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Solar irradiance measurements - Minimum through maximum solar activityThe Earth Radiation Budget Satellite (ERBS) and the NOAA-9 spacecraft solar monitors were used to measure the total solar irradiance during the period October 1984 to December 1989. Decreasing trends in the irradiance measurements were observed as sunspot activity decreased to minimum levels in 1986; after 1986, increasing trends were observed as sunspot activity increased. The magnitude of the irradiance variability was found to be approximately 0.1 percent between sunspot minimum and maximum (late 1989). When compared with the 1984 to 1989 indices of solar magnetic activity, the irradiance trends appear to be in phase with the 11-year sunspot cycle. Both irradiance series yielded 1,365/sq Wm as the mean value of the solar irradiance, normalized to the mean earth/sun distance. The monitors are electrical substitution, active-cavity radiometers with estimated measurement precisions and accuracies of less than 0.02 and 0.2 percent, respectively.
Document ID
19920048926
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lee, R. B., III
(NASA Langley Research Center Hampton, VA, United States)
Gibson, M. A.
(NASA Langley Research Center Hampton, VA, United States)
Shivakumar, N.
(NASA Langley Research Center Hampton, VA, United States)
Wilson, R.
(ST Systems Corp. Hampton, VA, United States)
Kyle, H. L.
(NASA Langley Research Center Hampton, VA, United States)
Mecherikunnel, A. T.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Metrologia
Volume: 28
ISSN: 0026-1394
Subject Category
Solar Physics
Accession Number
92A31550
Distribution Limits
Public
Copyright
Other

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