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NASA NTRS · 19930035243

Secondary instability in three-dimensional magnetic reconnection

Abstract

We consider the transition to turbulence in three-dimensional reconnection of a magnetic neutral sheet. We find that the transition can occur via a three-step process. First, the sheet undergoes the usual tearing instability. Second, the tearing mode saturates to form a two-dimensional quasi-steady state. Third, this secondary equilibrium is itself unstable when it is perturbed by three-dimensional disturbances. Most of this paper is devoted to the analysis and simulation of the three-dimensional linear stability properties of the two-dimensional saturated tearing layer. The numerical simulations are performed with a semi-implicit, pseudospectral-Fourier collocation algorithm. We identify a three-dimensional secondary linear stability which grows on the ideal timescale. An examination of the modal energetics reveals that the largest energy transfer is from the mean field to the three-dimensional field, with the two-dimensional field acting as a catalyst.

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BibTeXRIS

Dahlburg, R. B., Antiochos, S. K., Zang, T. A.. 1992-12-01. Secondary instability in three-dimensional magnetic reconnection. https://ntrs.nasa.gov/citations/19930035243

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