Using the dimensionality method in the analysis of the time evolution of solar cosmic rays in interplanetary space

Details Using the dimensionality method in the analysis of the time evolution of solar cosmic rays in interplanetary space Using the dimensionality method in the analysis of the time evolution of solar cosmic rays in interplanetary space

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kosis..30..566b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 30, no. 4, p. 566-571.

Physics

Charged Particles, Dimensional Analysis, Interplanetary Space, Solar Cosmic Rays, Solar Flares, Aeronomy, Geomagnetism, Interplanetary Magnetic Fields, Interplanetary Medium

Scientific paper

A simple and sufficiently accurate method for the analysis of solar cosmic ray propagation is presented which represents a further extension of the method proposed by Kuzhevskii et al. (1979). The method can be advantageously used in many cases where a detailed analysis of the behavior of particles is not required. Results obtained by the method proposed here are presented as an example.

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