Published August 1996
| Version v1
Journal article
DMSP satellite detections of gamma-ray bursts
- 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 six U.S. Air Force Defense Meteorological Satellite Program (DMSP) spacecraft, two of which are currently in use. Their 800-km altitude orbits give a field of view to 117 degree from the zenith. A great many bursts have been detected, usually in coincidence with detections by GRO or other satellites such as PVO or ULYSSES. The directions of the sources can be determined with considerable accuracy from such correlated observations, even when GRO/BATSE with its directional capabilities is not involved. Thus these DMSP data, especially in conjunction with other observations, should be helpful in trying to understand the true nature of gamma-ray bursts. copyright 1996 American Institute of Physics
Additional details
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 384
- Journal Issue
- 1
- Journal Page Range
- p. 545-549.
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Symposium on gamma ray bursts.
- Dates
- 25-27 Oct 1995.
- Place
- Huntsville, AL (United States).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 28076513
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC GAMMA BURSTS; GAMMA ASTRONOMY; GAMMA DETECTION; SATELLITES; SPECTRAL DENSITY; TIME DEPENDENCE
- Descriptors DEC
- ASTRONOMY; COSMIC RADIATION; DETECTION; FUNCTIONS; IONIZING RADIATIONS; PRIMARY COSMIC RADIATION; RADIATION DETECTION; RADIATIONS; SPECTRAL FUNCTIONS
Optional Information
- Secondary number(s)
- CONF-9510332--.