Anisotropic cosmic-ray diffusion in interplanetary space. V - Solar daily variations

Details Anisotropic cosmic-ray diffusion in interplanetary space. V - Solar daily variations Anisotropic cosmic-ray diffusion in interplanetary space. V - Solar daily variations

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18..406d&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 18, May-June 1978, p. 406-409.) Geomagnetism and Aeronomy, vol. 18, Dec. 1978, p. 272-274. Tra

Computer Science

Diurnal Variations, Interplanetary Space, Particle Diffusion, Solar Activity, Solar Cosmic Rays, Adiabatic Conditions, Anisotropy, Heat Transmission, Periodic Variations, Polarization (Waves), Spatial Distribution, Thermodynamic Cycles

Scientific paper

Current models developed to interpret the anisotropy of cosmic rays (as observed on the earth) do not take into consideration the changes caused in interplanetary space by changes in solar activity. In the present paper, three components of the cosmic-ray anisotropy vector are calculated within the framework of the theory of anisotropic diffusion. Convection, adiabatic cooling, and the heliolatitudinal distribution of solar activity are taken into account. The analysis is based on 1958-1968 data on the spatial distribution of cosmic ray density and gradients in interplanetary space.

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