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


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2006-11-08

AUTHORS

Ashok Ambastha, H. M. Antia

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. More... »

PAGES

219-230

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s11207-006-0234-y

DOI

http://dx.doi.org/10.1007/s11207-006-0234-y

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1013570015


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