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Proceedings Paper

Calibration and modeling of the SODART-OXS Bragg spectrometer on board the SRG satellite
Author(s): Ingolf Halm; Hans-Joachim Wiebicke; Finn Erland Christensen; Peter K. Frederiksen; Ib Lundgaard Rasmussen
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Paper Abstract

The SODART x-ray telescope includes an objective crystal spectrometer (OXS) providing a high energy resolving power by Bragg reflection upon crystals. To cover a wide energy range, 3 types of natural crystals, and a Co/C multilayer structure upon Si are used in the ranges 5-11 keV, 2-5 keV, 0.5-1.2 keV, and 0.16-0.42 keV. All types of crystal besides Si being an ideal crystal have been calibrated individually and after gluing onto the Bragg panel. The x-ray calibration procedures and result are discussed below. A ray-tracing program using the OXS calibration data and simulating the x- ray photon reflection on the mentioned crystals and the multilayers has been developed and is described also.

Paper Details

Date Published: 10 November 1998
PDF: 11 pages
Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); doi: 10.1117/12.330271
Show Author Affiliations
Ingolf Halm, Astrophysikalisches Institut Potsdam (Germany)
Hans-Joachim Wiebicke, Astrophysikalisches Institut Potsdam (Germany)
Finn Erland Christensen, Danish Space Research Institute (Denmark)
Peter K. Frederiksen, Danish Space Research Institute (Denmark)
Ib Lundgaard Rasmussen, Danish Space Research Institute (Denmark)


Published in SPIE Proceedings Vol. 3445:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX
Oswald H. W. Siegmund; Mark A. Gummin, Editor(s)

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