Share Email Print

Proceedings Paper

X-ray pencil beam characterization of silicon pore optics
Author(s): G. Vacanti; M. Ackermann; M. Vervest; M. Collon; R. Günther; C. Kelly; E. Wille; L. Cibik; M. Krumrey; P. Müller
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

The characterization of large aperture (> 2 meters), long focal length (> 10 meters) X-ray mirrors for X-ray astronomy with synchrotron radiation poses signi cant problems related to the available space at synchrotron radiation facilities. Intrafocal pencil beam characterization of part of the optics is advantageous if its results can be shown to have predictive capabilities with respect to the full system.

In this paper we present the routine characterization of silicon pore optics at the X-ray Pencil Beam Facility of the Physikalisch-Technische Bundesanstalt, located at the synchrotron radiation facility BESSY II (Berlin, Germany). In particular we show how measurements taken in the standard beamline con guration (detector at ve meters from the optics) can e ectively be used to predict the optical performance of the optics at their design focal length by comparing data taken on 20-meter focal length Silicon Pore Optics unit in the 20-meter beamline con guration (available only for a few weeks every year) with extrapolated 5-meter measurements.

Paper Details

Date Published: 26 September 2013
PDF: 9 pages
Proc. SPIE 8861, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VI, 88611K (26 September 2013); doi: 10.1117/12.2024837
Show Author Affiliations
G. Vacanti, cosine Science and Computing B.V. (Netherlands)
M. Ackermann, cosine Research B.V. (Netherlands)
M. Vervest, cosine Science and Computing B.V. (Netherlands)
M. Collon, cosine Research B.V. (Netherlands)
R. Günther, cosine Research B.V. (Netherlands)
C. Kelly, cosine Science and Computing B.V. (Netherlands)
E. Wille, European Space Agency, ESTEC (Netherlands)
L. Cibik, Physikalisch-Technische Bundesanstalt (Germany)
M. Krumrey, Physikalisch-Technische Bundesanstalt (Germany)
P. Müller, Physikalisch-Technische Bundesanstalt (Germany)

Published in SPIE Proceedings Vol. 8861:
Optics for EUV, X-Ray, and Gamma-Ray Astronomy VI
Stephen L. O'Dell; Giovanni Pareschi, Editor(s)

© SPIE. Terms of Use
Back to Top