Gamma-Ray and Optical Observation of the 1979 November 8 Solar Flare
Abstract
The solar flare on 1979 November 8 11h 21m 28s UT was observed by the Tel Aviv telescope of the Big Bear Solar Observatory and the High Resolution Gamma-Ray Spectrometer on the High Energy Astronomy Observatory HEAO 3. Photographs in Hα show the development of the flare and a subsequent Moreton wave. Although the flare was not detected with the high spectral resolution germanium detectors, the HEAO C-1 CsI shield detected a statistically significant signal above 80 keV, from 420 to 585 keV, and above 3.8 MeV. The temporal structure of microwave, optical, X-ray, and gamma-ray emission is consistent to within ~1 s with a simultaneous flare response at all energies. There is no evidence for either second-stage acceleration of charged particles (Bai and Ramaty, 1979) or a delay between gamma-ray and X-ray continuum emission due to energy-dependent electron energy loss times (Bai and Ramaty).
Additional Information
© 1982 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1980 December 8; accepted 1982 February 18. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract NAS7-100. The Tel Aviv Telescope is supported by the Atmospheric Sciences Section of the National Science Foundation under grant ATM79-11139. Space Radiation Laboratory SRL ID #: 1981-21.Attached Files
Published - 1981-21.pdf
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Additional details
- Eprint ID
- 45042
- Resolver ID
- CaltechAUTHORS:20140417-154129989
- NAS7-100
- NASA
- ATM79-11139
- NSF
- Created
-
2014-04-23Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1981-21