Share Email Print

Proceedings Paper

Performance of the scattering and crystal polarimeters for the SPECTRUM-X-Gamma mission
Author(s): Ronald F. Elsner; Martin C. Weisskopf; Robert Novick; Philip E. Kaaret; Eric H. Silver
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

X-ray scattering from a lithium disk and Bragg reflection from a mosaic graphite crystal can be exploited to measure the linear polarization of radiation emitted from cosmic X-ray sources. The sensitivity is enhanced if the polarimeters are placed at the focus of an X-ray telescope. Such devices form two of the components of the Stellar X-ray Polarimeter experiment scheduled to fly on the Spectrum-X-Gamma mission. The expected on-axis performance of the two components is described based on detailed Monte Carlo simulations. The polarimetry experiment is expected to provide sensitive measurements of linear polarization for many cosmic X-ray sources. The nature and utility of such observations is described for pulsing X-ray sources such as the Crab pulsar and Her X-1.

Paper Details

Date Published: 1 October 1990
PDF: 12 pages
Proc. SPIE 1317, Polarimetry: Radar, Infrared, Visible, Ultraviolet, and X-Ray, (1 October 1990); doi: 10.1117/12.22073
Show Author Affiliations
Ronald F. Elsner, NASA/Marshall Space Flight Ctr. (United States)
Martin C. Weisskopf, NASA/Marshall Space Flight Ctr. (United States)
Robert Novick, Columbia Univ. (United States)
Philip E. Kaaret, Columbia Univ. (United States)
Eric H. Silver, Lawrence Livermore National Lab. (United States)

Published in SPIE Proceedings Vol. 1317:
Polarimetry: Radar, Infrared, Visible, Ultraviolet, and X-Ray
Russell A. Chipman; John W. Morris, Editor(s)

© SPIE. Terms of Use
Back to Top