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-Reference-Cited by-同舟云学术

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

Published:1992-08 Issue:8 Volume:40 Page:1109-1137
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Nagashima K.,Fujimoto K.,Sakakibara S.,Morishita I.,Tatsuoka R.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference39 articles.

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2. Study and effect of magnetic clouds on the transient modulation of cosmic-ray intensity;Badruddin;Solar Phys.,1991

3. Causes of Forbush decreases and other cosmic ray variations;Barouch;J. geophys. Res.,1975

4. Understanding the heliosphere and its energetic particles;Burlaga,1983

5. Interplanetary Medium Data Book: Suppl. bf. 3A, 1977–1985, NSSDC/WDC-A 84-04;Couzens,1986

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