Influence of Magnetic Cloud Expansion on Its Fits

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F10%3A10080233" target="_blank" >RIV/00216208:11320/10:10080233 - 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

Influence of Magnetic Cloud Expansion on Its Fits

Original language description

Magnetic clouds observed between 1995 and 2003 are fitted using force-free cylindrical flux rope expansion and non-expansion models. The comparison reveals that the model with expansion provides better fits for larger expansion speeds and for magnetic clouds observed close to their axis. We conclude that expansion of magnetic clouds plays an important role in the MC evolution and should be accounted in space weather models.

Czech name

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Czech description

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Type

J_x - 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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Project

<a href="/en/project/GA205%2F09%2F0170" target="_blank" >GA205/09/0170: The role of solar wind disturbances in Space Weather</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

Name of the periodical

AIP Conference Proceedings

ISSN

0094-243X

e-ISSN

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Volume of the periodical

1216

Issue of the periodical within the volume

1

Country of publishing house

US - UNITED STATES

Number of pages

4

Pages from-to

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UT code for WoS article

000281438100093

EID of the result in the Scopus database

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