Inferred acoustic rates of solar p modes from several helioseismic instruments
Acoustic rates of excitation of solar p modes can be estimated from observations in order to place constraints on the modelling of the excitation process and the layers where it occurs in the star. For several reasons (including a poor signal to noise ratio and mode overlap), this estimation is diff...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2005-04, Vol.433 (1), p.349-356 |
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Sprache: | eng |
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