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	<journal>
		<journal_title>Solid Earth Discussions</journal_title>
		<journal_url>www.solid-earth-discuss.net</journal_url>
		<eissn>1869-9537</eissn>
		<volume_number>2</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/sed-2-69-2010</doi>
	<article_url>http://www.solid-earth-discuss.net/2/69/2010/</article_url>
	<abstract_html>http://www.solid-earth-discuss.net/2/69/2010/sed-2-69-2010.html</abstract_html>
	<fulltext_pdf>http://www.solid-earth-discuss.net/2/69/2010/sed-2-69-2010.pdf</fulltext_pdf>
	<start_page>69</start_page>
	<end_page>103</end_page>
	<publication_date>2010-03-09</publication_date>
	<article_title content_type="html">Candidates for multiple impact craters:  popigai and chicxulub as seen by EGM08, a global 5&apos;&amp;times;5&apos; gravitational model</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. Klokočník</name>
			<email>jklokocn@asu.cas.cz</email>
		</author>
		<author numeration="2" affiliations="2,3">
			<name>J. Kostelecký</name>
		</author>
		<author numeration="3" affiliations="3">
			<name>I. Pešek</name>
		</author>
		<author numeration="4" affiliations="2,4">
			<name>P. Novák</name>
		</author>
		<author numeration="5" affiliations="5">
			<name>C. A. Wagner</name>
		</author>
		<author numeration="6" affiliations="1,3">
			<name>J. Sebera</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Astronomical Institute, Academy of Sciences of the Czech Republic, Czech Republic</affiliation>
		<affiliation numeration="2" content_type="html">Research Institute for Geodesy, Topography and Cartography, Czech Republic</affiliation>
		<affiliation numeration="3" content_type="html">Department of Advanced Geodesy, Czech Technical University, Czech Republic</affiliation>
		<affiliation numeration="4" content_type="html">Department of Math, Faculty of Applied Sciences, University of West Bohemia, Czech Republic</affiliation>
		<affiliation numeration="5" content_type="html">Laboratory for Satellite Altimetry, NOAA, USA</affiliation>
	</affiliations>
	<abstract content_type="html">In 2008 the new Earth Gravitational Model (EGM08) was released. It contains
a complete set of spherical harmonic coefficients of the Earth&apos;s
gravitational potential (Stokes parameters) to degree 2190 and order 2159
that can be used for evaluation of various potential quantities with both
the unprecedented accuracy and high spatial resolution. Two such quantities,
the gravity anomaly and second-order radial derivative of the disturbing
potential, were computed over selected areas with known impact craters. The
displays of these derivatives for two such sites clearly show not only the
strong circular-like features known to be associated with them but also
other symmetrical structures which appear to make them multiple impact
sites. At Popigai, Siberia, the secondary circular features fall in a line
from the primary in the SE direction. At Chicxulub, Yucatán, there
appears to be one secondary crater close to the primary in the NE direction,
as well as possibly others in the vicinity of the main crater. Gravity
information alone is not proof of the impact craters but it is useful in
identifying candidate sites for further study, for future examination by
geologists and geophysicists.</abstract>
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</article>

