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Palle, P.L.; Perez Hernandez, F.; Regulo, C.; Roca Cortes, T.
Seismology of the sun and sun-like stars1988
Seismology of the sun and sun-like stars1988
AbstractAbstract
[en] Rotational splitting measurements of p-modes are calculated using different sources of data. For data obtained from years 1981 to 1985 is used to find out the stretches where each particular mode remains excited, then its splitting is measured and the mean found. Cross-correlation of power spectra confirms these finding, and this method is used to look for the 1=2 splitting. For 2<1<5 only one month of data is available and superposition of peak structures gives an upper limit for their splitting
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European Space Agency, 75 - Paris (France); 691 p; Dec 1988; p. 125-130; Symposium on seismology of the sun and sun-like stars; Tenerife (Spain); 26-30 Sep 1988
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