Influence of Magnetic Cloud Expansion on Its Fits

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355334" target="_blank" >RIV/67985815:_____/10:00355334 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.3395885" target="_blank" >http://dx.doi.org/10.1063/1.3395885</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.3395885" target="_blank" >10.1063/1.3395885</a>

Result language
angličtina
Original language name
Influence of Magnetic Cloud Expansion on Its Fits
Original language description
Magnetic clouds observed between 1995 and 2003 are fitted using force-free cylindrical flux rope models. The cloud parameters yielded by a static model are compared with those obtained from a modified model that includes magnetic cloud expansion. The deviations of these fits from measurements are quantified and compared with parameters measured by Wind. The comparison reveals that the model with expansion provides better fits for larger expansion speeds and for magnetic clouds observed close to their axis. We conclude that expansion of magnetic clouds plays an important role in the MC evolution and should be accounted in space weather models.
Czech name
—
Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Twelfth International Solar Wind Conference. Proceedings Paper
ISBN
978-0-7354-0759-6
ISSN
0094-243X
e-ISSN
—
Number of pages
4
Pages from-to
395-398
Publisher name
Melville
Place of publication
New York
Event location
Saint-Malo
Event date
Jun 21, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000281438100093

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