High-energy solar cosmic rays.

Details High-energy solar cosmic rays. High-energy solar cosmic rays.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..321z&link_type=abstract

Geomagn. Aeron., Vol. 29, No. 3, p. 321 - 325

Computer Science

Solar Cosmic Rays

Scientific paper

High-energy solar cosmic rays (SCR) are analyzed from 5 min data recorded by the high-mountain neutron monitor of Alma-Ata. Eight intensity increases during solar proton events with amplitudes of 0.4 - 2.0% are identified. The temporal intensity pattern is investigated for the events of May 7, 1978, and December 7 - 8, 1982. Integral SCR fluxes are computed for three cases; they agree with the spectra determined from the results of satellite measurements, measurements in the stratosphere, and measurements of high-latitude neutron monitors. The upper limit of the energy flux of SCR is determined and found to equal 9±1, 11±2, and 9.5±1.5 GeV for the three mentioned events, respectively.

Affiliated with

Also associated with

No associations

Rating

High-energy solar cosmic rays. 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 High-energy solar cosmic rays., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-energy solar cosmic rays. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1569932