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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-19-6607-2026</article-id><title-group><article-title>Physically constrained retrieval of fog visibility from millimeter-wavelength cloud radar observations</article-title><alt-title>Physically constrained retrieval of fog visibility from MMCR observations</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Li</surname><given-names>Xiaojie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Ge</surname><given-names>Jinming</given-names></name>
          <email>gejm@lzu.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Qiu</surname><given-names>Yucheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2">
          <name><surname>Lv</surname><given-names>Qiaoyi</given-names></name>
          <email>414562004@qq.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Song</surname><given-names>Wei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Jie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Chi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Liu</surname><given-names>Bochun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wang</surname><given-names>Jiapeng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Xia</surname><given-names>Hongwei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhu</surname><given-names>Yuhang</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Laboratory for Semi-Arid Climate Change of the Ministry of Education and the College of Atmospheric Sciences, Lanzhou University, Lanzhou, 730000, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Xiamen Key Laboratory of Straits Meteorology, Xiamen, 361012, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Tianjin Weather Modification Office, Tianjin, 300061, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Powerchina Sichuan Electric Power Engineering Co., Ltd., Chengdu, 610000, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jinming Ge (gejm@lzu.edu.cn) and Qiaoyi Lv (414562004@qq.com)</corresp></author-notes><pub-date><day>20</day><month>October</month><year>2026</year></pub-date>
      
      <volume>19</volume>
      <issue>20</issue>
      <fpage>6607</fpage><lpage>6623</lpage>
      <history>
        <date date-type="received"><day>24</day><month>February</month><year>2026</year></date>
           <date date-type="rev-request"><day>30</day><month>March</month><year>2026</year></date>
           <date date-type="rev-recd"><day>2</day><month>August</month><year>2026</year></date>
           <date date-type="accepted"><day>6</day><month>September</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Xiaojie Li et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026.html">This article is available from https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026.html</self-uri><self-uri xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e194">Fog severely degrades visibility (Vis) and poses substantial risks to transportation and aviation, yet quantitative monitoring remains challenging because conventional ground-based instruments provide spatially limited point observations and cannot resolve three-dimensional fog structure, while passive satellite retrievals have insufficient vertical resolution and difficulty separating fog from low cloud. Millimeter-wavelength cloud radar (MMCR) can penetrate fog and provide fine spatiotemporal resolution, but many radar Vis retrievals rely on empirical reflectivity–visibility relations. This study develops a physically constrained, observation-calibrated single-wavelength Ka-band MMCR retrieval that links reflectivity, liquid water content (LWC), geometric median radius, extinction, and Vis through lognormal droplet-size-distribution moments. A segment-wise mass-absorption LWC power law and an extinction-oriented radius power law are fitted to same-source FM-120 extinction-matching pseudo-targets, achieving a mean absolute fractional extinction error of 9.37 % on the development dataset. In ten spring-2025 DNQ3-conditioned cases, the present retrieval attains a mean absolute error of 0.092 km, while the local FM-120 and Liu et al. (2019) relations yield broadly comparable ranges and the Gultepe et al. (2009) relation departs more strongly. This method improves the physical self-consistency of single-band MMCR fog Vis retrieval without requiring auxiliary in-situ observations and provides technical support for three-dimensional coastal fog monitoring and traffic meteorological early warning.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42275076</award-id>
<award-id>42427804</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e206">Fog forms when moist air near the surface becomes saturated and water vapor condenses into droplets, often reducing horizontal visibility (Vis) to below 1 km. It is prevalent in valleys and in mountainous, urban, and coastal regions, where radiative cooling, moisture advection, evaporation, or orographic lifting can cause near-surface air to reach saturation. Fog poses substantial risks to port operations, maritime traffic safety, and regional economic activities <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx23 bib1.bibx9" id="paren.1"/>. As the core parameter for quantifying fog intensity and guiding operational decisions, Vis is defined as the maximum horizontal distance at which an observer with normal eyesight can distinguish a target against its background under current weather conditions <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx27 bib1.bibx30" id="paren.2"/>. Despite its operational importance, accurate measurement of Vis and characterization of fog structure remain challenging because of limitations in existing observational techniques.</p>
      <p id="d2e215">Various instruments have been used to conduct fog observations. Ground-based sensors such as optical visibility meters and fog droplet spectrometers provide high-precision point measurements but fail to capture the horizontal or vertical distribution of fog <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx6 bib1.bibx40" id="paren.3"/>. Laser-based active remote-sensing instruments (e.g., lidar, ceilometers) offer vertical profiling capabilities; however, their signals suffer severe attenuation in dense fog, often leading to signal saturation or complete loss <xref ref-type="bibr" rid="bib1.bibx38" id="paren.4"/>. Satellite passive imagers enable large-scale fog detection but struggle to distinguish fog from low-level clouds and lack vertical resolution to resolve internal stratification or microphysical structures <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx15" id="paren.5"/>. These limitations hinder reliable short-term fog nowcasting and proactive risk mitigation in transportation and maritime operations <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx1 bib1.bibx20 bib1.bibx13" id="paren.6"/>. In recent years, millimeter-wave cloud radar (MMCR) has gained prominence in fog monitoring due to its strong penetration, fine spatiotemporal resolution, and sensitivity to small hydrometeors. Field campaigns such as the 2021 Pingtan Sea Fog Experiment in China's Fujian Province have shown that Ka-band radar maintains robust signal integrity under dense fog conditions <xref ref-type="bibr" rid="bib1.bibx18" id="paren.7"/>. <xref ref-type="bibr" rid="bib1.bibx2" id="text.8"/> utilized dual-frequency radar to observe multi-layer fog, and by assimilating these radar data into the Applications de la Recherche à l'Opérationnel à Méso-Echelle (AROME) model, they reduced the fog-top height error by 64 % and largely improved visibility forecasts. In the absence of large hydrometeors, MMCR has gained prominence in fog monitoring for its strong penetration, fine resolution, and sensitivity to small hydrometeors <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx27 bib1.bibx30" id="paren.9"/>. The development of millimeter-wave radar has thus provided a new means for fog detection.</p>
      <p id="d2e240">Previous studies have advanced the quantification of fog visibility. Early work proposed an inverse relationship between <inline-formula><mml:math id="M1" display="inline"><mml:mi mathvariant="normal">Vis</mml:mi></mml:math></inline-formula> and LWC through bulk microphysical analysis. Subsequent studies showed that DSD strongly modulates extinction and visibility <xref ref-type="bibr" rid="bib1.bibx10" id="paren.10"/>. <xref ref-type="bibr" rid="bib1.bibx12" id="text.11"/> incorporated droplet number concentration into a multiparameter scheme, improving <inline-formula><mml:math id="M2" display="inline"><mml:mi mathvariant="normal">Vis</mml:mi></mml:math></inline-formula> estimates in numerical weather prediction models by up to 50 %. <xref ref-type="bibr" rid="bib1.bibx34" id="text.12"/> further incorporated effective droplet diameter. These studies indicate that fog microphysical properties can improve the physical consistency of visibility estimation <xref ref-type="bibr" rid="bib1.bibx37 bib1.bibx19 bib1.bibx7" id="paren.13"/>. Nevertheless, most radar-based <inline-formula><mml:math id="M3" display="inline"><mml:mi mathvariant="normal">Vis</mml:mi></mml:math></inline-formula> parameterizations remain empirical and are commonly obtained by directly fitting <inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="normal">Vis</mml:mi></mml:math></inline-formula> to <inline-formula><mml:math id="M5" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx14" id="paren.14"/>. Although <xref ref-type="bibr" rid="bib1.bibx25" id="text.15"/> introduced radar attenuation correction, the resulting retrieval still relies mainly on empirical relations. Approaches that account for microphysical effects often require auxiliary attenuation or microphysical measurements, restricting operational flexibility where supporting instruments are unavailable.</p>
      <p id="d2e297">In this study, we develop a physically based, observation-constrained visibility retrieval algorithm for single-wavelength Ka-band MMCR. Radar transmission theory and fog microphysics provide moment-based links among reflectivity (<inline-formula><mml:math id="M6" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>), liquid water content (LWC), effective radius (<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and extinction coefficient (<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>); however, these physical relations alone cannot resolve the ill-posedness inherent in single-wavelength radar measurements. We therefore use five years of FM-120 droplet size distributions as a priori microphysical constraints to inform the retrieval. Specifically, the observed microphysical ranges are used to (i) constrain the initialization and bounds of the mass-absorption-based LWC inversion and (ii) establish an extinction-oriented power-law relationship between the geometric median radius (<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and linear reflectivity (<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Section 2 describes the instrumentation and FM-120 processing. Section 3 presents the theoretical framework, the observed DSD regimes, and the two-step retrieval. Section 4 evaluates retrieval uncertainties associated with DSD shape, the constant-<inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> approximation, and perturbations in LWC and radius. Section 5 demonstrates the algorithm through a 2025 sea-fog case study and a ten-event consistency comparison. Section 6 summarizes the findings and limitations.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Instrumentation and data</title>
      <p id="d2e371">Dedicated monitoring campaigns have been conducted at DOB since 2019. The YLUKA2 solid-state Ka-band dual-polarization cloud radar provides reflectivity for the visibility retrieval. A DNQ3 visibility meter provides the near-surface point record for the ten-event consistency comparison, and an FM-120 spectrometer provides DSD and microphysical measurements for algorithm development and sensitivity analysis <xref ref-type="bibr" rid="bib1.bibx39" id="paren.16"/>.</p>
      <p id="d2e377">The YLUKA2 MMCR is installed at the highest point of DOB, with an antenna height of approximately 25 m. It operates at 34.50–35.50 GHz with an adjustable center frequency and integrates solid-state transmission, dual-transmitter/dual-receiver linear polarization, and fully coherent pulse-Doppler technology. Manufacturer specifications list 30 m spatial resolution, a 30 km maximum detection range, a 42 dB ground-clutter suppression ratio, and a minimum detectable reflectivity factor of <inline-formula><mml:math id="M12" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>30 dBZ at 10 km. The YLUKA2 MMCR performs sector Plan Position Indicator (PPI) scans at a fixed elevation angle of 2°, conducting continuous azimuthal surveillance between 60 and 300°. The YLUKA2 MMCR data used in this study are primarily affected by clear-sky ground clutter. As this method places high demands on data continuity, we recorded the ground clutter under clear-sky conditions and subsequently subtracted this clutter contribution to complete the ground clutter removal <xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx4 bib1.bibx21" id="paren.17"/>.</p>
      <p id="d2e390">The FM-120 operated continuously from 2019 through 2023. It measures droplets from 2–50 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m at 1 Hz in 30 non-equidistant size bins. The DSD observations are used to derive fog microphysical parameters, including <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWC, and <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, for algorithm development and sensitivity analysis.</p>
      <p id="d2e423">The DNQ3 visibility meter operates on the forward-scattering principle. It emits infrared pulses with a central wavelength of 0.87 <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, and the sensor receives light scattered at a forward angle. The instrument is approximately 153 m from the radar along azimuth 150°. Because this position is near the radar's minimum range, a nearby radar point whose temporal variation is most consistent with the DNQ3 trend is selected for matching. The ten spring-2025 cases were included when DNQ3 visibility remained continuously below 1000 m for at least 30 min and no other precipitation weather occurred during the interval.</p>
      <p id="d2e435">The DOB location and MMCR installation are shown in Fig. <xref ref-type="fig" rid="F1"/>.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e442"><bold>(a)</bold> Geographical location of DOB in Xiang'an District, Xiamen. The red mark denotes the observation station. The base map of the regional overview is provided by corresponding author Qiaoyi Lv; the inset satellite imagery is sourced from Baidu Maps, © Baidu Inc., used for academic research only. <bold>(b)</bold> The YLUKA2 MMCR installation at the observation site.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f01.jpg"/>

      </fig>

<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>FM-120 processing and observational constraints</title>
      <p id="d2e463">The FM-120 fog droplet spectrometer operated at the Datan Observation Base from 2019 through 2023. It measured droplets over a nominal diameter range of 2–50 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m in 30 non-equidistant channels at 1 Hz.</p>
      <p id="d2e474">A new event was defined when the gap between consecutive valid minutes exceeded 30 min. After quality control, the spectral-regime dataset aggregates 236037 contributing 1 Hz records into 4234 valid 1 min spectra from 28 events by summing particle counts and dividing by the summed sampling volume. For channel <inline-formula><mml:math id="M18" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, the 1 min number concentration was <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the particle count and <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is sampled volume. With <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in metres, <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in millimetres, <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>D</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in m<sup>−3</sup> mm<sup>−1</sup>, and <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in m<sup>−3</sup>, the discrete calculations were

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M29" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">LWC</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi></mml:munder><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mi mathvariant="italic">π</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msubsup><mml:mi>r</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi></mml:munder><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msubsup><mml:mi>D</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msubsup><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>[</mml:mo><mml:msup><mml:mi mathvariant="normal">mm</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>i</mml:mi></mml:munder><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>Q</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:msubsup><mml:mi>r</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>[</mml:mo><mml:mo>/</mml:mo><mml:mi mathvariant="normal">m</mml:mi><mml:mo>]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msubsup><mml:mi>r</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msubsup><mml:mi>r</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the size-dependent Mie extinction efficiency evaluated at 550 nm. Total number concentration and the number-weighted radius summary were obtained from the same discrete spectrum. All of these quantities share the same DSD source and therefore provide sample-internal conditioning variables rather than independent visibility observations; no separate historical interpolation or concentration-residual processing chain is implied by Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>).</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Observation-constrained retrieval development</title>
      <p id="d2e868">The classical Koschmieder law <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx16" id="paren.18"/> expresses <inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="normal">Vis</mml:mi></mml:math></inline-formula> as

          <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M32" display="block"><mml:mrow><mml:mi mathvariant="normal">Vis</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mi mathvariant="italic">ε</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mn mathvariant="normal">0.02</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

        where <inline-formula><mml:math id="M33" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> is the brightness-contrast threshold, typically set to 0.02, and <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the extinction coefficient (unit: <inline-formula><mml:math id="M35" display="inline"><mml:mrow><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>) at 550 nm. According to Mie scattering theory,

          <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M36" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mi mathvariant="normal">∞</mml:mi></mml:munderover><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">π</mml:mi><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">d</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:math></disp-formula>

        where <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the extinction efficiency for a droplet of radius <inline-formula><mml:math id="M38" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the fog DSD (unit: <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), which is commonly represented by a lognormal distribution <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx32" id="paren.19"/>:

          <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M41" display="block"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msqrt><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi></mml:mrow></mml:msqrt><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>r</mml:mi><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mi>exp⁡</mml:mi><mml:mfenced open="[" close="]"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mi>ln⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:math></disp-formula>

        Here, <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is total droplet number concentration, <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is geometric median radius, and <inline-formula><mml:math id="M44" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> is logarithmic spectral width. For a lognormal distribution, the <inline-formula><mml:math id="M45" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>th DSD moment can be written as

          <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M46" display="block"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mi>k</mml:mi></mml:msubsup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e1215">MMCR operates in the millimetre-wave band, where most fog droplets are in the Rayleigh regime. The attenuation-corrected radar reflectivity factor <inline-formula><mml:math id="M47" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> is proportional to the sixth DSD moment:

          <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M48" display="block"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">64</mml:mn><mml:msub><mml:mi>M</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">64</mml:mn><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msubsup><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">18</mml:mn><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:math></disp-formula>

        Because <inline-formula><mml:math id="M49" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> depend on different DSD moments, they cannot be linked uniquely without intermediate microphysical information. LWC and effective radius are defined by

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M51" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">LWC</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi>M</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">9</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">5</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

        where <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is water density. Eliminating <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M54" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> from the moment relations gives <xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx35" id="paren.20"/>

          <disp-formula id="Ch1.E9" content-type="numbered"><label>9</label><mml:math id="M55" display="block"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle></mml:msubsup><mml:msup><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mi>Z</mml:mi></mml:mrow><mml:mrow><mml:mn mathvariant="normal">48</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">LWC</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">5</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:msup></mml:mrow></mml:math></disp-formula>

        In the visible band, the extinction efficiency of sufficiently large fog droplets approaches 2 <xref ref-type="bibr" rid="bib1.bibx29" id="paren.21"/>. Figure <xref ref-type="fig" rid="F2"/> shows its radius dependence at 550 nm.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1506">Size dependence of <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at 550 nm. Red points mark radii associated with the FM-120 size bins. The constant value <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> is an asymptotic approximation rather than an exact representation over the sampled small-droplet range.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f02.png"/>

      </fig>

      <p id="d2e1542">For <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, extinction is <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">LWC</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Substitution of Eq. (<xref ref-type="disp-formula" rid="Ch1.E9"/>) gives

          <disp-formula id="Ch1.E10" content-type="numbered"><label>10</label><mml:math id="M60" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">LWC</mml:mi></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">3</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:msubsup><mml:msup><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mi>Z</mml:mi></mml:mrow><mml:mn mathvariant="normal">48</mml:mn></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">5</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:msup><mml:msup><mml:mi mathvariant="normal">LWC</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">32</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        All quantities are evaluated in consistent SI units, including <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, LWC, radius, and the conventional <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">mm</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> reflectivity factor. Combining Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>) with Koschmieder's relation yields

          <disp-formula id="Ch1.E11" content-type="numbered"><label>11</label><mml:math id="M63" display="block"><mml:mrow><mml:mi mathvariant="normal">Vis</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.91</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msubsup><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle></mml:msubsup><mml:msup><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">w</mml:mi></mml:msub><mml:mi>Z</mml:mi></mml:mrow><mml:mn mathvariant="normal">48</mml:mn></mml:mfrac></mml:mstyle></mml:mfenced><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">5</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:msup><mml:mi mathvariant="normal">LWC</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">32</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Equation (<xref ref-type="disp-formula" rid="Ch1.E10"/>) requires both LWC and <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, neither of which is uniquely determined by one MMCR reflectivity measurement. We therefore use two observation-constrained steps. The mass-absorption/TRR routine retrieves LWC and applies liquid-water attenuation correction, and the FM-120 development data provide the conditional radius–reflectivity relations.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>FM-120-observed spectral regimes and retrieval context</title>
      <p id="d2e1813">This section characterizes the morphology of fog droplet size distributions (DSDs) and the variation of microphysical parameters across fog intensity grades, drawing on long-term FM-120 observations. The results provide observational constraints for the visibility-retrieval parameterization developed in subsequent sections and delineate the applicability boundary of the single-lognormal closure assumption.</p>
<sec id="Ch1.S3.SS1.SSS1">
  <label>3.1.1</label><title>Data processing and spectral shape classification</title>
      <p id="d2e1824">Following standard classification criteria for fog DSD morphology, each 1 min spectrum is assigned to one of four definite shape categories: narrow unimodal, broad unimodal, shoulder, and bimodal. An additional uncertain status is reserved for samples with indistinct morphological features: spectra with a stability score below 0.80 are labeled as uncertain. Among them, 584 samples exhibit a weak two-peak pattern but are not classified as bimodal due to insufficient peak separation.</p>
      <p id="d2e1827">Across the full dataset, shoulder and broad-unimodal spectra account for the largest proportions, at 41.83 % and 33.54 %, respectively. Bimodal spectra make up 6.38 %, and narrow-unimodal spectra account for 4.32 %. The remaining 13.93 % fall into the uncertain status. Median normalized spectra and interquartile ranges for each shape category are shown in Fig. <xref ref-type="fig" rid="F3"/>a. Narrow-unimodal spectra have the smallest peak diameter and narrowest spectral width, while bimodal spectra exhibit a primary mode near 5 <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m and a secondary mode near 25 <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, with an overall spectral width substantially larger than that of unimodal spectra.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e1850">FM-120 spectral summaries from the spectral-regime dataset. <bold>(a)</bold> Median normalized spectra and interquartile ranges by fixed shape label. <bold>(b)</bold> Event-balanced hard-label composition in DSD-derived visibility bins; the dashed line marks the pre-specified 200 m split. <bold>(c)</bold> Minute-weighted, event-balanced, and label-resampling bimodal summaries.</p></caption>
            <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f03.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <label>3.1.2</label><title>Evolution of spectral shapes across visibility grades</title>
      <p id="d2e1876">To examine how DSD shapes vary with fog intensity, samples are grouped into four visibility grades according to meteorological fog classification standards, based on DSD-derived visibility: heavy fog (500 m <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m), dense fog (200 m <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> m), very dense fog (50 m <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m), and extremely dense fog (<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi>V</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> m). An event-balanced statistical approach is applied: the fraction of each shape category within each visibility bin is first calculated per event, then averaged across all events with equal event weights. The spectral shape composition across visibility grades is presented in Fig. <xref ref-type="fig" rid="F3"/>b.</p>
      <p id="d2e1935">Statistical results show that the proportion of bimodal spectra rises markedly as visibility decreases: Heavy fog (500–1000 m): bimodal spectra account for only 0.77 % (95 % confidence interval: 0.03 %–1.79 %), with unimodal and shoulder shapes dominating; Dense fog (200–500 m): the bimodal fraction increases to 4.22 % (95 % confidence interval: 1.45 %–7.96 %); Very dense fog (100–200 m): the bimodal fraction jumps to 24.07 % (95 % confidence interval: 9.11 %–40.04 %); The 50–100 m bin yields a point estimate of 35.90 % bimodal fraction, but only 3 events contribute to this interval with a confidence interval spanning 0 %–100 %, so it is not used for robust quantitative inference.</p>
      <p id="d2e1938">No DSD samples are available for the extremely dense fog (0–50 m) grade in this dataset. Overall, when visibility falls below 200 m, the deviation of fog DSD from a single lognormal distribution becomes pronounced, and bimodal structures emerge as a non-negligible spectral feature. Figure <xref ref-type="fig" rid="F3"/>c also presents bimodal fractions under alternative statistical frameworks (minute-weighted, event resampling), all of which show consistent trends.</p>
</sec>
<sec id="Ch1.S3.SS1.SSS3">
  <label>3.1.3</label><title>Comparison of microphysical parameters between two visibility strata</title>
      <p id="d2e1952">Building on the 200 m visibility threshold identified above, samples are further divided into a low-visibility stratum (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Mie</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m) and a high-visibility stratum (200 m <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Mie</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m). We compare the distribution of five microphysical parameters between the two strata: radar-equivalent reflectivity factor <inline-formula><mml:math id="M73" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>, total number concentration <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, liquid water content (LWC), effective radius <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and geometric median radius <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as illustrated in Fig. <xref ref-type="fig" rid="F4"/>.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2036">Timestamp-resolved FM-120 parameter distributions in the pre-specified strata <bold>(a)</bold> <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Mie</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">200</mml:mn></mml:mrow></mml:math></inline-formula> m and <bold>(b)</bold> 200 m <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Mie</mml:mi></mml:msub><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m. Rows show FM-120/DSD-derived radar-equivalent <inline-formula><mml:math id="M79" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> (dBZ), <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), LWC (g m<sup>−3</sup>), <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m), and the visibility-workflow geometric-median-radius proxy <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M86" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m). Each histogram is normalized within its stratum; dashed lines denote sample medians.</p></caption>
            <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f04.png"/>

          </fig>

      <p id="d2e2171">Distinct microphysical differences are observed between the two strata. The median <inline-formula><mml:math id="M87" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> in the low-visibility stratum is <inline-formula><mml:math id="M88" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.61 dBZ, 4.92 times the value of <inline-formula><mml:math id="M89" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.53 dBZ in the high-visibility stratum, a difference of approximately 6.92 dBZ corresponding to a 4.92-fold increase.</p>
      <p id="d2e2196">The median <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWC in the low-visibility stratum are <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mn mathvariant="normal">97.31</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<sup>−3</sup> and 0.21 g m<sup>−3</sup>, 2.19 times and 3.83 times the values in the high-visibility stratum (<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mn mathvariant="normal">44.34</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> m<sup>−3</sup>, 0.06 g m<sup>−3</sup>), respectively, also showing strong discriminative power.</p>
      <p id="d2e2290">Differences in radius parameters between the two strata are comparatively small. The geometric median radius <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and effective radius <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the low-visibility stratum are 13.57 and 11.90 <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, only 0.83 and 1.55 <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m larger than in the high-visibility stratum, with far weaker separability than reflectivity and LWC.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Mass-absorption-constrained LWC retrieval</title>
      <p id="d2e2340">In the visibility parameterization, accurate retrieval of liquid water content (LWC) and unattenuated radar reflectivity factor <inline-formula><mml:math id="M101" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> are essential. Therefore, we adopted the self-consistent LWC retrieval algorithm developed in Ge's research <xref ref-type="bibr" rid="bib1.bibx11" id="paren.22"/> to calculate LWC, and correct the absorption attenuation in the measured radar reflectivity <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e2364">The attenuation of millimeter-wave radar signals during propagation in fog is mainly caused by mass absorption of water droplets. Under the Rayleigh approximation, one-way liquid-water attenuation is proportional to LWC, <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>K</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mi mathvariant="normal">LWC</mml:mi></mml:mrow></mml:math></inline-formula>, independent of the droplet size distribution. Here, <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is determined by the radar wavelength, temperature, and complex refractive index of cloud droplets, and can be treated as a constant for a millimeter-wave radar operating at a fixed wavelength. Based on this, a self-consistent LWC retrieval framework is adopted: the radar radiative transfer equation is transformed into a Bernoulli differential equation and integrated within the cloud layer to establish a constrained relationship among the measured reflectivity factor <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the true reflectivity factor <inline-formula><mml:math id="M106" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>, and LWC. To obtain a closed-form solution, a segment-wise power-law relation is employed as a numerical closure. A bounded trust-region reflective (TRR) least-squares solver is used to optimize the parameter vector by minimizing the absolute dBZ residual between the measured and reconstructed reflectivity <xref ref-type="bibr" rid="bib1.bibx5" id="paren.23"/>. The reconstructed reflectivity is expressed as

            <disp-formula id="Ch1.E12" content-type="numbered"><label>12</label><mml:math id="M107" display="block"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mrow><mml:mi mathvariant="normal">mc</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">r</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>c</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msubsup><mml:mi mathvariant="normal">LWC</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">r</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mi>b</mml:mi></mml:mfrac></mml:mstyle></mml:msubsup><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.46</mml:mn><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:munderover><mml:msup><mml:mi>K</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mi mathvariant="normal">LWC</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">d</mml:mi><mml:mi>s</mml:mi></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          where the effect of gaseous attenuation on radiative transfer is neglected. Once LWC is retrieved, the accumulated attenuation can be readily computed and applied to correct the measured reflectivity. Given the substantial variability in liquid water path (LWP) along fog profiles detected by radar – as noted in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>, bimodal fog events exhibit significant enhancements in both <inline-formula><mml:math id="M108" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> and LWC – a 10-bin segmentation approach is applied to partition the profile into segments such that the LWP of each segment falls within the bounds prescribed by the TRR method. The numerical branch is selected according to the maximum original reflectivity within each segment: for a maximum not exceeding <inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 dBZ, the starting vector is <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>; for a maximum greater than <inline-formula><mml:math id="M111" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 dBZ, it is <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>. Both branches use lower bounds <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula> and upper bounds <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>. Each segment is fitted independently, with the accumulated attenuation derived from the retrieved LWC applied to its reflectivity prior to fitting. This approach requires neither ancillary instruments nor empirical coefficients, achieving LWC retrieval and attenuation correction through the self-consistent interdependencies among cloud physical variables.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Extinction-oriented conditional parameterization of <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></title>
      <p id="d2e2622">In addition to accurate LWC retrieval, determining <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a critical step. Although observational studies on <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> have been conducted previously, no empirical relationship between <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M119" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> has been established for fog. Given that both <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M121" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> are intimately linked to DSD, a strong power-law correlation is expected. Herein, we adopt the power-function form <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:msup><mml:mi>Z</mml:mi><mml:mi>b</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> to parameterize this relationship.</p>
      <p id="d2e2704">A single-frequency reflectivity measurement cannot determine <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> uniquely because total number concentration and spectral width also affect the sixth DSD moment. We therefore compare two sample-internal conditional parameterizations. The direct radius-space fit is used only as a comparison baseline. The selected extinction-oriented relation is fitted to extinction-matching pseudo-targets in the moment-closure development dataset; the pseudo-targets are constructed from reflectivity, LWC, and size-dependent Mie extinction co-derived from the same FM-120 DSD.</p>
      <p id="d2e2718">For each development row <inline-formula><mml:math id="M124" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, candidate radii from 1.00 to 20 <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m at 0.01 <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m spacing were inserted into Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>). The row-wise extinction-matching pseudo-target was

            <disp-formula id="Ch1.E13" content-type="numbered"><label>13</label><mml:math id="M127" display="block"><mml:mrow><mml:msubsup><mml:mi>r</mml:mi><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow><mml:mo>⋆</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:mi>arg⁡</mml:mi><mml:munder><mml:mo movablelimits="false">min⁡</mml:mo><mml:mrow><mml:mi>r</mml:mi><mml:mo>∈</mml:mo><mml:mi mathvariant="script">G</mml:mi></mml:mrow></mml:munder><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">closed</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>;</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mrow><mml:mi mathvariant="normal">lin</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">LWC</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">FM</mml:mi><mml:mn mathvariant="normal">120</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>|</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">FM</mml:mi><mml:mn mathvariant="normal">120</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M128" display="inline"><mml:mi mathvariant="script">G</mml:mi></mml:math></inline-formula> is the finite candidate grid. Thus <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msubsup><mml:mi>r</mml:mi><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow><mml:mo>⋆</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is a constructed radius pseudo-target, not an independently observed geometric median radius. A free power law was then fitted to these pseudo-targets by unweighted radius-space least squares:

            <disp-formula id="Ch1.E14" content-type="numbered"><label>14</label><mml:math id="M130" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">21.87</mml:mn><mml:msup><mml:mfenced open="[" close="]"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="normal">mm</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msup><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mn mathvariant="normal">0.20</mml:mn></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Linear <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the predictor for both relations, whereas dBZ is used only as a plotting coordinate. Against their respective fit targets, the direct relation has same-sample Pearson <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.74</mml:mn></mml:mrow></mml:math></inline-formula> and RMSE <inline-formula><mml:math id="M133" display="inline"><mml:mn mathvariant="normal">0.86</mml:mn></mml:math></inline-formula> <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, and the extinction-oriented relation has <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.73</mml:mn></mml:mrow></mml:math></inline-formula> and pseudo-target RMSE 1.64 <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m. Figure <xref ref-type="fig" rid="F5"/> displays the direct comparison baseline in panel (a) and the selected extinction-oriented relation in panel (b).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3001">Sample-internal radius–reflectivity fits. <bold>(a)</bold> Direct-fit subset with the FM-120-derived radius proxy. <bold>(b)</bold> Moment-closure development dataset with row-wise extinction-matching pseudo-targets. Linear <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is fitted, while dBZ is the display coordinate; equations, same-sample Pearson <inline-formula><mml:math id="M138" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>, and radius RMSE are shown to two decimal places.</p></caption>
          <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f05.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Evaluation of retrieval assumptions and uncertainties</title>
      <p id="d2e3043">The retrieval framework constructed in Sect. <xref ref-type="sec" rid="Ch1.S3"/> reduces reliance on direct visibility–reflectivity fitting, but its accuracy is ultimately governed by two algorithmic assumptions. The first is the constant extinction-efficiency approximation (<inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>), which replaces the size-dependent Mie efficiency shown in Fig. <xref ref-type="fig" rid="F2"/> with its large-particle asymptote. The second is the single-lognormal closure, which constrains the droplet size distribution to a parametric form that links reflectivity, liquid water content, and effective radius through shared moments. Both assumptions introduce structural biases whose magnitude depends on droplet size and spectral modality. Section 4.1 attributes the extinction-residual patterns revealed in Fig. <xref ref-type="fig" rid="F6"/> to these two sources: the weak-reflectivity bias is traced to the <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> approximation, while the broader residual reflects the lognormal closure and is partially mitigated by the extinction-oriented parameterization. Section 4.2 quantifies the analytical sensitivity of the retrieved extinction to perturbations in LWC and radius.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3084">Same-sample extinction-residual distributions for the moment-closure development dataset. <bold>(a, b)</bold> Three-dimensional residual density for the direct and extinction-oriented relations. <bold>(c, d)</bold> Direct-relation residual versus predicted radius and LWC; <bold>(e, f)</bold> corresponding extinction-oriented views. In <bold>(c)–(f)</bold>, colour denotes count per bin, white bands the interquartile range, and black curves the binned median; red references mark zero residual, and both methods share the residual scale.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f06.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>DSD effects on the radius–reflectivity relation and extinction retrieval</title>
      <p id="d2e3112">The DSD primarily affects the retrieval through the radius term.</p>
      <p id="d2e3115">To quantify the response to this structural variability, the direct and extinction-oriented relations are evaluated on the moment-closure development dataset. For each relation, the predicted radius is inserted into Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>) with the same row's <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">lin</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWC and compared with the same size-dependent Mie extinction reference. All quantities are same-sample and deterministic; there is no held-out subset or independent physical-radius observation. Accordingly, all <inline-formula><mml:math id="M142" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>, RMSE, signed-residual, and MAFE values in Sects. <xref ref-type="sec" rid="Ch1.S3.SS3"/> and <xref ref-type="sec" rid="Ch1.S4.SS1"/> are resubstitution diagnostics that measure numerical consistency with the development targets. The signed fractional residual and mean absolute fractional error (MAFE) are

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M143" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E15"><mml:mtd><mml:mtext>15</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">β</mml:mi><mml:mo mathvariant="normal" stretchy="true">^</mml:mo></mml:mover><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">FM</mml:mi><mml:mn mathvariant="normal">120</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">FM</mml:mi><mml:mn mathvariant="normal">120</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E16"><mml:mtd><mml:mtext>16</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">MAFE</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:mfenced close="|" open="|"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M144" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is the total number of rows in the moment-closure development dataset. For the <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">dBZ</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> subset, the signed mean of <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi mathvariant="italic">β</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is <inline-formula><mml:math id="M147" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25.32 %. The negative sign means that the closed-form extinction is lower on average than the same-row FM-120/Mie extinction; because visibility is inversely proportional to extinction, the closed-form result therefore tends toward visibility overestimation in this subset. This same-row, same-source signed mean is not an independent error estimate and is distinct from the signed mean and 22.01 % MAFE for the broader <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn><mml:mo>≤</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">dBZ</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> interval. The bimodal error structure visible in Fig. <xref ref-type="fig" rid="F6"/> can be attributed to the two algorithmic assumptions identified above. For weak-reflectivity cases, the predicted radii fall predominantly below 5 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, a range in which the actual Mie extinction efficiency at 550 nm deviates most strongly from the assumed constant value of 2 (Fig. <xref ref-type="fig" rid="F2"/>). Because the constant-<inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> approximation enters the analytical closure linking extinction to LWC and radius (Eq. <xref ref-type="disp-formula" rid="Ch1.E10"/>), this deviation systematically biases the closed-form extinction downward relative to the size-dependent Mie reference in the small-radius regime. The resulting extinction underestimation is consistent with the pronounced negative signed residual and elevated MAFE (22.01 %) observed in the weak-reflectivity bin of Fig. <xref ref-type="fig" rid="F6"/>. The residual that persists across the remaining reflectivity range arises primarily from the single-lognormal assumption: when the observed DSD departs from lognormality, as occurs increasingly at visibilities below 200 m where bimodal spectra become prevalent (Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>), the moment-based closure relating reflectivity, LWC, and radius no longer holds exactly. The extinction-oriented parameterization was designed to reduce precisely this distribution-shape error: by calibrating the radius–reflectivity relation against extinction-matching pseudo-targets rather than direct geometric radius proxies, it absorbs part of the departure from lognormality into the empirical power-law coefficients. The reduction in overall MAFE from 10.88 % to 9.37 %, and most notably from 12.25 % to 4.96 % at intermediate reflectivities, confirms the effectiveness of this strategy. The weak-reflectivity residual, however, is dominated by the <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> approximation and is not substantially improved by the extinction-oriented fitting alone.</p>
      <p id="d2e3378">Across the moment-closure development dataset, the direct relation yields an extinction MAFE of 10.88 %, whereas the extinction-oriented relation yields 9.37 %. The largest decrease occurs for <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn><mml:mo>≤</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">dBZ</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, from 12.25 % to 4.96 %.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Analytical sensitivity to LWC and <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></title>
      <p id="d2e3422">In practical application of the algorithm, reliable retrievals of LWC, <inline-formula><mml:math id="M154" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are essential for accurate visibility calculation via Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>). On one hand, the fog DSD does not strictly follow the lognormal distribution and may exhibit bimodal or multimodal characteristics, which introduces uncertainties into the calculation. On the other hand, both LWC and <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are derived from <inline-formula><mml:math id="M157" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> – while <inline-formula><mml:math id="M158" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> is simultaneously corrected during LWC retrieval via the self-consistent algorithm, residual deviations between the retrieved LWC and its true value still exist. Additionally, the corrected <inline-formula><mml:math id="M159" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> is influenced by LWC, which further propagates uncertainties to <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Furthermore, <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> itself is an estimated parameter, with a RMSE of 1.64 <inline-formula><mml:math id="M162" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m as shown in the validation results (Fig. <xref ref-type="fig" rid="F5"/>). To quantify the impact of these uncertainties on algorithm performance, we conducted perturbation simulations on both the retrieved LWC and empirically derived <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, with a focus on analyzing the resulting characteristics of retrieval errors. We define a relative extinction response <inline-formula><mml:math id="M164" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> that characterizes how retrieval extinction errors respond to perturbations in these two parameters. Let <inline-formula><mml:math id="M165" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M166" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> be multiplicative perturbations to <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWC. From Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>),

            <disp-formula id="Ch1.E17" content-type="numbered"><label>17</label><mml:math id="M168" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">pert</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="italic">α</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:msup><mml:msup><mml:mi mathvariant="italic">λ</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">32</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          so the relative extinction response is

            <disp-formula id="Ch1.E18" content-type="numbered"><label>18</label><mml:math id="M169" display="block"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi mathvariant="normal">ext</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">pert</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:msup><mml:mi mathvariant="italic">α</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">4</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle></mml:mrow></mml:msup><mml:msup><mml:mi mathvariant="italic">λ</mml:mi><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">32</mml:mn><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          <xref ref-type="bibr" rid="bib1.bibx11" id="text.24"/> reported that retrieved LWC can deviate from its true value by 50 % to 200 % under the self-consistent mass-absorption algorithm. In this study, the same fractional range applies to the empirically derived <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Both multipliers (<inline-formula><mml:math id="M171" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M172" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) are therefore varied from 0.50 to 2.00, spanning the physically plausible uncertainty range of these two parameters. Figure <xref ref-type="fig" rid="F7"/> displays the complete response range with a zero-centred normalization. The zero-response curve is <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi mathvariant="italic">α</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; same-signed perturbations partly compensate because radius and LWC enter with opposite-signed exponents. The larger LWC exponent produces a stronger analytical response to LWC perturbations. The ratio of the exponent magnitudes is <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">22</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">27</mml:mn><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">9</mml:mn><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">11</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">6</mml:mn><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1.83</mml:mn></mml:mrow></mml:math></inline-formula>, meaning that for any given fractional perturbation, the extinction response to LWC is approximately twice that of <inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. For instance, a 10 % increase in LWC raises the extinction by 8.1 %, whereas a 10 % increase in <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> lowers it by only 4.1 %. In practice, drizzle-sized droplets (diameter <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M178" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m) may appear near the fog top or during the mature-to-dissipation stage. Because the mass-absorption retrieval of LWC depends on the integrated liquid water mass (third DSD moment) rather than the sixth-moment reflectivity, it is intrinsically less sensitive to sparse large droplets; the attenuation coefficient <inline-formula><mml:math id="M179" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> remains closely tied to the bulk LWC, and no pronounced overestimation is expected. This is consistent with Fig. <xref ref-type="fig" rid="F7"/>, which shows that LWC perturbations dominate the extinction response. By contrast, the extinction-oriented <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M181" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> relation (Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/>) is calibrated against the FM-120 dataset, whose upper measurement limit is 50 <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m. When drizzle droplets dominate the radar sampling volume, they disproportionately increase reflectivity while contributing modestly to the geometric median radius inferred from the FM-120-constrained power law. Consequently, the parameterized <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> may be systematically biased high. Because <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> enters the visibility retrieval with a negative exponent (Eq. <xref ref-type="disp-formula" rid="Ch1.E10"/>), an overestimated <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> reduces the inferred extinction, partially offsetting the enhanced extinction from the larger droplets. The net retrieval error under drizzle contamination therefore depends on the competing effects of LWC (well constrained by mass absorption) and <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (poorly constrained by the FM-120-limited closure). A rigorous quantification of this trade-off requires dedicated observations extending into the drizzle regime.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e3888">Analytical relative extinction response to <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> multiplier <inline-formula><mml:math id="M188" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> and LWC multiplier <inline-formula><mml:math id="M189" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>. The black curve marks <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, the open circle marks the unperturbed state, and the diverging colour scale spans the complete calculated range.</p></caption>
          <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f07.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Application of the algorithm to visibility retrieval</title>
      <p id="d2e3944">Figures <xref ref-type="fig" rid="F8"/> and <xref ref-type="fig" rid="F9"/> illustrate the retrieved temporal and spatial evolution of fog microphysical parameters and visibility during a criterion-selected case on 2 March 2025. Influenced by a southern-branch trough, warm and humid southerly airflows advected over the observation site, producing a typical advection sea fog. The fog developed rapidly after 18:00 local standard time (LST) and reached maximum intensity around 21:00 LST. At the radar elevation angle of 2°, fog returns were detectable to a maximum range of approximately 10 km, and the fog-top height exceeded 350 m. Between 18:00 and 24:00 LST, the radar reflectivity factor <inline-formula><mml:math id="M191" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> generally decreased with increasing range, indicating a stable fog structure whose density decreased with altitude. During 20:00 to 22:00 LST, numerous range gates with <inline-formula><mml:math id="M192" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> exceeding <inline-formula><mml:math id="M193" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 dBZ were observed, with peak values approaching 0 dBZ. As shown in Fig. <xref ref-type="fig" rid="F8"/>, the polar scan at 20:29 LST reveals that high-<inline-formula><mml:math id="M194" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> regions were concentrated to the south and southwest of the observation site, where topographical undulations and man-made structures are distributed. The uneven underlying surface generates turbulence through surface friction, which promotes droplet coalescence and the formation of larger droplets, thereby enhancing <inline-formula><mml:math id="M195" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>.</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e3991">Polar radar scans at 20:29 LST on 2 March 2025: <bold>(a)</bold> measured radar reflectivity factor (dBZ) and <bold>(b)</bold> retrieved visibility (km). Range rings are in kilometres, and grey shading gives the displayed elevation context.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f08.png"/>

      </fig>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e4008">Application to the criterion-selected low-visibility case on 2 March 2025 (Local Standard Time, LST): <bold>(a)</bold> radar reflectivity (dBZ), <bold>(b)</bold> retrieved LWC (g m<sup>−3</sup>), <bold>(c)</bold> retrieved geometric median radius <inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M198" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m), and <bold>(d)</bold> retrieved visibility (km), shown versus LST and range (km); <bold>(e)</bold> visibility time series (km) comparing the DNQ3 visibility meter, the present retrieval, the local site-specific FM-120 relation, Liu et al. (2019, Eq. 7), and Gultepe et al. (2009, Fig. 10b), with provenance and equations in Table <xref ref-type="table" rid="T1"/>.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f09.png"/>

      </fig>

      <p id="d2e4067">To assess retrieval performance, the present method was cross-validated against DNQ3 forward-scattering visibility-meter observations and three direct empirical visibility–reflectivity relations (Table <xref ref-type="table" rid="T1"/>). Near-range radar data are susceptible to ground-clutter contamination, and the minimum detection range is approximately 150 m; the comparison point was therefore selected at 300 m along the 150° azimuth, where the temporal variation correlated most closely with DNQ3. A systematic height difference exists between the DNQ3 sensor at 1.5  m a.g.l. and the radar detection altitude of approximately 30 m at this range, arising from the 25 m antenna height and the beam elevation geometry. Notably, at 21:30 and 22:30 LST, DNQ3 visibility increased markedly while the radar retrievals did not show a corresponding rise. The intense radar echo around 21:00 LST indicates vigorous fog processes that induced droplet sedimentation; the resulting larger particles reduced the total droplet number concentration and raised near-surface visibility as measured by DNQ3 at 1.5 m, while the radar, sampling at a higher altitude, was less affected. Furthermore, the present retrieval is based on backscatter whereas DNQ3 exploits forward scattering, so inherent principle-related differences also contribute to the observed discrepancies. Comparison of FM-120-derived Mie-scattering visibility against DNQ3 shows the same tendency: the retrieval is lower than DNQ3 during the early-to-mature fog stage and converges during dissipation. It should also be noted that the FM-120 fog spectrometer has a limited observation range for large droplets, so variations in the median radius cannot be fully captured in the fitting process when large fog droplets are present, leading to larger biases in the fitted median-radius values.</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e4075">Direct visibility–reflectivity relations used in Figs. <xref ref-type="fig" rid="F9"/>e and <xref ref-type="fig" rid="F10"/>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="4cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="9.5cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left">Relation</oasis:entry>
         <oasis:entry colname="col2" align="left">Equation</oasis:entry>
         <oasis:entry colname="col3" align="left">Provenance and comparison role</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left">Local FM-120</oasis:entry>
         <oasis:entry colname="col2" align="left"><inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:mi mathvariant="normal">Vis</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mi mathvariant="normal">m</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">20.15</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.07</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>z</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3" align="left">Site-specific fit: 732 finite pairs on 23 dates to 882 5 min records. Local baseline only.</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left">Liu et al. (2019)</oasis:entry>
         <oasis:entry colname="col2" align="left"><inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:mi mathvariant="normal">Vis</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>[</mml:mo><mml:mi mathvariant="normal">m</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">40</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.069</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>z</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3" align="left">Eq. (7) of Liu et al. (2019): 33.44 GHz Ka-band radar and a forward-scatter visibility meter at Ningbo Beilun Port, 15–16 March 2015; reported correlation coefficient 0.732.</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1" align="left">Gultepe et al. (2009)</oasis:entry>
         <oasis:entry colname="col2" align="left"><inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:mi mathvariant="normal">Vis</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mi mathvariant="normal">km</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.04</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.098836</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>z</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, equivalently <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:mn mathvariant="normal">40</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.098836</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi>z</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> m</oasis:entry>
         <oasis:entry colname="col3" align="left">Fig. 10b of Gultepe et al. (2009): 1 s FRAM-L/Lunenburg data on 27 June 2006; <inline-formula><mml:math id="M203" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> was calculated from FMD/FM-100 DSDs rather than observed directly by radar; reported RMSE 0.2367 km and correlation <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.7118</mml:mn></mml:mrow></mml:math></inline-formula>.</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d2e4272">The local and Liu et al. (2019) prefactors are 0.02015 and 0.040 km, respectively, for the kilometre axes in Figs. <xref ref-type="fig" rid="F9"/>e and <xref ref-type="fig" rid="F10"/>. The local relation was derived by weighted nonlinear least-squares fitting of 5 min aggregated visibility–reflectivity pairs from FM-120 DSD observations, with elevated weight applied to the low-reflectivity regime where visibility sensitivity is highest (Table <xref ref-type="table" rid="T1"/>). Because the radar sampling volume and the DNQ3 point measurement differ in geometry and representativeness, and DNQ3 data also conditioned the event selection and range-gate matching, the comparison in Fig. <xref ref-type="fig" rid="F10"/> assesses local consistency and reasonable range rather than ranking methods.</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e4285">DNQ3-conditioned local-consistency comparison: DNQ3 visibility-meter observations versus <bold>(a)</bold> the present retrieval, <bold>(b)</bold> the local site-specific FM-120 relation, <bold>(c)</bold> Liu et al. (2019, Eq. 7), and <bold>(d)</bold> Gultepe et al. (2009, Fig. 10b); equations and provenance are given in Table <xref ref-type="table" rid="T1"/>. Axes are in kilometres; red lines show <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> agreement and colour denotes counts per displayed bin.</p></caption>
        <graphic xlink:href="https://amt.copernicus.org/articles/19/6607/2026/amt-19-6607-2026-f10.png"/>

      </fig>

      <p id="d2e4321">Taken together, Figs. <xref ref-type="fig" rid="F8"/>–<xref ref-type="fig" rid="F10"/> present the algorithm outputs used only for a DNQ3-conditioned reasonable-range and local-consistency comparison in the criterion-selected coastal low-visibility cases. Owing to systematic differences between the radar sampling volume and the DNQ3 point measurement, as well as the conditioning of event selection and range-gate matching on DNQ3 data, this evaluation reflects local consistency under conditioned samples rather than independent retrieval validation. A stricter quantitative evaluation requires more completely collocated observations over additional fog regimes and explicit characterization of inter-instrument systematic differences.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d2e4336">This study presents a physically constrained, observation-calibrated visibility retrieval algorithm for single-wavelength Ka-band millimeter-wave cloud radar. DSD moment analysis confirms that single-wavelength reflectivity cannot uniquely determine both droplet number concentration and geometric median radius, motivating the introduction of two intermediate microphysical constraints. The first is a segment-wise mass-absorption LWC power law that operates on contiguous 4–10-gate segments with reflectivity-dependent starting vectors, a strong-branch retry, and branch-specific attenuation accumulation. The second is an extinction-oriented radius–reflectivity parameterization calibrated against same-source FM-120 DSD observations, enabling closed-form calculation of the extinction coefficient and hence visibility. Compared with purely empirical visibility–reflectivity relations, the proposed method provides clearer physical underpinnings and better internal self-consistency. The main findings are summarized as follows.</p>
      <p id="d2e4339">During algorithm development, the dominant error sources are identified as the constant extinction efficiency (<inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>) approximation and the single-lognormal DSD assumption. Multi-year FM-120 observations reveal high morphological diversity in coastal fog spectra: broad-unimodal spectra dominate, whereas bimodal spectra become increasingly prevalent below 200 m visibility. Both LWC and <inline-formula><mml:math id="M207" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> exhibit strong discriminability across fog-intensity regimes, and this contrast is exploited to optimize the mass-absorption retrieval framework following <xref ref-type="bibr" rid="bib1.bibx11" id="text.25"/>.</p>
      <p id="d2e4368">The single-lognormal closure introduces inherent uncertainty into the radius–reflectivity relation. The extinction-oriented parameterization mitigates systematic extinction retrieval errors without additional observational inputs, with more pronounced improvement in dense fog characterized by relatively high reflectivity, achieving a mean absolute fractional extinction error of 9.37 % on the development dataset. Both intermediate quantities (<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWC) carry retrieval uncertainties, and LWC perturbations exert a stronger influence on the final visibility estimate than median-radius perturbations. Within the perturbation range of 0.50–2.00 times the baseline values, the relative change in extinction spans from <inline-formula><mml:math id="M209" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>67.7 % to <inline-formula><mml:math id="M210" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>209.4 %. Nevertheless, the covariation of <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and LWC can partly compensate for individual errors, as reflected in the analytical sensitivity response.</p>
      <p id="d2e4407">Evaluation on ten criterion-selected spring low-visibility fog events shows that the near-surface visibility retrieved by the proposed method achieves the lowest error statistics among the four compared relations, with a mean absolute error (MAE) of 0.092 km and a relative error (RE) of 42.86 %, followed by the local site-specific FM-120 relation (MAE <inline-formula><mml:math id="M212" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.123 km, RE <inline-formula><mml:math id="M213" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 50.53 %) and Liu et al. (2019) (MAE <inline-formula><mml:math id="M214" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.160 km, RE <inline-formula><mml:math id="M215" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 85.30 %), whereas the Gultepe et al. (2009) relation departs most strongly (MAE <inline-formula><mml:math id="M216" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.533 km, RE <inline-formula><mml:math id="M217" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 310.63 %). The present retrieval, the local FM-120 relation, and Liu et al. (2019) yield broadly comparable visibility ranges, consistent with their shared origin in Fujian Province coastal-fog observations, while the larger departure of Gultepe et al. (2009) reflects regional and latitudinal differences in fog microphysics. However, owing to the spatial mismatch between the radar sampling volume and the ground point measurement, as well as the conditioning of event selection and range-gate matching on DNQ3 data, this evaluation reflects local consistency under conditioned samples rather than independent retrieval validation.</p>
      <p id="d2e4454">Several limitations of this study must be acknowledged. First, independent in situ LWC measurements and standardized hydrometeor phase data are unavailable, so the retrieved microphysical parameters cannot be validated against reference truth. Second, near-range retrieval results may still be affected by residual ground clutter, as the full quantitative performance of the clutter-filtering algorithm cannot be completely verified. Third, the study samples are limited to spring warm fog at a single southeast coastal site, so the generalizability of the algorithm to other fog types (e.g., radiation fog, orographic fog) and other climate regions remains to be tested.</p>
      <p id="d2e4457">Future work will pursue three directions. First, dual-wavelength cloud radar observations will be incorporated to further constrain LWC retrieval using differential attenuation characteristics, reducing the non-uniqueness of microphysical parameter estimation. Second, a multi-source synergistic visibility retrieval scheme will be developed by combining lidar, microwave radiometer, and fog-spectrometer observations to add phase identification, vertical structure, and microphysical constraints. Third, observational samples from diverse climate zones and fog types will be accumulated to improve parameterization robustness and generalizability, and to carry out targeted error evaluation for transportation and civil aviation operational applications.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d2e4464">The instrumental data used in this work are provided by the Key Innovation Team of Marine Severe Weather Mechanism and Forecasting, Fujian Meteorological Bureau. The intermediate variable data (including liquid water content, LWC; effective droplet radius, <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and the final visibility (Vis) retrieval program calculated from these variables, which are presented in this paper, are available upon reasonable request to the corresponding author(s).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e4481">The underlying research data can be obtained from the corresponding author Qiaoyi Lv (414562004@qq.com) upon reasonable request.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e4487">Xiaojie Li developed the research concepts and methodology for fog visibility retrieval, performed formal statistical and computational analyses of radar data, conducted field investigations at the observation base, created data visualizations, and drafted the original manuscript. Jinming Ge contributed to the conceptualization of the study and refinement of the retrieval methodology, supervised the overall research process, acquired financial support for the project, managed project administration, provided key research resources, and reviewed and edited the manuscript (corresponding author). Yucheng Qiu curated and processed fog observation data, validated the retrieval algorithm results, and participated in field investigations. Qiaoyi Lv provided research resources, conducted field investigations, curated experimental data, and reviewed and edited the manuscript (corresponding author). Wei Song performed formal analysis of fog microphysical parameters and refined the retrieval methodology. Jie Zhang, Chi Zhang, Bochun Liu, Jiapeng Wang, Hongwei Xia, and Yuhang Zhu participated in field investigations, created visualizations of radar and visibility data, and curated the collected observation data.</p>

      <p id="d2e4490">All authors read and approved the final version of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e4496">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e4502">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e4508">The authors would like to extend their gratitude to the Key Innovation Team of Marine Severe Weather Mechanism and Forecasting, Fujian Meteorological Bureau, for providing valuable observational data, the geographical base map of Fig. 1a, and fruitful discussions on research questions, as well as kind support in daily work.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e4513">This research has been supported by the National Natural Science Foundation of China (grant nos. 42275076 and 42427804) and the Research Project of Aerospace New Meteorological Technology Co., Ltd. (grant no. BW230315-015).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e4520">This paper was edited by Chao Liu and reviewed by three anonymous referees.</p>
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