On the relation between the long-term variations of cosmic rays and the solar activities

Details On the relation between the long-term variations of cosmic rays and the solar activities On the relation between the long-term variations of cosmic rays and the solar activities

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....4..113k&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 4. (A81-12386 02-93) T

Physics

Cosmic Rays, Diurnal Variations, Solar Activity Effects, Solar Corona, Anisotropy, Harmonic Analysis, Secular Variations, Solar Cycles, Sunspot Cycle

Scientific paper

The unusual variations in the relation between the anisotropy of the tridiurnal variation and the intensity of solar coronal green line since 1968 are discussed. It was shown that the polarity of the solar general magnetic field is reversed at about the time of the maximum values of sunspot numbers; the sunspots are more active than the solar corona during the 19th solar cycle. However, the solar corona are more active than the sunspots during the 20th solar cycle, so that the intensities of the solar coronal green line at low heliographic latitudes had the maximum value of secular variation since 1968.

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