Rotational splitting of low L solar p-mode

Details Rotational splitting of low L solar p-mode Rotational splitting of low L solar p-mode

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..125p&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 125-130 (SEE N89-25819 19-92)

Physics

5

P Waves, Power Spectra, Solar Oscillations, Solar Rotation, Spectrum Analysis, Cross Correlation, Data Reduction, Solar Physics

Scientific paper

Rotational splitting measurements of less than 5 p-modes are calculated using different sources of data. For l=1, 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 l=2 splitting. For l between 2 and 5, only 1 month of data is available and superposition of peak structures gives an upper limit for their splitting.

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