Physics – Space Physics
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ijrsp..16..281v&link_type=abstract
Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 16, June 1987, p. 281-285.
Physics
Space Physics
Gamma Ray Bursts, Microwave Emission, Particle Acceleration, Solar Radiation, Solar Radio Bursts, Shock Wave Propagation, Solar Flares
Scientific paper
The relationships of solar gamma ray (GR) emissions with microwave (MW) and other radio bursts have been studied. The GR emissions are found to start about 1-2 min after the onset of MW emissions (on 17 GHz) or about 0.5 min before the peak of MW emissions. This time delay may be due to differences in acceleration times for accelerating the electrons for MW emissions and protons, ions and nuclei for gamma ray (also line) emissions. Further, the GR emission flares are found to be associated fairly well with type-II and type-IV radio bursts while the gamma ray line (GRL) emission flares show higher association with the type-II and type-IV radio bursts. The type-II bursts start about 6 min after the onset of GR emissions while the type-IV bursts start about 2 min before the onset of GR emissions, which show that the GR emissions and the type-II (also type-IV) may not be produced simultaneously by shock waves.
No associations
LandOfFree
Relationship of solar gamma ray emissions with microwaves and other radio bursts 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 Relationship of solar gamma ray emissions with microwaves and other radio bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relationship of solar gamma ray emissions with microwaves and other radio bursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1817991