NASA NTRS · 19840052844
The inconstant solar constant
Abstract
The Active Cavity Radiometer Irradiance Monitor (ACRIM) of the Solar Maximum Mission satellite measures the radiant power emitted by the sun in the direction of the earth and has worked flawlessly since 1980. The main motivation for ACRIM's use to measure the solar constant is the determination of the extent to which this quantity's variations affect earth weather and climate. Data from the solar minimum of 1986-1987 is eagerly anticipated, with a view to the possible presence of a solar cycle variation in addition to that caused directly by sunspots.
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Willson, R. C., Hudson, H., Woodard, M.. 1984-06-01. The inconstant solar constant. https://ntrs.nasa.gov/citations/19840052844
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