Modeling Heliospheric Phenomena with the Multi-Scale Fluid-Kinetic Simulation Suite

被引：0

作者：

Pogorelov, N. V. ^{[1
]}

Borovikov, S. N. ^{[2
]}

Heerikhuisen, J. ^{[2
]}

Kryukov, I. A. ^{[2
]}

Zank, G. P. ^{[2
]}

机构：

[1] Univ Alabama, Dept Phys, 320 Sparkman Dr, Hunsville, AL 35805 USA

[2] Univ Alabama, Ctr Space Plasma & Aeronom Res, Hunsville, AL 35805 USA

来源：

NUMERICAL MODELING OF SPACE PLASMA FLOWS ASTRONUM-2009 | 2010年 / 429卷

关键词：

INTERSTELLAR MAGNETIC-FIELD; ADAPTIVE MESH REFINEMENT; SOLAR-WIND; ASYMMETRIES; HELIOSHEATH; PLASMA; MHD;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Numerical approaches are outlined that are implemented in the Multi-Scale Fluid-Kinetic Simulation Suite (MS-FLUKSS). A comparison is presented of different methods implemented in MS-FLUKSS to remove spurious magnetic charge from the computational region. The suite application is shown to modeling the solar wind (SW) interaction with the local interstellar medium (LISM) under 22nd and 23rd solar minimum condutions.

引用

页码：266 / +

页数：3

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