IMF-sense-dependent cosmic ray anisotropy produced from diffusion-convection in heliosphere

Details IMF-sense-dependent cosmic ray anisotropy produced from diffusion-convection in heliosphere IMF-sense-dependent cosmic ray anisotropy produced from diffusion-convection in heliosphere

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5....9n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 9-12 (SEE N85-34991 23-93)

Computer Science

Anisotropy, Convection, Diffusion, Heliosphere, Interplanetary Magnetic Fields, Solar Cosmic Rays, Annual Variations, Coefficients, Comparison, Diurnal Variations, Particle Telescopes, Polar Coordinates, Simulation

Scientific paper

The authors discuss the characteristics of the daily variations caused
by the IMF-sense-dependent 2nd order anisotropy obtained on the same
condition as adopted by Munakata and Nagashima (1984). A brief
comparison of these variations with observations will also be made in
order to demonstrate their existence.

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