Propagation of a toroidal magnetic cloud trough the inner heliosphere.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030128" target="_blank" >RIV/67985815:_____/03:01030128 - 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
Propagation of a toroidal magnetic cloud trough the inner heliosphere.
Original language description
An analytical solution for a potential magnetic field with arbitrary intensity around a toroidal magnetic cloud has been found. The background external field may have a gradient. The solution is used for calculation of magnetic cloud propagation.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/IBS1003006" target="_blank" >IBS1003006: Solar influence on space weather</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
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Solar wind ten. Proceedings of the tenth international solar wind conference.
ISBN
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ISSN
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e-ISSN
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Number of pages
3
Pages from-to
180-182
Publisher name
American Institute of Physics
Place of publication
Melville
Event location
Pisa [IT]
Event date
Jun 17, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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