Are the shapes of the p-mode peaks `distorted' by the solar cycle when they are observed in long, multi-year power frequency spectra?

Details Are the shapes of the p-mode peaks `distorted' by the solar cycle when they are observed in long, multi-year power frequency spectra? Are the shapes of the p-mode peaks `distorted' by the solar cycle when they are observed in long, multi-year power frequency spectra?

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp.624e..91c&link_type=gif

Proceedings of SOHO 18/GONG 2006/HELAS I, Beyond the spherical Sun (ESA SP-624). 7-11 August 2006, Sheffield, UK. Editor: Karen

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