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- W1996572743 abstract "Context. The long and almost continuous observations by Kepler show clear evidence of a granulation background signal in a large sample of stars, which is interpreted as the surface manifestation of convection. It has been shown that its characteristic timescale and rms intensity fluctuation scale with the peak frequency (νmax) of the solar-like oscillations. Various attempts have been made to quantify the observed signal, to determine scaling relations for its characteristic parameters, and to compare them to theoretical predictions. Even though they are consistent on a global scale, large systematic differences of an unknown origin remain between different methods, as well as between the observations and simulations." @default.
- W1996572743 created "2016-06-24" @default.
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- W1996572743 date "2014-10-01" @default.
- W1996572743 modified "2023-10-15" @default.
- W1996572743 title "The connection between stellar granulation and oscillation as seen by the<i>Kepler</i>mission" @default.
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- W1996572743 doi "https://doi.org/10.1051/0004-6361/201424313" @default.
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