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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</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/acp-4-2543-2004</article-id>
<title-group>
<article-title>Improved sky imaging for studies of enhanced UV irradiance</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sabburg</surname>
<given-names>J. M.</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>Long</surname>
<given-names>C. N.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Centre for Astronomy, Solar Radiation and Climate, Faculty of Sciences, Univ. Southern Queensland, Toowoomba, Australia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Pacific Northwest National Laboratory, Richland, WA, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>14</day>
<month>12</month>
<year>2004</year>
</pub-date>
<volume>4</volume>
<issue>11/12</issue>
<fpage>2543</fpage>
<lpage>2552</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2004 J. M. Sabburg</copyright-statement>
<copyright-year>2004</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Generic License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by-nc-sa/2.5/">https://creativecommons.org/licenses/by-nc-sa/2.5/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/2543/2004/acp-4-2543-2004.html">This article is available from https://acp.copernicus.org/articles/4/2543/2004/acp-4-2543-2004.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/4/2543/2004/acp-4-2543-2004.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/4/2543/2004/acp-4-2543-2004.pdf</self-uri>
<abstract>
<p>A recent World Meteorological Organisation report discussed the importance of
continued study of the effect of clouds on the solar UV radiation reaching the earth&apos;s
surface. The report mentions that the use of all-sky imagery offers the potential to
understand and quantify cloud effects more accurately. There are an increasing number of
studies investigating the enhancement of surface solar, UV irradiance, and UV actinic
flux, using automated CCD and sky imagers. This paper describes new algorithms
applicable to a commercially available all-sky imager (TSI-440), for research
investigating cloud enhanced spectral UV irradiance. Specifically, these include three
new algorithms relating to cloud amount at different spatial positions from 1) zenith and
2) from the solar position and 3) the visible brightness of clouds surrounding the sun. A
possible relationship between UV enhancement and the occurrence of near-sun cloud
brightness is reported based on this preliminary data. It is found that a range of
wavelength dependent intensities, from 306 to 400 nm, can occur in one day for UV
enhancements. Evidence for a possible decreasing variation of intensity with longer
wavelengths is also presented.</p>
</abstract>
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</article-meta>
</front>
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