Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points

J. Reid, C. E. Parnell, A. W. Hood, P. K. Browning

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)
18 Downloads (Pure)

Abstract

The squashing factor of a magnetic field, Q, is commonly used as an indicator of magnetic reconnection, but few studies seek to evaluate how reliable it is in comparison with other possible reconnection indicators. By using a full, self-consistent, three-dimensional, resistive magnetohydrodynamic experiment of interacting magnetic strands constituting a coronal loop, Q and several different quantities are determined. Each is then compared with the necessary and sufficient condition for reconnection, namely the integral along a field line of the component of the electric field parallel to the magnetic field. Among the reconnection indicators explored, we find the squashing factor less successful when compared with alternatives, such as Ohmic heating. In a reconnecting magnetic field devoid of null points, our work suggests that Q, being a geometric measure of the magnetic field, is not a reliable indicator of the onset or a diagnostic of the location of magnetic reconnection in some configurations.
Original languageEnglish
Article numberA92
Number of pages14
JournalAstronomy & Astrophysics
Volume633
DOIs
Publication statusPublished - 16 Jan 2020

Keywords

  • Sun: corona
  • Sun: magnetic fields
  • Magnetic reconnection
  • Magnetohydrodynamics (MHD)

Fingerprint

Dive into the research topics of 'Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points'. Together they form a unique fingerprint.

Cite this