A normal incidence high resolution X-ray telescope for solar coronal observations

Details A normal incidence high resolution X-ray telescope for solar coronal observations A normal incidence high resolution X-ray telescope for solar coronal observations

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sao..repts....g&link_type=abstract

Semiannual Progress Report, 1 Feb. - 31 Jul. 1987 Smithsonian Astrophysical Observatory, Cambridge, MA.

Computer Science

Performance

Performance Tests, Postflight Analysis, Solar Corona, X Ray Telescopes, H Alpha Line, High Resolution, Mirrors, Moments Of Inertia, Reflectance

Scientific paper

The preflight preparation of the multilayer mirror fabrication and testing, integration and testing, and WSMR activities are described. Post-flight analysis shows that all payload systems and subsystems performed well within acceptable limits, with the sole exception of the light-blocking prefilters. Suggested corrective actions were discussed. Refurbishment and reflight are then described.

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