Onboard performance of the RT-2 detectors

Details Onboard performance of the RT-2 detectors Onboard performance of the RT-2 detectors

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sosyr..45..123r&link_type=abstract

Solar System Research, Volume 45, Issue 2, pp.123-134

Computer Science

Performance

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Onboard performance of the RT-2 detectors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Onboard performance of the RT-2 detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Onboard performance of the RT-2 detectors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-770200