Solar flare activity and the changes of proton fluxes in the distant heliosphere

Details Solar flare activity and the changes of proton fluxes in the distant heliosphere Solar flare activity and the changes of proton fluxes in the distant heliosphere

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..327k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, no. 5, 1988, p. 327, 328.

Astronomy and Astrophysics

Astronomy

2

Heliosphere, Solar Activity Effects, Solar Flares, Solar Protons, Plasma Turbulence, Solar Corona, Voyager Project

Scientific paper

In an interval of three years, proton fluxes occurred at the time of enhanced solar activity, which is expressed in terms of the number of flares. The proton fluxes were attenuated at distances of 12-19 AU, especially between Aug. 1983 and Feb. 1984, at a time when solar flare and coronal radio activity was very low; it was at this time that a plasma emission on about 3 kHz, probably originating after Lanzerotti et al. (1985) from the turbulent plasma medium of distant heliopausa, was indicated. The results may also prove important for forecasting long-lasting fluctuations of proton fluxes at distances of 10-20 AU in the heliosphere.

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