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- W2077288081 abstract "The solar‐like spectrophotometric variations due to nonradial oscillations were simulated using a series of synthetic spectra computed and interpolated from stellar model atmospheres, each in complete equilibrium but at varying effective temperatures. The simulations are in good agreement with observations of the Sun done by others. We have demonstrated how the p‐mode signal is distributed as a function of wavelength between 350 and 1000 nm and more specifically how most of the signal is concentrated at shorter wavelengths. We attribute this to the high density of spectral lines at shorter wavelengths, as well as the tendency of the majority of the lines to weaken with increasing effective temperature. Our simulations are also in agreement with the observational studies that report that stronger lines show larger relative variations. We also reproduce the observed exceptions to this trend for lines such as Balmer lines and Ca ii H and K." @default.
- W2077288081 created "2016-06-24" @default.
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- W2077288081 date "2002-03-01" @default.
- W2077288081 modified "2023-09-25" @default.
- W2077288081 title "Simulating Spectrophotometric Fluctuations of<i>p</i>‐Mode Oscillations in Solar‐like Stars" @default.
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- W2077288081 doi "https://doi.org/10.1086/339256" @default.
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