The High Energy Astronomy Observatory - Mission B (HEAO-B) is a satellite observatory for the purpose of performing a detailed X-ray survey of the celestial sphere 'b'. Measurements will be made of stellar radiation in the range of 0.2 to 20 keV. The central part of the Observatory is an X-ray telescope, into the focus of which a variety of imaging instruments and spectrographs may be introduced. The telescope has a resolution of about 1 arc second, so that the instruments must be placed with extreme precision. This is obtained by a mechanical system of toggles and stops and a motor drive system controlled by a position sensing potentiometer with a resolution of about 1.5 deg.
Focal plane transport assembly controls for the high energy astronomy observatory x-ray telescope
Hochenergie-astronomisches Observatorium mit Roentgen-Teleskop
IEEE Transactions on Nuclear Science ; NS-26 , 1Pt.1 ; 536-541
1979
6 Seiten, 3 Bilder, 18 Quellen
Aufsatz (Zeitschrift)
Englisch
The high energy astronomy observatory x-ray telescope
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|Space infrared telescope facility (SIRTF) focal plane
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|HEAO-A - The first high energy astronomy observatory
AIAA | 1978
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