Multi-Spectral Solar Telescope Array. II - Soft X-ray/EUV reflectivity of the multilayer mirrors

Details Multi-Spectral Solar Telescope Array. II - Soft X-ray/EUV reflectivity of the multilayer mirrors Multi-Spectral Solar Telescope Array. II - Soft X-ray/EUV reflectivity of the multilayer mirrors

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991opten..30.1067b&link_type=abstract

Optical Engineering (ISSN 0091-3286), vol. 30, Aug. 1991, p. 1067-1075.

Physics

Optics

10

Cassegrain Optics, Extreme Ultraviolet Radiation, Layers, Optical Reflection, Rocket-Borne Instruments, X Ray Telescopes, Ceramic Coatings, Monte Carlo Method, Optical Materials, Protective Coatings, Quantum Efficiency

Scientific paper

The Multispectral Solar Telescope Array is a rocket-borne observatory which encompasses seven compact soft X-ray/EUV, multilayer-coated, and two compact far-UV, interference film-coated, Cassegrain and Ritchey-Chretien telescopes. Extensive measurements are presented on the efficiency and spectral bandpass of the X-ray/EUV telescopes. Attention is given to systematic errors and measurement errors.

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