1 February 1991 Performance of the Multi-Spectral Solar Telescope Array V: temperature diagnostic response to the optically thin solar plasma
Author Affiliations +
We have developed compact soft x-ray, extreme ultraviolet (BUY), and far-ultraviolet (FUV) multilayer coated telescopes for the study of the solar chromosphere, corona, and corona/solar wind interface. Because these systems operate at short wavelengths (-40 A <2< 1550 A), the modest apertures of4O mm - 127 mm allow observations at very high angular resolution (0. 1 - 0.7 arc second). In addition to permitting traditional normal incidence optical configurations (such as Cassegrain, Ritchey-Chrétien, and Herschelian configurations) to be used at soft x-ray/EUV wavelengths, multilayer coatings also allow a narrow wavelength band (/& - 15 - 100) to be selected for imaging. The resulting telescopes provide a very powerful and flexible diagnostic instrument for the study of both the fine scale structure of the chromosphere/corona interface and the large scale structure of the corona and corona/solar wind interface. In previous papers we have described a new solar rocket payload, the Multi-Spectral Solar Telescope Array (MSSTA), which is composed of 17 of these compact telescopes. In the present paper, we report on the ability of the MSSTA payload to obtain temperature diagnostic information about the optically thin solar plasma. We also discuss applications of this information to studies of coronal structure.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Craig Edward DeForest, Craig Edward DeForest, Charles C. Kankelborg, Charles C. Kankelborg, Maxwell J. Allen, Maxwell J. Allen, Elizabeth S. Paris, Elizabeth S. Paris, Thomas D. Willis, Thomas D. Willis, Joakim F. Lindblom, Joakim F. Lindblom, Ray H. O'Neal, Ray H. O'Neal, Arthur B. C. Walker, Arthur B. C. Walker, Troy W. Barbee, Troy W. Barbee, Richard B. Hoover, Richard B. Hoover, Efim S. Gluskin, Efim S. Gluskin, "Performance of the Multi-Spectral Solar Telescope Array V: temperature diagnostic response to the optically thin solar plasma", Proc. SPIE 1343, X-Ray/EUV Optics for Astronomy, Microscopy, Polarimetry, and Projection Lithography, (1 February 1991); doi: 10.1117/12.23210; https://doi.org/10.1117/12.23210


The Stanford/Msfc Multi-Spectral Solar Telescope Array
Proceedings of SPIE (July 27 1989)
MAGRITTE optomechanical design and mirror manufacturing
Proceedings of SPIE (February 17 2004)
Active sun telescope array
Proceedings of SPIE (January 31 1991)

Back to Top