<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>5</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/acpd-5-4641-2005</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/5/4641/2005/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/5/4641/2005/acpd-5-4641-2005.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/5/4641/2005/acpd-5-4641-2005.pdf</fulltext_pdf>
	<start_page>4641</start_page>
	<end_page>4677</end_page>
	<publication_date>2005-07-12</publication_date>
	<article_title content_type="html">Screening the ESA ATSR-2 World Fire Atlas (1997–2002)</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. W. Mota</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>J. M. C. Pereira</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>D. Oom</name>
		</author>
		<author numeration="4" affiliations="2">
			<name>M. J. P. Vasconcelos</name>
		</author>
		<author numeration="5" affiliations="3">
			<name>M. Schultz</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Departamento de Engenharia Florestal, Instituto Superior de Agronomia, Tapada da Ajuda 1349-017 Lisboa, Portugal</affiliation>
		<affiliation numeration="2" content_type="html">Centro de Cartografia, Instituto de Investigaç&amp;#227;o Cient&amp;#237;fica Tropical, Tv. Conde da Ribeira 9,  1300-142 Lisboa, Portugal.</affiliation>
		<affiliation numeration="3" content_type="html">Max Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The European Space Agency (ESA) World Fire Atlas (WFA), for the period
1997&amp;ndash;2002, is built using night time data from the Along Track Scanning
Radiometer (ATSR) onboard the Second European Remote-Sensing Satellite
(ERS-2). The spatial resolution of the data is 1 km and the satellite
revisiting period is 3&amp;nbsp;days at the equator. The WFA is the first and longest
archive of global fire observations and has been used in numerous biomass
burning studies. Known limitations of the WFA are the inclusion of warm
surfaces, gas flares, and city lights, and an underestimation of actual
global fire activity, due to the time of satellite overpass. Nevertheless,
it has been considered that the WFA contains a relatively small proportion
of observations that do not correspond to vegetation fires. We used
ancillary land cover, night-lights and volcanic activity datasets, combined
with statistical techniques to detect the occurrence of space-time clusters,
to screen the algorithm&amp;nbsp;2 (308&amp;deg;K threshold) WFA data for the period
1997&amp;ndash;2002. During the study period, the annual percentage of false alarms
and non-vegetation fires varied from a minimum value of 20.6% in 1997 to
a maximum of 27.9% in 1998. Gas flares and hot bare soils are the major
sources of false alarms and non-vegetation fires.</abstract>
	<references>
	</references>
</article>

