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--.