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Article Dans Une Revue Solar Physics Année : 2004

εBoo Inversion of simulated rotational profile

Résumé

The detection of solar oscillations on etaBoo is now established. We explore here what we can expect from the inversion of similar data by COROT to recover the rotational profile of the star. We show that the observation of a few low-l mixed modes in the excited high frequency range gives access to the rotational gradient if it is large enough.

Dates et versions

hal-03786291 , version 1 (23-09-2022)

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Jérémie Lochard, Davoud-Reza Samadi, Marie-José Goupil. εBoo Inversion of simulated rotational profile. Solar Physics, 2004, 220, pp.199-205. ⟨10.1023/B:SOLA.0000031376.55932.b6⟩. ⟨hal-03786291⟩
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