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Activity cycle of solar filaments

✍ Scribed by K. J. Li; Q. X. Li; P. X. Gao; J. Mu; H. D. Chen; T. W. Su

Book ID: 107582774
Publisher: Springer-Verlag
Year: 2007
Tongue: English
Weight: 248 KB
Volume: 28
Category: Article
ISSN: 0250-6335
DOI: 10.1007/s12036-007-0012-8

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As a sequel to our recent identification of the high-speed stream as the candidate structure in the solar wind at 1 AU, that is primarily responsible for the geomagnetic disturbances occasionally noticed after 'disparition brusques' (DBs) of solar filaments (Sastri et al., 1985), we report here that

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