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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/acpd-10-11009-2010</article-id>
<title-group>
<article-title>Probabilistic model of shattering effect on in-cloud measurements</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shcherbakov</surname>
<given-names>V.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gayet</surname>
<given-names>J.-F.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Febvre</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Heymsfield</surname>
<given-names>A. J.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mioche</surname>
<given-names>G.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Laboratoire de Météorologie Physique, UMR/CNRS 6016, Université Blaise Pascal, 24 avenue des Landais, 63177 Aubière Cedex, France</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>LaMP – Institut Universitaire de Technologie de Montluçon, Avenue A. Briand-BP 2235, 03101 Montluçon Cedex, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>National Center for Atmospheric Research, Boulder, Colorado, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>26</day>
<month>04</month>
<year>2010</year>
</pub-date>
<volume>10</volume>
<issue>4</issue>
<fpage>11009</fpage>
<lpage>11045</lpage>
<permissions>
<license xlink:type="simple">
<license-p>This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.</license-p>
</license>
</permissions>
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<abstract>
<p>A probabilistic model of the ice shattering effects on
in-cloud measurements performed with instruments designed with
inlets, which have the circular cross-section, is
presented. Applications are made for the Polar Nephelometer and PMS FSSP
instruments. The model provides rough estimates of the effects on
microphysical measurements and assigns the key parameters that govern the
efficiency of ice shattering. It is shown that experimental data are less
affected by the shattering for clouds that have a lower proportion of large
particles. The effects on derived integral microphysical parameters are
shown to be very sensitive to the effective diameter of the ice fragments.
The smaller the fragments from a given cloud particle are, the higher their
effects are. Errors on Polar Nephelometer measurements
were evaluated. It is shown that the ice particle shattering leads to the
overestimation of the extinction coefficient. For example, for a given
distribution with the effective diameter of 68 &amp;mu;m and with fragment
effective diameters of 10 &amp;mu;m the extinction is overestimated
by 25%. With larger particles having an effective diameter of 89 &amp;mu;m,
the error increases up to 37%. As for the FSSP-300 instrument, under the
same conditions the extinction coefficient is overrated by 17% and the
number particle concentration is overestimated by 30%. The discussion of
the results points out the main hypothesis which may seriously limit the
reliability of the modelling results. Nevertheless, the magnitudes of the
errors on extinction and particle concentration are of the same orders of
those reported in the literature from experimental assessments.</p>
</abstract>
<counts><page-count count="37"/></counts>
</article-meta>
</front>
<body/>
<back>
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</article>