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Solar Irradiance Measurements: Minimum through Maximum Solar Activity

1991; IOP Publishing; Volume: 28; Issue: 3 Linguagem: Inglês

10.1088/0026-1394/28/3/032

1681-7575

R B Lee, Michael A. Gibson, Netra D. Shivakumar, Robert S. Wilson, H. Lee Kyle, Ann T. Mecherikunnel,

Solar Radiation and Photovoltaics

The 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% 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 Wm-2 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%, respectively.