Cosmic-ray variations associated with evanescence of solar filaments.

Details Cosmic-ray variations associated with evanescence of solar filaments. Cosmic-ray variations associated with evanescence of solar filaments.

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..263b&link_type=abstract

Geomagn. Aeron., Vol. 31, No. 2, p. 263 - 265

Physics

Cosmic Rays: Variations, Cosmic Rays: Solar Modulation

Scientific paper

Forty-three cases of evanescence of solar filaments were identified between 1984 - 1988 during periods of no geoeffective solar flares and no coronal hole crossings of the effective heliolongitudes. In approximately one-half of the cases (and in virtually all cases for the central portion of the solar disk) a small Forbush decrease is observed on earth several days after the filament evanescence.

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