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Observations of Solar Irradiance Variability

Willson, R. C., Gulkis, S., Janssen, M., Hudson, H. S., Chapman, G. A.·1981·Science

Abstract

High-precision measurements of total solar irradiance, made by the active cavity radiometer irradiance monitor on the Solar Maximum Mission satellite, show the irradiance to have been variable throughout the first 153 days of observations. The corrected data resolve orbit-to-orbit variations with uncertainties as small as 0.001 percent. Irradiance fluctuations are typical of a band-limited noise spectrum with high-frequency cutoff near 0.15 day –1 ; their amplitudes about the mean value of 1368.31 watts per square meter approach ± 0.05 percent. Two large decreases in irradiance of up to 0.2 percent lasting about 1 week are highly correlated with the development of sunspot groups. The magnitude and time scale of the irradiance variability suggest that considerable energy storage occurs within the convection zone in solar active regions.

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Metadata

Authors
Willson, R. C., Gulkis, S., Janssen, M., Hudson, H. S., & Chapman, G. A.
Venue
Science
Published
1981-02-13
Volume
211
Issue
4483
Pages
700-702
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2018635133
Cited by
407
References
0
FWCI
50.80
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Observations of Solar Irradiance Variability. https://app.cochat.ai/papers/10.1126/science.211.4483.700
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Willson, R. C., Gulkis, S., Janssen, M., Hudson, H. S., & Chapman, G. A. (1981). Observations of Solar Irradiance Variability. Science. https://doi.org/10.1126/science.211.4483.700

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.