Astronomy and Astrophysics – Astronomy
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..177b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, May 1985, p. 177-182.
Astronomy and Astrophysics
Astronomy
1
Abundance, Helium Isotopes, Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Solar Activity Effects
Scientific paper
The positions of solar flares identified in the He3-rich Solar Flares Catalog of Slivka (1982) were compared with magnetic field patterns for selected areas of the solar disk during the period 1968-1978. A high concentration of He3 solar flares was found in magnetically active longitudes; practically all of the flare events occurred in or near a well-defined magnetic field boundary surrounded by a field of the opposite polarity. The patterns of the magnetic field lines in the magnetically active longitudes are shown in synoptic charts. It is concluded that the geometry of the magnetic field may contribute to the enrichment of flare particles by H3.
No associations
LandOfFree
Characteristic patterns of solar magnetic fields around the positions of flares with enhanced helium-3 abundance 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 Characteristic patterns of solar magnetic fields around the positions of flares with enhanced helium-3 abundance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristic patterns of solar magnetic fields around the positions of flares with enhanced helium-3 abundance will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1631591