Paper
22 December 1992 Scintillating fiber calorimeter as a detector for the observation of GeV cosmic gamma rays
Shoji Torii, Katsuaki Kasahara, Tadayoshi Doke, T. Kashiwagi, Jun Kikuchi, Heihachiro Murakami, A. Nakamoto, Toshinori Yuda, Kimiaki Masuda, Y. Muraki, V. V. Akimov, N. G. Leikov
Author Affiliations +
Abstract
A scintillating fiber sampling calorimeter telescope (SSCT) intended to be operated onboard a satellite for cosmic gamma-ray observation in the range from 200 MeV to 200 GeV is presented. SSCT consists of a target part and a main part that includes a calorimeter with imaging capability, which are separated by a distance of 60-70 cm. A gamma ray enters the target and is converted into a pair of electrons which in turn develops into an electron-photon cascade that is observed in the main part. The gamma-ray direction is measured by pointing the energy-weighted centers observed in the two parts. The shower particle are detected using 2 mm square fibers which are bundled into a 2 mm thick flat belt. A pair of belts crossing at a right angle is inserted between lead plates. Experimental results show that the energy resolution of the calorimeter is 20 percent/sq root E(GeV) below a few GeV. The angular resolution is 1.6 deg at 1 GeV and 0.34 deg at 10 GeV.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Shoji Torii, Katsuaki Kasahara, Tadayoshi Doke, T. Kashiwagi, Jun Kikuchi, Heihachiro Murakami, A. Nakamoto, Toshinori Yuda, Kimiaki Masuda, Y. Muraki, V. V. Akimov, and N. G. Leikov "Scintillating fiber calorimeter as a detector for the observation of GeV cosmic gamma rays", Proc. SPIE 1734, Gamma-Ray Detectors, (22 December 1992); https://doi.org/10.1117/12.138591
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Particles

Sensors

Gamma radiation

Electrons

Lead

Spatial resolution

Signal attenuation

RELATED CONTENT

IBIS science prospects
Proceedings of SPIE (March 11 2003)
TIGRE prototype gamma-ray balloon instrument
Proceedings of SPIE (September 21 2006)

Back to Top