The Ultra High Resolution XUV Spectroheliograph

Details The Ultra High Resolution XUV Spectroheliograph The Ultra High Resolution XUV Spectroheliograph

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990opten..29..698w&link_type=abstract

Optical Engineering (ISSN 0091-3286), vol. 29, July 1990, p. 698-710.

Other

4

Image Analysis, Solar Atmosphere, Solar Corona, Spectroheliographs, X Ray Telescopes, Extreme Ultraviolet Radiation, Solar Flares, Solar Observatories, Solar Spectrometers, Solar Wind, Space Station Freedom

Scientific paper

The Ultra High Resolution XUV Spectroheliograph (UHRXS), a solar observatory planned for the Space Station Freedom, is described. The UHRXR instruments include nine XUV Ritchey-Chretien telescopes covering a spectral range of 70-350 A, which will provide images of solar atmosphere structures ranging in temperature from 50,000 to 20,000,000 K. The images will be obtained with spatial resolution that is an order of magnitude better than any other currently planned solar satellite experiment.

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