Disappearing solar filaments and geomagn
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J. Hanumath Sastri
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Article
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1986
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Springer
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English
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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