English

Evolution of Filament Barbs

Solar and Stellar Astrophysics 2010-01-12 v1

Abstract

We present a selected few cases in which the sense of chirality of filament barbs changed within as short as hours. We investigate in detail a quiescent filament on 2003 September 10 and 11. Of its four barbs displaying such changes only one overlay a small polarity inversion line inside the EUV filament channel (EFC). No magnetic elements with magnitude above the noise level were detected at the endpoints of all barbs. In particular, a pair of barbs first approached toward and then departed from each other in H-alpha, with the barb endpoints migrating as far as ~10". We conclude that the evolution of the barbs was driven by flux emergence and cancellation of small bipolar units at the EFC border.

Cite

@article{arxiv.1001.1572,
  title  = {Evolution of Filament Barbs},
  author = {Rui Liu and Yan Xu and Haimin Wang},
  journal= {arXiv preprint arXiv:1001.1572},
  year   = {2010}
}

Comments

To appear in the Proceedings of the 25th NSO Workshop

R2 v1 2026-06-21T14:32:57.899Z