Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cospar........k&link_type=abstract
Presented at the 28th COSPAR, Jul. 1990
Astronomy and Astrophysics
Astronomy
Astronomy, Gamma Rays, Radiation Counters, Scintillation Counters, X Ray Sources, Background Radiation, Collimators, Shielding
Scientific paper
New phoswich counters were developed that will be capable of detecting low flux hard x rays/gamma rays from astronomical objects. The new phoswich counter consists of a small inorganic scintillator with a fast decay time (the detection part) glued to the interior bottom surface of a rectangular well-shaped block of another inorganic scintillator with a slow decay time (the shielding part). Here, the well-shaped shielding part acts as an active collimator as well as an active shield. A detector system was built which consists of 64 such phoswich counters: newly developed scintillator (GSO) is used for the detection part and CsI(Tl) is used for the shielding part. The total geometrical area of the 64 detection parts is about 740 sq cm and its 3 sigma sensitivity is expected to reach below 10-5/sq cm/s/keV up to 700 keV. With several improvements such detectors will be able to detect hard x rays/gamma rays at a flux level around 10-6/sq cm/s/keV up to 2 MeV.
Gunji Shuichi
Kamae Teturo
Miyazaki Satoshi
Nishimura Jun
Sekimoto Yutaro
No associations
LandOfFree
Detector to study low-flex hard X ray/gamma ray sources 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 Detector to study low-flex hard X ray/gamma ray sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detector to study low-flex hard X ray/gamma ray sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1093329