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KONUS-W gamma-ray burst experiment for ISTP WIND spacecraftThe primary task of the KONUS-W experiment to be flown on board the WIND spacecraft is to observe gamma-ray bursts and solar flares with moderate and high time resolution. The scientific objectives of the experiment include the study of continuum energy spectra and spectral features of these events in the energy range of 10 keV to 10 MeV as well as their time histories in soft, medium, and hard energy bands with a time resolution up to 2 ms. The general design and operation of the KONUS-W gamma-ray detector are briefly described, and the nomial program of burst observations is examined.
Document ID
19930056113
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Aptekar', R. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dement'ev, I. V.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Frederiks, D. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Golenetskij, S. V.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Il'inskij, V. N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mazets, E. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Panov, V. N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sokolova, Z. YA.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Sheshin, L. O.
(Russian Academy of Sciences, Physical-Technical Inst. St. Petersburg, Russia)
Cline, T. L.
(NASA Goddard Space Flight Center Greenbelt, MD, 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
Spacecraft Instrumentation
Accession Number
93A40110
Distribution Limits
Public
Copyright
Other

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