Published September 1, 1991 | Version v1
Journal article

Burst detection capability of the Mars Observer gamma-ray spectrometer

  • 1. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109 (United States)
  • 2. Department of Planetary Sciences, University of Arizona, Tucson, Arizona 85721 (United States)
  • 3. Los Alamos National Laboratory, Los Alamos, New Mexico 87544 (United States)
  • 4. Goddard Space Flight Center, Building 21, Room 173A, Greenbelt, Maryland 20771 (United States)

Description

This paper describes the gamma-ray burst detection capability of the gamma-ray spectrometer on board the Mars Observer spacecraft. The instrument is designed to respond to significant bursts by suspending its observation of the martian surface in favor of optimizing the collection of pre-burst, burst, and post-burst data. The results are expected to contribute to our understanding of gamma-ray bursts through a high-energy resolution search for line emission, by the examination of spectral shapes and by comprising one leg of an arrival time network to determine the direction of origin

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
265
Journal Issue
1
Journal Page Range
p. 353-358.
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Gamma ray burst conference.
Dates
17-18 Oct 1991.
Place
Huntsville, AL (United States).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
25041161
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMIC GAMMA BURSTS; DATA PROCESSING; DETECTION; GAMMA ASTRONOMY; GAMMA SPECTROMETERS; SENSITIVITY
Descriptors DEC
ASTRONOMY; COSMIC RADIATION; IONIZING RADIATIONS; MEASURING INSTRUMENTS; PRIMARY COSMIC RADIATION; RADIATIONS; SPECTROMETERS

Optional Information

Secondary number(s)
CONF-9110310--.