Physics
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508...33c&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
Physics
Solar Cycles, Solar Activity
Scientific paper
The rate of supply of energy to the low-degree p modes of the Sun is investigated using both long and short time-duration Fourier transforms. We see that, although on average the energy supply rate to the modes is independent of solar activity, there is a period of high solar activity where the energy-supply rate is increased. Furthermore we see that the correlations between the mode line width and the power in the modes are different on the falling phase of cycle 22 and the rising phase of cycle 23 with a strong correlation between the energy supply rate and the mode power on the rising phase of cycle 23.
Chaplin William J.
Elsworth Yvonne
Isaak George R.
New Roger
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