22-year intensity variations of galactic cosmic rays and the evolution of the heliospheric current sheet

Details 22-year intensity variations of galactic cosmic rays and the evolution of the heliospheric current sheet 22-year intensity variations of galactic cosmic rays and the evolution of the heliospheric current sheet

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...48s&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 7, p. 48-50.

Physics

Annual Variations, Current Sheets, Galactic Cosmic Rays, Heliosphere, Solar Activity Effects, Interplanetary Magnetic Fields, Particle Energy

Scientific paper

In order to explain certain properties of 22-year variations of the intensity and anisotropy of galactic cosmic rays, the notion of a modulation region that is without spherical symmetry and is closely connected with the heliospheric current sheet is put forward. A qualitative explanation of differences in the intensity modulation levels at the minima of even and odd solar cycles is offered.

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