Composition anomalies in solar flares

Details Composition anomalies in solar flares Composition anomalies in solar flares

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5..128m&link_type=abstract

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

Computer Science

Abundance, Chemical Composition, Energetic Particles, Heavy Elements, Solar Flares, Abnormalities, Cosmic Rays, Heavy Ions, Mass Ratios

Scientific paper

Flares with anomalies in He-3 and Fe enrichment and unusual abundances of heavy ions are discussed. Enrichment in heavy elements including O, Ne, Mg, Si, S-Ca group, and Fe is found in small flares enriched in He-3 and Fe; the flares enriched in He-3 and all heavy elements through Fe show depletion of the carbon abundance. An extreme case of the carbon abundance depletion with the C/O ratio of 0.01 contrasting with the normal solar flare C/O ratio of 0.5 indicates new constraints on acceleration models for small Fe-rich events.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-949289