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Solar Maximum Mission experiment - Initial observations by the active cavity radiometerThe Active Cavity Radiometer on board the SMM is providing high-quality measurements of the solar irradiance. After correction for the solar distance, the orbital displacement of the satellite, and the relativistic shift of irradiance due to the satellite motion, the observed standard deviation is in the range 10-15 parts per million in a 96-minute integration. Measurable solar variations occur on time scales of a few minutes to a few days. The total amplitude of the variations in the daily averages from February 16 to March 31, 1980, was 0.10% based upon 96-minute averages.
Document ID
19810051980
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Willson, R. C.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Hudson, H. S.
(California, University La Jolla, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Subject Category
Solar Physics
Accession Number
81A36384
Funding Number(s)
CONTRACT_GRANT: NSG-5322
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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