Ambastha, Ashok ; Antia, H. M. (2006) Possibility of excitation of low-l p-modes by energetic solar transients Solar Physics, 238 (2). pp. 219-230. ISSN 0038-0938
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Official URL: http://www.springerlink.com/content/x05684p1150k31...
Related URL: http://dx.doi.org/10.1007/s11207-006-0234-y
Abstract
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.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer-Verlag. |
| ID Code: | 12236 |
| Deposited On: | 10 Nov 2010 04:56 |
| Last Modified: | 12 May 2011 09:52 |
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