Forbush effect in solar proton intensity

Details Forbush effect in solar proton intensity Forbush effect in solar proton intensity

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978izyak..42.1026v&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, June 1977.) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheska

Physics

Cosmic Rays, Forbush Decreases, Proton Flux Density, Solar Protons, Decay Rates, Energy Spectra, Galactic Radiation, Interplanetary Medium, Radiation Spectra, Solar Cosmic Rays, Solar Spectra, Spectral Energy Distribution

Scientific paper

Observed Forbush decreases in the intensity of low-energy (1 to 30 MeV) cosmic-ray protons of solar and galactic origin are discussed. It is shown that for solar cosmic rays, a general decline in intensity is always observed after the decay phase of a Forbush decrease. Some typical examples of Forbush decreases in the intensity of solar cosmic-ray protons are examined, and an experimentally obtained energy spectrum of a Forbush decrease in solar proton intensity is analyzed. A 'spurious' Forbush decrease in solar proton intensity is also described which is believed to have been caused by the passage or formation of an interplanetary inhomogeneity between the sun and the point of observation.

Affiliated with

Also associated with

No associations

Rating

Forbush effect in solar proton intensity 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 Forbush effect in solar proton intensity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Forbush effect in solar proton intensity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1297589