Continuous Transition from Fast Magnetic Reconnection to Slow Reconnection and Change of the Reconnection System Structure

  • Nitta S
12Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.

Abstract

This paper analytically investigates a series of two-dimensional MHD reconnection solutions over a wide variation of magnetic Reynolds number ($R_{em}^*$). A new series of solutions explains a continuous transition from Petschek-like fast regime to a Sweet-Parker-like slow regime. The inflow region is obtained from a Grad-Shafranov analysis used by Nitta et al. 2002 and the outflow region from a shock-tube approximation used by Nitta 2004, 2006. A single X-point (Petschek-like) solution forms for a sufficiently small $R_{em}^*$. As $R_{em}^*$ gradually increases, the solutions shifts to an X-O-X solution with a magnetic island between two X-points. When $R_{em}^*$ increases further, the island collapses to a new elongated current sheet with Y-points at both ends (Sweet-Parker-like). These reconnection structures expand self-similarly as time proceeds. As $R_{em}^*$ increases, the reconnection rate and the reducible fraction of the initial magnetic energy of the system decrease as power-law functions of $R_{em}^*$.

Cite

CITATION STYLE

APA

Nitta, S. (2007). Continuous Transition from Fast Magnetic Reconnection to Slow Reconnection and Change of the Reconnection System Structure. The Astrophysical Journal, 663(1), 610–624. https://doi.org/10.1086/518104

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free