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Title: DMSP satellites as gamma-ray burst detectors

Conference ·
OSTI ID:10112595
; ;  [1];  [2]
  1. Los Alamos National Lab., NM (United States)
  2. Sandia National Labs., Albuquerque, NM (United States)

Gamma-ray burst detectors are aboard three US Air Force Defense Meteorological Satellite Program (DMSP) spacecraft, in orbit at 800 km altitude, with corresponding fields of view to 117{degree} from the zenith. A large number of bursts have been detected by DMSP, usually confirming and supplementing data from GRO and other spacecraft. The location of a gamma-ray burst source detected by several DMSP spacecraft is considerably restricted by knowledge of the several fields of view. Often non-detection of a strong burst by one or more DMSP spacecraft is even more informative in narrowing the possible area of the burst. The DMSP data in conjunction with observations by other spacecraft can lead to reasonable positional information when more accurate positions are not available from GRO or other data.

Research Organization:
Los Alamos National Lab., NM (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States); Department of Defense, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
10112595
Report Number(s):
LA-UR-93-4313; CONF-9310252-1; ON: DE94004977
Resource Relation:
Conference: 2. gamma-ray burst workshop,Huntsville, AL (United States),20-22 Oct 1993; Other Information: PBD: [1993]
Country of Publication:
United States
Language:
English

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