Multi-Spectral Solar Telescope Array. V - Temperature diagnostic response to the optically thin solar plasma

Details Multi-Spectral Solar Telescope Array. V - Temperature diagnostic response to the optically thin solar plasma Multi-Spectral Solar Telescope Array. V - Temperature diagnostic response to the optically thin solar plasma

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991opten..30.1125d&link_type=abstract

Optical Engineering (ISSN 0091-3286), vol. 30, Aug. 1991, p. 1125-1133.

Physics

Optics

7

Optical Thickness, Plasma Temperature, Rocket-Borne Instruments, Solar Corona, Solar Wind, Spaceborne Telescopes, Cassegrain Optics, Layers, Reflecting Telescopes, Solar Spectra

Scientific paper

The compact soft X-ray/EUV/FUV multilayer coated telescopes developed for solar chromosphere, corona, and corona/solar-wind interface studies permit the use of conventional (Cassegrain, Herschelian, etc.) configurations. The multilayer coatings also allow a narrow-wavelength band to be selected for imaging. NASA's Multi-Spectral Solar Telescope Array is composed of 17 of these compact telescopes; attention is given to their ability to obtain temperature-diagnostic information concerning the solar plasma.

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