The Third Interplanetary Network
Abstract
The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds Wind, up to ~7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10-7 erg cm-2 or 1 photon cm-2 s-1. It detects ~335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.
- Publication:
-
Gamma Ray Bursts 2010
- Pub Date:
- August 2011
- DOI:
- 10.1063/1.3621810
- Bibcode:
- 2011AIPC.1358..385H
- Keywords:
-
- gamma-ray sources (astronomical);
- spacecraft;
- gravitational lenses;
- gravitational waves;
- 98.70.Rz;
- 94.05.Hk;
- 95.30.Sf;
- 95.85.Sz;
- gamma-ray sources;
- gamma-ray bursts;
- Spacecraft/atmosphere interactions;
- Relativity and gravitation;
- Gravitational radiation magnetic fields and other observations