Fitting of expanding magnetic clouds: A statistical study

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F09%3A00206945" target="_blank" >RIV/00216208:11320/09:00206945 - 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

Fitting of expanding magnetic clouds: A statistical study

Original language description

The cloud parameters yielded by a static model are compared with those obtained from a modified model that includes magnetic cloud expansion. The dynamic model provides better fits than static one in 70 % of investigated MCs. We conclude that the expansion of magnetic clouds plays an important role in the MC formation and propagation

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

2009

Confidentiality

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

Name of the periodical

Planetary and Space Science

ISSN

0032-0633

e-ISSN

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Volume of the periodical

57

Issue of the periodical within the volume

12

Country of publishing house

GB - UNITED KINGDOM

Number of pages

6

Pages from-to

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UT code for WoS article

000271365200006

EID of the result in the Scopus database

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