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Reflectometry of surfaces of 1.7-m mirror of WSO-UV space telescope
Author(s): Oleg Vlasenko; Mikhail Sachkov
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Paper Abstract

Reflectometry is one of the widely used method to study rough optical surfaces. Here we present results of first measurement of mirror samples of T-170M Primary Mirror. These measurements were made by using compact HOROS-S instrument for 3D Bidirectional reflectance distribution function (BRDF) determination constructed by Jena Fraunhofer Institute of Applied Optics.

Paper Details

Date Published: 6 July 2018
PDF: 6 pages
Proc. SPIE 10699, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, 1069933 (6 July 2018); doi: 10.1117/12.2312900
Show Author Affiliations
Oleg Vlasenko, Institute of Astronomy (Russian Federation)
Mikhail Sachkov, Institute of Astronomy (Russian Federation)


Published in SPIE Proceedings Vol. 10699:
Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
Jan-Willem A. den Herder; Shouleh Nikzad; Kazuhiro Nakazawa, Editor(s)

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