Hard x-ray, gamma-ray, and neutron detector physics XII
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Hard x-ray, gamma-ray, and neutron detector physics XII 2-4 August 2010, San Diego, California, United States by R. B. James

  • 575 Want to read
  • ·
  • 29 Currently reading

Published by SPIE in Bellingham, Wash .
Written in English

Subjects:

  • Semiconductor nuclear counters,
  • Congresses,
  • Optical detectors,
  • Optical radiometry,
  • Gamma ray detectors,
  • X-ray optics

Book details:

Edition Notes

Includes bibliographical references and index.

StatementRalph B. James, Larry A. Franks, Arnold Burger, editors ; sponsored and published by SPIE
SeriesProceedings of SPIE -- v. 7805., Proceedings of SPIE--the International Society for Optical Engineering -- v. 7805.
ContributionsSPIE (Society)
Classifications
LC ClassificationsTA1775 .H3747 2010, QC371 .S67 v. 7805
The Physical Object
Pagination1 v. (various pagings) :
ID Numbers
Open LibraryOL25231502M
ISBN 10081948301X
ISBN 109780819483010
LC Control Number2011293431
OCLC/WorldCa674693610

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Hard X-Ray, Gamma-Ray, and Neutron Detector Physics II Article (PDF Available) in Proceedings of SPIE - The International Society for Optical Engineering October with Reads. Page 1. PROCEEDINGS OF SPIE Volume Proceedings of SPIE, X, v. SPIE is an international society advancing an interdisciplinary approach to the science and application of light. Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XIII. Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XV Introduction Article (PDF Available) in Proceedings of SPIE - The International Society for Optical Engineering August with 66 Reads. An X-ray, or X-radiation, is a penetrating form of high-energy electromagnetic X-rays have a wavelength ranging from 10 picometres to 10 nanometres, corresponding to frequencies in the range 30 petahertz to 30 exahertz (3×10 16 Hz to 3×10 19 Hz) and energies in the range eV to keV.X-ray wavelengths are shorter than those of UV rays and typically longer than those of.

Gamma ray detectors -- Congresses. Semiconductor nuclear counters -- Congresses. Hard X-ray, gamma-ray, and neutron detector physics XVII: August , San Diego, California, United States / Larry Franks [and three others], editors ; sponsored by SPIE. Jay Theodore Cremer Jr., in Advances in Imaging and Electron Physics, Books on Neutron, X-Ray, and Gamma Sources, Optics, and Detectors after More recent publications between and on primarily neutron, and secondarily, X-ray and gamma sources, optics and detectors, and related topics are included in the following incomplete list. Proc. SPIE , Hard X-Ray, Gamma-Ray, and Neutron Detector Physics, pg (19 October ); doi: / Read Abstract + The difference is sped of fast neutrons and gamma rays has been investigated as a mechanism for distinguishing neutron and gamma interactions in . The detection of thermal neutrons has traditionally been accomplished with 3 He-tubes, but with the recent shortage of 3 He, much research has gone into finding suitable replacements. Both relatively inefficient 10 B- and 6 LiF-coated silicon diodes and HgI 2 have been known for many years, and engineered structures in Si that have been filled with 10 B and 6 LiF have shown promise.

Hard X-ray, gamma-ray, and neutron detector physics II 31 July-2 August, , San Diego, [California] USA by. Want to read; 9 Currently reading; Published by SPIE in Bellingham, Washington. Written in English Subjects: X-ray optics -- Congresses., Gamma ray detectors -- .   Get this from a library! Hard X-ray, gamma-ray, and neutron detector physics X: August , San Diego, California, USA. [Arnold Burger; Larry A Franks; R B James; SPIE (Society); United States. Defense Threat Reduction Agency.;].   Get this from a library! Hard X-ray, gamma-ray, and neutron detector physics II: 31 July-2 August, , San Diego, [California] USA. [R B James; Richard C Schirato; Society of Photo-optical Instrumentation Engineers.;]. adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A.