Conference paper
Effect of mirror curvature on the angular resolution of silicon pore optics
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 |
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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 |