✦ LIBER ✦

Solar, geomagnetic and seismic activity

✍ Scribed by A. Mazzarella; A. Palumbo

Book ID: 112771610
Publisher: Italian Physical Society
Year: 1988
Tongue: English
Weight: 527 KB
Volume: 11
Category: Article
ISSN: 1124-1896
DOI: 10.1007/bf02533129

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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