The Lockheed OSO-8 program. Task 2: Analysis of data from the high resolution ultraviolet spectrometer experiment

Details The Lockheed OSO-8 program. Task 2: Analysis of data from the high resolution ultraviolet spectrometer experiment The Lockheed OSO-8 program. Task 2: Analysis of data from the high resolution ultraviolet spectrometer experiment

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980lock.rept.....b&link_type=abstract

Final Report, 19 Nov. 1977 - 31 Aug. 1980 Lockheed Missiles and Space Co., Sunnyvale, CA.

Computer Science

Carbon, Coronal Loops, Emission Spectra, Line Spectra, Silicon, Solar Flares, Oso-8, Spectroheliographs, Spectrum Analysis, Time Series Analysis, Ultraviolet Spectrometers

Scientific paper

The complete set of C 4 time sequences generated by the University of Colorado high resolution ultraviolet spectrometer experiment on OSO-8 were examined in a comprehensive and systematic fashion. As a result a new limit is placed on the acoustic flux passing through the transition zone of the Sun's atmosphere. It is found to be three orders of magnitude too small to heat the corona, and is consistent with zero. In collaborative efforts, the properties of transient C 4 brightenings were examined in considerable detail.

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