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Elongation of Flare Ribbons View all abstracts by submitter

Jiong Qiu   Submitted: 2017-07-08 12:59

We present an analysis of the apparent elongation motion of flare ribbons along the polarity inversion line (PIL), as well as the shear of flare loops in several two-ribbon flares. Flare ribbons and loops spread along the PIL at a speed ranging from a few to a hundred km s-1. The shear measured from conjugate footpoints is consistent with the measurement from flare loops, and both show the decrease of shear toward a potential field as a flare evolves and ribbons and loops spread along the PIL. Flares exhibiting fast bidirectional elongation appear to have a strong shear, which may indicate a large magnetic guide field relative to the reconnection field in the coronal current sheet. We discuss how the analysis of ribbon motion could help infer properties in the corona where reconnection takes place.

Authors: Qiu, J., Longcope, D. W., Cassak, P. A., Priest, E. R.
Projects: None

Publication Status: The Astrophysical Journal, Volume 838, Issue 1, article id. 17, 17 pp. (2017)
Last Modified: 2017-07-11 11:23
Go to main E-Print page  Gradual Solar Coronal Dimming and Evolution of Coronal Mass Ejection in the Early Phase  The eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection  Edit Entry  Download Preprint  Delete Entry 

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