The Multi-Spectral Solar Telescope Array ( MSSTA) was a sounding rocket payload built by Arthur B. C. Walker Jr. at Stanford University in the 1990s to test ultraviolet imaging of the Sun using normal incidence EUV-reflective multilayer optics. MSSTA contained a large number of individual telescopes (> 10), all trained on the Sun and all sensitive to slightly different of ultraviolet light. Like all sounding rockets, MSSTA flew for approximately 14 minutes per mission, about 5 minutes of which were in space—just enough time to test a new technology or yield "first results" science. MSSTA is one of the last solar observing instruments to use photographic film rather than a digital camera system such as a CCD. MSSTA used film instead of a CCD in order to achieve the highest possible spatial resolution and to avoid the electronics difficulty presented by the large number of detectors that would have been required for its many telescopes.
MSSTA and its sister rocket, NIXT, were prototypes for normal incidence extreme ultraviolet imaging telescopes that are in use today, as well as the historic EIT instrument aboard the SOHO spacecraft, and the TRACE spacecraft. MSSTA flew three times: once in 1991 (NASA Sounding Rocket flight 36.049), once in 1994 (flight 36.091),
and once in 2002 (flight 36.194).
Several Stanford Ph.D. degrees in Physics resulted from the MSSTA program. These include those earned by Joakim Lindblom, Maxwell J. Allen, Ray H. O'Neal, Craig Edward DeForest, Charles C. Kankelborg, Hakeem Oluseyi, Dennis S. Martinez-Galarce, and Paul F.X. Boerner.
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