1992
DOI: 10.1017/s0033822200013710
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On a Plausible Physical Mechanism Linking the Maunder Minimum to the Little Ice Age

Abstract: To understand better the Earth's climate, we need to know precisely how much radiation the Sun generates. We present here a simple physical mechanism describing the convective processes at the time of low sunspot activity. According to this model, the kinetic energy increased during the Maunder Minimum, causing a decrease of the solar radiation that was sufficient to produce a little Ice Age.

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Cited by 17 publications
(1 citation statement)
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“…Extrapolating back to the Maunder minimum, when the Sun's open magnetic flux was almost zero [ Solanki et al , 2000] we obtain approximately 2.5 Wm −2 . Based on different arguments other authors have proposed a much larger increase (4–5 Wm −2 by Hoyt and Schatten [1993]; 6.8 Wm −2 by Nesmes‐Ribes and Manganey [1992]).…”
Section: Total Solar Irradiancementioning
confidence: 99%
“…Extrapolating back to the Maunder minimum, when the Sun's open magnetic flux was almost zero [ Solanki et al , 2000] we obtain approximately 2.5 Wm −2 . Based on different arguments other authors have proposed a much larger increase (4–5 Wm −2 by Hoyt and Schatten [1993]; 6.8 Wm −2 by Nesmes‐Ribes and Manganey [1992]).…”
Section: Total Solar Irradiancementioning
confidence: 99%