Abstract

We examine the effect of accuracy of high-order spectral element methods, with or without adaptive mesh refinement (AMR), in the context of a classical configuration of magnetic reconnection in two space dimensions, the so-called Orszag–Tang (OT) vortex made up of a magnetic X-point centred on a stagnation point of the velocity. A recently developed spectral-element adaptive refinement incompressible magnetohydrodynamic (MHD) code is applied to simulate this problem. The MHD solver is explicit, and uses the Elsässer formulation on high-order elements. It automatically takes advantage of the adaptive grid mechanics that have been described elsewhere in the fluid context (Rosenberg et al 2006 J. Comput. Phys. 215 59–80); the code allows both statically refined and dynamically refined grids. Tests of the algorithm using analytic solutions are described, and comparisons of the OT solutions with pseudo-spectral computations are performed. We demonstrate for moderate Reynolds numbers that the algorithms using both static and refined grids reproduce the pseudo-spectral solutions quite well. We show that low-order truncation—even with a comparable number of global degrees of freedom—fails to correctly model some strong (sup-norm) quantities in this problem, even though it satisfies adequately the weak (integrated) balance diagnostics.

Highlights

  • In geophysical and astrophysical flows, the Reynolds numbers are large, and nonlinear terms appearing in the primitive equations lead to strong mode coupling and multiple scale interactions

  • We examine in this paper the accuracy of an adaptive mesh refinement (AMR) code using spectral elements by comparing its output to exact solutions in simplified cases and to computations using a pseudo-spectral code at the same Reynolds numbers on a classical configuration of magnetic reconnection in two-dimensional geometry

  • We have presented an explicit spectral element method for solving the equations of incompressible magnetohydrodynamics

Read more

Summary

Introduction

In geophysical and astrophysical flows, the Reynolds numbers are large, and nonlinear terms appearing in the primitive equations lead to strong mode coupling and multiple scale interactions. In the case of coupling to a magnetic field, and using the magnetohydrodynamic (MHD) approximation valid for the description of the large-scale dynamics, few such techniques have been developed and tested (see [26, 22, 23, 15]). Another venue is to develop adaptive mesh refinement (AMR) methods. We consider effects of low order versus high order local approximations in section 5, and section 6 is the conclusion, in which we summarize the results, and offer some observations about the performance of the method and some directions for future work

Setup and theory
Algorithm description for MHD
Time stepping
Tests with exact solutions
The Orszag-Tang vortex
High versus low order
Discussion and Conclusion
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.