Computer Science
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..111e&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 111-114 (SEE N85-34991 23-93)
Computer Science
Diurnal Variations, Energy Dissipation, Particle Trajectories, Solar Cosmic Rays, Anisotropy, Energy Spectra, Interplanetary Magnetic Fields, Interplanetary Space, Magnetic Field Configurations
Scientific paper
The method of calculating energy losses along regular particle trajectories is applied to obtain the predicted cosmic ray anisotropies from 200 to 500 GV. The tilt angle of the interplanetary neutral sheet varies to simulate a 22-year cycle magnetic cycle. The calculated values of solar diurnal and semidiurnal, and sidereal diurnal intensity waves are compared with observations.
Erdos Géza
Kota József
Merényi Erzsébet
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