Cosmic-ray variations associated with the disappearance of filaments on the sun

Details Cosmic-ray variations associated with the disappearance of filaments on the sun Cosmic-ray variations associated with the disappearance of filaments on the sun

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..345b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Mar.-Apr. 1991, p. 345-347. In Russian.

Physics

2

Coronal Holes, Forbush Decreases, Periodic Variations, Solar Flares, Solar Longitude, Diurnal Variations, Magnetic Storms, Solar Limb

Scientific paper

Forty-three cases of the disappearance of solar filaments were observed
in 1984-1988 during periods when geoefficient solar flares were absent
and there was no generation of coronal holes through efficient solar
longitudes. In about half the cases, small Forbush decreases were
observed on the earth several days after the filament disappearance.

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