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<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>7</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/acpd-7-7603-2007</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/7/7603/2007/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/7/7603/2007/acpd-7-7603-2007.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/7/7603/2007/acpd-7-7603-2007.pdf</fulltext_pdf>
	<start_page>7603</start_page>
	<end_page>7624</end_page>
	<publication_date>2007-05-31</publication_date>
	<article_title content_type="html">Evidence of gravity waves into the atmosphere during the March 2006 total solar eclipse</article_title>
	<authors>
		<author numeration="1" affiliations="1,3">
			<name>C. S. Zerefos</name>
			<email>zerefos@geol.uoa.gr</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>E. Gerasopoulos</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>I. Tsagouri</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>B. Psiloglou</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>A. Belehaki</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>T. Herekakis</name>
		</author>
		<author numeration="7" affiliations="2">
			<name>A. Bais</name>
		</author>
		<author numeration="8" affiliations="2">
			<name>S. Kazadzis</name>
		</author>
		<author numeration="9" affiliations="3">
			<name>C. Eleftheratos</name>
		</author>
		<author numeration="10" affiliations="4">
			<name>N. Kalivitis</name>
		</author>
		<author numeration="11" affiliations="4">
			<name>N. Mihalopoulos</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">National Observatory of Athens, V. Pavlou &amp; I. Metaxa, P. Penteli, 15236, Athens, Greece</affiliation>
		<affiliation numeration="2" content_type="html">Aristotle University of Thessaloniki, Physics Department, Laboratory of Atmospheric Physics, Thessaloniki, Greece</affiliation>
		<affiliation numeration="3" content_type="html">Foundation for Biomedical Research, Academy of Athens, Greece</affiliation>
		<affiliation numeration="4" content_type="html">University of Crete, Chemistry Department, Environmental and Chemical Processes Laboratory, Crete, Greece</affiliation>
	</affiliations>
	<abstract content_type="html">This study aims at testing the hypothesis according to which the movement of
the moon&apos;s shadow sweeping the ozone layer at supersonic speed during a
solar eclipse creates gravity waves in the atmosphere. An experiment was
conducted to study fluctuations of the ozone layer, the Ionosonde Total
Electron Content (ITEC) and the peak electron density height (hmF2) in the
ionosphere, as well as at a number of other parameters before, during and
after the total solar eclipse. We found the existence of dominant
oscillations with periods ranging between 30&amp;ndash;40 min in most of the
parameters. Cross-spectrum analyses between total ozone and various
atmospheric parameters resulted to statistically significant square
coherences between the observed oscillations, while the respective phase
spectra show that the perturbation originates in the stratosphere and
reaches the various layers at speeds around 20 km min&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. Additional
evidence supporting these findings was provided by the amplitude of the
oscillations in the ionospheric electron density, which increased upwards
from 160 to 220 km height.</abstract>
	<references>
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</article>

