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| Title: |
Gamma-ray detectors (greater than 10 MeV)
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| Author(s): |
Owens, Alan; Dunphy, Philip P.
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| Abstract: |
Photons in the energy region above 10 MeV can provide unique information about the highest energy particles produced in solar flares. Measurements of the energy spectra, temporal behavior and anisotropies of the incident photons, can give valuable insights into the particle acceleration process. The detection techniques used at these energies, typical instruments which use these techniques, and future solar missions are reviewed.
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| NASA Center: |
NASA (non Center Specific)
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| Publication Date: |
JAN 1, 1988
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| Document Source: |
Other Sources |
| No Digital Version Available: |
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| Document ID: |
19890040750
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| Accession ID: |
89A28121
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| Publication Information: |
Solar Physics, 118, 1-2,, ISSN 0038-0938, Number of Pages = 17 |
| Contract-Grant-Task Number: |
NAGW-534 |
| Keywords: |
ENERGETIC PARTICLES; GAMMA RAY SPECTROMETERS; HIGH ENERGY ELECTRONS; SOLAR FLARES; ENERGY SPECTRA; RADIATION DETECTORS; SATELLITE INSTRUMENTS;
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| Notes: |
Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 291-307. |
| Accessibility: |
Unclassified; Copyright; Unlimited; Publicly available; |
| Updated/Added to NTRS: |
2004-11-03 |
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