Additive self-helicity as a kink mode threshold

Research output: Contribution to journalArticlepeer-review

13 Scopus citations

Abstract

In this paper, we propose that additive self-helicity, introduced by Longcope and Malanushenko, plays a role in the kink instability for complex equilibria, similar to twist helicity for thin flux tubes. We support this hypothesis by a calculation of additive self-helicity of a twisted flux tube from the simulation of Fan and Gibson. As more twist gets introduced, the additive self-helicity increases, and the kink instability of the tube coincides with the drop of additive self-helicity, after the latter reaches the value of HA2 1.5 (where Φ is the flux of the tube and HA is the additive self-helicity). We compare the additive self-helicity to twist for a thin subportion of the tube to illustrate that HA2 is equal to the twist number, studied by Berger and Field, when the thin flux tube approximation is applicable. We suggest that the quantity HA2 could be treated as a generalization of a twist number, when the thin flux tube approximation is not applicable. A threshold on a generalized twist number might prove extremely useful studying complex equilibria, just as the twist number itself has proven useful studying idealized thin flux tubes. We explicitly describe a numerical method for calculating additive self-helicity, which includes an algorithm for identifying a domain occupied by a flux bundle and a method of calculating potential magnetic field confined to this domain. We also describe a numerical method to calculate twist of a thin flux tube, using a frame parallelly transported along the axis of the tube.

Original languageEnglish
Pages (from-to)580-592
Number of pages13
JournalAstrophysical Journal
Volume702
Issue number1
DOIs
StatePublished - 2009

Keywords

  • Instabilities
  • Magnetic fields
  • Sun: corona
  • Sun: coronal mass ejections (CMEs)
  • Sun: flares
  • Sun: magnetic fields

Fingerprint

Dive into the research topics of 'Additive self-helicity as a kink mode threshold'. Together they form a unique fingerprint.

Cite this