Share Email Print
cover

Proceedings Paper

New type of imaging x-ray detector using a capillary plate
Author(s): Hirohisa Sakurai; S. Saito; Motosaku Noma; Shuichi Gunji; Makiko Tsukahara; Tsutomu Tamura
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

We constructed an optical imaging x-ray detector with a capillary gas proportional counter (CGPC), a focusing mirror system, and an image intensified CCD camera. The CGPC consists of an absorption region for x-rays, which also operates as a drift region of electron clouds, and a gas proportional scintillation region in a capillary plate. With a gas mixture of Xe plus 2% CH4 at 1 atm and a gas gain 8000, the light output from the CGPC is several tens thousand times larger than that of a typical NaI(Tl) scintillator and it is enough to image electron clouds due to a few tens keV x rays. To investigate the imaging ability, images for tracks due to (alpha) particles (241Am) of 5.5 MeV were taken in the gas mixture of Xe plus CH4, for the several reduced fields in the drift region. We confirmed that the images were most clearly observed at around the reduced fields of 40 V/cm(DOT)atm.

Paper Details

Date Published: 15 October 1997
PDF: 7 pages
Proc. SPIE 3114, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VIII, (15 October 1997); doi: 10.1117/12.278899
Show Author Affiliations
Hirohisa Sakurai, Yamagata Univ. (Japan)
S. Saito, Yamagata Univ. (Japan)
Motosaku Noma, Yamagata Univ. (Japan)
Shuichi Gunji, Yamagata Univ. (Japan)
Makiko Tsukahara, IBM Japan, Ltd. (Japan)
Tsutomu Tamura, Yonezawa Engineering High School (Japan)


Published in SPIE Proceedings Vol. 3114:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VIII
Oswald H. W. Siegmund; Mark A. Gummin, Editor(s)

© SPIE. Terms of Use
Back to Top