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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-9-1993-2016</article-id><title-group><article-title>Evaluation of three lidar scanning strategies for <?xmltex \hack{\break}?>turbulence measurements</article-title>
      </title-group><?xmltex \runningtitle{Evaluation of three lidar scanning strategies for turbulence measurements}?><?xmltex \runningauthor{J. F. Newman et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff6">
          <name><surname>Newman</surname><given-names>Jennifer F.</given-names></name>
          <email>jennifer.newman@nrel.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Klein</surname><given-names>Petra M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Wharton</surname><given-names>Sonia</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff8">
          <name><surname>Sathe</surname><given-names>Ameya</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4533-0551</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff7">
          <name><surname>Bonin</surname><given-names>Timothy A.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Chilson</surname><given-names>Phillip B.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Muschinski</surname><given-names>Andreas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Meteorology, University of Oklahoma, Norman, OK,
USA </institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Atmospheric, Earth and Energy Division, Lawrence Livermore
National Laboratory, Livermore, CA, USA </institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>DTU Wind Energy, Risø Campus, Roskilde, Denmark</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Advanced Radar Research Center, University of Oklahoma,
Norman, OK, USA </institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>NorthWest Research Associates, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff6"><label>a</label><institution>now at: National Wind Technology Center, National Renewable
Energy Laboratory, Golden, CO, USA</institution>
        </aff>
        <aff id="aff7"><label>b</label><institution>now at: Cooperative Institute for Research in the
Environmental Sciences, University of Colorado, and National Oceanic
and Atmospheric Administration/Earth System Research Laboratory,
Boulder, CO, USA</institution>
        </aff>
        <aff id="aff8"><label>c</label><institution>now at: DONG Energy, Copenhagen, Denmark</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jennifer F. Newman (jennifer.newman@nrel.gov)</corresp></author-notes><pub-date><day>3</day><month>May</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>5</issue>
      <fpage>1993</fpage><lpage>2013</lpage>
      <history>
        <date date-type="received"><day>23</day><month>October</month><year>2015</year></date>
           <date date-type="rev-request"><day>24</day><month>November</month><year>2015</year></date>
           <date date-type="rev-recd"><day>18</day><month>April</month><year>2016</year></date>
           <date date-type="accepted"><day>20</day><month>April</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016.html">This article is available from https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016.pdf</self-uri>


      <abstract>
    <p>Several errors occur when a traditional Doppler beam swinging (DBS) or
velocity–azimuth display (VAD) strategy is used to measure turbulence with
a lidar. To mitigate some of these errors, a scanning strategy was recently
developed which employs six beam positions to independently estimate the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> velocity variances and covariances. In order to assess the
ability of these different scanning techniques to measure turbulence, a Halo
scanning lidar, WindCube v2 pulsed lidar, and ZephIR continuous wave lidar
were deployed at field sites in Oklahoma and Colorado with collocated sonic
anemometers.</p>
    <p>Results indicate that the six-beam strategy mitigates some of the errors
caused by VAD and DBS scans, but the strategy is strongly affected by errors
in the variance measured at the different beam positions. The ZephIR and
WindCube lidars overestimated horizontal variance values by over 60 %
under unstable conditions as a result of variance contamination, where
additional variance components contaminate the true value of the variance.
A correction method was developed for the WindCube lidar that uses variance
calculated from the vertical beam position to reduce variance contamination
in the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance components. The correction method reduced
WindCube variance estimates by over 20 % at both the Oklahoma and
Colorado sites under unstable conditions, when variance contamination is
largest. This correction method can be easily applied to other lidars that
contain a vertical beam position and is a promising method for accurately
estimating turbulence with commercially available lidars.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Atmospheric turbulence, a measure of small-scale fluctuations in wind speed,
impacts a number of fields, including air quality
<xref ref-type="bibr" rid="bib1.bibx11" id="paren.1"><named-content content-type="pre">e.g.,</named-content></xref>, aviation <xref ref-type="bibr" rid="bib1.bibx9" id="paren.2"><named-content content-type="pre">e.g.,</named-content></xref>, and
numerical weather prediction <xref ref-type="bibr" rid="bib1.bibx5" id="paren.3"><named-content content-type="pre">e.g.,</named-content></xref>. In particular,
lidar-measured turbulence is a significant parameter in the wind energy
industry, where high-resolution measurements are often needed in remote
locations. Wind power production can differ substantially as a result of
turbulence <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx10" id="paren.4"><named-content content-type="pre">e.g.,</named-content></xref>, and
turbulence can induce damaging loads on the turbine blades, reducing the
turbine's reliability and expected lifetime <xref ref-type="bibr" rid="bib1.bibx19" id="paren.5"><named-content content-type="pre">e.g.,</named-content></xref>.
Thus, turbulence is an extremely important parameter to measure in the wind
farm site selection and design process.<?xmltex \hack{\newpage}?></p>
      <p>In the wind power industry, turbulence is typically estimated from cup
anemometer measurements on meteorological towers. Measurements from cup
anemometers are limited by tower height and can be plagued by issues with
overspeeding and slow response times, which can lead to inaccurate mean wind
speed and turbulence measurements <xref ref-type="bibr" rid="bib1.bibx18" id="paren.6"/>. Sonic
anemometers can measure turbulence much more accurately than cup anemometers
but are also limited by tower height. In response to these issues, remote
sensing devices, such as sodars (sound detection and ranging) and lidars
(light detection and ranging), have recently emerged as a promising
alternative to anemometers on towers. Although the ability of wind lidars to
accurately measure mean horizontal wind speeds has been well-documented in
the literature
<xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx32 bib1.bibx30 bib1.bibx2 bib1.bibx25 bib1.bibx37" id="paren.7"><named-content content-type="pre">e.g.,</named-content></xref>,
the measurement of turbulence with lidars is still an active area of research
<xref ref-type="bibr" rid="bib1.bibx35" id="paren.8"/>.</p>
      <p>While cup anemometers measure wind speed at a small point in space, remote
sensing devices report an average wind speed from a probe volume (typically
30–150 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> in the vertical) and usually take measurements less
frequently than tower-mounted instruments. These differences in spatial and
temporal resolution lead to differences in the turbulence measured by cup
anemometers and remote sensing devices <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx45 bib1.bibx22" id="paren.9"><named-content content-type="pre">e.g.,</named-content></xref>. While turbulent scales of motion
can range from milliseconds to hours and from centimeters to kilometers
<xref ref-type="bibr" rid="bib1.bibx41" id="paren.10"><named-content content-type="pre">e.g.,</named-content></xref>, lidars are only capable of measuring turbulent
motions with timescales on the order of seconds and spatial scales on the
order of tens of meters. In addition to differences in spatial and temporal
sampling, the scanning strategy used by the remote sensing device can also
induce errors in the different turbulence components
<xref ref-type="bibr" rid="bib1.bibx34" id="paren.11"/>.</p>
      <p>Most commercially available lidars employ a Doppler beam swinging
<xref ref-type="bibr" rid="bib1.bibx40" id="paren.12"><named-content content-type="pre">DBS;</named-content></xref> technique or a velocity–azimuth display
<xref ref-type="bibr" rid="bib1.bibx6" id="paren.13"><named-content content-type="pre">VAD;</named-content></xref> technique to collect wind speed
measurements. Using lidar DBS and VAD scans, the variances of the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>,
and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> velocity components are not directly measured; rather, the DBS and
VAD techniques combine radial velocity measurements from different points
around the scanning circle to calculate instantaneous values of the velocity
components. The time series of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> are then used to calculate
the velocity variances, whereby it is implicitly assumed that the
instantaneous velocity values are constant across the scanning circle. In
turbulent flow, this assumption is not valid even if the mean flow is
homogenous across the scanning circle, and the standard DBS and VAD approach
for computing variances is thus flawed by variance contamination errors
<xref ref-type="bibr" rid="bib1.bibx34" id="paren.14"/>. A different variance calculation approach was
proposed by <xref ref-type="bibr" rid="bib1.bibx33" id="text.15"/> using a novel six-beam scanning technique,
which utilizes the radial velocity variance values from six lidar beam
positions to independently calculate the six unique components of the
Reynolds stress tensor, i.e., the velocity variances and covariances.</p>
      <p><xref ref-type="bibr" rid="bib1.bibx37" id="text.16"/> evaluated the six-beam technique at the Danish National
Test Center for Large Wind Turbines in Høvsøre, Denmark, using the
WindScanner lidar developed at Denmark Technical University.
<xref ref-type="bibr" rid="bib1.bibx37" id="text.17"/> found that the six-beam technique measured higher values
of variance than the VAD technique for all stability classes, with values
that were greater in magnitude and closest to the cup anemometer values under
stable conditions. These findings are in contrast to observations presented
by <xref ref-type="bibr" rid="bib1.bibx36" id="text.18"/> for the same site, which indicates that lidars measure
much larger values of variance under unstable conditions due to the larger
turbulent motions present under these conditions. <xref ref-type="bibr" rid="bib1.bibx37" id="text.19"/>
attribute this difference to the wind directions selected for each of the
studies; while only westerly wind directions were analyzed in the six-beam
study, <xref ref-type="bibr" rid="bib1.bibx36" id="text.20"/> analyzed only data that were associated with
easterly wind directions. Since the WindScanner used by <xref ref-type="bibr" rid="bib1.bibx37" id="text.21"/>
was located 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> east of the coast of the North Sea, data from the
westerly wind direction could be influenced by the land–sea transition. As
discussed by <xref ref-type="bibr" rid="bib1.bibx37" id="text.22"/>, this transition likely caused an internal
boundary layer to develop, which, in conjunction with the current atmospheric
stability regime, would affect the turbulent scales of motion intercepted by
the lidar and the cup anemometer.</p>
      <p>The six-beam technique, like the DBS and VAD techniques, is affected by
volume averaging within the lidar probe volume. All three of these techniques
also assume the three-dimensional flow is horizontally homogeneous across the
scanning circle used by the lidar, which is often not a valid assumption
<xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx24" id="paren.23"><named-content content-type="pre">e.g.,</named-content></xref>, especially in complex
terrain <xref ref-type="bibr" rid="bib1.bibx3" id="paren.24"><named-content content-type="pre">e.g.,</named-content></xref>. All lidar scanning strategies are
subject to sources of error, and the magnitude of these errors is largely
dependent on atmospheric stability, measurement height, and the particular
type of lidar used <xref ref-type="bibr" rid="bib1.bibx36" id="paren.25"><named-content content-type="pre">e.g.,</named-content></xref>. Wind energy developers and
researchers must know how accurately their lidar can measure turbulence under
different conditions if they want to use turbulence information for resource
assessment or site suitability studies.</p>
      <p>The main goals of this study are to evaluate the accuracy of lidar turbulence
measurements and to provide guidance about lidar scanning strategies for wind
energy applications. To this end, three main research questions are addressed
in this work: (1) how well do two commonly used scanning strategies (the DBS
and VAD techniques) measure turbulence under different stability conditions?
(2) How well does the new six-beam technique measure turbulence under
different stability conditions? (3) Can new data processing techniques
reduce the errors in velocity variance calculations from lidar DBS scans? To
address these questions, turbulence measured with the various techniques is
compared to turbulence measured by three-dimensional sonic anemometers on tall towers at
sites in Oklahoma and Colorado. Sonic anemometer data from the Boulder
Atmospheric Observatory (BAO) in Colorado are used to quantify the additional
terms that occur as a result of variance contamination and to develop
improved data processing techniques that reduce variance contamination
errors. Data from the Southern Great Plains Atmospheric Radiation
Measurement (ARM) site in Oklahoma provide a second location to test the new
processing techniques with the DBS scan.</p>
      <p>To the authors' knowledge, this work represents the first time the six-beam
technique has been experimentally validated with high-frequency sonic
anemometers and commercially available lidars. The use of commercially
available lidars allows for an evaluation of turbulence measured with lidar
technologies and scanning strategies that are commonly employed in the wind
energy industry.</p><?xmltex \hack{\vspace{-3mm}}?>
</sec>
<sec id="Ch1.S2">
  <title>Lidar scanning strategies and estimation of turbulence parameters</title>
<sec id="Ch1.S2.SS1">
  <title>Current lidar technology</title>
      <p>One frequently used lidar in the wind energy industry is the Leosphere
WindCube lidar, a pulsed Doppler lidar that emits short pulses of laser
energy to measure radial wind speed. The time series of the returned signal
is then split up into blocks that correspond to range gates and processed to
estimate the average radial wind speed at each range gate. The sign and
magnitude of the radial wind speed are determined from the Doppler shift of
the returned signal with respect to the original signal
<xref ref-type="bibr" rid="bib1.bibx17" id="paren.26"/>. The Leosphere WindCube v2 model was used in
this work.</p>
      <p>Another type of Doppler lidar using pulsed 1.5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> lasers is the
Halo Streamline manufactured by Halo Photonics (Pearson et al., 2009). The
Halo Streamline (thereafter referred to as Halo lidar) is a scanning lidar,
which allows the user to configure and choose different types of scanning
routines. In our study, the Halo was used to evaluate both a six-beam and a VAD
scanning technique, which are further detailed in the next section.</p>
      <p>Unlike the WindCube and Halo lidars, the ZephIR is a continuous wave lidar
and focuses the laser beam at different heights to obtain wind speed
measurements. The ZephIR must collect velocity measurements individually at
each measurement height, so it takes approximately 15 s to complete a full
volumetric scan with 10 measurement heights. The probe length of the focused
ZephIR beam increases with height and, thus, the size of the range gates is
not constant. (The probe length is approximately 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> at a range of
100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, but much smaller closer to the ground;
<xref ref-type="bibr" rid="bib1.bibx39" id="altparen.27"/>.) The ZephIR continuously receives
backscattered radiation, so it can collect data at ranges as low as
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. However, the ZephIR cannot determine the direction of the
Doppler shift in the received time series, and there is a 180<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
ambiguity in the wind direction. The ZephIR 300, which was used in this work,
has an attached met station with wind direction measurements, which can
provide an estimate for the remotely measured wind direction
<xref ref-type="bibr" rid="bib1.bibx39" id="paren.28"/>. However, this estimated wind direction was not
always accurate during our field campaign in Colorado, and wind direction
information from the sonic anemometers had to be used to correct the ZephIR
wind direction measurements.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>General conventions</title>
      <p>In this work, we follow standard meteorological conventions for <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and
<inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> is the east–west component (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>u</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> for wind coming from the
west), <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> is the north–south component (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> for wind coming from the
south), and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> is the vertical component (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> for upward motion). Lidar
data are presented using a spherical coordinate system, where <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> is the
azimuthal angle of the lidar beam measured clockwise from true north and
<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> is the elevation angle of the lidar beam measured from the ground. The
radial velocity, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, measured by the lidar is defined as positive
for motion away from the lidar and negative for motion toward the lidar.</p>
      <p>All three lidar systems evaluated in this study use some variant of
a plan-position indicator (PPI) scan to measure the three-dimensional wind
components, where the lidar takes measurements at several azimuth angles
around a scanning circle at a constant elevation angle. In a horizontally
homogeneous atmosphere, the radial velocity values measured by a lidar
completing a PPI scan should take the following form <xref ref-type="bibr" rid="bib1.bibx44" id="paren.29"/>:

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>u</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:mi>v</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:mi>w</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          When calculating velocity variances from Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>), two
different approaches can be used. The standard method is to apply DBS or VAD
analysis techniques to the PPI data to compute instantaneous values of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> for each time stamp. The variances are then computed using

                <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>u</mml:mi><mml:mi>i</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>u</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where the index <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1, 2, 3 refers to the three velocity components <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> and the overbar denotes temporal averaging.</p>
      <p>The second method involves first computing the variance of the radial
velocities given by Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>):

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mi mathvariant="normal">r</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            The variances and covariances of the velocity components <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>
create a set of six unknown variables. By using six different beam positions
(i.e., different combinations of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>), a set of equations can
be solved for the six unknown variables <xref ref-type="bibr" rid="bib1.bibx33" id="paren.30"/>.</p>
      <p>The different lidar scanning and data analysis approaches for computing mean
values and variances of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> are discussed in more detail in the
following sections. For reference, a schematic of the DBS and VAD scanning
strategies can be found in Sect. 12.4.3 of <xref ref-type="bibr" rid="bib1.bibx44" id="text.31"/>.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>WindCube v2: DBS technique</title>
      <p>The WindCube v2 measures wind speed with a DBS technique, where an optical
switch is used to point the lidar beam in the four cardinal directions
(north, east, south, and west) at an elevation angle of 62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> from the
ground. Equations for the instantaneous radial velocities measured at the
four beam positions can be derived by letting <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, 90,
180, and 270<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>):

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>u</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the instantaneous values of the velocity
components at the four beam positions, and the index <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">4</mml:mn></mml:math></inline-formula>
describes the values measured by the <?xmltex \hack{\mbox\bgroup}?>north-,<?xmltex \hack{\egroup}?> east-, south-, and west-pointing
beams, respectively. Some WindCube lidars, including the model used here, add
a vertically pointing beam position, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, which provides a direct
measurement of the vertical velocity, <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). It takes the
WindCube lidar 1 s to collect data at each beam location, and steer the
beam to the next beam location such that a full DBS scan takes approximately
4–5 s. However, the WindCube velocity algorithm calculates the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>,
and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> components every  second using the current radial velocity and the
radial velocities obtained from the previous three beam locations
<xref ref-type="bibr" rid="bib1.bibx31" id="paren.32"/>.</p>
      <p>In lidar studies, Eqs. (<xref ref-type="disp-formula" rid="Ch1.E4"/>)–(<xref ref-type="disp-formula" rid="Ch1.E7"/>) are usually solved for <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> assuming that the flow is homogenous, i.e., the mean values of
the three-dimensional wind components do not change across the scanning
circle <xref ref-type="bibr" rid="bib1.bibx31" id="paren.33"><named-content content-type="pre">e.g.,</named-content></xref>. Letting <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, equations for the mean velocity values can be
found:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E8"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E9"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E10"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi>Q</mml:mi><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> (degrees) is the
wind direction. The <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> equation is a slightly modified version of
the true DBS solution and is used by Leosphere to calculate the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> velocity
for the WindCube lidar <xref ref-type="bibr" rid="bib1.bibx36" id="paren.34"><named-content content-type="pre">e.g.,</named-content></xref>. If a fifth vertical
beam is used, the mean value of the vertical velocity component can also be
calculated as <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>.</p>
      <p>Equations (<xref ref-type="disp-formula" rid="Ch1.E8"/>)–(<xref ref-type="disp-formula" rid="Ch1.E10"/>) are derived assuming that the values
of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> remain constant across the scanning circle. While this
assumption is valid when computing mean values in homogenous flow,
instantaneous velocity values will be highly variable due to the nature of
turbulent flow, and the computation of instantaneous velocity values with
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E8"/>)–(<xref ref-type="disp-formula" rid="Ch1.E10"/>) is inaccurate. However, the standard DBS
velocity variance calculation method uses Eqs. (<xref ref-type="disp-formula" rid="Ch1.E8"/>)–(<xref ref-type="disp-formula" rid="Ch1.E10"/>)
to compute instantaneous values of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>, which leads to the
variance contamination errors discussed in the literature
<xref ref-type="bibr" rid="bib1.bibx34" id="paren.35"/>.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>WindCube v2: novel method to reduce DBS variance contamination</title>
      <p>The errors associated with the standard DBS variance method can be
illustrated by applying Reynolds decomposition to the instantaneous velocity
values at each beam position. For the first and third beam positions, the
following set of equations is obtained:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E11"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E12"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E13"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E14"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:msub><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where the mean values <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> can be assumed to
be constant across the scanning circle but the turbulent velocity
fluctuations will differ (<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>≠</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>≠</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>). Combining Eqs. (<xref ref-type="disp-formula" rid="Ch1.E4"/>)–(<xref ref-type="disp-formula" rid="Ch1.E7"/>), an equation
for the instantaneous velocity at beam position 1 can then be derived:

                <disp-formula id="Ch1.E15" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. Comparing Eqs. (<xref ref-type="disp-formula" rid="Ch1.E15"/>) and (<xref ref-type="disp-formula" rid="Ch1.E9"/>)
illustrates how turbulent fluctuations at the different beam positions,
reflected by nonzero values of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow></mml:math></inline-formula>, affect the
computation of instantaneous velocity values.</p>
      <p>Taking the variance of Eq. (<xref ref-type="disp-formula" rid="Ch1.E15"/>) gives the following equation:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E16"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            The terms involving <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow></mml:math></inline-formula> appear because
data are being combined from two different beam positions to estimate the <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance. These terms can be further modified by taking into account that
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. For homogeneous flow,
we can assume that time-averaged correlations between different velocity
components (i.e., turbulent fluxes) become independent of the position along
the scanning circle as long as both components are measured at the same
location; thus, <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, etc. If the velocity components are measured at different
beam positions, the fluxes can be expressed using autocorrelation functions:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E17"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mrow><mml:mi>v</mml:mi><mml:mi>w</mml:mi></mml:mrow></mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E18"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E19"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            whereby the autocorrelation functions of the different velocity
components describe the spatial and temporal correlation of the instantaneous
velocity components measured at beam positions 1 and 3. Equation <xref ref-type="disp-formula" rid="Ch1.E16"/> then becomes the following:</p>
      <p><disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close="" open="["><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E20"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced close="]" open="."><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>Equation (<xref ref-type="disp-formula" rid="Ch1.E20"/>) can then be solved for <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>
to give a general expression for the actual <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance that is measured
when data are combined from different beam positions in the DBS technique:</p>
      <p><disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced open="[" close="]"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E21"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>When we apply the standard DBS approach we inherently assume that
the velocity fluctuations at the different beam positions are the same, i.e.,
we assume that <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1 and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 1. Thus, the DBS equation for the
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance becomes
            <disp-formula id="Ch1.E22" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mtext>DBS</mml:mtext><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close="]" open="["><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>Equation (<xref ref-type="disp-formula" rid="Ch1.E21"/>) can thus be recast into
            <disp-formula id="Ch1.E23" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>DBS</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>Similarly, an equation for the actual <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance given in terms of the DBS variance can be derived:</p>
      <p><disp-formula id="Ch1.E24" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>u</mml:mi><mml:mtext>DBS</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>Given the actual spatial separation and time shift between
different lidar beams, the autocorrelation function values are all less than
1 and the correction terms in
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E23"/>)–(<xref ref-type="disp-formula" rid="Ch1.E24"/>)
may become significant. In particular, the second term in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E23"/>)–(<xref ref-type="disp-formula" rid="Ch1.E24"/>) contains the ratio <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi></mml:mrow></mml:math></inline-formula>, which is approximately equal to 3.54 for the WindCube v2
elevation angle of 62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. This illustrates that ignoring the
contribution of fluctuations in the instantaneous velocity for the WindCube
v2 can lead to a large overestimation of the horizontal velocity variances
during convective conditions when <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is large. The actual
values of the autocorrelation functions will depend on atmospheric stability
and wind speed, which complicates applying corrections to the DBS variance
calculations. However, Eqs. (<xref ref-type="disp-formula" rid="Ch1.E23"/>) and (<xref ref-type="disp-formula" rid="Ch1.E24"/>)
provide the advantage that the variances of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> computed from the DBS
equations can be corrected if the vertical velocity component is measured
with a direct vertical beam, as was the case in our study, and estimates of
the autocorrelation functions can be made.</p>
      <p>In Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>, sonic anemometer and lidar measurements are used to
evaluate the autocorrelation functions, and the feasibility of applying the
correction algorithm (Eqs. <xref ref-type="disp-formula" rid="Ch1.E23"/>–<xref ref-type="disp-formula" rid="Ch1.E24"/>) under a
range of different stability conditions is discussed.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <title>ZephIR 300: VAD technique</title>
      <p>The ZephIR lidar employs a rotating mirror to conduct a 50-point VAD scan at
each measurement height, using a similar elevation angle to the WindCube
lidar (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for the ZephIR compared to <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> = 62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
for the WindCube lidar). For the VAD technique, the radial velocities
measured by the instrument should create a rectified cosine curve as
a function of azimuth angle <xref ref-type="bibr" rid="bib1.bibx23" id="paren.36"/>, as in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>). In a standard VAD analysis, the curve is assumed to
fit the following equation:

                <disp-formula id="Ch1.E25" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">r</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mtext>max</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> (degrees) is the azimuthal angle of the lidar beam, <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>)
is the offset of the curve from the zero-velocity line, <inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) is the amplitude of the curve, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mtext>max</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>
(degrees) is the phase shift of the curve. Assuming a homogeneous flow field
with no convergence or divergence, the horizontal wind speed, wind direction,
and vertical wind speed are then derived from the following relations:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E26"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>b</mml:mi><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E27"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mi>W</mml:mi><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mtext>max</mml:mtext></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E28"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mi>w</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>a</mml:mi><mml:mrow><mml:mi>sin⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mtext>max</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> are typically determined from
a least-squares approach. The values of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> can then be derived from
the horizontal wind speed, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">h</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and the wind direction.</p>

<table-wrap id="Ch1.T1" specific-use="star"><caption><p>Overview of instruments used to evaluate different scanning
strategies during LABLE 2 and LATTE.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.90}[.90]?><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="110.965748pt"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="justify" colwidth="56.905512pt"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry namest="col1" nameend="col6" align="center">Campaign instrumentation </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Instrument</oasis:entry>  
         <oasis:entry colname="col2">Campaign</oasis:entry>  
         <oasis:entry colname="col3">Measurement range</oasis:entry>  
         <oasis:entry colname="col4">Temporal resolution</oasis:entry>  
         <oasis:entry colname="col5">Scanning strategy</oasis:entry>  
         <oasis:entry colname="col6">Owner</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">WindCube v2</oasis:entry>  
         <oasis:entry colname="col2">LABLE 2</oasis:entry>  
         <oasis:entry colname="col3">40–200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">DBS</oasis:entry>  
         <oasis:entry colname="col6">LLNL</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Pulsed Doppler lidar</oasis:entry>  
         <oasis:entry colname="col2">LATTE</oasis:entry>  
         <oasis:entry colname="col3">12  measurement heights</oasis:entry>  
         <oasis:entry colname="col4">Full scan: 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> elevation angle</oasis:entry>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> range gates</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">ZephIR 300</oasis:entry>  
         <oasis:entry colname="col2">LATTE</oasis:entry>  
         <oasis:entry colname="col3">10–200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">0.07 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">VAD</oasis:entry>  
         <oasis:entry colname="col6">LLNL</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Continuous wave Doppler lidar</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">10 measurement heights</oasis:entry>  
         <oasis:entry colname="col4">Full scan: 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> elevation angle</oasis:entry>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">Variable range gate size  <?xmltex \hack{\hfill\break}?>(0.1–44 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Halo Streamline Pro</oasis:entry>  
         <oasis:entry colname="col2">LABLE 2</oasis:entry>  
         <oasis:entry colname="col3">105 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>–9.6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">Six-beam</oasis:entry>  
         <oasis:entry colname="col6">OU</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Scanning Doppler lidar</oasis:entry>  
         <oasis:entry colname="col2">LATTE</oasis:entry>  
         <oasis:entry colname="col3">30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> range gates</oasis:entry>  
         <oasis:entry colname="col4">Full scan: 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">s</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">45<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> elevation angle</oasis:entry>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Gill Windmaster Pro</oasis:entry>  
         <oasis:entry colname="col2">LABLE 2</oasis:entry>  
         <oasis:entry colname="col3">60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4">10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">–</oasis:entry>  
         <oasis:entry colname="col6">Lawrence Berkeley</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Three-dimensional sonic anemometer</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">National <?xmltex \hack{\hfill\break}?>Laboratory</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">RM Young</oasis:entry>  
         <oasis:entry colname="col2">LATTE</oasis:entry>  
         <oasis:entry colname="col3">50, 100, 150, 200, 250,</oasis:entry>  
         <oasis:entry colname="col4">30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">–</oasis:entry>  
         <oasis:entry colname="col6">OU</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Three-dimensional  sonic anemometers</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">and 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, NW booms</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Campbell Scientific CSAT3</oasis:entry>  
         <oasis:entry colname="col2">LATTE</oasis:entry>  
         <oasis:entry colname="col3">50, 100, 150, 200, 250,</oasis:entry>  
         <oasis:entry colname="col4">60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5">–</oasis:entry>  
         <oasis:entry colname="col6">NCAR</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Three-dimensional sonic anemometers</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">and 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, SE booms</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p>Equations (<xref ref-type="disp-formula" rid="Ch1.E26"/>)–(<xref ref-type="disp-formula" rid="Ch1.E28"/>) are derived from the first-order
coefficients of a Fourier decomposition of the radial velocity field, while
higher-order terms in the Fourier decomposition are related to divergence and
deformation <xref ref-type="bibr" rid="bib1.bibx6" id="paren.37"/>. Although these higher-order terms
are typically ignored in VAD analysis of lidar data, neglecting the terms can
lead to errors in the estimated wind speed and direction
<xref ref-type="bibr" rid="bib1.bibx21" id="paren.38"><named-content content-type="pre">e.g.,</named-content></xref>. Errors in the turbulent components can
arise as a result of variance contamination. Similar to the DBS technique,
the VAD technique involves combining data from different beam positions with
the assumption that the instantaneous velocity field is homogeneous across
the scanning circle.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <title>Six-beam technique</title>
      <p>As discussed in the previous two sections, the use of either the DBS or the
VAD technique introduces a number of known systematic errors into lidar
turbulence calculations. Some of these errors can be mitigated when applying
the second variance calculation method (Eq. <xref ref-type="disp-formula" rid="Ch1.E3"/>), which
involves solving a set of equations for different combinations of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> to obtain all six components of the covariance matrix.</p>
      <p>In this work, the six-beam technique developed by <xref ref-type="bibr" rid="bib1.bibx33" id="text.39"/> was
evaluated using the user-configurable Halo lidar. <xref ref-type="bibr" rid="bib1.bibx33" id="text.40"/>
developed the technique by using a minimization algorithm to determine the
optimum combination of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> values that minimizes the random
errors in the variance estimates. The optimal configuration found was as
follows: five beams at an elevation angle of 45<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> that are equally
spaced 72<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> apart (i.e., located at azimuths of 0, 72, 144, 216, and
288<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) and one vertically pointed beam. This scanning strategy is
hereafter referred to as the six-beam technique.</p>
      <p>Solving Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) with the chosen values of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>, the equations for the variances <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> based on the
six-beam technique are

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>u</mml:mi><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mi>b</mml:mi></mml:mrow><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn>0.4</mml:mn><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mn>1.05</mml:mn><mml:mfenced open="(" close=")"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E29"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="1em"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:mn>0.15</mml:mn><mml:mfenced open="(" close=")"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mi>b</mml:mi></mml:mrow><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mn>1.2</mml:mn><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>-</mml:mo><mml:mn>0.25</mml:mn><mml:mfenced close=")" open="("><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E30"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="1em"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:mn>0.65</mml:mn><mml:mfenced close=")" open="("><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E31"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>w</mml:mi><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mi>b</mml:mi></mml:mrow><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where subscript <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula> indicates that the horizontal velocity variances are
computed applying the six-beam technique, and subscripts 1–6 refer to the
beam positions, with beams 1–5 spaced 72<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> apart in the scanning
circle and beam 6 pointing vertically upward.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p><bold>(a)</bold> Google Earth image of the state of Colorado. Location
of BAO site is denoted by red marker. <bold>(b)</bold> Google Earth image of the
BAO site. Instrument locations are denoted by red markers. Approximate
distance between instruments is indicated by blue line and label. Only the
initial location of the WindCube lidar is shown.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f01.jpg"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Measurement campaigns</title>
      <p>The DBS and six-beam strategies were evaluated at a field site in Oklahoma,
while all three scanning strategies were evaluated at a field site in
Colorado. As the Colorado site featured a large amount of three-dimensional sonic
anemometer verification data, this site will be described first and will be
primarily used to draw conclusions about the accuracy of lidar turbulence
measurements. These results will be corroborated by data collected during the
Oklahoma experiment. Instruments used to evaluate the various scanning
techniques are summarized in
Table <xref ref-type="table" rid="Ch1.T1"/>.<?xmltex \hack{\newpage}?></p>
<sec id="Ch1.S3.SS1">
  <title>Lower Atmospheric Thermodynamics and Turbulence Experiment (LATTE)</title>
      <p>LATTE was conducted from 10 February to 28 March 2014, with a small-scale extension of
the project from 28 March to 28 April 2014. LATTE was conducted at the
BAO, a National Oceanic and Atmospheric
Administration (NOAA) facility located in Erie,
Colorado (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a). The BAO site is situated approximately
25 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> east of the foothills of the Rocky Mountains. Although the
diurnal heating cycle can induce upslope and downslope winds in the vicinity
of a mountain range <xref ref-type="bibr" rid="bib1.bibx13" id="paren.41"><named-content content-type="pre">e.g.,</named-content></xref>, these effects are only
expected to influence flow at the BAO when the synoptic-scale pressure
gradient is weak <xref ref-type="bibr" rid="bib1.bibx15" id="paren.42"/>. During LATTE, winds were primarily
northerly and westerly throughout the lower boundary layer and appeared to be
mainly associated with the upper-level flow pattern.</p>
      <p>One of the primary goals of LATTE was to evaluate the accuracy of lidar
turbulence measurements. Thus, the 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> tower at the BAO was
instrumented with three-dimensional sonic anemometers at six different heights. As a result
of a collaboration with the National Center for Atmospheric Research (NCAR),
NorthWest Research Associates, and the NOAA Earth System Research Laboratory (ESRL), we were able
to mount two sonic anemometers at each measurement height on opposite booms
such that at each height there would be at least one set of three-dimensional sonic
anemometer measurements that were not strongly influenced by the wake of the
tower. A Halo lidar owned by the University of Oklahoma (OU) along with
a WindCube v2 and ZephIR 300 lidar, both owned by Lawrence Livermore National
Laboratory (LLNL), were deployed at the BAO for LATTE, in addition to several
instruments owned by NCAR. The OU Halo lidar was located approximately
600 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> south-southwest of the 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> tower so that it could be
used to verify wind speeds from an NCAR wind profiler. The WindCube was
located in the same enclosure as the 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> tower from 14 to 28
February 2014, then moved to the same location as the OU Halo lidar from 1
March to 28 April 2014. The ZephIR remained in the tower enclosure for the
duration of the experiment (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Lower Atmospheric Boundary Layer Experiment (LABLE) 2</title>
      <p>LABLE took place in two phases: LABLE 1 was conducted from 18 September to 13 November 2012 and
LABLE 2 was conducted from 12 June to 2 July 2013. LABLE 2 was a multi-lidar
experiment designed to test different scanning strategies and will be
discussed in this work. Detailed information on the research goals and
instrumentation of LABLE can be found in <xref ref-type="bibr" rid="bib1.bibx20" id="text.43"/>. Both LABLE
campaigns took place at the central facility of the Southern Great Plains
ARM site. The ARM site is operated by the
Department of Energy and serves as a field site for an extensive suite of
various in situ and remote sensing instruments <xref ref-type="bibr" rid="bib1.bibx27" id="paren.44"/>.
The location of the ARM site in northern Oklahoma is shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>a.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p><bold>(a)</bold> Google Earth image of the state of Oklahoma. Location
of Southern Great Plains ARM site is denoted by red marker. <bold>(b)</bold>
Google Earth image of the central facility of the Southern Great Plains ARM
site. Instrument locations are denoted by red markers. Approximate distances
between instruments are indicated by blue lines and labels.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f02.jpg"/>

        </fig>

      <p>Locations of the lidars deployed during LABLE 2 are shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>b. The ARM Halo lidar is a scanning lidar operated by the
ARM site and is nearly identical to the OU Halo lidar. The Galion lidar is
a lidar rented by OU that has identical hardware to the two scanning Halo
lidars. Data from three-dimensional sonic anemometers on a 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> tower were also
available at the ARM site but could not be used to verify the six-beam lidar
measurements as the tower was too short to overlap with the scanning lidar
measurement heights (first range gate is 105 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>). Data from the
60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> sonic anemometer could be directly compared to corresponding
measurements from the WindCube lidar, which has a first range gate of
40 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, so only data from the WindCube lidar are shown in this work.
Results from the scanning lidar portion of LABLE 2 are presented
in <xref ref-type="bibr" rid="bib1.bibx28" id="text.45"/>.<?xmltex \hack{\vspace{-3mm}}?></p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Data processing</title>
<sec id="Ch1.S4.SS1">
  <title>Coordinate rotation</title>
      <p>A coordinate rotation was applied to the sonic
anemometer and lidar data to reduce the effects of alignment and tilt errors
on the variance estimates <xref ref-type="bibr" rid="bib1.bibx14" id="paren.46"/>. Following the procedure
outlined by <xref ref-type="bibr" rid="bib1.bibx18" id="text.47"/>, the coordinate axes were first
rotated such that the mean meridional wind speed, <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, was set to
0 and <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> was aligned with the 10 min mean wind direction. In the next
step, the coordinate axes were rotated such that <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>w</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> was equal to
0.</p>
      <p>Typically, the coordinate rotation is applied to the raw wind speed
components before the variance is calculated, such that the variance is also
defined in the new coordinate system. However, instead of first rotating the
raw wind speed components, the variance values themselves from the old
coordinate system can also be rotated such that <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> is aligned with the mean
wind direction and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is forced to 0, as in <xref ref-type="bibr" rid="bib1.bibx37" id="text.48"/>.
The rotated variance components are described as follows:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E32"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mtext>rot</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E33"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mtext>rot</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>cos⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi>sin⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E34"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mtext>rot</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> is the mean wind direction and the subscript rot
refers to variance components in the rotated coordinate system. This rotation
has the same effect as applying the first coordinate rotation to the original
wind speed components before taking the variance. Thus, in comparisons with
the six-beam technique, only the first coordinate rotation was applied to the
lidar and sonic data to be consistent with the coordinate rotation used by
<xref ref-type="bibr" rid="bib1.bibx37" id="text.49"/>.</p>
      <p>It was determined during our analysis that the covariance term
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> in
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E32"/>)–(<xref ref-type="disp-formula" rid="Ch1.E33"/>)
is also affected by variance contamination when a DBS or VAD scan is used, in
addition to the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance components. At the BAO, variance
contamination caused WindCube values of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> to differ largely
from the sonic values under unstable conditions. However, the
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> term measured by the sonics at both sites was near-zero
throughout the day and only had a negligible effect on the coordinate
rotations for the sonic variance. Thus, the <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> term was
neglected in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E32"/>) and (<xref ref-type="disp-formula" rid="Ch1.E33"/>) for
rotation of the lidar data.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Quality control</title>
      <p>The actual sampling frequencies of the sonic anemometers and lidars drifted
slightly around their prescribed sampling frequencies throughout the
measurement campaigns, which is problematic for the calculation of variance.
Thus, the raw wind speed data from the different instruments were linearly
interpolated onto temporal grids with constant spacing that matched the
sampling frequency of each instrument (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">Hz</mml:mi><mml:mo>/</mml:mo><mml:mn>0.25</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">Hz</mml:mi></mml:mrow></mml:math></inline-formula> for the
WindCube v2, 0.067 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> for the ZephIR, 0.033 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> for the Halo
lidar, and 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> (60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula>) for the north (south) sonic
anemometers at the BAO tower). The sonic anemometer data were additionally
averaged to form 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data streams. The 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data streams
were used in further calculations, as they served to reduce high-frequency
noise in the sonic anemometer data as well as reduce processing time. (Values
of the 30 min variance calculated from the 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> data streams did
not differ significantly from values calculated from the raw sonic anemometer
data streams.) The 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> sonic anemometer data at the ARM site were
also interpolated to a 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> grid. No averaging was needed for the
ARM sonic data, as the output frequency of the ARM sonic anemometers is
already 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula> (Table <xref ref-type="table" rid="Ch1.T1"/>).</p>
      <p>The spike filter developed by <xref ref-type="bibr" rid="bib1.bibx16" id="text.50"/> and adapted by
<xref ref-type="bibr" rid="bib1.bibx42" id="text.51"/> was used to flag outliers in the data. A 10 min
window was shifted through the raw lidar and sonic anemometer data, and any
point that was more than 3.5 standard deviations from the 10 min block
average was flagged as a possible spike and removed from the data set. This
process was repeated until no more spikes were detected. For each pass
through the spike filter, the factor of 3.5 standard deviations was increased
by 0.1 standard deviations.</p>
      <p>By default, WindCube radial velocities that were associated with
signal-to-noise ratios (SNRs) lower than <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn>23</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">dB</mml:mi></mml:mrow></mml:math></inline-formula> were flagged as
missing values. For the scanning lidars, SNR thresholds were set to <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn>23</mml:mn></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn>17</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">dB</mml:mi></mml:mrow></mml:math></inline-formula> for the horizontal and vertical beams, respectively. The
ZephIR lidar obtains an estimate of the mean noise level by taking
measurements with the shutter closed before each full scan. Only signals with
power that exceeds a threshold of 5 standard deviations above this mean
noise level are used to estimate the velocity <xref ref-type="bibr" rid="bib1.bibx39" id="paren.52"/>.</p>
      <p>As Doppler lidars use the Doppler shift from aerosols to estimate radial
velocity, they are adversely affected by the presence of precipitation
particles, which can result in beam attenuation and increased vertical
velocities <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx29" id="paren.53"><named-content content-type="pre">e.g.,</named-content></xref>. Thus,
lidar data that were collected when rain gauges at the different field sites
recorded precipitation were flagged as erroneous data.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Selection of averaging times</title>
      <p>In order to mitigate the effects of random errors on variance calculations,
<xref ref-type="bibr" rid="bib1.bibx26" id="text.54"/> and <xref ref-type="bibr" rid="bib1.bibx42" id="text.55"/> recommend averaging
products of perturbations over a period of time that is longer than the local
averaging length, <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, the averaging time that is used to calculate mean
values from which the perturbations are derived. In this work, the variance
of each velocity component was defined as the mean value of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:msubsup><mml:mi>u</mml:mi><mml:mi>i</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (calculated using <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn>10</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:math></inline-formula>) over a 30 min
period, with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> corresponding to the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> estimates,
respectively. The typical averaging period for wind energy studies is
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, but a 30 min averaging period was used in this work to
reduce the effects of noise on variance estimates, as in <xref ref-type="bibr" rid="bib1.bibx37" id="text.56"/>.
The variance calculated with this method is hereafter referred to as the
“30 min variance”, although it differs from the standard calculation of
30 min variance. These variance estimates represent turbulent motions with
timescales from 0.01 s to 10 min, with the smallest scales of turbulence
only measured by the sonic anemometers.</p>
      <p>Mesoscale motions can also induce errors in variance calculations, as the
mean of each variable can change significantly over the averaging period used
to calculate variance as a result of a frontal passage or wind direction
shift <xref ref-type="bibr" rid="bib1.bibx42" id="paren.57"/>. Thus, raw wind speed data were detrended
using a linear detrend method for each hour-long record. The detrending
method served to reduce high variance values that were associated with large
shifts in wind speed or wind direction.</p>
</sec>
<sec id="Ch1.S4.SS4">
  <title>Stability classification</title>
      <p>At the BAO, temperature and wind speed data were available at multiple
heights on the tower, so the gradient Richardson number, Ri, was
used as a stability parameter. Ri is defined by the following
equation <xref ref-type="bibr" rid="bib1.bibx1" id="paren.58"/>:

                <disp-formula id="Ch1.E35" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>R</mml:mi><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi>g</mml:mi><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>o</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mrow><mml:mo>(</mml:mo><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>U</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) is the gravitational acceleration, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (K) is
the surface temperature, and <inline-formula><mml:math display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>U</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>)
and <inline-formula><mml:math display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">K</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) are the vertical
gradients of horizontal wind speed and potential temperature, respectively.
In this work, the potential temperature gradient was approximated by adding
the dry adiabatic lapse rate, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Γ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, to the temperature
gradient, and the derivatives of temperature and wind speed were approximated
by using a finite differencing approach, similar to the procedure used by
<xref ref-type="bibr" rid="bib1.bibx4" id="text.59"/>:

                <disp-formula id="Ch1.E36" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>R</mml:mi><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>g</mml:mi><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">Γ</mml:mi><mml:mi mathvariant="normal">d</mml:mi></mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>z</mml:mi><mml:mi>U</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>U</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> correspond to two different measurement heights, and
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mi>U</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> refer to the differences in measurement levels
for <inline-formula><mml:math display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula>. As wind shear was often extremely low during the daytime
hours at the BAO, a bulk wind shear quantity was used in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E36"/>), i.e., <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> was assumed for wind
speed, with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. This bulk approximation
eliminated the extremely large negative Ri values that were often
produced at the BAO under unstable conditions as a result of the small
difference between <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>U</mml:mi><mml:mrow><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p>Due to unexpected tower maintenance at the ARM site, it was not often
possible to measure the temperature and wind speed at two heights
simultaneously. Thus, the Monin–Obukhov length, <inline-formula><mml:math display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> (m), from the
60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> sonic was used to define stability instead. <inline-formula><mml:math display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> is defined by
the following equation:

                <disp-formula id="Ch1.E37" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>L</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>u</mml:mi><mml:mo>∗</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mi mathvariant="italic">κ</mml:mi><mml:mi>g</mml:mi><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) is the friction velocity,
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> (K) is the mean virtual potential temperature at the
measurement height, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">κ</mml:mi></mml:math></inline-formula> is the von Kármán constant (commonly set
to 0.4), and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>)
is the heat flux measured at the surface <xref ref-type="bibr" rid="bib1.bibx1" id="paren.60"><named-content content-type="pre">e.g.,</named-content></xref>. Negative
values of both <inline-formula><mml:math display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> and Ri indicate unstable conditions while
positive values indicate stable conditions. As the data sets analyzed in this
work are relatively small, only a broad classification of conditions as
either stable or unstable was made.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Comparison of turbulence parameters: LATTE</title>
      <p>Figure <xref ref-type="fig" rid="Ch1.F3"/> demonstrates the typical diurnal cycle of
turbulence (<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>v</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>) at the BAO, with
low values of turbulence occurring during the evening and overnight hours
(approximately 00:00–12:00 UTC) and high values of turbulence occurring
during daytime, convective conditions (approximately 12:00–00:00 UTC).
(Note that for all LATTE plots, data from the NCAR sonics are shown, unless
the mean wind direction corresponded to the NCAR sonic wake sector, in which
case the OU sonics were used. Local time is UTC<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>.) During this period, the
wind direction generally shifted between easterly/southeasterly and northerly
(Fig. <xref ref-type="fig" rid="Ch1.F3"/>e). However, from approximately 18:00 UTC 23 March
to 06:00 UTC 24 March, winds were primarily from the west/northwest, which
is the direction of the Rocky Mountains. Flow from the mountains was
associated with higher mean wind speeds and variances of the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
velocity components in comparison to the rest of the period (Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p>
      <p>The following sections focus on measurements from 25 March 2014, which was
a calm, clear day with no precipitation when all three lidars had good data
availability. Variance estimates from each lidar and scanning strategy are
compared to similar measurements made by the sonic anemometers and the other
lidars. For most comparison plots, variance estimates from the measurement
height where the lidar data availability was greatest are shown. For the
WindCube and ZephIR lidars, which only collect measurements up to
200 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>, data from 100 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> are shown. For the
Halo lidar, which has a minimum range gate of 105 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>, data from
200 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> are shown.</p>
<sec id="Ch1.S5.SS1">
  <title>DBS technique: WindCube</title>
      <p>During the overnight hours of 25 March, variance values computed from the
WindCube DBS data agreed well with sonic anemometer data, but between 15:00
and 21:00 UTC the WindCube substantially overestimated the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance (Fig. <xref ref-type="fig" rid="Ch1.F4"/>a and b). <xref ref-type="bibr" rid="bib1.bibx36" id="text.61"/> attribute this
overestimation to variance contamination, which artificially increases the
lidar-measured variance and is most prominent under unstable conditions, when
the effects of volume averaging are minimized due to the relatively large
turbulent eddy sizes. In Sect. <xref ref-type="sec" rid="Ch1.S2.SS4"/>, we presented a framework
that further details the causes of variance contamination errors and provides
equations for correcting variances computed from lidar DBS scans. These
equations are now evaluated using sonic and lidar data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>30 min <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance,
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance, <bold>(d)</bold> mean wind speed,
and <bold>(e)</bold> mean wind direction at 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from sonic
anemometers at BAO and <bold>(f)</bold> Richardson number calculated from tower
data. Data are shown from 22 to 26 March 2014, and tick marks for each date
correspond to 00:00 UTC on that day.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f03.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>30 min <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance, and
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance at 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from sonic anemometers and
WindCube DBS technique at BAO and <bold>(d)</bold> Richardson number calculated
from tower data. Data are shown from 25 March 2014. In <bold>(a)</bold> and
<bold>(b)</bold>, solid blue line indicates DBS-calculated variance and dashed
black line indicates corrected variance. In <bold>(c)</bold>, solid blue line
indicates DBS-calculated <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance and dashed blue line indicates <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>
variance calculated from vertically pointing beam. The corrected <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance data show substantial improvement over the uncorrected data set
during unstable conditions.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f04.pdf"/>

        </fig>

<sec id="Ch1.S5.SS1.SSS1">
  <title>Variance correction</title>
      <p>As discussed in Sect. <xref ref-type="sec" rid="Ch1.S2.SS4"/>, instantaneous velocity values
calculated from lidar DBS data contain extra terms, for example, the
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow></mml:math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="Ch1.E15"/>), which become large
under convective conditions. The addition of these extra terms can cause the
WindCube to overestimate the magnitude of the instantaneous <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
velocity and contaminate the true value of the variance, as shown in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E23"/>) and (<xref ref-type="disp-formula" rid="Ch1.E24"/>) and seen in Fig. <xref ref-type="fig" rid="Ch1.F4"/>a, b. Since these extra terms cannot be easily quantified
from lidar data, sonic anemometer data were used to examine the impacts of
temporal and spatial changes in the instantaneous velocity components on the
resultant variance estimates.</p>
      <p>At the BAO tower, two sonic anemometers were located approximately 11.5 m
apart on opposite booms at each measurement height, which were used to
simulate the measurement technique used by the WindCube lidar. First, sonic
data were projected into the directions of the WindCube beam positions and
projected data from the south sonic were shifted forward in time by 2 s to simulate the time it takes the WindCube lidar beam to move from
one side of the scanning circle to the other. The time-shifted and projected
sonic data were then used to calculate values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p>Sonic anemometer data from 22 to 26 March 2014 were used to estimate values
of the autocorrelation functions for times when neither sonic was waked by
the tower. Mean values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> under unstable
conditions were 0.96, 0.81, and 0.66, respectively. Under stable conditions,
the average values were 0.95, 0.71, and 0.69. These values indicate that the
<inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and particularly <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> wind components do change significantly in
both space and time and that values of <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> become decorrelated more quickly
than values of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> as a result of the presence of smaller turbulent
scales of motion in the vertical direction.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>30 min <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance,
and <bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance at 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from sonic
anemometers and lidar VAD techniques at BAO and <bold>(d)</bold>
Richardson number calculated from tower data. Data are shown from 25
March 2014. Comparison of the Halo and ZephIR VAD-processed data
suggests that a lower elevation angle may be advantageous (e.g.,
lower <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values measured by the Halo lidar, which uses a lower elevation angle, shown in <bold>b</bold>).
Note the smaller <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values shown here for the Halo and ZephIR (VAD)
as compared to the Wind Cube (DBS) in Fig. <xref ref-type="fig" rid="Ch1.F4"/>.</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f05.pdf"/>

          </fig>

      <p>The mean values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> calculated from the sonic
data were then used with
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E23"/>) and (<xref ref-type="disp-formula" rid="Ch1.E24"/>)
to correct the WindCube DBS variance values, where the value of
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> in the correction equations was taken to be the velocity
variance measured by the WindCube vertical beam. Corrected <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance values on 25 March 2014 are indicated by the black dashed lines in
Fig. <xref ref-type="fig" rid="Ch1.F4"/>. The variance correction does not significantly change
variance values under stable conditions, when the value of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>
is small, but it serves to reduce estimates of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> by over 20 % under unstable conditions, bringing them
closer to the values measured by the sonics. In reality, the values of the
autocorrelation functions needed for the correction should be smaller than
the values that were calculated for the sonics, as the sonics were only
located 11.5 m apart while the WindCube scanning cone has a diameter of 106 m
at a measurement height of 100 m. Thus, there is still some variance
contamination present in the corrected <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values shown in
Fig. <xref ref-type="fig" rid="Ch1.F4"/>, as the values of the autocorrelation functions used
in the correction do not fully represent the degree of decorrelation that
occurs between the WindCube beams.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Thirty-minute <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance, and
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance at 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from sonic anemometers and Halo
lidar six-beam technique at BAO and <bold>(d)</bold> Richardson number calculated
from tower data. Data are shown from 25 March 2014. Note the high agreement
between the six-beam Halo method and sonic in <bold>(c)</bold> as compared to the
VAD Halo method in Fig. <xref ref-type="fig" rid="Ch1.F5"/>c for <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance. (The difference
in vertical variance accuracy is also likely related to the different
turbulent scales present at 100 and 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>.)</p></caption>
            <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f06.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>30 min mean velocity values (left panels) and variance values
(right panels) for <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>,
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(d)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(e)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and
<bold>(f)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> measured by Halo lidar and calculated from projected
sonic data. Values of <bold>(g)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance and <bold>(h)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance
are also shown for reference, where sonic values are from standard variance
calculation and Halo values are from six-beam calculation. Mean wind speed
from sonic is shown in <bold>(i)</bold> and Richardson number from tower is shown
in <bold>(j)</bold>. Data are shown from 25 March 2014 at 200 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>
at the BAO tower.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f07.pdf"/>

          </fig>

      <p>Another method to calculate values of the autocorrelation functions is to use
a least-squares approach to find the values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that provide the best estimate for the sonic variance. This method
yielded similar values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> to the values calculated from
the sonic data and much lower values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in comparison to the sonic
values (approximately 0.29 under unstable conditions and 0.13 under stable
conditions). True estimates of the autocorrelation functions for the
distances spanned by the WindCube beams would require either sonic
anemometers at different towers or a numerical model that provides wind speed
data with high spatial and temporal resolution.</p>
</sec>
<sec id="Ch1.S5.SS1.SSS2">
  <?xmltex \opttitle{Methods for estimating $w$ variance}?><title>Methods for estimating <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance</title>
      <p>Contamination errors also affect the variance of the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> component if it is
computed applying the DBS method, although it generally does not lead to
variance overestimates, as volume averaging for the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> component is more
significant than it is for the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> components <xref ref-type="bibr" rid="bib1.bibx36" id="paren.62"/>.
However, the WindCube v2 lidar utilizes a vertical beam position once per
scan to obtain a direct measurement of the vertical velocity directly above
the lidar, which is only minimally affected by variance contamination. Both
the vertical beam method and the DBS method (Eq. <xref ref-type="disp-formula" rid="Ch1.E10"/>) were
investigated in this work to determine the advantage of having a vertically
pointed beam position to measure <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance. At the BAO, the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance
measured by the WindCube lidar's vertical beam was much higher and more
accurate than the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance calculated from the DBS equations,
particularly under convective conditions (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c). This is
not surprising, as the vertical beam variance is a measure of the variance
directly above the lidar (barring the effects of volume averaging), while the
DBS-estimated variance is an average across the scanning circle. Thus, in all
further plots, <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance from the WindCube lidar is calculated from the
vertical beam.<?xmltex \hack{\newpage}?></p>
</sec>
</sec>
<sec id="Ch1.S5.SS2">
  <title>VAD technique: ZephIR, Halo</title>
      <p>During post-processing, a VAD technique <xref ref-type="bibr" rid="bib1.bibx6" id="paren.63"/> was used
to calculate variance from the six-beam Halo data. The five off-vertical
beams were fit to a sine curve to estimate the horizontal wind speed, wind
direction, and vertical wind speed from each scan. This information was then
used to create a time series for the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> components from which
the variance could be calculated. Variance from the Halo VAD technique was
compared to the variance estimated by the ZephIR lidar, which employs
a 50-point VAD at each height as part of its scanning strategy, as well as
variance measured by the sonic anemometers.</p>
      <p>While the ZephIR-estimated <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance values were quite close to those
measured by the sonic anemometers and the Halo lidar (Fig. <xref ref-type="fig" rid="Ch1.F5"/>a), the ZephIR overestimated the <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance under
unstable conditions during some half-hourly periods (Fig. <xref ref-type="fig" rid="Ch1.F5"/>b), which could indicate that the ZephIR lidar VAD
technique is also affected by variance contamination, similar to the WindCube
lidar. Although the WindCube and ZephIR lidars use similar elevation angles
(Table <xref ref-type="table" rid="Ch1.T1"/>), the overestimation of <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance by the
ZephIR lidar was not nearly as large as it was for the WindCube lidar. The
ZephIR has variable range gate sizes and takes nearly 4 times as long to
complete a full scan from 10 to 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> as the WindCube lidar, so the
lower temporal resolution of the ZephIR scans may have caused it to measure
lower variance values than the WindCube lidar. The Halo lidar produced the
most accurate VAD-estimated <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values throughout the day
(Fig. <xref ref-type="fig" rid="Ch1.F5"/>a and b), suggesting that a VAD technique with
a lower elevation angle can measure horizontal variance values more
accurately. The Halo lidar used an elevation angle of 45<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> while the
WindCube and ZephIR lidars used elevation angles of 62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and
60<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, respectively. Although the values of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>w</mml:mi></mml:mrow></mml:math></inline-formula> were likely larger for the Halo lidar, since it used a wider
scanning cone, the contribution of the <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> term to the
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance in Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>) is smaller for lower values of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>.
Additionally, the temporal resolution of the Halo lidar likely led to the
measurement of lower variance values than the WindCube and ZephIR lidars,
which may have masked the effects of variance contamination.</p>
      <p>The ZephIR and Halo lidars measured similar <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance values with
the VAD technique, which were underestimates in comparison to the
sonic anemometer values for nearly all stability conditions throughout
the day (Fig. <xref ref-type="fig" rid="Ch1.F5"/>c). As previously discussed, the most
accurate lidar method for measuring the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance appears to be the
use of a vertical beam position to obtain a direct measurement of the
vertical wind speed (Figs. <xref ref-type="fig" rid="Ch1.F4"/>c and <xref ref-type="fig" rid="Ch1.F6"/>c).</p>
</sec>
<sec id="Ch1.S5.SS3">
  <title>Halo: six-beam technique</title>
      <p>Variance measured using the six-beam technique with the Halo lidar is
compared to variance measured by the sonic anemometers in Fig. <xref ref-type="fig" rid="Ch1.F6"/>. Similar to the WindCube lidar, the six-beam
technique includes a vertically pointed beam to obtain a direct measurement
of the vertical velocity. Vertical variance estimated by the Halo six-beam
technique was much higher and more accurate than the vertical variance
measured by the Halo VAD technique (Figs. <xref ref-type="fig" rid="Ch1.F5"/>c and <xref ref-type="fig" rid="Ch1.F6"/>c). However, larger discrepancies occurred in the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values. During strongly unstable conditions from 17:00 to
21:00 UTC, the Halo six-beam technique often underestimated the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance in comparison to the sonic anemometers
(Fig. <xref ref-type="fig" rid="Ch1.F6"/>a and b). In some extreme cases, the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance values became negative, which should be mathematically impossible
given the definition of variance (<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>=</mml:mo><mml:mover accent="true"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>u</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>).</p>
      <p>In order to determine the cause of this horizontal variance underestimation
and the negative variance values, it is instructive to examine the equations
used to calculate the variance components with the six-beam technique
(Eqs. <xref ref-type="disp-formula" rid="Ch1.E29"/>–<xref ref-type="disp-formula" rid="Ch1.E31"/>).
Equations (<xref ref-type="disp-formula" rid="Ch1.E29"/>) and (<xref ref-type="disp-formula" rid="Ch1.E30"/>) for the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance, respectively, both include the term <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>,
meaning that the variance calculated from the vertical beam radial velocity
is subtracted from the combination of the other terms. Thus, when
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r6</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is large, as is often the case under
convective conditions (Fig. <xref ref-type="fig" rid="Ch1.F6"/>c), or overestimated due
to instrument noise, a large value is subtracted in
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E29"/>) and (<xref ref-type="disp-formula" rid="Ch1.E30"/>), and the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance can become negative if the other radial variances are not measured
accurately. The other negative terms in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E29"/>) and (<xref ref-type="disp-formula" rid="Ch1.E30"/>) could also decrease the horizontal variance components
and cause them to become negative. Similarly, if the positive terms in
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E29"/>) and (<xref ref-type="disp-formula" rid="Ch1.E30"/>) are underestimated,
the variance values would also likely be underestimated. Although negative
values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>v</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula> only comprised approximately 5 %
of the horizontal variance values at 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> during the 5-day analysis
period, the underestimation of horizontal variance components by the six-beam
technique is a significant issue that warrants further investigation.</p>
      <p>Velocity data from the 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> sonic anemometers were projected into
the directions of the different Halo beam locations in order to assess the
accuracy of the measurements from each beam position. Time series plots of
the 30 min mean radial wind speeds and radial variance values measured by
the sonics and Halo lidar on 25 March 2014 are shown in
Fig. <xref ref-type="fig" rid="Ch1.F7"/>. During the afternoon of 25 March, mean
wind speeds were very low (Fig. <xref ref-type="fig" rid="Ch1.F7"/>i), which is
reflected by the low radial wind speeds measured by the Halo lidar and
calculated from the projected sonic data
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>a–f). Some minor differences in the
radial wind speeds measured by the Halo and sonic anemometer were evident in
the late afternoon, as well as strongly underestimated and negative Halo <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values (Fig. <xref ref-type="fig" rid="Ch1.F7"/>g and h). The
largest discrepancies between the radial variance values also occurred in the
late afternoon, when the Halo strongly underestimated the variance of the
radial velocity at the third, fourth, and fifth beam positions
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>c–e). In the initial six-beam
equations, terms <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> have
positive coefficients in the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance equation
(Eq. <xref ref-type="disp-formula" rid="Ch1.E29"/>), and terms <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> have positive coefficients in the <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance equation while the <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> term has
a negative coefficient (Eq. <xref ref-type="disp-formula" rid="Ch1.E30"/>). The actual coefficients of
the radial beam variances will change once the coordinate rotation is applied
(Eqs. <xref ref-type="disp-formula" rid="Ch1.E32"/>–<xref ref-type="disp-formula" rid="Ch1.E34"/>), but for the most
part weighted values of <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:msubsup><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> are
added to the weighted values of the other radial beam variances to obtain
values for the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance. Thus, if the variance measured at beam
positions 3, 4, and 5 is underestimated, the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance will also
be underestimated. Similar trends were also observed on 24 March 2014 (not
shown).</p>
      <p>Several factors may have caused the Halo lidar to underestimate the variance
at certain beam positions more strongly than at other beam positions. One
possible explanation for the variance discrepancies could be the presence of
horizontal heterogeneity across the lidar scanning circle. The six-beam
technique requires the assumption that flow is homogeneous in the scanning
circle encompassed by the five off-vertical beams, and this assumption may
not have been valid at the BAO, which is located in the vicinity of complex
terrain, especially at a measurement height of 200 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>
Horizontal heterogeneity and high values of variance could cause large
amounts of scatter about the VAD sine curve <xref ref-type="bibr" rid="bib1.bibx44" id="paren.64"/>. The
differences between the instantaneous radial velocities and the fit VAD sine
curve (Eq. <xref ref-type="disp-formula" rid="Ch1.E25"/>) were examined for 25 March, but no noticeable
differences were evident for the different beam positions, although residuals
were much larger under unstable conditions. A modeled flow field and lidar
simulator would likely be needed to definitively quantify the effect of
horizontal heterogeneity on the variances measured by the different lidar
beam positions.</p>
      <p>Relative intensity noise (RIN) also may have affected the variance values
measured by the Halo lidar on 25 March. RIN results from spontaneous
radiation emissions from the laser, which cause intensity fluctuations in the
laser oscillator <xref ref-type="bibr" rid="bib1.bibx8" id="paren.65"/>. In a coherent heterodyne lidar, RIN
appears as pink noise; i.e., it is mainly present in the low-frequency part
of the Doppler spectrum <xref ref-type="bibr" rid="bib1.bibx12" id="paren.66"/>. Since low wind speeds would
also be detected in the low frequency part of the spectrum, RIN can impact
the accuracy of Doppler velocity measurements under low wind speeds.
<xref ref-type="bibr" rid="bib1.bibx30" id="text.67"/> found that a ZephIR lidar most strongly underestimated the
turbulence intensity measured by cup anemometers when weak wind speeds were
measured.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="Ch1.F7"/> but for 6 March 2014.
Richardson number is not shown, because the 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> temperature sensor
had data quality issues on this day (possibly related to tower icing).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f08.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>Thirty-minute <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r1</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r2</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(c)</bold>
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r3</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <bold>(d)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r4</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and <bold>(e)</bold> <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mtext>r5</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> variance values
measured by WindCube lidar and calculated from projected sonic data, where
positions 1–4 are located at azimuths of 0, 90, 180, and 270<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>,
respectively, at an elevation angle of 62<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and position 5 is pointed
vertically. Values of <bold>(f)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance and <bold>(g)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance
are also shown for reference, where sonic values are from standard variance
calculation and WindCube values are shown from DBS calculation (solid blue
line), five-beam calculation (green line), and corrected DBS calculation
(dashed black line). Mean wind speed from sonic anemometer is shown in
<bold>(h)</bold>. Data are shown from the BAO on 25 March 2014 at
100 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> (left panels) and from the ARM site on 23 June 2013 at
60 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> (right panels). The WindCube five-beam method results in
large underestimates of <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance, especially under convective
conditions at the BAO, while much better agreement is seen with the new
variance correction method.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f09.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p>Thirty-minute <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> variance, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance,
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance, <bold>(d)</bold> mean wind
speed,<?xmltex \hack{\break}?><bold>(e)</bold> mean wind direction, and
<bold>(f)</bold> Monin–Obukhov length at 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from sonic anemometer at
the ARM site. Data are shown from 19 to 23 June 2013, and tick marks for each
date correspond to 00:00 UTC on that day.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f10.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p>Averaged <bold>(a)</bold> <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> spectra, <bold>(b)</bold> <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> spectra, and
<bold>(c)</bold> <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> spectra for unstable conditions measured by the south BAO
sonic at 50 and 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and the ARM sonic at 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>. Black line
denotes theoretical <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> slope for inertial subrange. Note the larger
amount of energy contained at the lowest frequency scales at the BAO for the
<inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> component at both measurement heights.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/1993/2016/amt-9-1993-2016-f11.pdf"/>

        </fig>

      <p>As several of the Halo radial beams measured radial wind speeds that were
close to 0 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> during the afternoon of 25 March
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>a–f), it is possible that RIN caused
the Halo lidar to underestimate the variance at certain beam positions. To
further investigate this possibility, mean radial velocity and variance
values were calculated for 6 March 2014, a date from the campaign when
atmospheric conditions were less strongly convective and wind speeds were
higher during the late afternoon (Fig. <xref ref-type="fig" rid="Ch1.F8"/>).
Although there were some small biases in the radial wind speed measurements
from the Halo lidar (Fig. <xref ref-type="fig" rid="Ch1.F8"/>a–f), there were
no large discrepancies in the radial variance measurements on 6 March and no
strongly underestimated or negative <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>g–h). This suggests that the six-beam
technique is more accurate when wind speeds are higher, as radial variance
estimates are more accurate under higher wind speed conditions and more
accurate horizontal variance estimates are produced as a result. However, it
is difficult to make this assessment with the limited data set available. For
the 5-day period selected for this study, there was no clear trend between
the mean radial wind speed measured at each beam location and the error in
Halo-measured variance at each beam location. It should be noted that the
mean wind speeds measured during the afternoon of 25 March rarely exceeded
3 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, which is below the typical cut-in speed for a modern
wind turbine <xref ref-type="bibr" rid="bib1.bibx7" id="paren.68"><named-content content-type="pre">e.g.,</named-content></xref>. Thus, variance measurements under
low wind speeds would likely not be used for wind energy applications.</p>
</sec>
<sec id="Ch1.S5.SS4">
  <title>Application of six-beam technique to WindCube lidar</title>
      <p>A technique similar to the six-beam strategy can be applied to the WindCube
data by substituting the DBS values of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula> into
Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). The <inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>v</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> term
drops out because either <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi></mml:mrow></mml:math></inline-formula> is equal to 0 for
every beam position, resulting in five equations and five unknowns. Similar
to the Halo six-beam technique, these equations can be solved simultaneously
to obtain values of the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance, which can then be rotated
into the coordinate system aligned with the mean wind.</p>
      <p>Variance measured by the individual WindCube beams is compared to variance
calculated from projected sonic data in Fig. <xref ref-type="fig" rid="Ch1.F9"/>.
Similar to the Halo lidar (Figs. <xref ref-type="fig" rid="Ch1.F7"/> and
<xref ref-type="fig" rid="Ch1.F8"/>), the variance of the radial velocities was
sometimes overestimated by the WindCube lidar and sometimes underestimated.
Although there were no large discrepancies between the WindCube and sonic
radial variance under unstable conditions (14:00–23:00 UTC), the five-beam
technique produced large <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance underestimates and several
negative variance values (Fig. <xref ref-type="fig" rid="Ch1.F9"/>f and g). Thus,
even when a lidar with better temporal resolution and a smaller scanning
circle than the Halo lidar is used, the simultaneous use of all the radial
beam velocity variances to calculate the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance can result in
large uncertainties, especially during unstable conditions.</p>
      <p>In summary, at this site, the WindCube and Halo lidars were not able to
measure the radial beam variances accurately enough to estimate the
horizontal variance values with a five- or six-beam technique, possibly
because wind speeds at the site were often too low to accurately measure
variance with lidars. In the next section, the five-beam technique is
evaluated at the ARM site, where mean wind speeds were much higher in
comparison to the BAO.<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S5.SS5">
  <title>Note on the effects of temporal resolution</title>
      <p>The temporal resolution between the sonic anemometers and the lidars at the
BAO is drastically different; while the NCAR and OU sonics collect data at
frequencies of 60 and 30 Hz, respectively, the lidars collect data at a
frequency of 1 Hz, with most scanning strategies taking much longer than 1 s. In order to examine the effect of temporal resolution on variance
estimates, the sonic data streams were artificially degraded in temporal
resolution and then used to calculate the three-dimensional variance
components. Temporal resolutions of 1, 4, 15, and 30 s were selected to
represent the time it takes the WindCube to update the wind vector, the time
for a full WindCube scan, the time for a full ZephIR scan, and the time for a
full Halo six-beam scan, respectively. On 25 March 2014, the use of either
1 or 4 s temporal resolution resulted in percent errors around 5 % for <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> and 10 % for <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> while the use of either 15 or 30 s resolution
resulted in larger errors of 20 to 50 % in the variance estimates (not
shown). Thus, the temporal resolution of the lidar scans likely influenced
the variance estimates in addition to the scanning strategy used,
particularly for the ZephIR and Halo lidars.<?xmltex \hack{\vspace{-3mm}}?></p>
</sec>
</sec>
<sec id="Ch1.S6">
  <title>Comparison of turbulence parameters: LABLE 2</title>
      <p>Plots of the 30 min variance, mean wind speed and direction, and
Monin–Obukhov length from the 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> sonic over 5 days at the ARM
site are shown in Fig. <xref ref-type="fig" rid="Ch1.F10"/>. Diurnal trends in the LABLE 2
turbulence parameters are similar to those seen in the LATTE data: turbulence
is fairly low during overnight, stable conditions before increasing during
daytime, convective conditions. However, mean wind speeds at the ARM site
were generally much higher than at the BAO, and winds were nearly constantly
from the south/southeast. In addition, variance values were generally much
higher at the ARM site. In comparison to the BAO, the ARM site is located in
much simpler terrain and SNR values tended to be much higher, so lidar
variance measurements are expected to be more accurate.</p>
      <p>Time series of 30 min radial variance values estimated at
60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from projected sonic data and WindCube lidar data during
LABLE 2 on 23 June 2013 are shown in the right panels of
Fig. <xref ref-type="fig" rid="Ch1.F9"/>. In contrast to the case shown
from the BAO (left panels in Fig. <xref ref-type="fig" rid="Ch1.F9"/>),
variance values are higher throughout the day and the WindCube lidar
nearly always underestimated the radial variance values calculated
from the projected sonic data
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>a–e). However, when applying the
DBS method, the WindCube again overestimated the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance
under unstable conditions as a result of variance contamination
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>f and g).</p>
      <p>The five-beam method and the variance correction method described in Sect. <xref ref-type="sec" rid="Ch1.S5.SS1.SSS1"/> were also applied to the 60m WindCube data at the ARM
site. Values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> obtained from the sonics at
the BAO were used in the variance correction equations (Eqs. <xref ref-type="disp-formula" rid="Ch1.E23"/>–<xref ref-type="disp-formula" rid="Ch1.E24"/>) to determine how well this
correction worked at a different site. At the ARM site, both the five-beam
method and variance correction method produced nearly identical variance
values under stable conditions, while the five-beam method produced much
lower variance values under unstable conditions (Fig. <xref ref-type="fig" rid="Ch1.F9"/>f, g). However, none of the five-beam <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values were negative, in contrast to the BAO data. This likely
occurred because the WindCube underestimated the variance from the radial
velocities by approximately the same amount throughout the day. In
particular, the WindCube measured lower <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance values than the sonic
anemometer during nearly all time periods on 23 June 2013 at the ARM site
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>e, right panel) while the WindCube
measured <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> variance values that were approximately the same as or slightly
higher than those measured by the sonic anemometers at the BAO (Fig. <xref ref-type="fig" rid="Ch1.F9"/>e, left panel). Similar to the six-beam
equations, the value of the vertical variance is subtracted from the sum of
the other terms in the five-beam equations. As discussed in Sect. <xref ref-type="sec" rid="Ch1.S5.SS3"/>, when the value of the vertical variance is large or the
vertical variance is overestimated, this can cause the calculated <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>
variance to become negative. This did not occur at the ARM site, as values of
the vertical variance were much smaller than variance values from the other
beam positions under unstable conditions, in contrast to the BAO, where the
vertical variance values were similar to the variance estimated from the
horizontal radial beams. Thus, the vertical variance term had a much larger
influence on the <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values for the example shown at the BAO
than it did at the ARM site.</p>
      <p>Velocity spectra from the two sites were calculated in order to examine the
scales of turbulence measured at the different locations. Averaged spectra
for unstable conditions are shown in Fig. <xref ref-type="fig" rid="Ch1.F11"/> for the 60 m
ARM sonic data and the 50 and 100 m BAO sonic data. The spectral power
calculated from the ARM site data is much higher than for the BAO data, which
is reflected by the higher values of variance measured at the ARM site in
comparison to the BAO (Figs. <xref ref-type="fig" rid="Ch1.F3"/> and <xref ref-type="fig" rid="Ch1.F10"/>). The
largest difference between the spectral shapes occurs for the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula> spectra,
where the peak in the ARM site spectrum is shifted to higher frequencies in
comparison to the BAO spectra at both 50 and 100 m. Thus, the vertical
turbulent scales present during the campaign at the ARM site appear to be
generally smaller than those measured at the BAO site under unstable
conditions. This caused the WindCube lidar to often underestimate the <inline-formula><mml:math display="inline"><mml:mi>w</mml:mi></mml:math></inline-formula>
variance at the ARM site, as the effects of temporal resolution and volume
averaging are more significant for smaller turbulent scales. SNR values were
also generally higher at the ARM site than at the BAO, so lower amounts of
noise in the raw velocity data also likely led to the measurement of smaller
vertical variance values. In addition, differences in season and measurement
site characteristics may have affected the turbulent scales observed at the
two sites. Higher mean wind speeds at the ARM site (Fig. <xref ref-type="fig" rid="Ch1.F9"/>h) also likely led to more accurate variance
values in comparison to the BAO.
<?xmltex \hack{\vspace{-3mm}}?></p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <title>Summary and conclusions</title>
      <p>The VAD and DBS scanning strategies, a novel correction method for the DBS
strategy, and the six-beam lidar scanning strategy <xref ref-type="bibr" rid="bib1.bibx33" id="paren.69"/> were
evaluated at two measurement sites: the Southern Great Plains ARM site and
the Boulder Atmospheric Observatory. As a 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> tower with 12
sonic anemometers was located at the BAO, the evaluation primarily focused on
data collected there.</p>
      <p>One of the primary disadvantages of using a VAD or DBS technique with a high
scanning elevation angle is the variance contamination that can occur as a
result of differences in the instantaneous velocity at different parts of the
scanning circle. In our work, the VAD and DBS techniques often measured
variance values that were 60–80 % larger than those measured by a sonic
anemometer as a result of variance contamination. Although using a smaller
scanning cone mitigates the effects of horizontal heterogeneity on wind speed
estimates, it also increases the contribution of variance contamination (Eqs. <xref ref-type="disp-formula" rid="Ch1.E23"/>–<xref ref-type="disp-formula" rid="Ch1.E24"/>). In this work, a method was
developed to correct DBS-estimated variance values for contamination. The
additional variance terms were quantified using estimates of the
autocorrelation functions <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from sonic
anemometer data at the BAO and vertical variance measured by the WindCube's
vertical beam. This correction method was not expected to completely
eliminate variance contamination, as estimations of the autocorrelation
functions from the sonic anemometers were not fully representative of the
decorrelation that actually occurs across the DBS scanning circle. In
addition, it was assumed that turbulent fluxes remain constant across the
scanning circle, which is not always true. However, the correction method
still reduced WindCube variance overestimates by over 20 % under unstable
conditions at both the BAO and the ARM site. The correction method can be
applied to other lidars that have a vertical beam position and does not
require the use of a scanning lidar or complex calculations. Thus, it is a
method that can be easily used by wind farm managers or researchers with
commercially available lidars.</p>
      <p>Another way to reduce variance contamination is to combine the radial
velocity variance values and solve a set of equations to calculate the
variance. This method was suggested by <xref ref-type="bibr" rid="bib1.bibx33" id="text.70"/> as a scanning
strategy with six beam positions, and it can also be applied to the five beam
positions used by the WindCube lidar. At the BAO, the calculation of
horizontal variance with the five- and six-beam equations often led to
variance underestimates and even negative <inline-formula><mml:math display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> variance values
(Figs. <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F9"/>). The
technique appears to be strongly affected by inaccurate variance measurements
from one or more beam positions, which could be due to the low wind speeds
and low SNR values measured at the BAO. At the ARM site, wind speeds were
much higher and the WindCube lidar nearly always underestimated the radial
velocity variances, likely as a result of the smaller turbulent scales
present at the ARM site. The uniform underestimation of the radial velocity
variances around the scanning circle led to more accurate five-beam variance
estimates at the ARM site.</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>The authors would like to thank the staff of the Southern Great Plains ARM
site, Tim Lim from NCAR, Lucas Root from NorthWest Research Associates,
Shiril Tichkule from the University of Colorado at Boulder, Bruce Bartram and
Daniel Wolfe from NOAA/ESRL's Physical Sciences Division, Marc Fischer and
Sebastien Biraud from Lawrence Berkeley National Laboratory, the Boundary
Layer Integrated Sensing and Simulation group at OU, and the technical
support staff at Campbell Scientific, Leosphere, and Halo Photonics for their
assistance during the experiments. We would also like to acknowledge the
efforts of two reviewers, whose comments and suggestions helped improve the
manuscript. LABLE 2 data were obtained from the Atmospheric Radiation
Measurement (ARM) Climate Research Facility, a US Department of Energy
Office of Science user facility sponsored by the Office of Biological and
Environmental Research. J. F. Newman and S. Wharton received funding from the
Laboratory Directed Research and Development (LDRD) award number 12-ERD-069
from the Lawrence Livermore National Laboratory. Livermore National
Laboratory is operated by Lawrence Livermore National Security, LLC, for the
US Department of Energy, National Nuclear Security Administration, under
contract DE-AC52-07NA27344.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: M. Rapp</p></ack><ref-list>
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a lidar. To mitigate some of these errors, a scanning strategy was recently
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anemometers.</p><p class="p">Results indicate that the six-beam strategy mitigates some of the errors
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in the variance measured at the different beam positions. The ZephIR and
WindCube lidars overestimated horizontal variance values by over 60 %
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