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<journal-meta>
<journal-id journal-id-type="publisher">ISPRS-Archives</journal-id>
<journal-title-group>
<journal-title>The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences</journal-title>
<abbrev-journal-title abbrev-type="publisher">ISPRS-Archives</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2194-9034</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/isprsarchives-XL-7-W3-219-2015</article-id>
<title-group>
<article-title>Discuss on Satellite-Based Particulate Matter Monitoring Technique</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Li</surname>
<given-names>B.</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>Hou</surname>
<given-names>L.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Beijing Institute of Space Mechanics and Electricity (BISME), Beijing, China</addr-line>
</aff>
<pub-date pub-type="epub">
<day>28</day>
<month>04</month>
<year>2015</year>
</pub-date>
<volume>XL-7/W3</volume>
<fpage>219</fpage>
<lpage>223</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2015 B. Li</copyright-statement>
<copyright-year>2015</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
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<self-uri xlink:href="https://isprs-archives.copernicus.org/articles/XL-7-W3/219/2015/isprs-archives-XL-7-W3-219-2015.pdf">The full text article is available as a PDF file from https://isprs-archives.copernicus.org/articles/XL-7-W3/219/2015/isprs-archives-XL-7-W3-219-2015.pdf</self-uri>
<abstract>
<p>Satellite measurements for atmospheric pollutants monitoring provide full mapping, large spatial coverage, and high spatial
resolution. Retrieved aerosol optical depth (AOD) from satellite data as the key parameter has been used in the study on particulate
matter (PM) distributions which is complementary to ground-based measurements. Based on the empirical relations between aerosol
optical properties and PM10 or PM2.5 concentration and its influencing factors, combining the Beijing-Tianjin-Hebei regional PM
distribution feature, the specifications including bands, viewing angles and polarization measuring requirements of the on-orbit PM
monitoring instrument are discussed. The instrument is designed to obtain the data for retrieving atmospheric AOD, shape and size
of particles, refractive index, aerosol single scattering albedo (SSA), etc. The major pollutant PM2.5 concentration can be retrieved
from the remote sensing data especially, and its global distribution can be mapped as well. The progress of conventional aerosol
retrieval method using visible data is presented along with its limitation for serious haze-fog condition. Adding ultra violet (UV)
bands to obtain UV aerosol index (UVAI) is useful for monitoring the main constituents of haze.</p>
</abstract>
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