2015
DOI: 10.1016/j.jcp.2014.10.003
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Numerical study of the plasma tearing instability on the resistive time scale

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Cited by 5 publications
(3 citation statements)
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“…In general, plasma physics is non linear and the formation of internal layers is a common feature in this context. Such an occurrence of local areas where the solution develops steep gradients is for instance dealt with in [15] using AP-methods. More sophisticated numerical methods remain yet to be developed along with AP schemes to address efficiently such problems: either local mesh refinements in the framework of unstructured grids, or patch techniques to perform local mesh refinement for Cartesian meshes [28].…”
Section: Towards Plasma Physics Simulationsmentioning
confidence: 99%
“…In general, plasma physics is non linear and the formation of internal layers is a common feature in this context. Such an occurrence of local areas where the solution develops steep gradients is for instance dealt with in [15] using AP-methods. More sophisticated numerical methods remain yet to be developed along with AP schemes to address efficiently such problems: either local mesh refinements in the framework of unstructured grids, or patch techniques to perform local mesh refinement for Cartesian meshes [28].…”
Section: Towards Plasma Physics Simulationsmentioning
confidence: 99%
“…The Micro-Macro as well as the duality based methods have been developed to heterogeneous anisotropy ratios in [48,60]. The Micro-Macro approach has been extended to closed magnetic field lines thanks to a regularization of the problem introduced in [114] and also implemented in [63]. Note that, an asymptotic preserving method based on a lagrangian integration along the anisotropy direction is proposed in [28].…”
Section: Generalization To Non Adapted Coordinatesmentioning
confidence: 99%
“…Indeed standard approaches have some difficulties in specific areas such as the so-called "O point" or "X point" [82,70,126] where the coordinate system is singular. Moreover, the goal pursued here is to easily account for changes in the magnetic field topology, with for instance the creation of magnetic islands [15,7,83,87,63,139,122,140]. To this end, the numerical methods developed within this section are free from any assumption relating the magnetic field to the mesh or the coordinate system.…”
Section: Introductionmentioning
confidence: 99%