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Advanced techniques for high resolution spectroscopic observations of cosmic gamma-ray sourcesAn advanced gamma-ray spectrometer that is currently in development is described. It will obtain a sensitivity of 0.0001 ph/sq cm./sec in a 6 hour balloon observation and uses innovative techniques for background reduction and source imaging.
Document ID
19850026635
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Matteson, J. L. (California Univ., San Diego La Jolla, CA, United States)
Pelling, M. R. (California Univ., San Diego La Jolla, CA, United States)
Peterson, L. E. (California Univ., San Diego La Jolla, CA, United States)
Lin, R. P. (California Univ. Berkeley, United States)
Anderson, K. A. (California Univ. Berkeley, United States)
Pehl, R. H. (California Univ. Lawrence Berkeley Lab. Gif-sur-Yvette, France)
Hurley, K. C. (Centre d'Etude Spatiale des Rayonnements)
Vedrenne, G. (Centre d'Etude Spatiale des Rayonnements)
Sniel, M. (Centre d'Etude Spatiale des Rayonnements)
Durouchoux, P. (CEA)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 3
Subject Category
Space Radiation
Report/Patent Number
OG-9.2-9
Accession Number
85N34948
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850026549Collected WorksNineteenth International Cosmic Ray Conference. OG Sessions, Volume 3
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