The Ultra High Resolution XUV Spectroheliograph. III - A modified configuration for a free flying platform

Details The Ultra High Resolution XUV Spectroheliograph. III - A modified configuration for a free flying platform The Ultra High Resolution XUV Spectroheliograph. III - A modified configuration for a free flying platform

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1546..265w&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

Physics

Far Ultraviolet Radiation, Flying Platforms, Solar Physics, Spectroheliographs, Extreme Ultraviolet Radiation, High Resolution, Solar X-Rays

Scientific paper

The Ultra-High Resolution XUV Spectroheliograph (UHRXS) is a comprehensive solar observatory capable of studying solar phenomena at soft X-ray, XUV, EUV, and VUV wavelengths with normal incidence imaging multilayer telescopes capable of very high angular resolution (about 0.1 arcsec), and spectrographs able to achieve high spectral resolution. This instrument has been selected by NASA for flight as an attached payload on the Space Station Freedom. Recent developments have made it clear that accommodations for attached payloads on Freedom will not become available during the initial operations of Freedom and may never be available. We have studied the changes that must be made to place the UHRXS instrument on a Free Flying Platform such as the Delta Launched Explorer Bus. We report on the configuration, performance, and accommodation on a free flying platform of the revised UHRXS concept.

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