✦ LIBER ✦

Solar Phenomena and Geomagnetism

Book ID: 109543491
Publisher: Nature Publishing Group
Year: 1944
Tongue: English
Weight: 384 KB
Volume: 153
Category: Article
ISSN: 0028-0836
DOI: 10.1038/153452a0

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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