Dynamics of a toroidal magnetic cloud in the solar wind.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010050" target="_blank" >RIV/67985815:_____/01:01010050 - 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
Dynamics of a toroidal magnetic cloud in the solar wind.
Original language description
The problem to find the diamagnetic force acting on a toroidal object in an inhomogoneous magnetic field is solved analytically. The obtained solution is used for calculations of the repulsing diamagnetic force acting on isolated objects in the solar corona such as magnetic clouds of a toroidal shape and for the determination of their velocity profilies.
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
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Journal of Geophysical Research. Space physics
ISSN
0148-0227
e-ISSN
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Volume of the periodical
106
Issue of the periodical within the volume
A6
Country of publishing house
US - UNITED STATES
Number of pages
10
Pages from-to
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UT code for WoS article
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EID of the result in the Scopus database
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