A solar proton event of possible non-flare origin

Details A solar proton event of possible non-flare origin A solar proton event of possible non-flare origin

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5..192d&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 5. (A81-12386 02-93) T

Physics

Solar Flux, Solar Protons, Angular Distribution, Energy Spectra, Proton Energy, Proton Flux Density, Solar Magnetic Field

Scientific paper

The sun showed little activity in the period August 18-23, 1978. A filament, near central meridian passage, disappeared at approximately 0120 U.T. on August 23, with a SSC recorded at earth at 0247 U.T. on August 27 that appears to be associated with it. On August 25, the low-energy proton detector on board the ISEE-3 spacecraft detected a particle increase which commenced prior to mid-day, and lasted until about 1730 U.T. on August 27. Data for the event are displayed and the possible origin of the particles is discussed.

Affiliated with

Also associated with

No associations

Rating

A solar proton event of possible non-flare origin 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 A solar proton event of possible non-flare origin, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A solar proton event of possible non-flare origin will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-949300