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The Lockheed OSO-8 program. Task 2: Analysis of data from the high resolution ultraviolet spectrometer experimentThe 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.
Document ID
19810008447
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Bruner, E. C., Jr. (Lockheed Missiles and Space Co. Sunnyvale, CA, United States)
Date Acquired
September 4, 2013
Publication Date
September 30, 1980
Subject Category
Solar Physics
Report/Patent Number
NASA-CR-163918
LMSC-D766867
Accession Number
81N16966
Funding Number(s)
CONTRACT_GRANT: NAS5-22411
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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