Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355335" target="_blank" >RIV/67985815:_____/10:00355335 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.3395886" target="_blank" >http://dx.doi.org/10.1063/1.3395886</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.3395886" target="_blank" >10.1063/1.3395886</a>

Result language
angličtina
Original language name
Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes
Original language description
It is widely accepted that magnetic disturbances around fast interplanetary magnetic clouds can play an important role in their geo-effectiveness. An analytical solution for magnetic field in the sheath region of a cylindrical magnetic cloud with an elliptical cross-section is proposed. Upstream magnetic field can have an arbitrary direction. Normal magnetic field components are conserved through the bow shock with a high accuracy.
Czech name
—
Czech description
—

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)<br>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
399-402
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
000281438100094

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