NASA NTRS · 19910064267
Multi-Spectral Solar Telescope Array. V - Temperature diagnostic response to the optically thin solar plasma
Abstract
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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Deforest, Craig E., Kankelborg, Charles C., Allen, Max J., Paris, Elizabeth S., Willis, Tom D., Lindblom, Joakim F., O'Neal, Ray H., Walker, Arthur B. C., Jr., Barbee, Troy W., Jr., Hoover, Richard B.. 1991-08-01. Multi-Spectral Solar Telescope Array. V - Temperature diagnostic response to the optically thin solar plasma. https://ntrs.nasa.gov/citations/19910064267
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