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Fig. 10.


Results of fitting power spectra constructed with sensitivities calculated including the effects of rotation, but using a model calculated assuming sensitivities ignoring the effects of rotation. Results are shown for the G2 star with no field, the 6173 Å line, and a rotation velocity of 6 km s−1. The ratio of the FWHM of the modes to the rotation rate is set to 1.0. The symbols show the results of fitting the spectrum of one l at a time. The solid blue line shows the results of fitting the spectra of all l with 0 ≤ l ≤ 3 together. In all cases a global search was performed to ensure that the global minimum has been found.

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