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Conference paper

Effect of mirror curvature on the angular resolution of silicon pore optics

In Proceedings of Spie 2021, Volume 11822, pp. 118220F-118220F-8
From

National Space Institute, Technical University of Denmark1

Astrophysics and Atmospheric Physics, National Space Institute, Technical University of Denmark2

Department of Physics, Technical University of Denmark3

Neutrons and X-rays for Materials Physics, Department of Physics, Technical University of Denmark4

Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna5

ESTEC6

Silicon Pore Optics are a novel technology for focusing high-energy photons, where pairs of mirror plates stacked into mirror modules. This paper presents a study of the angular resolution of SPO mirror assemblies, using a selection of sagittal mirror curvatures. Results were achieved by ray-tracing the different configurations of the mirror with the ray tracing software SPORT, or Silicon Pore Optics Ray Tracer, using an observation of the Crab Nebula originally obtained by Chandra.

It is found that a true Wolter geometry most closely reproduces the original image, while geometries with a conic approximation on either their primary or secondary mirrors create the most diffuse image. A geometry with conic approximations on both primary and secondary mirrors falls in between the two extremes.

Language: English
Publisher: SPIE - International Society for Optical Engineering
Year: 2021
Pages: 118220F-118220F-8
Proceedings: SPIE Optical Engineering + Applications 2021
Series: Proceedings of Spie - the International Society for Optical Engineering
Journal subtitle: Optics for Euv, X-ray, and Gamma-ray Astronomy X
ISBN: 1510644822 , 1510644830 , 9781510644823 and 9781510644830
ISSN: 1996756x and 0277786x
Types: Conference paper
DOI: 10.1117/12.2594530
ORCIDs: Jegers, Arne S. , Ferreira, Desiree Della Monica , Bergbäck Knudsen, Erik , Massahi, Sonny , Svendsen, Sara , Lindquist Henriksen, Peter and Gellert, Nis Christian

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