3-D MHD simulations of CMES by coupled coronal and heliospheric models.

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F02%3A01020165" target="_blank" >RIV/67985815:_____/02:01020165 - 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

3-D MHD simulations of CMES by coupled coronal and heliospheric models.

Original language description

Merging of coronal and heliospheric magnetohydrodynamic (MHD) models in demonstrated for a 3-D idealized case involving a magnetic flux rope, shock, streamer belt, and current sheet. The disruption of a sheared coronal arcade launches a coronal mass ejection, vhich evolves during its propagation through interplanetary space.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/IAA3003003" target="_blank" >IAA3003003: Origin and evolution of dynamic phenomena in the solar wind</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2002

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Solar variabiliy: from core to outer frontiers.

ISBN

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ISSN

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e-ISSN

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Number of pages

4

Pages from-to

95-98

Publisher name

ESA Publication Division

Place of publication

Noordwijk

Event location

Praha [CZ]

Event date

Sep 9, 2002

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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