Diagnostics of the interplanetary medium on the basis of observations of cosmic-ray fluctuations

Details Diagnostics of the interplanetary medium on the basis of observations of cosmic-ray fluctuations Diagnostics of the interplanetary medium on the basis of observations of cosmic-ray fluctuations

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2444g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Statistics

Computation

Cosmic Rays, Interplanetary Magnetic Fields, Interplanetary Medium, Radiant Flux Density, Computational Astrophysics, Correlation

Scientific paper

Aspects of the diagnostics of the interplanetary medium on the basis of cosmic-ray intensity data are examined in connection with the use of a power-spectrum relationship between cosmic-ray intensity and IMF strength. This approach is used to consider two problems: (1) the relationship between the spectral characteristics of cosmic rays and the IMF components, with emphasis on the contribution of the Bz component; and (2) the frequency characteristics of cosmic rays and the Bz component before the arrival of disturbances.

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