MultiSpectral Solar Telescope Array VII: a status report

Details MultiSpectral Solar Telescope Array VII: a status report MultiSpectral Solar Telescope Array VII: a status report

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2011..489w&link_type=abstract

Proc. SPIE Vol. 2011, p. 489-503, Multilayer and Grazing Incidence X-Ray/EUV Optics II, Richard B. Hoover; Arthur B. Walker; Eds

Physics

Optics

Scientific paper

The Multi Spectral Solar Telescope ARray (MSSTA) is a rocket borne solar observatory that utilizes an array of multilayer coated telescopes to observe the solar atmosphere from the chromosphere to the corona, over a broad spectral range (VUV--soft X-rays). The instrumentation of the MSSTA is continuously evolved to incorporate new instrument concepts, and to improve its ability to investigate specific topics related to the structure and dynamics of the solar atmosphere.

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