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Onboard performance of the RT-2 detectors |
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| Authors: | A. R. Rao J. P. Malkar M. K. Hingar V. K. Agrawal Sandip K. Chakrabarti Anuj Nandi D. Debnath T. B. Kotoch R. Sarkar T. R. Chidambaram P. Vinod S. Sreekumar Y. D. Kotov A. S. Buslov V. N. Yurov V. G. TyshkeVich A. I. Arkhangelsky R. A. Zyatkov |
| Affiliation: | 1. Tata Institute of Fundamental Research, Mumbai, India 2. S.N. Bose National Centre for Basic Sciences, Kolkata, India 3. India Centre for Space Physics, Kolkata, India 4. Vikram Sarabhai Space Center, Thiruvananthapuram, India 5. National Research Nuclear University “MEPhI” (NRNU MEPhI), Moscow, Russia |
| Abstract: | The RT-2 Experiment onboard the CORONAS-PHOTON satellite is designed to study the spectral, temporal, and spatial details of solar hard X-ray flares in the 15–150 keV range. Above this energy (and upto 1000 keV), it also acts as an omni-directional gamma-ray detector with a capability to study gamma-ray bursts (GRB), bright solar flares, and X-ray pulsars. With an ensemble of hard X-ray detectors with different fields of view and coding devices, it also has the capability to investigate the spectrum of Cosmic Diffuse X-ray Background. The performance of the detectors from 2009 February to November is described in this paper. Results obtained on a few GRBs and solar flares are also briefly discussed. |
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