Damping of coronal loop oscillations by resonant absorption of quasi-mode kink oscillations

Details Damping of coronal loop oscillations by resonant absorption of quasi-mode kink oscillations Damping of coronal loop oscillations by resonant absorption of quasi-mode kink oscillations

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..629g&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Solar Coronal Loops: Oscillations

Scientific paper

Damped quasi-mode kink oscillations in cylindrical flux tubes are capable of explaining the observed rapid damping of the coronal loop oscillations when the ratio of the inhomogneity length scale to the radius of the loop is allowed to vary from loop to loop. They do not need to invoke anomalously low Reynolds numbers. The theoretical expressions for the decay time by Hollweg & Yang (1988) and Ruderman & Roberts (2002) are used to estimate the ratio of the length scale of inhomogneity compared to the loop radius for a collection of loop oscillations.

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