7 November 1994 X-ray spectroheliographs with the Bragg focusing optics for the CORONAS project: design, fabrication, and optical testing
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Abstract
Two x-ray spectroheliographs have been designed for obtaining solar images in about 8.42 angstrom and in 1.86 angstrom spectral regions with high spatial and spectral resolution. In both devices unique optical elements-focusing Bragg crystal mirrors are used. Technologies of their production are described here. These mirrors were tested in the x-ray region for their iamging and dispersive properties. These calibration results are presented.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sergey V. Kuzin, Sergey V. Kuzin, Eugeny A. Andreev, Eugeny A. Andreev, Viatcheslav V. Korneev, Viatcheslav V. Korneev, Viktor V. Krutov, Viktor V. Krutov, Mikhail M. Mitropolsky, Mikhail M. Mitropolsky, Andrey A. Pertzov, Andrey A. Pertzov, Vladimir N. Stasevich, Vladimir N. Stasevich, Igor I. Sobelman, Igor I. Sobelman, Igor P. Tindo, Igor P. Tindo, Igor A. Zhitnik, Igor A. Zhitnik, } "X-ray spectroheliographs with the Bragg focusing optics for the CORONAS project: design, fabrication, and optical testing", Proc. SPIE 2283, X-Ray and Ultraviolet Spectroscopy and Polarimetry, (7 November 1994); doi: 10.1117/12.193192; https://doi.org/10.1117/12.193192
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