Hall MHD on Block-Adaptive Grids

被引：0

作者：

Toth, Gabor ^{[1
]}

Ma, Ying-Juan ^{[2
]}

Gombosi, Tamas I. ^{[1
]}

机构：

[1] Univ Michigan, Ctr Space Environm Modeling, 2455 Hayward Ave, Ann Arbor, MI 48109 USA

[2] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA

来源：

NUMERICAL MODELING OF SPACE PLASMA FLOWS: ASTRONUM-2008 | 2009年 / 406卷

关键词：

MAGNETOHYDRODYNAMICS; SCHEME;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This proceedings paper is based on a much longer research paper that was published during the conference (Toth et al. 2008). We present a, conservative second order accurate finite volume discretization of the magnetohydrodynamics equations including the Hall term on three dimensional block adaptive grids with Cartesian or generalized coordinates. Both explicit and implicit time integration schemes are developed. The parallel scaling and robustness are demonstrated by three dimensional simulations of planetary magnetospheres.

引用

页码：287 / +

页数：2

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