Physics
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..119c&link_type=abstract
In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,
Physics
3
Sun: Activity, Sun: Oscillations
Scientific paper
The line-width, velocity power and rate of supply of energy to the low-degree p modes of the Sun are investigated over falling phase of cycle 22 and the rising phase of cycle 23 by fitting in the Fourier transform domain. We see that for the first time for low-degree modes we are able to parameterise the solar activity dependence as a function of the angular degree of the mode.
Chaplin William J.
Elsworth Yvonne
Isaak George R.
New Roger
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