Astronomical nacelle stabilized by means of an ultraviolet detector with a photomultiplier

Details Astronomical nacelle stabilized by means of an ultraviolet detector with a photomultiplier Astronomical nacelle stabilized by means of an ultraviolet detector with a photomultiplier

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978esasp.135..403h&link_type=abstract

In ESA European Sounding Rocket, Balloon and Related Res., with Emphasis on Expt. at High Latitudes p 403-406 (SEE N79-31637 2

Computer Science

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7

Balloon-Borne Instruments, Gondolas, Instrument Packages, Telescopes, Ultraviolet Radiation, Celestial Bodies, Galaxies, High Altitude Balloons, Photomultiplier Tubes

Scientific paper

A polyvalent nacelle developed during an international cooperation program is described. The structural characteristics, primary stabilization are discussed. The Schmidt Cassegrain anastigmatic flat field (SCAP) ultraviolet optical system is analyzed in detail. A description of current scientific programs includes research on weak blue stars, ultraviolet spectrometry of galaxy centers, and detection of H2 galactic regions at 1900 A.

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