Multi-Spectral Solar Telescope Array. IV - The soft X-ray and extreme ultraviolet filters

Details Multi-Spectral Solar Telescope Array. IV - The soft X-ray and extreme ultraviolet filters Multi-Spectral Solar Telescope Array. IV - The soft X-ray and extreme ultraviolet filters

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991opten..30.1134l&link_type=abstract

Optical Engineering (ISSN 0091-3286), vol. 30, Aug. 1991, p. 1134-1141.

Computer Science

6

Layers, Optical Filters, Ultraviolet Telescopes, X Ray Telescopes, Aluminum, Beryllium, Carbon, Extreme Ultraviolet Radiation, Mirrors, Molybdenum

Scientific paper

NASA's Multi-Spectral Solar Telescope Array uses various combinations of thin foil filters composed of Al, C, Te, Be, Mo, Rh, and phthalocyanine to achieve the requisite radiation-rejection characteristics. Such rejection is demanded by the presence of strong EUV radiation at longer wavelengths where the specular reflectivity of multilayer mirrors can cause 'contamination' of the image in the narrow band defined by the Bragg condition.

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