Published July 1, 1994 | Version v1
Journal article

DMSP satellites as gamma-ray burst detectors

  • 1. Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)
  • 2. Sandia National Laboratory, Albuquerque, New Mexico 87185 (United States)

Description

Gamma-ray burst detectors are aboard three U. S. 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 from GRO or other data

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
307
Journal Issue
1
Journal Page Range
p. 34-38.
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
2. gamma-ray burst workshop.
Dates
20-22 Oct 1993.
Place
Huntsville, AL (United States).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
26034051
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CHARGED PARTICLE DETECTION; COORDINATES; COSMIC GAMMA BURSTS; COUNTING RATES; GAMMA DETECTION; KEV RANGE 10-100; KEV RANGE 100-1000; TIMING PROPERTIES
Descriptors DEC
COSMIC RADIATION; DETECTION; ENERGY RANGE; IONIZING RADIATIONS; KEV RANGE; PRIMARY COSMIC RADIATION; RADIATION DETECTION; RADIATIONS

Optional Information

Secondary number(s)
CONF-9310252--.