Intensity perturbations of cosmic rays after weak proton flares on the sun

Details Intensity perturbations of cosmic rays after weak proton flares on the sun Intensity perturbations of cosmic rays after weak proton flares on the sun

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..308b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Mar.-Apr. 1990, p. 308-310. In Russian.

Physics

Solar Cosmic Rays, Solar Flares, Solar Protons, Diurnal Variations, Geomagnetism, Interplanetary Magnetic Fields, Nocturnal Variations, Solar Neutrons

Scientific paper

A cosmic-ray intensity decrease effect (at an energy of not less than 4
GeV) has been observed during nighttime/morning hours after solar flares
generating particles with energies not greater than 100 MeV/nucleon.
However, no effect of relativistic solar protons or neutrons with an
energy greater than about 300 MeV was observed after weak proton flares.

Affiliated with

Also associated with

No associations

Rating

Intensity perturbations of cosmic rays after weak proton flares on the sun 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 Intensity perturbations of cosmic rays after weak proton flares on the sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Intensity perturbations of cosmic rays after weak proton flares on the sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1380842