Computer Science
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..378d&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 378-383. In Russian.
Computer Science
Cosmic Rays, Distance, Interplanetary Medium, Modulation Transfer Function, Radiation Transport, Solar Wind, Kinetic Equations, Magnetic Flux, Plasma-Electromagnetic Interaction, Shock Waves, Solar Magnetic Field, Transition Points
Scientific paper
The kinetic equation is used to obtain an equation for cosmic-ray transport in interplanetary space in the presence of the solar wind with frozen-in magnetic inhomogeneities (medium 1) and shock waves and fast plasma formations (medium 2). An analysis is made of the character of the distance dependence of the modulating properties of the two media, having different velocities. It is shown that two modulation regions (near and far) arise, with a smooth transition between them; in the near region the main role in the modulation is played by medium 1, while in the far field the main role is played by medium 2. The results obtained are compared with space probe (IMP-8, Voyager 1 and 2, and Pioneer-10) studies.
Dorman Lev I.
Shogenov Kh. V.
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