Spectroscopic capabilities of the Solar-A satellite

Details Spectroscopic capabilities of the Solar-A satellite Spectroscopic capabilities of the Solar-A satellite

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..401y&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 401-406 (1988).

Physics

1

X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

The Wide Band Spectrometer (WBS) will be flown on the Solar-A satellite to observe a flare photon spectrum from soft X-rays to gamma-rays. The WBS consists of three spectrometers: a soft X-ray spectrometer of a gas proportional counter covering the 2-30 keV band, hard X-ray spectrometer of a NaI scintillation counter covering the 20-400 keV band and gamma-ray spectrometer of two BGO scintillation counters covering the 0.2-100 MeV band. The details of the spectral capabilities of the Wide Band Spectrometer are described.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic capabilities of the Solar-A satellite 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 Spectroscopic capabilities of the Solar-A satellite, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic capabilities of the Solar-A satellite will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-909090