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<article language="en">
	<journal>
		<journal_title>Astrophysics and Space Sciences Transactions</journal_title>
		<journal_url>www.astrophys-space-sci-trans.net</journal_url>
		<issn>1810-6528</issn>
		<eissn>1810-6536</eissn>
		<volume_number>5</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/astra-5-35-2009</doi>
	<article_url>http://www.astrophys-space-sci-trans.net/5/35/2009/</article_url>
	<abstract_html>http://www.astrophys-space-sci-trans.net/5/35/2009/astra-5-35-2009.html</abstract_html>
	<fulltext_pdf>http://www.astrophys-space-sci-trans.net/5/35/2009/astra-5-35-2009.pdf</fulltext_pdf>
	<start_page>35</start_page>
	<end_page>38</end_page>
	<publication_date>2009-08-06</publication_date>
	<article_title content_type="html">On expansion of magnetic clouds in the solar wind</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>M. Vandas</name>
			<email>vandas@ig.cas.cz</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>A. Geranios</name>
		</author>
		<author numeration="3" affiliations="3,4">
			<name>E. Romashets</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Astronomical Institute, Academy of Sciences of the Czech Republic,  14131 Praha 4, Czech Republic</affiliation>
		<affiliation numeration="2" content_type="html">Physics Department, University of Athens, Panepistimioupoli-Kouponia,  Athens 15771, Greece</affiliation>
		<affiliation numeration="3" content_type="html">Prairie View A&amp; M University, Mail Stop 2250, PO Box 519,  Prairie View TX 77446, USA</affiliation>
		<affiliation numeration="4" content_type="html">Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave  Propagation of Russian Academy of Sciences, Troitsk, 142190, Russia</affiliation>
	</affiliations>
	<abstract content_type="html">Magnetic clouds are supposed to be large
interplanetary flux ropes propagating away from the Sun. Due to enhanced
inner magnetic pressure, they expand during their travel.
We have analyzed 21 magnetic clouds from Wind observations and fitted them
by our model.
Comparison of the time-dependent model with observations
is shown for several cases with a detailed discussion.
The model describes behavior of compared quantities satisfactorily.
In addition to magnetic field vectors, also velocity vectors were modeled
and it was found that radial velocity component behaves as expected.
Analysis of velocity components put models under a more strict test and
yields more confidence into models and derived magnetic cloud parameters.</abstract>
	<references>
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</article>
