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- W2904845810 abstract "Abstract This chapter describes several aspects of stars that inform us about the Sun, especially characteristics that might have changed significantly on our star's journey to its present evolutionary state. The focus is on stellar “chromospheres,” an important byproduct of magnetic “activity,” because this is a key area in solar physics today and one in which the stars can be most informative. The main topic is why chromospheres exist: the warm, extensive outer atmospheres of cool stars, a consequence of nonradiative heating mainly devolving from magnetic effects. Ancillary topics consider two different aspects of the underlying magnetic activity: the rotation–age–activity connection, primary signature of magnetic evolution over time; and activity cycles, outward manifestations of an enigmatic, poorly understood, and perhaps equally poorly synchronized magnetic clock deep in the stellar interior." @default.
- W2904845810 created "2018-12-22" @default.
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- W2904845810 date "2019-01-01" @default.
- W2904845810 modified "2023-09-24" @default.
- W2904845810 title "Stellar and Solar Chromospheres and Attendant Phenomena" @default.
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- W2904845810 doi "https://doi.org/10.1016/b978-0-12-814334-6.00002-9" @default.
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