Analysis of Aerobee 17.012 data

Details Analysis of Aerobee 17.012 data Analysis of Aerobee 17.012 data

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975lock.reptt....c&link_type=abstract

Final Report Lockheed Missiles and Space Co., Palo Alto, CA.

Computer Science

Sound

Aerobee Rocket Vehicle, Data Processing, Data Reduction, Ionospheric Sounding, Cosmic Rays, Galactic Clusters, Proportional Counters, Supernova Remnants, X Ray Sources

Scientific paper

The results are summarized of reduction and analysis of data acquired during the flight of NASA-Aerobee 17.012CG. This rocket was launched from White Sands Missile Range on 6 April 1974 at 0410 U.T. The primary instrument in the experiment payload was a singly focussing x-ray reflector system sensitive in the range from 0.18 to 3 keV. X-ray detectors for this system consisted of two gas flow proportional counters with fields of view defined by apertures of 0.1 deg and 0.3 deg at the reflector focus. A Bragg spectrometer utilizing KAP crystals was included in the payload with the objective of detecting the Lyman alpha line of 0 VIII at 18.97A in the Puppis supernova remanant. A 35 mm camera photographed the star field every 1.6 sec throughout the flight to provide aspect information.

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