Paper
24 July 2014 A setup for soft proton scattering on x-ray mirrors
Sebastian Diebold, Josef Jochum, Eckhard Kendziorra, Emanuele Perinati, Andrea Santangelo, Chris Tenzer
Author Affiliations +
Abstract
Protons with energies between tens of keV and some MeV can degrade the performance of X-ray detectors and contribute to the instrument background. In-orbit measurements showed that the flux of soft protons funneled through Wolter-type mirrors is considerably larger than expected from simulations. Up to now, just very few results from laboratory experiments have been reported and the data is not sufficient to pinpoint the best analytical description of the physical process or to validate simulation codes. In order to improve this situation, a small angle scattering experiment to measure the proton reflection properties of X-ray mirrors has been set up at the accelerator facility of the University of Tübingen. The experimental setup and initial preliminary results obtained with samples of eROSITA mirror shells are presented.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sebastian Diebold, Josef Jochum, Eckhard Kendziorra, Emanuele Perinati, Andrea Santangelo, and Chris Tenzer "A setup for soft proton scattering on x-ray mirrors", Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91444S (24 July 2014); https://doi.org/10.1117/12.2054887
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Scattering

Sensors

Laser scattering

X-rays

Mirrors

Collimators

X-ray detectors

RELATED CONTENT

NuSTAR on-ground calibration: I. Imaging quality
Proceedings of SPIE (September 17 2012)
Time-resolved techniques: an overview
Proceedings of SPIE (January 01 1991)
X-ray study of concave surface roughness
Proceedings of SPIE (September 06 1999)
X-Ray Scattering Of Superpolished Flat Mirror Samples
Proceedings of SPIE (March 24 1982)

Back to Top