Forbush decrease and geomagnetic storms in relation to varying interplanetary parameters

Details Forbush decrease and geomagnetic storms in relation to varying interplanetary parameters Forbush decrease and geomagnetic storms in relation to varying interplanetary parameters

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ijrsp...5..330a&link_type=abstract

(Symposium on Earth's Near Space Environment, New Delhi, India, Feb. 18-21, 1975.) Indian Journal of Radio and Space Physics, vo

Physics

Space Physics

2

Cosmic Rays, Forbush Decreases, Magnetic Storms, Solar Activity Effects, Solar Cycles, Solar Flares, Sudden Storm Commencements, Time Lag

Scientific paper

Using the hourly neutron monitor data for the present solar cycle, the characteristics of all the Forbush decreases (FDs) have been studied. Statistically, the rigidity spectral exponent is found to be about 0.8 plus or minus 0.2. It is seen that most of the FDs occur in coincidence with sudden storm commencements and the largest FDs are produced by solar flares occurring near the central meridian.

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