A photograph of the FOXSI team in front of the FOXSI-2 sounding rocket on the launch pad.
The Focusing Optics X-ray Solar Imager, or FOXSI, is a sounding rocket payload built by UC Berkeley and led by Säm Krucker to test high energy grazing-incidence focusing optics paired with solid-state pixelated detectors to observe the Sun. FOXSI is composed of seven identical Wolter-I telescope modules, as well as Silicon and Cadmium Telluride strip detectors originally developed for the HXT telescope on the Japanese Hitomi mission. The FOXSI payload flew two times, most recently in 2014 and previously in 2012. Like most sounding rockets, FOXSI flew for approximately 15 minutes per mission and observed the Sun for about 5 minutes while in space. During its first flight, FOXSI successfully imaged a solar microflare in the hard x-ray band for the first time.
FOXSI's third mission, led by Lindsay Glesener of the University of Minnesota, had a successful launch on September 7, 2018 from White Sands, New Mexico. This iteration of the payload included a combination of Silicon and improved Cadmium Telluride detectors, as well as one CMOS soft x-ray detector. Two of the telescope modules were updated from 7-shell to 10-shell configurations, and the payload also introduced collimator technology to reduce the impact of singly-reflected rays.
A high resolution render of the FOXSI-2 payload.
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Fox, Karen (July 27, 2015). "A Next-Generation X-Ray Telescope Launches". NASA. Retrieved July 27, 2015.
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Buitrago-Casas, J. C.; Glesener, L.; Christe, S.; Ramsey, B.; Elsner, R.; Courtade, S.; Vievering, J.; Subramania, A.; Krucker, S.; Bale, S. (2017). "Methods for reducing singly reflected rays on the Wolter-I focusing mirrors of the FOXSI rocket experiment". Optics for EUV, X-Ray, and Gamma-Ray Astronomy VIII. Proceedings of SPIE. 10399. p. 103990J. Bibcode:2017SPD....4830504B. doi:10.1117/12.2274675. ISBN 9781510612556.