The Solar/Stellar Coronal Explorer and the Solar/Stellar Coronal Observatory

Details The Solar/Stellar Coronal Explorer and the Solar/Stellar Coronal Observatory The Solar/Stellar Coronal Explorer and the Solar/Stellar Coronal Observatory

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1546..281w&link_type=abstract

In: Multilayer and grazing incidence X-ray/EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991 (A93-39658 15

Astronomy and Astrophysics

Astronomy

Astronomical Observatories, Cool Stars, Solar Corona, Solar Observatories, Spaceborne Astronomy, Stellar Coronas, Angular Velocity, Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, Stellar Rotation, Surface Temperature

Scientific paper

The Solar/Stellar Coronal Explorer (SSCE) carries six identical Ritchey-Chretien Telescopes of 127 mm aperture each; their images will be recorded by multianode microchannel-array detectors. The mirrors of five of the telescopes are coated with multilayer reflecting structures that select narrow XUV wavelength bands corresponding to strong emission lines emitted by solar or stellar coronal plasmas. Also noted here is a larger explorer mission concept, that of the Solar/Stellar Coronal Observatory, which will undertake more extensive spectroscopic observations.

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