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- W2023879986 abstract "We present a mathematical model that predicts the variation of illuminance during a solar eclipse, considering continuous effects of limb darkening. We assume that (1) the Sun and the Moon constitute perfect spheres, (2) the Moon crosses the Sun with a constant apparent velocity, and (3) sunspots, prominences, and coronae can be neglected. We compare predictions of this model with actual measurements made by M<TEX>$ddot{o}$</TEX>llmann & Vollmer (2006) during a total solar eclipse in Turkey, and with predictions of existing models. The new model is shown to describe the actual phenomenon more accurately than existing models." @default.
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- W2023879986 date "2012-10-31" @default.
- W2023879986 modified "2023-10-18" @default.
- W2023879986 title "ILLUMINANCE DURING A SOLAR ECLIPSE WITH LIMB DARKENING: A MATHEMATICAL MODEL" @default.
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- W2023879986 doi "https://doi.org/10.5303/jkas.2012.45.5.111" @default.
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