Variations of cosmic ray intensity and the solar wind

Details Variations of cosmic ray intensity and the solar wind Variations of cosmic ray intensity and the solar wind

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q.340v&link_type=abstract

(Mezhdunarodnyi Seminar po Uskoreniiu Chastits i Iadernykh Reaktsii v Kosmose, 6th, Leningrad, USSR, Aug. 19-21, 1974.) Akademii

Physics

Cosmic Rays, Interplanetary Medium, Magnetohydrodynamic Flow, Solar Wind, Galactic Radiation, Photosphere, Plasma Flux Measurement, Solar Flares, Time Response

Scientific paper

An attempt is made to study the structure of the interplanetary medium
and the solar plasma sources on the basis of the intensity variations of
galactic cosmic rays. The analysis is based on the adoption and further
development of Mustel's (1965) hypothesis in which the active regions
are treated as sources of quasi-stationary plasma flows.

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