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

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..453n&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 34, May 1986, p. 453-467.

Physics

5

Anisotropy, Cosmic Rays, Heliosphere, Convection, Diffusion, Harmonic Radiation, Interplanetary Magnetic Fields, Solar Magnetic Field, Solar Wind

Scientific paper

An IMF-sense-dependent first order (or unidirectional) anisotropy of cosmic rays, which is produced perpendicularly to the ecliptic from the radial density gradient in the solar system, has been confirmed by Swinson. In the present paper, the authors point out the existence of IMF-sense-dependent higher order anisotropies, based on the simulation of cosmic ray diffusion-convection in the heliomagnetosphere. In order to confirm their existence, the authors demonstrate some examples of the observed cosmic ray daily variation which is supposed to be due to these anisotropies.

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