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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

โœ Scribed by E. V. Ivanov; G. V. Rudenko; V. G. Fainshtein


Book ID
110164068
Publisher
SP MAIK Nauka/Interperiodica
Year
2009
Tongue
English
Weight
230 KB
Volume
49
Category
Article
ISSN
0016-7932

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Daily images of the white light corona between 3 and 10 R| have been recorded by a coronagraph aboard the OSO-7 unmanned satellite since October 3, 1971. Images for the years 1972 and 1973 have been examined for persistent coronal forms. For most of 1972 there passed over the Sun's east limb a regul