A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F03%3A04033544" target="_blank" >RIV/68378289:_____/03:04033544 - 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
A global three dimensional hybrid simulation of the interaction between a weakly magnetized obstacle and the solar wind.
Original language description
We study an interaction between the solar wind flow and a conductive obstacle with a weak dipole magnetic field using a three dimensional implementation of the hybrid code. We show that the hybrid approach is capable of describing most of structures formed due to the interaction between the solar wind and a magnetized planet like the bow shock, proton foreshock, magnetopause, magnetosheath, northern and southern cusps and current sheath.
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
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
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Continuities
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
Name of the periodical
AIP conference proceedings. International solar wind conference /10./
ISSN
0094-243X
e-ISSN
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Volume of the periodical
679
Issue of the periodical within the volume
CP679
Country of publishing house
US - UNITED STATES
Number of pages
4
Pages from-to
485-488
UT code for WoS article
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EID of the result in the Scopus database
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