High energy flare physics group summary
Abstract
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Society Solar Physics Division Meeting are reviewed. Oral and poster papers were presented on observatories and instruments available for the upcoming solar maximum. Among these are the space-based Gamma Ray Observatory, the Solar Flare and Cosmic Burst Gamma Ray Experiment on the Ulysses spacecraft, the Soft X Ray Telescope on the spacecraft Solar-A, and the balloon-based Gamma Ray Imaging Device. Ground based observatories with new capabilities include the BIMA mm-wave interferometer (Univ. of California, Berkeley; Univ. of Illinois; Univ. of Maryland), Owens Valley Radio Observatory and the Very Large Array. The highlights of the various instrument performances are reported and potential data correlations and collaborations are suggested.
- Publication:
-
Developments in Observations and Theory for Solar Cycle 22
- Pub Date:
- 1989
- Bibcode:
- 1989dots.work....1R
- Keywords:
-
- Solar Flares;
- Solar Instruments;
- Solar Observatories;
- Solar Physics;
- Gamma Ray Observatory;
- Gamma Ray Telescopes;
- Radio Interferometers;
- Solar Cycles;
- Ulysses Mission;
- Very Large Array (Vla);
- X Ray Telescopes;
- Solar Physics