Deformation of ICME and MC on 1-30 AU Seen by Voyager 2 and WIND

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F10%3A10077595" target="_blank" >RIV/00216208:11320/10:10077595 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Deformation of ICME and MC on 1-30 AU Seen by Voyager 2 and WIND
Original language description
The Interplanetary Coronal Mass Ejections (ICMEs) which propagate in the solar wind with supersonic velocities create the shock prior to their leading edge. The shock standoff distance depends on the ICME's velocity, form and expansion. The study of thestandoff distance can provide us an additional information about the shape of ICMEs.
Czech name
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Czech description
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Project
<a href="/en/project/GA205%2F07%2F0694" target="_blank" >GA205/07/0694: Application of fast monitors for the study of instabilities in the solar wind and foreshock region</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach

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

Article name in the collection
WDS'10 Proceedings of Contributed Papers: Part II - Physics of Plasmas and Ionized Media
ISBN
978-80-7378-140-8
ISSN
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e-ISSN
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Number of pages
7
Pages from-to
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Publisher name
Matfyzpress
Place of publication
Praha
Event location
Praha
Event date
Jun 1, 2010
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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