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- W2081718277 abstract "Abstract The optical behavior of active chromosphere stars is reviewed, with particular reference to determination of the parameters (size, temperature, location, magnetic field strength) that characterize a stellar active region. Three areas of ground-based observational technique are highlighted for their contributions and future promise. Doppler Imaging, the reconstruction of the surface brightness distributions of spotted stars by analysis of distortions in spectral line profiles, promises to yield information on location and time evolution of active regions. Magnetic field measurements, especially those utilizing infrared FTS data, will in the future provide complementary data that will permit investigations of the field evolution of spots. Lastly, asteroseismology, utilizing either very high precision radial velocity or intensity measures, will provide input on internal structures of stars. Since parameters such as stellar convection zone depth are crucial input information for modeling the stellar dynamo, asteroseismology will aid the refinement of theoretical models of stellar activity." @default.
- W2081718277 created "2016-06-24" @default.
- W2081718277 creator A5026305817 @default.
- W2081718277 date "1987-01-01" @default.
- W2081718277 modified "2023-10-16" @default.
- W2081718277 title "The unknown, remembered gate: Present and future observations of active chromosphere stars" @default.
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- W2081718277 doi "https://doi.org/10.1016/0083-6656(87)90020-1" @default.
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