Possibility of Excitation of Low-ℓ P-Modes by Energetic Solar Transients

Details Possibility of Excitation of Low-ℓ P-Modes by Energetic Solar Transients Possibility of Excitation of Low-ℓ P-Modes by Energetic Solar Transients

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..238..219a&link_type=abstract

Solar Physics, Volume 238, Issue 2, pp.219-230

Physics

6

Scientific paper

We examine the temporal variation of power in low-ℓ modes using GONG data for the period of May 1995 October 2005 and compare this with disk-integrated flare and CME indices. A poor correlation between the running means of Flare Index and mode power is found. A similar result is found for CME Index also. Variations in the running mean mode power corresponding to ℓ = 0 modes with different radial orders are generally stochastic in nature. This behaviour is also reflected in the distribution of mode power.

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