Cosmic-ray variations connected with the evolution of the parameters of recurrent high-speed streams of the solar wind

Details Cosmic-ray variations connected with the evolution of the parameters of recurrent high-speed streams of the solar wind Cosmic-ray variations connected with the evolution of the parameters of recurrent high-speed streams of the solar wind

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25.1000d&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Nov.-Dec. 1985, p. 1000-1002. In Russian.

Physics

Cosmic Rays, Periodic Variations, Plasma-Electromagnetic Interaction, Solar Wind Velocity, Coronal Holes, Radiant Flux Density, Solar Corona, Solar Cycles, Time Dependence

Scientific paper

Preliminary results of an analysis of a typical high-speed recurrent high-speed stream (HHS) of the solar wind for May-October 1973 are presented. It is shown that the recurrent HHS parameters and the associated cosmic-ray variations change not randomly but regularly with time. It is concluded that the duration of recurrent HHS existence should be taken into account in investigations of HHSs and related phenomena.

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