Abstract
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented. The reliability of this technique was tested with TRACE 171 Å observations. The application of this technique to a flare-induced kink-mode oscillation, revealed a 3500 km spatial periodicity which occur along the loop edge. We establish a reduction in oscillatory power, for these spatial periodicities, of 45% over a 322 s interval. We relate the reduction in oscillatory power to the physical damping of these loop-top oscillations.
| Original language | English |
|---|---|
| Pages (from-to) | 288-295 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 3 |
| Issue number | s247 |
| DOIs | |
| Publication status | Published - 2007 |
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