Paper
25 November 1996 Japanese sounding rocket experiment with the solar XUV Doppler telescope
Taro Sakao, Saku Tsuneta, Hirohisa Hara, Ryouhei Kano, Tsuyoshi Yoshida, Shin'ichi Nagata, Toshifumi Shimizu, Takeo Kosugi, Katsuhiko Murakami, Wakuna Wasa, Masao Inoue, Katsuhiro Miura, Koji Taguchi, Kazuo Tanimoto
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Abstract
We present an overview of an ongoing Japanese sounding rocket project with the Solar XUV Doppler telescope. The telescope employs a pair of normal incidence multilayer mirrors and a back-thinned CCD, and is designed to observe coronal velocity field of the whole sun by measuring line- of-sight Doppler shifts of the Fe XIV 211 angstroms line. The velocity detection limit is estimated to be better than 100 km/s. The telescope will be launched by the Institute of Space and Astronautical Science in 1998, when the solar activity is going to be increasing towards the cycle 23 activity maximum. Together with the overview of the telescope, the current status of the development of each telescope components including multilayer mirrors, telescope structure, image stabilization mechanism, and focal plane assembly, are reviewed. The observation sequence during the flight is also briefly described.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Taro Sakao, Saku Tsuneta, Hirohisa Hara, Ryouhei Kano, Tsuyoshi Yoshida, Shin'ichi Nagata, Toshifumi Shimizu, Takeo Kosugi, Katsuhiko Murakami, Wakuna Wasa, Masao Inoue, Katsuhiro Miura, Koji Taguchi, and Kazuo Tanimoto "Japanese sounding rocket experiment with the solar XUV Doppler telescope", Proc. SPIE 2804, Missions to the Sun, (25 November 1996); https://doi.org/10.1117/12.259721
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Cited by 5 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Space telescopes

Extreme ultraviolet

Rockets

Charge-coupled devices

Multilayers

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