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<article language="en">
	<journal>
		<journal_title>Atmospheric Measurement Techniques Discussions</journal_title>
		<journal_url>www.atmos-meas-tech-discuss.net</journal_url>
		<eissn>1867-8610</eissn>
		<volume_number>3</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/amtd-3-269-2010</doi>
	<article_url>http://www.atmos-meas-tech-discuss.net/3/269/2010/</article_url>
	<abstract_html>http://www.atmos-meas-tech-discuss.net/3/269/2010/amtd-3-269-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-meas-tech-discuss.net/3/269/2010/amtd-3-269-2010.pdf</fulltext_pdf>
	<start_page>269</start_page>
	<end_page>299</end_page>
	<publication_date>2010-01-27</publication_date>
	<article_title content_type="html">Automatic cloud classification of whole sky images</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Heinle</name>
			<email>ahe@informatik.uni-kiel.de</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>A. Macke</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. Srivastav</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Excellence Cluster &quot;The Future Ocean&quot;, Department of Computer Science, Kiel University, Kiel, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Leibniz Institute of Marine Sciences at Kiel University (IFM-GEOMAR), Kiel, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The recently increasing development of whole sky imagers enables temporal and
spatial high-resolution sky observations. One application already performed in
most cases is the estimation of fractional sky cover. A distinction between different
cloud types, however, is still in progress. Here, an automatic cloud classification
algorithm is presented, based on a set of mainly statistical features describing
the color as well as the texture of an image. The &lt;i&gt;k&lt;/i&gt;-nearest-neighbour classifier
is used due to its high performance in solving complex issues, simplicity of
implementation and low computational complexity. Seven different sky conditions
are distinguished: high thin clouds (cirrus and cirrostratus), high patched cumuliform
clouds (cirrocumulus and altocumulus), stratocumulus clouds, low cumuliform clouds,
thick clouds (cumulonimbus and nimbostratus), stratiform clouds and clear sky.
Based on the Leave-One-Out Cross-Validation the algorithm achieves an accuracy of
about 97%, outperforming previous algorithms with accuracies of at most 62%.
An additional test run of random images is presented, still yielding a success rate
of about 75%, or up to 88% if only &quot;serious&quot; errors with respect to radiation
impact are considered. Reasons for the decrement in accuracy are discussed, and
ideas to further improve the classification results, especially in problematic
cases, are investigated.</abstract>
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</article>

