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Gamma ray burst source locations with the Ulysses/Compton/PVO networkThe new interplanetary gamma-ray burst network will determine source fields with unprecedented accuracy. The baseline of the Ulysses mission and the locations of Pioneer-Venus Orbiter and of Mars Observer will ensure precision to a few tens of arc seconds. Combined with the event phenomenologies of the Burst and Transient Source Experiment on Compton Observatory, the source locations to be achieved with this network may provide a basic new understanding of the puzzle of gamma ray bursts.
Document ID
19930056064
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cline, T. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Hurley, K. C.
(California Univ. Berkeley, United States)
Boer, M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sommer, M.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Niel, M.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Fishman, G. J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kouveliotou, C.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Meegan, C. A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Paciesas, W. S.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Wilson, R. B.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Gamma-ray bursts; Proceedings of the Workshop, Univ. of Alabama, Huntsville, Oct. 16-18, 1991 (A93-40051 16-93)
Publisher: American Institute of Physics
Subject Category
Space Radiation
Accession Number
93A40061
Funding Number(s)
CONTRACT_GRANT: JPL-958056
CONTRACT_GRANT: NAG5-1560
Distribution Limits
Public
Copyright
Other

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