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- W1595897162 abstract "We review this topic with sections on the theory of interior nuclear fusion energy generation in the Sun, the role of surface magnetism including the origin of active regions and the 11-year solar cycle, the measured total solar irradiance in watts-m − 2 , the solar wind, coronal mass ejections, and the minute effects of orbital modulation. We briefly summarize the evolution of the luminous output of the Sun during its pre-main sequence phase when the solar system was young. Finally, we review recent findings concerning the behavior of the solar cycle as inferred from the variations in the production rates of certain radioisotopes that are sensitive to solar activity. We conclude with an examination of the Sun in a stellar context, specifically, how solar magnetic activity and variations in its luminous output in the visible band of the electromagnetic spectrum compare to that of other solar-type stars." @default.
- W1595897162 created "2016-06-24" @default.
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- W1595897162 date "2015-01-01" @default.
- W1595897162 modified "2023-09-24" @default.
- W1595897162 title "Energy from the Sun☆" @default.
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- W1595897162 doi "https://doi.org/10.1016/b978-0-12-409548-9.09510-5" @default.
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