Local-time-dependent pre-IMF-shock decrease and post-shock increase of cosmic rays, produced respectively by their IMF-collimated outward and inward flows across the shock responsible for Forbush decrease

Details Local-time-dependent pre-IMF-shock decrease and post-shock increase of cosmic rays, produced respectively by their IMF-collimated outward and inward flows across the shock responsible for Forbush decrease Local-time-dependent pre-IMF-shock decrease and post-shock increase of cosmic rays, produced respectively by their IMF-collimated outward and inward flows across the shock responsible for Forbush decrease

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40.1109n&link_type=ejournal

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 8, Aug. 1992, p. 1109-1137.

Physics

23

Collimation, Cosmic Rays, Forbush Decreases, Interplanetary Magnetic Fields, Shock Waves, Diurnal Variations, Shock Fronts

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