XUV Doppler telescope with multilayer optics

Hirohisa Hara; Ryouhei Kano; Shin'ichi Nagata; Taro Sakao; Toshifumi Shimizu; Saku Tsuneta; Tsuyoshi Yoshida; Takeo Kosugi

doi:10.1117/12.278872

11 July 1997 XUV Doppler telescope with multilayer optics

Hirohisa Hara, Ryouhei Kano, Shin'ichi Nagata, Taro Sakao, Toshifumi Shimizu, Saku Tsuneta, Tsuyoshi Yoshida, Takeo Kosugi

Author Affiliations +

Proceedings Volume 3113, Grazing Incidence and Multilayer X-Ray Optical Systems; (1997) https://doi.org/10.1117/12.278872
Event: Optical Science, Engineering and Instrumentation '97, 1997, San Diego, CA, United States

Abstract

We present an overview of a sounding-rocket experiment that is scheduled to be launched by the Institute of Space and Astronautical Science (ISAS) in January 1998, the rising phase of the 11-year activity cycle of the sun. The purpose of this experiment is (1) to obtain whole-sun images taken in an XUV emission line, Fe XIV 211 A, using the normal incidence multilayer optics with a high spectral resolution of about 40, and (2) to carry out the velocity-field measurement with a detection limit as high as 100 km/s.

Citation Download Citation

Hirohisa Hara, Ryouhei Kano, Shin'ichi Nagata, Taro Sakao, Toshifumi Shimizu, Saku Tsuneta, Tsuyoshi Yoshida, and Takeo Kosugi "XUV Doppler telescope with multilayer optics", Proc. SPIE 3113, Grazing Incidence and Multilayer X-Ray Optical Systems, (11 July 1997); https://doi.org/10.1117/12.278872

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