The Ability of Cos-B to Measure Gamma-Ray Bursts
Abstract
The COS-B satellite for gamma-ray astronomy, launched on 7 August, 1975, features as part of the main instrument a 1.1 m2, 10 mm thick, plastic scintillator for the vetoing of charged particle events. This detector which has an average effective area of 360 cm2 for gamma rays in the interval 0.1 to 1 MeV has been instrumented to detect and record the temporal structure of cosmic gamma ray bursts. The instrument will be sensitive to gamma bursts down to 3% of the typical intensities measured by the Vela satellite system. The best time resolution achievable is 1.6 ms. The satellite will be placed in a 100 000 km eccentric orbit and with absolute timing accuracies of fractions of a millisecond achievable, a long base line is available for the triangulation of the source position, given comparable data from other satellites.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- June 1976
- DOI:
- 10.1007/BF00645532
- Bibcode:
- 1976Ap&SS..42..103B
- Keywords:
-
- Cos-B Satellite;
- Cosmic X Rays;
- Gamma Rays;
- Satellite Observation;
- X Ray Astronomy;
- Data Systems;
- Energy Spectra;
- Radiation Detectors;
- Satellite-Borne Instruments;
- Scintillation Counters;
- Spaceborne Astronomy;
- X Ray Sources;
- Instrumentation and Photography;
- Charged Particle;
- Temporal Structure;
- Effective Area;
- Satellite System;
- Source Position