Ambastha, Ashok ; Antia, H. M. (2004) Variations in low-l solar P-modes with flare activity Proceedings of the SOHO 14 / GONG 2004 Workshop on Helio- and Asteroseismology: Towards a Golden Future . pp. 289-292.
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Official URL: http://articles.adsabs.harvard.edu/cgi-bin/nph-iar...
Abstract
We have studied the temporal variation of power in low-l modes and compared it with solar disk integrated flareindex. GONG power spectrum data for the period of May 1995-December 2001 has been used. Variations in the running mean mode power corresponding to l=0 modes with different radial orders (n = 16,17,...,28) are found to be generally stochastic in nature. A comparison of the temporally varying p-mode power with the disk-integrated flare-index does not show any unambiguous correlations.
Item Type: | Article |
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Source: | Copyright of this article belongs to European Space Agency. |
Keywords: | Sun: Activity; Sun: Oscillations |
ID Code: | 75678 |
Deposited On: | 24 Dec 2011 15:10 |
Last Modified: | 18 May 2016 19:37 |
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