Distortion of the p-mode peak profiles by the solar-cycle frequency shifts: do we need to worry?

Monthly Notices of the Royal Astronomical Society(2008)

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Abstract
We seek to address whether solar-cycle frequency shifts of the Sun's low-l p modes ‘distort’ the underlying shapes of the mode peaks, when those peaks are observed in power frequency spectra made from data spanning large fractions, or more, of the cycle period. We present analytical descriptions of the expected profiles, and validate the predictions through use of artificial seismic time-series da...
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methods: data analysis,methods: statistical,Sun: helioseismology
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