The solar cycle dependence of low-degree p-mode parameters

Details The solar cycle dependence of low-degree p-mode parameters The solar cycle dependence of low-degree p-mode parameters

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..103t&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

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Solar Oscillations

Scientific paper

Thanks to the extension of the SOHO mission it is possible to analyze with a good accuracy the dependence of the low-degree p-mode parameters on the solar cycle. We have constructed from the LOI-proxy data (MDI) two time series of 784 days each, one taken at low activity and the other one at high activity. We have focused on analyzing the solar-cycle dependence of the linewidth, the splitting, the asymmetry and the frequency shift of the low-degree p modes. It turns out that some of these parameters exhibit a significant dependence on solar cycle moreover there is also a dependence on m the azimuthal order.

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