A systems approach to mechanisms for a white light coronagraph X-ray XUV telescope

Details A systems approach to mechanisms for a white light coronagraph X-ray XUV telescope A systems approach to mechanisms for a white light coronagraph X-ray XUV telescope

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aeme.symp...77m&link_type=abstract

In NASA. Marshall Space Flight Center The 15th Aerospace Mech. Symp. p 77-90 (SEE N81-22388 13-39)

Computer Science

Coronagraphs, Spacecraft Instruments, Ulysses Mission, X Ray Telescopes, Extreme Ultraviolet Radiation, Solar Atmosphere, Solar Observatories

Scientific paper

A combined instrument package containing nine mechanisms was designed and developed for the international solar polar mission (ISPM). This complement of instruments, commonly called the CXX, is the only imaging system on either the NASA or ESA spacecraft and consists of a white light coronagraph mounted parallel to a combined X-ray and extreme ultra-violet (XUV) telescope. Requirements for and implementation of mechanisms in the CXX instrument are discussed.

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