Features of the modulation of galatic cosmic rays in 1982

Details Features of the modulation of galatic cosmic rays in 1982 Features of the modulation of galatic cosmic rays in 1982

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2349b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Diffuse Radiation, Galactic Cosmic Rays, Solar Activity, Solar Cycles, Solar Magnetic Field, Magnetic Moments, Periodic Variations

Scientific paper

A correlation has been observed between diurnal variations of galactic cosmic rays (GCR) at R = 331 GV and variations of the magnetic moment of the sun M. A sharp increase in M was observed in 1982, which might have led to variations in the GCR modulation. Changes in M lead to an increase in the magnetic field strength in the heliosphere, leading in turn to an increase in the fluctuation level of the IMF, which in turn is responsible for GCR modulation.

Affiliated with

Also associated with

No associations

Rating

Features of the modulation of galatic cosmic rays in 1982 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Features of the modulation of galatic cosmic rays in 1982, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Features of the modulation of galatic cosmic rays in 1982 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1757865