Correlation between the parameters of coronal mass ejections and features of their propagation in the corona with the large-scale structure of the solar magnetic field

Correlation between the parameters of coronal mass ejections (CMEs) that are detected on the LASCO coronographs and are associated with eruptive prominences and the distances of CME axes from the coronal streamer belt has been analyzed. The deviations of CME trajectories from the radial direction ha...

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Bibliographic Details
Published inGeomagnetism and Aeronomy Vol. 49; no. 8; pp. 1096 - 1100
Main Authors Ivanov, E. V., Rudenko, G. V., Fainshtein, V. G.
Format Journal Article
LanguageEnglish
Published Dordrecht SP MAIK Nauka/Interperiodica 01.12.2009
Springer Nature B.V
Subjects
Astrophysics
Corona
Correlation analysis
Earth and Environmental Science
Earth Sciences
Geophysics/Geodesy
Magnetic fields
Sun
Coronal Mass Ejection
Solar Phys
Angular Size
Source Surface
Neutral Line
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Summary:Correlation between the parameters of coronal mass ejections (CMEs) that are detected on the LASCO coronographs and are associated with eruptive prominences and the distances of CME axes from the coronal streamer belt has been analyzed. The deviations of CME trajectories from the radial direction have been investigated.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0016-7932
1555-645X
0016-7940
DOI:10.1134/S001679320908009X