?pagebreak page875?><p id="d1e2913">Uncertainties <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>B</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> due to the forward model parameters
<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:mfenced><mml:mi mathvariant="monospace">T</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>
that describe the snow particle model were examined in <xref ref-type="bibr" rid="bib1.bibx67" id="text.52"/>
as
              <disp-formula id="Ch1.E16" content-type="numbered"><label>16</label><mml:math id="M137" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>B</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>b</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>b</mml:mi></mml:msub><mml:msubsup><mml:mi mathvariant="bold">K</mml:mi><mml:mi>b</mml:mi><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the Jacobian of the forward model reflectivities with
respect to the parameters <inline-formula><mml:math id="M139" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the
covariance matrix for the parameters. The Jacobian <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> depends on
the estimated state <inline-formula><mml:math id="M142" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula> and is computed at each iterative step.  At
each step, the forward model is used to calculate reflectivity perturbations
that result from perturbations of the parameters <inline-formula><mml:math id="M143" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M144" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M145" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>,
and <inline-formula><mml:math id="M146" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>.  The ratio of each reflectivity perturbation to its parameter
perturbation gives an element of the Jacobian.  The parameter perturbation
affects the reflectivity via changes to the corresponding particle scattering
properties.  The perturbed scattering properties are precomputed with DDSCAT
<xref ref-type="bibr" rid="bib1.bibx7" id="paren.53"/> by using the perturbed parameter to generate
discrete dipole models following the process described in <xref ref-type="bibr" rid="bib1.bibx67" id="text.54"/>.  <xref ref-type="bibr" rid="bib1.bibx67" id="text.55"/> found the resulting forward
model uncertainties to be near 5 dB, increasing to as high as 15 dB for very
broad distributions.</p>
      <p id="d1e3090"><inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>F</mml:mi><mml:mi mathvariant="normal">ss</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> quantifies uncertainties due to other assumptions
and limitations in the forward model reflectivity calculation. <xref ref-type="bibr" rid="bib1.bibx67" id="text.56"/>
looked at uncertainties due to the random component of dipole placement
within discrete dipole approximation (DDA) models for a particular particle shape and found them negligible. Other sources include the assumption of the shape of the distribution as exponential, the choice of particle shape, and the discretization
and truncation of the integrations over size distribution.</p>
      <p id="d1e3108">Errors due to the assumed exponential shape were evaluated using a
dataset of 4080 SVI-measured, discrete, 5 min-long snow PSDs from C3VP. Simulated reflectivities and snowfall rates were calculated
using the B8pr-30 particle model and the <xref ref-type="bibr" rid="bib1.bibx43" id="text.57"/>
terminal velocity model. Exponential distributions were fit to the
observed discrete PSDs using orthogonal distance regression <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx22" id="paren.58"/>
with uncertainty estimates per <xref ref-type="bibr" rid="bib1.bibx65" id="text.59"/>. The fitted
distributions were scaled in number concentration to match the snowfall
rates simulated from the discrete distributions. The fitted distributions
were then used to simulate reflectivities for comparison against those
from the discrete distributions. Errors are negligible at high reflectivities
but increase as reflectivity decreases (Fig. <xref ref-type="fig" rid="Ch1.F4"/>).
Bias is negligible, and the total uncertainty is modeled as
              <disp-formula id="Ch1.E17" content-type="numbered"><label>17</label><mml:math id="M148" display="block"><mml:mrow><mml:msubsup><mml:mi>s</mml:mi><mml:mi>F</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mfenced open="(" close=")"><mml:mi mathvariant="normal">dB</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mo>-</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:mfenced><mml:mo>/</mml:mo><mml:mn mathvariant="normal">16</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            reaching a maximum of 1 dB of uncertainty at <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e3188">Actual rms errors and the fitted model for uncertainty due to the assumed exponential size distribution.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f04.png"/>

          </fig>

      <p id="d1e3197">Uncertainties due to shape were evaluated using the same SVI dataset
to which the alternate particle shapes Ep (ellipsoidal) and B8pr-45
(branched spatial particle with a larger aspect ratio than B8pr-30) from <xref ref-type="bibr" rid="bib1.bibx67" id="text.60"/> were applied to simulate reflectivities.
These alternate shapes are constrained to have the same mass-dimension
relationship as used for the B8pr-30 particle model used in this work,
so differences are due only to particle shape. Figure <xref ref-type="fig" rid="Ch1.F5"/>
shows total and variance-only rms errors. From these results we estimate the shape uncertainty to be 2 dB.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e3207">Errors in reflectivity for the
Ep and B8pr-45 shapes compared to the B8pr-30 shape. Errors shown
are total (bias <inline-formula><mml:math id="M150" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> variance) and variance only.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f05.png"/>

          </fig>

      <p id="d1e3223">Finally, truncation and discretization errors were evaluated using
the same SVI PSD dataset. These are errors that result from the discrete
treatment of the integrations over size distribution, errors due to both the limited maximum <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the particle model and in the limited resolution of the particle model. Truncation errors were evaluated
using analytic exponential PSDs fitted to the SVI PSD dataset as<?pagebreak page876?> described
previously. The particle model backscatter properties were augmented
to <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">40</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> by linearly extrapolating backscatter
efficiencies, and then reflectivities were calculated using integrations to both the standard (maximum <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">18</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula>) and augmented
size ranges. The bias and scatter of the truncation errors were <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> and 0.42 dB. To evaluate discretization errors, a high-resolution
version of the particle model backscatter properties was created by
interpolating backscatter efficiencies so that the particle size resolution
of the particle model was increased by a factor of 2. Reflectivities were then calculated and compared against those from the standard-resolution
particle model. The bias and scatter of the discretization errors
were 0.00 and 0.02 dB.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e3285">Histograms of errors for truncation
and discretization.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f06.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Snowfall rate and uncertainties</title>
      <p id="d1e3303">The snowfall rate <inline-formula><mml:math id="M155" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula> in units of liquid water depth per unit time
is
            <disp-formula id="Ch1.E18" content-type="numbered"><label>18</label><mml:math id="M156" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9.0}{9.0}\selectfont$\displaystyle}?><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">liq</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi mathvariant="normal">M</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi mathvariant="normal">M</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">max</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:munderover><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mi>m</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:mfenced><mml:mi>V</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:mfenced><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is particle mass, <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mi>V</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is fall speed, and <inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">liq</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the density of liquid water. Particle mass is
provided by Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>). Fall speed is assumed to equal terminal velocity, which is calculated from the model of <xref ref-type="bibr" rid="bib1.bibx43" id="text.61"/>
using particle mass, the horizontally projected area from Eq. (<xref ref-type="disp-formula" rid="Ch1.E8"/>), and environmental pressure and temperature from collocated observations.
Uncertainties for the estimated snowfall rate are determined in a
manner similar to that used for the forward model uncertainties. The
total variance <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is decomposed as
            <disp-formula id="Ch1.E19" content-type="numbered"><label>19</label><mml:math id="M161" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where the terms on the right represent the variances resulting from (1)
retrieved state uncertainties, (2) particle model parameter uncertainties, (3)
uncertainties in the fall-speed model and its parameters, and (4) assuming an exponential form for the PSD, respectively.</p>
      <p id="d1e3556">Contributions from uncertainties in the retrieved state and in the particle
model parameters are determined using linearized error propagation (e.g.,
following a form like Eq. <xref ref-type="disp-formula" rid="Ch1.E16"/>).  For
<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, which gives the snowfall rate variance that results
from uncertainties in the particle model parameters, this means that the
Jacobian <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is calculated for the snowfall rate with
respect to the particle model parameters <inline-formula><mml:math id="M164" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M165" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M166" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>, and
<inline-formula><mml:math id="M167" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, following the process described for the reflectivity Jacobian in
Sect. <xref ref-type="sec" rid="Ch1.S3.SS1.SSS2"/>.  Then
            <disp-formula id="Ch1.E20" content-type="numbered"><label>20</label><mml:math id="M168" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>b</mml:mi></mml:msub><mml:msubsup><mml:mi mathvariant="bold">K</mml:mi><mml:mrow><mml:mover accent="true"><mml:mi>b</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mo>,</mml:mo><mml:mi>P</mml:mi></mml:mrow><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the covariance matrix for the particle model
parameters as determined in <xref ref-type="bibr" rid="bib1.bibx67" id="text.62"/>.</p>
      <p id="d1e3700"><?xmltex \hack{\newpage}?>Fall-speed contributions are handled following <xref ref-type="bibr" rid="bib1.bibx66" id="text.63"/>. Snowfall rate uncertainties
due to the assumed exponential form of the size distribution are determined
using the SVI PSD dataset in an approach analogous to that for Eq. (<xref ref-type="disp-formula" rid="Ch1.E17"/>).
In this approach, number concentrations for the fitted exponential
distributions were scaled so that reflectivities were matched, and then snowfall rate errors were evaluated. The fractional uncertainty in
snowfall rate was found to be
            <disp-formula id="Ch1.E21" content-type="numbered"><label>21</label><mml:math id="M170" display="block"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.06</mml:mn><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi>P</mml:mi></mml:mfenced><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          from which the necessary variance can be determined. Uncertainties
from each of the four sources are treated as uncorrelated.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Retrieval performance tests with ground-based radar observations</title>
      <p id="d1e3746">During C3VP, a vertically pointing W-band radar (the Jet Propulsion Laboratory's Airborne Cloud Radar, ACR) was deployed on the ground at CARE. In
all, about 28 h of ACR radar profiles of snowfall were recorded at
approximately 2.8 s intervals. These observations represent 17 distinct snow
events that occurred over 18 d between 3 November 2006 and 2 March 2007;
however, most of the accumulations were concentrated during nine of the events
(Table <xref ref-type="table" rid="Ch1.T1"/>).  These observations include portions
of three of the cases that were used to develop the snow particle microphysical
models (cases SYN1, LES1, and LES2, <xref ref-type="bibr" rid="bib1.bibx67" id="altparen.64"/>).  Of the nearly
36 000 ACR profiles in these observations, approximately 7300 are from cases
SYN1, LES1, and LES2.  Further, as described in <xref ref-type="bibr" rid="bib1.bibx67" id="text.65"/>, ACR reflectivities from 12 of the events between 2 December 2006 and 26 February 2007 were used to constrain the snow particle models' scattering properties to give unbiased reflectivities.  This overlap should be kept in mind when evaluating
the retrieved snowfall rates and estimated accumulation, but it should not
substantially affect the assessments of retrieval uncertainties, uncertainty sources, and information content metrics that follow.</p>
      <p id="d1e3757">The retrieval was applied to the ACR reflectivities observed in the
single range bin nearest the surface, at 197 m above ground level
(AGL). Temperatures and pressures needed by the retrieval to perform
snow detection, calculate fall speeds, and establish the a priori states were obtained from nearby surface meteorology observations. Because of the short distance to the target range bin, attenuation along the
path was neglected.  The retrieved snowfall rates produce a <inline-formula><mml:math id="M171" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M172" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>
relationship that is most similar to that developed by
<xref ref-type="bibr" rid="bib1.bibx27" id="text.66"/> for an aggregate particle model denoted
as the <xref ref-type="bibr" rid="bib1.bibx16" id="text.67"/> aggregate (HA) (Fig. <xref ref-type="fig" rid="Ch1.F7"/>).  For warmer temperatures and mid-range reflectivities, the <inline-formula><mml:math id="M173" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M174" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> relationship becomes more similar to that of <xref ref-type="bibr" rid="bib1.bibx30" id="text.68"/> and the LR3 relationship of Kulie and Bennartz.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e3802"><inline-formula><mml:math id="M175" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M176" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> values as a function of
temperature for this retrieval compared against those from  M07, <xref ref-type="bibr" rid="bib1.bibx38" id="text.69"/>; L08, <xref ref-type="bibr" rid="bib1.bibx30" id="text.70"/>; and KB09_LR3, KB09_HA,
and KB09_SS, <xref ref-type="bibr" rid="bib1.bibx27" id="text.71"/>.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f07.png"/>

      </fig>

      <?pagebreak page877?><p id="d1e3834"><?xmltex \hack{\newpage}?>For comparisons, snowfall rate observations were
obtained at 1 min intervals from the Vaisala FD12P <xref ref-type="bibr" rid="bib1.bibx62" id="paren.72"/>
and scaled to provide unbiased accumulations relative to the nearby
Dual Fence Intercomparison Reference, or DFIR <xref ref-type="bibr" rid="bib1.bibx8" id="paren.73"/>.
The retrieved ACR snowfall rates, <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, were matched to the
nearest-in-time observed snowfall rate, <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Table}?><label>Table 1</label><caption><p id="d1e3874">Accumulations by event for the ACR
retrievals. Duration shows the elapsed time of ACR observations
for which retrievals were performed. Fractional differences are relative
to FD12P accumulations.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry rowsep="1" namest="col3" nameend="col5" align="center">Accumulations </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Date</oasis:entry>
         <oasis:entry colname="col2">Duration</oasis:entry>
         <oasis:entry colname="col3">ACR</oasis:entry>
         <oasis:entry colname="col4">FD12P</oasis:entry>
         <oasis:entry colname="col5">Fractional</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M182" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry namest="col3" nameend="col4" align="center"><?xmltex \hack{\hspace*{8mm}}?><inline-formula><mml:math id="M183" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> LWE </oasis:entry>
         <oasis:entry colname="col5">difference, %</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">3 Nov 2006</oasis:entry>
         <oasis:entry colname="col2">0.98</oasis:entry>
         <oasis:entry colname="col3">0.065</oasis:entry>
         <oasis:entry colname="col4">0.11</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">40.9</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2 Dec 2006</oasis:entry>
         <oasis:entry colname="col2">0.16</oasis:entry>
         <oasis:entry colname="col3">0.007</oasis:entry>
         <oasis:entry colname="col4">0.00</oasis:entry>
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">6 Dec 2006</oasis:entry>
         <oasis:entry colname="col2">4.00</oasis:entry>
         <oasis:entry colname="col3">0.86</oasis:entry>
         <oasis:entry colname="col4">0.80</oasis:entry>
         <oasis:entry colname="col5">7.5 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">7 Dec 2006</oasis:entry>
         <oasis:entry colname="col2">1.08</oasis:entry>
         <oasis:entry colname="col3">0.038</oasis:entry>
         <oasis:entry colname="col4">0.093</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">59.1</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">8 Dec 2006</oasis:entry>
         <oasis:entry colname="col2">0.34</oasis:entry>
         <oasis:entry colname="col3">0.018</oasis:entry>
         <oasis:entry colname="col4">0.00</oasis:entry>
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">17 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">0.09</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.3</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">04</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.00</oasis:entry>
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">19 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">0.46</oasis:entry>
         <oasis:entry colname="col3">0.061</oasis:entry>
         <oasis:entry colname="col4">0.13</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">53.1</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">20 Jan 2007<inline-formula><mml:math id="M188" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">0.32</oasis:entry>
         <oasis:entry colname="col3">0.004</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.8</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">04</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">1329 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">20 Jan 2007<inline-formula><mml:math id="M190" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">0.59</oasis:entry>
         <oasis:entry colname="col3">0.079</oasis:entry>
         <oasis:entry colname="col4">0.0</oasis:entry>
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">22 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">4.29</oasis:entry>
         <oasis:entry colname="col3">0.89</oasis:entry>
         <oasis:entry colname="col4">0.87</oasis:entry>
         <oasis:entry colname="col5">2.2 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">23 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">0.76</oasis:entry>
         <oasis:entry colname="col3">0.017</oasis:entry>
         <oasis:entry colname="col4">0.00</oasis:entry>
         <oasis:entry colname="col5">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">26 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">0.93</oasis:entry>
         <oasis:entry colname="col3">0.045</oasis:entry>
         <oasis:entry colname="col4">0.085</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">47.1</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">27 Jan 2007</oasis:entry>
         <oasis:entry colname="col2">3.36</oasis:entry>
         <oasis:entry colname="col3">0.57</oasis:entry>
         <oasis:entry colname="col4">1.06</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">46.2</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">19 Feb 2007</oasis:entry>
         <oasis:entry colname="col2">0.97</oasis:entry>
         <oasis:entry colname="col3">0.26</oasis:entry>
         <oasis:entry colname="col4">0.18</oasis:entry>
         <oasis:entry colname="col5">44.4 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">22 Feb 2007</oasis:entry>
         <oasis:entry colname="col2">2.72</oasis:entry>
         <oasis:entry colname="col3">0.40<inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.23<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">73.9 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">26 Feb 2007</oasis:entry>
         <oasis:entry colname="col2">2.41</oasis:entry>
         <oasis:entry colname="col3">0.58</oasis:entry>
         <oasis:entry colname="col4">0.64</oasis:entry>
         <oasis:entry colname="col5">9.4 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1 Mar 2007</oasis:entry>
         <oasis:entry colname="col2">4.23</oasis:entry>
         <oasis:entry colname="col3">1.14<inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">1.57<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">27.4</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Season</oasis:entry>
         <oasis:entry colname="col2">26.3</oasis:entry>
         <oasis:entry colname="col3">5.04<inline-formula><mml:math id="M198" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">5.77<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12.6</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e3877">Two distinct events, indicated as <inline-formula><mml:math id="M179" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula>, occurred
on 20 January 2007. <inline-formula><mml:math id="M181" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> Accumulations
adjusted to remove anomalies indicated in Fig. <xref ref-type="fig" rid="Ch1.F8"/>.</p></table-wrap-foot></table-wrap>

      <p id="d1e4465">Time series of <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> show a high degree of agreement over
most of the observing period (Fig. <xref ref-type="fig" rid="Ch1.F8"/>a). This is not extraordinary given the dependence of the retrieval's particle microphysical
and scattering properties on portions of the C3VP data.  Two notable exceptions
occur near time indices 25 000 and 32 500, however, when the FD12P recorded
snowfall rates above 1 <inline-formula><mml:math id="M203" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> LWE <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, while the retrieved values are substantially smaller. Examining the time series of ACR
reflectivities shows that the ACR did not observe high reflectivities during
these periods (Fig. <xref ref-type="fig" rid="Ch1.F8"/>b). The first of these anomalies occurred on 22 February 2007 from 11:20 to 12:05 UTC, while the second occurred on 1 March 2007 between 22:15 and 22:50 UTC. For both, the ACR operator made note of the heavy snowfall, suggesting that both the
FD12P and the ACR observed similar snowfall rates.
Based on soundings, Environment Canada forecasts, and ACR operator
observations, these anomalies appear to correspond to melting aloft, ice pellets, and freezing rain <xref ref-type="bibr" rid="bib1.bibx63" id="paren.74"/>.  These conditions could also have
been favorable for formation of large, heavy aggregates.  It seems likely that
the conditions produced snowfall whose properties were strongly inconsistent
with the particle properties assumed in the retrieval, although reflectivities
did not change substantially.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e4532"><bold>(a)</bold> Time series
of snowfall rates retrieved from ACR reflectivities and observed.
<bold>(b)</bold> Corresponding time series of ACR reflectivities. Each
time index indicates a 2.8 s observation by the ACR. Snowfall rates
retrieved for the ACR used the reflectivity in the range bin nearest
the surface, at 197 m AGL.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f08.png"/>

      </fig>

      <?pagebreak page879?><p id="d1e4546">Accumulations were calculated from both <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with and
without the two anomalies described above (Fig. <xref ref-type="fig" rid="Ch1.F9"/>).  Accumulations agree
substantially during the first 16 h but diverge somewhat beyond that, again
noting the dependence of the retrieval's assumed microphysical and scattering
properties on portions of the C3VP data. With the anomalies included the final
difference between the accumulations is 2 <inline-formula><mml:math id="M208" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula>. With the anomalies removed
that difference is reduced to 0.7 <inline-formula><mml:math id="M209" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula>. For individual events, absolute
fractional differences between the ACR and FD12P accumulations can range to
50 % and upwards (Table <xref ref-type="table" rid="Ch1.T1"/>), but these large values
are associated mainly with events with small accumulations.  For events with
larger accumulations, the absolute fractional differences are mostly below
30 %. At seasonal timescales, the random components in event-total
accumulations are likely uncorrelated, leading to offsetting errors when
calculating seasonal accumulations. The time series of absolute fractional
differences between the ACR-derived and FD12P accumulations begins with large
fractional differences. Within 5 h and over the initial three events, the
fractional differences reduce to less than 5 % and then remain below 20 % for the remainder of the season.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e4600">Snow accumulations
computed from <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. The accumulations are for
17 snow events observed by the ACR on 18 d between 3 November 2006
and 2 March 2007, but accumulations are principally from nine events
(Table <xref ref-type="table" rid="Ch1.T1"/>). The events were concatenated
sequentially in time, and the time axis indicates the cumulative time over all events. <bold>(a)</bold> Accumulations from all observations and corresponding
retrieval results, <bold>(b)</bold> accumulations with two anomalous periods identified
in Fig. <xref ref-type="fig" rid="Ch1.F8"/> removed, and
<bold>(c)</bold> fractional differences in accumulations shown in <bold>(b)</bold>, with
distinct colors indicating individual events.</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f09.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Snowfall rate uncertainties</title>
      <p id="d1e4660">Uncertainties in instantaneous snowfall rate estimates, taken to be
the square root of the total variance evaluated as shown in Eq. (<xref ref-type="disp-formula" rid="Ch1.E19"/>),
were evaluated by binning the fractional uncertainties by snowfall
rate and then averaging and taking standard deviations. Mean fractional uncertainties range from 150 % to 185 %, and the range for <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> standard
deviation extends from about 145 % to 190 % (Fig. <xref ref-type="fig" rid="Ch1.F10"/>).
The fractional uncertainties generally increase with increasing snowfall
rate, but above 0.5 <inline-formula><mml:math id="M213" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> LWE <inline-formula><mml:math id="M214" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M215" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> the means and standard deviations
diminish and result from only a small number of samples in each bin.
For comparison, uncertainties for FD12P precipitation rates at 5 min
resolution were estimated at 0.03 <inline-formula><mml:math id="M216" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M217" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M218" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for rates
less than 0.05 <inline-formula><mml:math id="M219" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M220" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M221" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, 50 % for rates up to 0.5 <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M224" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and 30 % for rates larger than 0.5 <inline-formula><mml:math id="M225" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M227" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
by <xref ref-type="bibr" rid="bib1.bibx66" id="text.75"/> based on comparisons against the Precipitation Occurrence Sensor System.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e4819">Instantaneous fractional uncertainties
in snowfall rate. The central line shows mean fractional uncertainties
and the error bars show <inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> standard deviation.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f10.png"/>

        </fig>

      <p id="d1e4838">To evaluate the importance of each source of uncertainty, variances
from each of the sources from Eq. (<xref ref-type="disp-formula" rid="Ch1.E19"/>) (retrieved state, microphysical parameters, fall-speed parameterization, or exponential distribution) were extracted separately, and then fractions of total variance
were calculated. To allow the trends in each source to be shown as
a function of snowfall rate (Fig. <xref ref-type="fig" rid="Ch1.F11"/>),
the fractions were binned by snowfall rate and averaged. As snowfall
rates increase up to 0.5 <inline-formula><mml:math id="M229" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M230" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M231" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, the variance due
to the retrieved state becomes a more significant contributor to the
total variance, while the contributions from the other sources diminish.
The contribution due to the assumed exponential PSD shape is not significant.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e4875">Instantaneous fractional
variances for snowfall rate resolved by source.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f11.png"/>

        </fig>

      <p id="d1e4884">The instantaneous uncertainties for snowfall rate include uncertainties
due to random errors and biases in the retrieval components and observations.
For accumulations or mean rates evaluated over longer time periods,
errors due to random sources may be reduced and remaining errors can
be more representative of biases in the retrieval. The reductions
in random errors depend on their correlations in time, however <xref ref-type="bibr" rid="bib1.bibx60" id="paren.76"><named-content content-type="pre">e.g.,</named-content></xref>. When random errors within events are assumed perfectly positively
correlated, end-of-event <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulations have fractional
uncertainties from 1.5 % to 52.4 % (Fig. <xref ref-type="fig" rid="Ch1.F12"/>).
In actuality, the random error sources likely decorrelate with increasing
separation in time. While the scales for these decorrelations are
not known, with<?pagebreak page880?> even a modest amount of decorrelation in the errors
the uncertainties are reduced substantially. After applying a negative
exponential decorrelation model with a decorrelation scale of 0.5 h to intra-event errors, the fractional uncertainties at the ends
of individual events are 1.3 % to 18.8 %. The most significant reductions
due to decorrelation occur with the longer-duration events. The end-of-season
<inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulation uncertainties, calculated assuming inter-event
uncertainties are uncorrelated, are reduced from 64.9 % for perfectly
correlated to 11.8 % for decorrelated intra-event errors.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e4918">End-of-event accumulations and uncertainties.
The <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulation uncertainties are estimated assuming intra-event
errors are perfectly correlated (orange) and decorrelated using a
negative exponential model with a decorrelation scale of 0.5 h
(purple). <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> accumulations (blue-green) are shown for comparison
except for those equal to zero, which are omitted. For clarity, the <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulations are plotted at <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.02</mml:mn></mml:mrow></mml:math></inline-formula> h (purple/orange)
of their actual durations.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f12.png"/>

        </fig>

      <p id="d1e4975">Agreement between observed <inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> event accumulations and those
from <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> generally improves for events with larger accumulations
and durations (Fig.<xref ref-type="fig" rid="Ch1.F12"/>). Of the seven
events with accumulations larger than 0.2 <inline-formula><mml:math id="M240" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> and durations of 1 <inline-formula><mml:math id="M241" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>
and longer, the <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> accumulations for six fall within or
near the uncertainty bounds of the <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulations with perfectly
correlated errors, while four out of seven are within or near the
much narrower bounds for errors with decorrelations. This result is
also true for the season as a whole. For the duration of 26.3 h
and accumulation of 5.05 <inline-formula><mml:math id="M244" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> from <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the difference compared
to the <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">FD</mml:mi><mml:mn mathvariant="normal">12</mml:mn><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> seasonal accumulation of 5.77 <inline-formula><mml:math id="M247" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula> is <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12.6</mml:mn></mml:mrow></mml:math></inline-formula> %. The
difference is similar to the <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi mathvariant="normal">ACR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> accumulation uncertainty of
11.7 % for decorrelated errors.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Information content</title>
      <p id="d1e5124">The optimal estimation results allow easy calculation of a number
of metrics that quantify retrieval performance in terms of information
content <xref ref-type="bibr" rid="bib1.bibx52 bib1.bibx56" id="paren.77"/>. These include
the averaging kernel matrix
            <disp-formula id="Ch1.E22" content-type="numbered"><label>22</label><mml:math id="M250" display="block"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi mathvariant="sans-serif">T</mml:mi></mml:msup><mml:msubsup><mml:mi mathvariant="bold">S</mml:mi><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold">K</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          the Shannon information content
            <disp-formula id="Ch1.E23" content-type="numbered"><label>23</label><mml:math id="M251" display="block"><mml:mrow><mml:mi>H</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msub><mml:mi>log⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mfenced close="|" open="|"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold">S</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>x</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          and the degrees of freedom for signal
            <disp-formula id="Ch1.E24" content-type="numbered"><label>24</label><mml:math id="M252" display="block"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi>S</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Tr</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="bold">A</mml:mi></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          Briefly, the diagonal values of <inline-formula><mml:math id="M253" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula> indicate the degree to
which the corresponding retrieved state variables are determined by
the observations (values nearer 1) versus by the a priori (values nearer 0). <inline-formula><mml:math id="M254" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> measures how well the observations serve to narrow the possible retrieved states in comparison to the a priori state. Its value can be interpreted as describing the binary bits of resolution of the observing system
<xref ref-type="bibr" rid="bib1.bibx28" id="paren.78"/>. <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi>S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> quantifies the number of independent
quantities that are determined by the observations. See <xref ref-type="bibr" rid="bib1.bibx52" id="text.79"/>
for a more complete discussion in the context of retrieval theory.</p>
      <p id="d1e5303">For the ACR retrievals, values for <inline-formula><mml:math id="M256" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> vary between 0.4 and 1.2 (Fig. <xref ref-type="fig" rid="Ch1.F13"/>), indicating that the measurements
resolve between 1.3 and 2.3 distinct states. Values for <inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi>s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> show
that the retrieval produces somewhat less than one independent piece
of information that is significant compared to the measurement and
forward model uncertainties. Figure <xref ref-type="fig" rid="Ch1.F13"/>c, d show the diagonal elements of <inline-formula><mml:math id="M258" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula>. While the element relevant
to <inline-formula><mml:math id="M259" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, is
consistently positive, the element for <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M262" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, is near zero and is at times negative. These results show that <inline-formula><mml:math id="M263" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> is moderately to strongly constrained by the reflectivity observation,
while <inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is largely dependent on the a priori
constraint.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e5416">Distributions of information
content metrics for the ACR retrieval. </p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f13.png"/>

        </fig>

      <?pagebreak page881?><p id="d1e5426">The size distribution plays a significant role in determining the
values of these metrics. Information content <inline-formula><mml:math id="M265" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> increases as the distribution
narrows (Fig. <xref ref-type="fig" rid="Ch1.F14"/>a). The increase in <inline-formula><mml:math id="M266" display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> accompanies a substantial increase in the magnitude of the
sensitivity of the forward model to <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F14"/>b). In contrast, the sensitivity to <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> has a constant value of
10 owing to the reflectivity in <inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being a linear function of
<inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> (and so is not shown in Fig. <xref ref-type="fig" rid="Ch1.F14"/>).  This increased
sensitivity to <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> allows the observed reflectivity to
better constrain the retrieved state, particularly the value of
<inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>. As a result,
<inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> increases from 0.4 to 0.95 as
<inline-formula><mml:math id="M274" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> increases (Fig. <xref ref-type="fig" rid="Ch1.F14"/>c). The behavior of <inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F14"/>d) is quite different.
The values are small and are positive for small values of <inline-formula><mml:math id="M276" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> but become negative as <inline-formula><mml:math id="M277" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> increases.  This behavior results from the positive a
priori correlation between <inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and the opposing signs of the sensitivities of <inline-formula><mml:math id="M280" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to these two variables. While the forward model is
strongly sensitive to <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>, its sensitivity to
<inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is 3–4 times smaller in magnitude.  Consequently, the
retrieved value of <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> is influenced more strongly by
the observations, while the retrieved value of <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is
influenced more by the a priori estimate of the state. This difference is
reflected in panels (c) and (d) of Fig. <xref ref-type="fig" rid="Ch1.F14"/>.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F14"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e5679">Information
content metrics and the forward model Jacobian as functions of <inline-formula><mml:math id="M285" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f14.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Discussion and conclusions</title>
      <p id="d1e5705">While millimeter-wavelength, single-frequency radar reflectivity observations
alone would seem to have limited utility for retrieving snowfall properties,
the results herein demonstrate capabilities for quantifying snowfall
rate, accumulation, and aspects of the snow PSD. The results were obtained by applying the radar observations to constrain a priori information
appropriate to a broad range of snowfall regimes. The results indicate
that the approach would provide useful information when applied to
observations such as those from satellite-borne radars, which observe
a range of snowfall regimes and for which radar observables are limited
to reflectivity.</p>
      <?pagebreak page882?><p id="d1e5708">The results demonstrate the ability of the retrieval to produce reliable
estimates of snow accumulation, particularly over timescales involving multiple events and more than several hours of snowfall duration, in spite of
large uncertainties in retrieved instantaneous snowfall rates. For the C3VP
season, the retrieval reproduced the observed accumulation within 13 % at the
end of the season. These results were achieved by omitting two particular time
periods during which the retrieval's particle property assumptions were likely
very inconsistent with the observed snowfall. Without this adjustment, the
end-of-season absolute difference was 18.9 %, illustrating the need for
adequate discrimination of the precipitation phase in the retrieval process.
Keeping in mind that certain a priori assumptions of the retrieval were also
sourced from the C3VP observations, these results are probably best viewed as
indicating proper function of the retrieval.  The time series of seasonal
accumulation shows that while the initial fractional differences reach almost
80 %, the differences diminish with time and increasing accumulation, reaching
values of less than 5 % within 5 h. These results are partly due to offsetting errors between events; however, for individual events, best
agreement between the observed and retrieved snow accumulations were achieved
for events that were longer in duration and produced more substantial
accumulations. The observed accumulations for these events were mostly near or
within the tighter uncertainty bounds produced by a decorrelating error model
applied to the retrieved accumulation.  The modest decorrelation used in the
model produces uncertainties in the retrieved event accumulations of only 1 %
to 20 %. Thus, despite large instantaneous snowfall rate uncertainties for these single-frequency, millimeter-wavelength retrievals, retrieved rates can be
expected to prove of value for quantifying accumulations over events, months, seasons, and longer.</p>
      <p id="d1e5711">Uncertainties in instantaneous retrieval-estimated snowfall rate are
dominated by uncertainties in the retrieved state (the uncertainties
in the estimated PSD), followed by uncertainties in particle model
parameters and, to a lesser extent, the uncertainties in the fall-speed model. Uncertainties due to the assumption of an exponential PSD form are negligible. There is a degree of ambiguity here. The uncertainties
in the particle model parameters contribute to the uncertainties in
the estimated snowfall rate due to the appearance of the mass term
in Eq. (<xref ref-type="disp-formula" rid="Ch1.E18"/>) but also contribute to uncertainties
in the retrieved state. We treat these as independent contributions
to the uncertainty. There is likely some covariance that could reduce
total uncertainties, but this is not addressed in the treatment of snowfall rate uncertainty presented here.</p>
      <p id="d1e5716">Retrieval performance, quantified in terms of information content
metrics, is determined by the sensitivity of the observations to the
desired state vector, the uncertainties assessed for the forward models
and measurements, and the explicit assumptions about the uncertainty
in the a priori knowledge of the state. For W-band modeled reflectivities
in dB, the magnitudes of sensitivities for <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> are 3–4 times those for <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, and sensitivities
are opposite in sign. This contributes to <inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>
being better constrained by the retrieval than is <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>.
The consequences of these sensitivities are described more fully in
Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>. To the extent that process
information can be gleaned from changes in the slope parameter over
time or space, the retrieval may be useful for process analyses when
more direct observations of PSD are not available.</p>
      <p id="d1e5774">Model-measurement uncertainties are dominated by uncertainties in
the particle model parameters (e.g., the coefficients and exponents
of the mass- and area-dimension relationships, Table <xref ref-type="table" rid="Ch1.T2"/>),
and it is the uncertainties in mass parameters that are the most substantial
contributor <xref ref-type="bibr" rid="bib1.bibx67" id="paren.80"/>. For these near-surface observations,
contributions to uncertainties in W-band radar reflectivity from shape,
the assumption of an exponential form for the PSD, and the discrete-truncated
form of the integrations over size distribution were not significant.
For longer wavelength radars that might be used in similar applications
(e.g., the MRR or KAZR), shape uncertainty will likely be even smaller due to less prevalent non-Rayleigh scattering.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Table}?><label>Table 2</label><caption><p id="d1e5785">Contributions to uncertainties in
forward-modeled and observed reflectivity.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="center"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Source</oasis:entry>
         <oasis:entry colname="col2">Reflectivity, dB</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Observed reflectivity</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Particle model</oasis:entry>
         <oasis:entry colname="col2">5–15</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Shape</oasis:entry>
         <oasis:entry colname="col2">2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Assumed exponential</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Truncation</oasis:entry>
         <oasis:entry colname="col2">0.42</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Discretization</oasis:entry>
         <oasis:entry colname="col2">0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Random dipole locations</oasis:entry>
         <oasis:entry colname="col2">0</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e5892">These baseline results suggest several avenues for improving such
single-frequency, radar reflectivity-based snowfall retrievals. Improved
constraints on snow PSD parameters, through either reduced a priori
uncertainties or better observational constraints, are paramount.
For ground- or aircraft-based observations, ancillary measurements
of snow PSDs can improve the a priori constraints. For retrievals
from satellite-borne radar where such measurements are not available,
the a priori state is given by more broadly applicable relationships
for PSD parameters like those presented here. To the extent that a
priori states for specific snowfall regimes might have smaller uncertainties,
knowledge of regime-specific PDFs for snow PSD parameters would improve
retrieval results provided the correct regime can be diagnosed by
the retrieval. Coincident dual-frequency radar observations may also
provide improved constraints on the snow PSD parameters <xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx39" id="paren.81"/>
but among current satellite-borne instruments, the CPR is single-frequency,
and while the GPM DPR provides dual-frequency observations, the DPR
sensitivities limit observations to heavier snowfall <xref ref-type="bibr" rid="bib1.bibx58" id="paren.82"/>
and implementation of dual-frequency snowfall retrieval has proven
difficult <xref ref-type="bibr" rid="bib1.bibx20" id="paren.83"/>. Finally, model-measurement uncertainties
can be reduced by reducing uncertainties in particle mass estimates.
This may require a more synergistic approach in which improved PSD
information is coupled with additional observations such as Doppler
velocity to better constrain the assumed particle model used in the
retrieval, e.g., moving toward the approach used by <xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx67" id="text.84"/>
with ground-based observations. The methods presented here, easily
adaptable to other observing systems providing multiple frequency
or collocated Doppler velocity observations, provide the basis from
which such improvements can be tested and evaluated.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<?pagebreak page883?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Retrieval interpretation</title>
      <p id="d1e5919">To interpret the behavior of the retrieval, we refer to the discussion
of the information content metrics (Sect. <xref ref-type="sec" rid="Ch1.S4.SS2"/>).
The small values for <inline-formula><mml:math id="M292" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
indicate its value is determined primarily by the a priori information
and the negative signs do not fit the normal paradigm used to explain
the <inline-formula><mml:math id="M293" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula> matrix. Their explanation reveals details of the significant
behavior of this retrieval. In the application of the retrieval to
a single radar bin, the value of <inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
is given by
          <disp-formula id="App1.Ch1.S1.E25" content-type="numbered"><label>A1</label><mml:math id="M295" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{8.5}{8.5}\selectfont$\displaystyle}?><mml:mtable columnspacing="1em" rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mfenced open="[" close=""><mml:mrow><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>N</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:msup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced open="" close="]"><mml:mrow><mml:mi>s</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi>N</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mover accent="true"><mml:mi mathvariant="italic">λ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mfenced></mml:mrow></mml:mfenced><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mphantom style="vphantom"><mml:mpadded style="vphantom" width="0pt"><mml:msup><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mpadded></mml:mphantom></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msup><mml:mfenced open="[" close="]"><mml:mrow><mml:msubsup><mml:mi>s</mml:mi><mml:mi>y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable><?xmltex \hack{$\egroup}?></mml:mrow></mml:math></disp-formula>
        where the carets indicate retrieved values. In the first set of brackets
on the right side, the sign of the first term is clearly positive,
while that of the second term depends on the signs of the covariance
and the two partial derivatives, which are the elements of the Jacobian
of the forward model. As was shown earlier (Fig. <xref ref-type="fig" rid="Ch1.F14"/>),
<inline-formula><mml:math id="M296" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> is positive
while <inline-formula><mml:math id="M297" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> is
negative. The covariance for the retrieved state changes very little
from the a priori covariance, which is positive and represents a substantial
correlation between <inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>.
This second term, then, is negative and as the magnitude of <inline-formula><mml:math id="M300" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula>
increases, the sign of <inline-formula><mml:math id="M301" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
changes from positive to negative.</p>
      <p id="d1e6299">These terms represent competing influences on the retrieved value
of <inline-formula><mml:math id="M302" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>. These competing influences arise from
the a priori covariance and from the Jacobian of the forward model.
The positive covariance requires that a positive adjustment in <inline-formula><mml:math id="M303" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>
be accompanied by a positive adjustment in <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>.
In contrast, the Jacobian terms have differing signs. If the difference
between the observed and forward model reflectivity calls for a positive
adjustment to <inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>, the corresponding adjustment
to <inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> would be negative.</p>
      <p id="d1e6369">Figure <xref ref-type="fig" rid="App1.Ch1.S1.F15"/> shows this process schematically.
The size distribution that represents the initial state is shown by
the soid line. Assuming that the forward modeled reflectivity for
this state overestimates the observed reflectivity (a positive error),
two responses are possible: <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> could be increased,
narrowing the distribution; and <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> could be
decreased, reducing the amplitude of the distribution. Absent the
covariance between <inline-formula><mml:math id="M309" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>,
the retrieval would apply both adjustments, likely giving more weight
to the adjustment of <inline-formula><mml:math id="M311" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> because of the stronger
sensitivity of the forward model to that variable. These adjustments
are represented by the heavy arrows labeled <inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>. Because of the positive covariance
between <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>,
however, an increase in <inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> produces an opposing
response that increases <inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, shown by the upward-pointing
heavy arrow. The resulting size distribution is shown by the dashed
line.</p>
      <p id="d1e6521">For small <inline-formula><mml:math id="M318" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (broad distributions), the magnitude of <inline-formula><mml:math id="M319" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula>
is relatively small, so the covariance-driven adjustment is small
and does not overcome the initial reduction in <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>.
In these cases, <inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> decreases in response to
a positive error in the modeled reflectivity. This net response is
consistent with the sensitivity of the forward model to <inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M323" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced open="[" close="]"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> is positive. For
large <inline-formula><mml:math id="M324" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (narrower distributions), the magnitude of <inline-formula><mml:math id="M325" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:msub><mml:mi mathvariant="normal">dBZ</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula>
is larger. The covariance-driven adjustment is larger also and does
overcome the initial reduction in <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>. As a
result, <inline-formula><mml:math id="M327" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> increases in response to the positive
error in the modeled reflectivity. Since this net response opposes
the sensitivity of the forward model, <inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:mi mathvariant="bold">A</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
is negative.</p>
      <p id="d1e6699">The combination of the strong positive covariance between <inline-formula><mml:math id="M329" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and the comparatively weak sensitivity
of the reflectivity to <inline-formula><mml:math id="M331" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> limits the behavior
of the retrieval. For narrower distributions, the retrieval is prevented
from simultaneously increasing <inline-formula><mml:math id="M332" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and decreasing
<inline-formula><mml:math id="M333" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> in response to a positive error in reflectivity.
The opposing behavior, decreasing <inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and
increasing <inline-formula><mml:math id="M335" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> in response to a negative error
in reflectivity, is also restricted. While correct in a climatological
sense since <inline-formula><mml:math id="M336" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M337" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
are positively correlated, in nature there are likely scenes for which
such responses would give a more accurate retrieval. This reasoning
demonstrates how other measurements, specifically those with better
sensitivity to <inline-formula><mml:math id="M338" display="inline"><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, would benefit the retrieval.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.S1.F15"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e6839">Schematic illustration of the
retrieval process. The solid line represents the initial state of
the retrieval, while the dashed line shows the adjusted state assuming the initial state overestimates the observed reflectivity. The arrows
labeled <inline-formula><mml:math id="M339" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">λ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M340" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
show the expected responses of the retrieval based on the sensitivities
of the forward model. The arrow labeled <inline-formula><mml:math id="M341" display="inline"><mml:mrow><mml:mi>s</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>o</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>
shows the response due to positive covariance between <inline-formula><mml:math id="M342" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://amt.copernicus.org/articles/14/869/2021/amt-14-869-2021-f15.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>

<?pagebreak page884?><app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><title>Particle model</title>
      <p id="d1e6935">The properties here are for the particle shape denoted as “B8pr-30”
from <xref ref-type="bibr" rid="bib1.bibx67" id="text.85"/>, an idealized eight-arm branched spatial particle. Values for the parameters of the mass- and area-dimension
power functions are
          <disp-formula id="App1.Ch1.S2.Ex1"><mml:math id="M344" display="block"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">α</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.723</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.248</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">γ</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.379</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.813</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
        with error covariance matrix
          <disp-formula id="App1.Ch1.S2.Ex2"><mml:math id="M345" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">S</mml:mi><mml:mi>b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mtable class="matrix" columnalign="center center center center" framespacing="0em"><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.592</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.212</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.090</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.023</mml:mn></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.212</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.142</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.011</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.007</mml:mn></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.090</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.011</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.335</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.103</mml:mn></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mn mathvariant="normal">0.023</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.007</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.103</mml:mn></mml:mtd><mml:mtd><mml:mn mathvariant="normal">0.046</mml:mn></mml:mtd></mml:mtr></mml:mtable><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        These values are appropriate for use with particle size <inline-formula><mml:math id="M346" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
in centimeters, mass in grams and area in square centimeters. The
radar backscatter and extinction cross sections are given in Table <xref ref-type="table" rid="App1.Ch1.S2.T3"/> versus particle size.</p>

<?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S2.T3" specific-use="star"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{B1}?><?xmltex \def\figurename{Table}?><label>Table B1</label><caption><p id="d1e7087">Backscatter and extinction
properties for the snow particle model.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="center"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="center"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:colspec colnum="7" colname="col7" align="center"/>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M350" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M351" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">bk</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry rowsep="1" colname="col1"><inline-formula><mml:math id="M353" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col2"><inline-formula><mml:math id="M354" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M355" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col3"><inline-formula><mml:math id="M356" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M357" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M358" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col6"><inline-formula><mml:math id="M359" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M360" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col7"><inline-formula><mml:math id="M361" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M362" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.025</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M363" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.16253</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">17</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M364" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.52024</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">3.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M365" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.60708</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M366" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.31323</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.050</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M367" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.20475</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M368" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.77890</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">3.250</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M369" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.64139</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M370" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.21088</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.075</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M371" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.27182</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M372" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.00664</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">3.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M373" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.66119</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M374" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.22600</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.100</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M375" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.06847</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M376" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.89618</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">4.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M377" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.55864</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M378" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.74061</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.125</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M379" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.40498</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M380" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.67138</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">4.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M381" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.77554</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M382" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.11609</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.150</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M383" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.92314</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M384" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.58903</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">5.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M385" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.06798</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.58860</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.200</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M387" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.17250</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M388" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.30976</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">5.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M389" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.93705</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M390" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.00667</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.250</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M391" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.91396</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M392" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.14038</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">6.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M393" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.04092</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M394" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.83080</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.300</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M395" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.35436</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.48681</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">6.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M397" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.75512</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M398" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.35067</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.350</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.56280</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.25304</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">7.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.49787</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M402" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.13047</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.400</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M403" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.54761</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M404" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.31046</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">7.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.30734</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.10512</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.450</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M407" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.58963</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M408" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.69409</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">8.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M409" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.13418</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M410" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.07034</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.500</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M411" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.11161</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M412" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.52071</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">8.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.88081</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M414" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.06213</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.600</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M415" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.93929</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M416" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.16523</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">9.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.94080</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M418" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.59293</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.700</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.75650</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M420" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.00793</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">9.500</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M421" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.01596</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M422" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.74101</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.800</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M423" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.06043</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M424" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.20526</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">10.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.07686</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M426" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.12076</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">0.900</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M427" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.97542</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M428" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.93081</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">11.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M429" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.33291</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M430" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.46061</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1.000</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M431" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.65231</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M432" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.27755</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">12.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M433" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.94999</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M434" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.90676</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1.250</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M435" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.82454</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M436" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.67311</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">13.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M437" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.45403</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M438" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.27318</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1.500</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M439" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.56830</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.30096</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">14.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M441" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.63279</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M442" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.81244</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1.750</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M443" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.83188</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M444" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.75812</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">15.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M445" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.90939</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M446" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.58772</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2.000</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M447" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.34684</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M448" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.01675</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">09</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">16.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M449" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.39329</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M450" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.18269</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2.250</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M451" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.10293</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M452" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.33794</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">17.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M453" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.07551</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">07</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M454" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.86569</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2.500</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.38623</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M456" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.90102</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5">18.000</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M457" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.05353</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M458" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.83543</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">06</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2.750</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M459" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.50482</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M460" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.53761</mml:mn><mml:mi>e</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">08</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e9066">Most data used in this work, particularly those from C3VP, have been compiled and made available in <xref ref-type="bibr" rid="bib1.bibx64" id="text.86"/> (<uri>https://doi.org/10.5281/zenodo.4302575</uri>).  Other data are available in the
literature cited herein.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e9078">TSL'E and NBW developed the retrieval method from an initial concept by TSL'E.
NBW performed the analyses and prepared the manuscript with contributions from TSL'E.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e9084">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e9090">Work by Tristan S. L'Ecuyer and Norman B. Wood was performed at the University of Wisconsin–Madison and at Colorado State University for the Jet Propulsion Laboratory,
California Institute of Technology, sponsored by the National Aeronautics
and Space Administration.  We extend our appreciation to Peter Rodriguez and David Hudak of Environment and Climate Change Canada for managing and making available C3VP observations used in this work.  We thank Max Maahn
and two anonymous reviewers for providing their feedback on this paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e9095">This research has been supported by the National Aeronautics and Space Administration, Jet Propulsion Laboratory (grant no. G-39690-1).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e9101">This paper was edited by Alexis Berne and reviewed by Maximilian Maahn and two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>What millimeter-wavelength radar reflectivity reveals about snowfall:  an information-centric analysis</article-title-html>
<abstract-html><p>The ability of single-frequency, millimeter-wavelength radar reflectivity
observations to provide useful constraints for retrieval of snow particle
size distribution (PSD) parameters, snowfall rates, and snowfall accumulations
is examined. An optimal estimation snowfall retrieval that allows
analyses of retrieval uncertainties and information content is applied
to observations of near-surface W-band reflectivities from multiple
snowfall events during the 2006–2007 winter season in southern Ontario.
Retrieved instantaneous snowfall rates generally have uncertainties
greater than 100&thinsp;%, but single-event and seasonal snow accumulations
from the retrieval results match well with collocated
measurements of accumulations. Absolute fractional differences are
mainly below 30&thinsp;% for individual events that have more substantial
accumulations and, for the season, 12.6&thinsp;%. Uncertainties in retrieved
snowfall rates are driven mainly by uncertainties in the retrieved
PSD parameters, followed by uncertainties in particle model parameters
and, to a lesser extent, the uncertainties in the fall-speed model. Uncertainties attributable to assuming an exponential distribution
are negligible. The results indicate that improvements to PSD and
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