Approximate fitting of expanding magnetic clouds: a statistical study
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F09%3A00334783" target="_blank" >RIV/67985815:_____/09:00334783 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Approximate fitting of expanding magnetic clouds: a statistical study
Original language description
Magnetic clouds observed during 1995 - 2003 years are fitted using a force-free cylindrical flux rope model that includes magnetic cloud expansion. The distribution of comparison results according expansion velocity shows that the expansion of clouds plays a significant role in MC's inner structure formation.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/1QS300120506" target="_blank" >1QS300120506: Development of methods for space weather forecasts and impacts of space weather on the ionosphere-atmosphere system</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2009
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Planetary and Space Science
ISSN
0032-0633
e-ISSN
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Volume of the periodical
57
Issue of the periodical within the volume
12
Country of publishing house
US - UNITED STATES
Number of pages
6
Pages from-to
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UT code for WoS article
000271365200006
EID of the result in the Scopus database
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