Observations of high-energy (E≥10 MeV) gamma-rays with the PHEBUS instrument
Abstract
The PHEBUS instrument aboard GRANAT has observed several high energy (E 10 MeV) gamma-ray bursts since 1990. We describe here the characteristics of these high energy bursts with respect of the longitude of the associated H flare. We discuss our results in the context of the transport of high energy particles in the solar atmosphere.
- Publication:
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Advances in Solar Physics
- Pub Date:
- 1994
- DOI:
- Bibcode:
- 1994LNP...432..197V
- Keywords:
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- Solar Gamma-Ray Bursts;
- Solar Gamma-Ray Bursts: Particle Acceleration