Forbush decreases in cosmic-ray intensity and large-scale magnetic configuration of interplanetary shocks.

Details Forbush decreases in cosmic-ray intensity and large-scale magnetic configuration of interplanetary shocks. Forbush decreases in cosmic-ray intensity and large-scale magnetic configuration of interplanetary shocks.

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ncimc..23..217b&link_type=abstract

Nuovo Cimento C, Vol. 23C, N. 3, p. 217 - 226

Physics

4

Cosmic Rays: Forbush Effect, Cosmic Rays: Shock Waves

Scientific paper

The author presents the results of an analysis to study the effects of shock front, sheath region and driver gas (ejecta) on the transient decreases of cosmic-ray intensity. A shock structure is considered which explains the results. The essential feature of this structure is that the extent of the shock front is much more than the ejecta and magnetic turbulence is usually present in the limited region of sheath. Based on this, the author explains the observation that all the shock-associated disturbances do not produce Forbush decreases on reaching the Earth.

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