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- W1840989508 abstract "Excitation of solar oscillations is attribued to turbulent motions in the solar convective zone. It is also currently believed that oscillations of low massive stars (M <2 Mo) - which possess an upper convective zone - are stochastically excited by turbulent convection in their outer layers. A recent theoretical work (Samadi & Goupil, 2001 ; Samadi et al, 2001) supplements and reinforces this theory. This allows the use of any available model of turbulence and emphasizes some recent unsolved problems which are brought up by these new theoretical developments." @default.
- W1840989508 created "2016-06-24" @default.
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- W1840989508 date "2001-08-22" @default.
- W1840989508 modified "2023-09-27" @default.
- W1840989508 title "Stochastic excitation of stellar oscillations" @default.
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- W1840989508 hasPublicationYear "2001" @default.
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