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Markus J. Aschwanden   Submitted: 2008-09-02 14:16

Coronal loops that exhibit kink-mode oscillations have generally been assumed to have a constant density and temperature during the observed time interval. Analyzing their intensities in an EUV waveband, however, clearly shows that their brightness varies in a way that is consistent with a temperature cooling through the EUV passband, which limits their detection time, observed damping time, and number of observable periods. We study kink-mode oscillations of eight loops observed during the so-called ``harmonica event'' on 2001-Apr-15, 21:58-22:27 UT in 171 ang . We find loop densities of n_e=1.4pm0.6 imes 109 cm-3, loop widths of w=2.0pm2.6 Mm, and e-folding cooling times of aucool=17pm7 min, when they cool through the peak temperature T=0.95 MK of the 171 ang band. We conclude that oscillations of a single loop can not be detected longer than 10-20 min in one single filter and appropriate light curve modeling is necessary to disentangle the subsequent oscillation phases of multiple near-cospatial loops.

Authors: Markus J. Aschwanden and Jaume Terradas
Projects: TRACE

Publication Status: ApJ Lett. (accepted, Sept 1, 2008; in press)
Last Modified: 2008-09-03 07:49
Go to main E-Print page  Modeling and Observations of Photospheric Magnetic Helicity  The Effect of Radiative Cooling on Coronal Loop Oscillations  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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