XUV Doppler telescope with multilayer optics

Details XUV Doppler telescope with multilayer optics XUV Doppler telescope with multilayer optics

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spie.3113..420h&link_type=abstract

Conference Paper, SPIE Proceedings, Vol. 3113, p. 420-429.

Physics

Optics

2

X Ray Telescopes, Far Ultraviolet Radiation, Solar Activity, X Ray Optics, Solar Spectra, Emission Spectra, Doppler Effect, Line Spectra, Spectral Resolution, Velocity Distribution

Scientific paper

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.

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