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Variation of the Solar He I 10830 A Line: 1977 - 1980Daily measurements of the equivalent width of the 10830 A He I line integrated over the visible disk show: (1) an increase from about 32 to about 74 mA in the monthly mean values from the minimum to the maximum of the current solar cycle; (2) the monthly mean values are more smoothly varying than most other indices of solar activity; (3) rotation modulates the daily values in a highly variable manner with amplitudes as large as plus or minus 20%; (4) the apparent synodic rotation period is 29 days rather than the expected 27 days associated with active regions; (5) despite great differences in the appearance of the sun in 3933 A Ca I and 10830 A He I, the central intensity of the former correlates with the equivalent width of the latter with a value r = 0.97.
Document ID
19820009166
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Harvey, J. W.
(Kitt Peak National Observatory Tucson, AZ, United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1981
Publication Information
Publication: NASA. Goddard Space Flight Center Variations of the Solar Constant
Subject Category
Solar Physics
Accession Number
82N17040
Distribution Limits
Public
Copyright
Public Use Permitted.
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