Use of the EGRET (Energetic Gamma-Ray Experiment Telescope) instrument in studies of the origin of the cosmic radiation
Conference
·
OSTI ID:5984259
The Energetic Gamma-Ray Telescope (EGRET) onboard the Gamma Ray Observatory will provide the first detailed map of the galaxy showing both intensity and spectral variations at >20 MeV gamma-ray energies. Possible reasons for gamma-ray spectral variations are considered under the hypothesis that point sources of cosmic rays exist. We show how the spectrum and intensity of cosmic rays in the vicinity of such objects can depend on propagation effects, injection conditions and model geometry in a number of special cases. 21 refs., 4 figs.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- DOE Contract Number:
- W-7405-ENG-48
- OSTI ID:
- 5984259
- Report Number(s):
- UCRL-101129; CONF-8904216-4; ON: DE89013785
- Resource Relation:
- Conference: Gamma ray observatory science workshop, Greenbelt, MD, USA, 10 Apr 1989; Other Information: Portions of this document are illegible in microfiche products
- Country of Publication:
- United States
- Language:
- English
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GALAXIES
GAMMA DETECTION
COSMIC PROTONS
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GAMMA SPECTRA
GAMMA TRANSPORT THEORY
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GALAXIES
GAMMA DETECTION
COSMIC PROTONS
COSMIC RADIATION
DISTRIBUTION FUNCTIONS
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GAMMA RADIATION
GAMMA SPECTRA
GAMMA TRANSPORT THEORY
MAPPING
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BARYONS
CAMERAS
DETECTION
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
FERMIONS
FUNCTIONS
HADRONS
IONIZING RADIATIONS
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PROTONS
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TRANSPORT THEORY
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