Forbush decreases at high rigidities

Details Forbush decreases at high rigidities Forbush decreases at high rigidities

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..160e&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Computer Science

Energy Dissipation, Forbush Decreases, Interplanetary Magnetic Fields, Particle Trajectories, Shock Wave Propagation, Interplanetary Space, Protons

Scientific paper

A method of calculating energy losses along regular trajectories in a model Interplanetary Magnetic Field (IMF) is extended to describe Forbush events at high rigidities. A simple IMF model is adopted, yet the gross features of Forbush events are reproduced. Computed intensity profiles of 70-GV protons are presented for both halves of the 22-year solar magnetic cycle.

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