Discovery of Spatial Periodicities in a Coronal Loop Using Automated Edge-Tracking Algorithms
Abstract
A new method for automated coronal loop tracking, in both spatial and temporal domains, is presented. Applying this technique to TRACE data, obtained using the 171 Å filter on 1998 July 14, we detect a coronal loop undergoing a 270 s kink-mode oscillation, as previously found by Aschwanden et al. However, we also detect flare-induced, and previously unnoticed, spatial periodicities on a scale of 3500 km, which occur along the coronal loop edge. Furthermore, we establish a reduction in oscillatory power for these spatial periodicities of 45% over a 222 s interval. We relate the reduction in detected oscillatory power to the physical damping of these loop-top oscillations.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- June 2008
- DOI:
- 10.1086/587735
- arXiv:
- arXiv:0802.1971
- Bibcode:
- 2008ApJ...680.1523J
- Keywords:
-
- methods: data analysis;
- Sun: corona;
- Sun: evolution;
- Sun: oscillations;
- techniques: image processing;
- Astrophysics
- E-Print:
- 7 pages, 11 figures