盘吸积至磁化恒星的3D MHD模拟：数值方法与示例模拟
太阳与恒星天体物理
2009-01-28 v1
摘要
我们展示了使用基于我们课题组先前开发的“立方球”网格的Godunov型代码，对具有偶极子和更复杂磁场的旋转恒星进行全局3D MHD盘吸积模拟的结果。我们描述了该代码和网格，并展示了模拟结果的示例。
引用
@article{arxiv.0901.4269,
title = {3D MHD Simulations of Disk Accretion onto Magnetized Stars: Numerical Approach and Sample Simulations},
author = {Marina M. Romanova and Alexander V. Koldoba and Galina V. Ustyugova and Akshay K. Kulkarni and Min Long and Richard V. E. Lovelace},
journal= {arXiv preprint arXiv:0901.4269},
year = {2009}
}
备注
7 pages, 3 figures. Proceedings of the 3RD International Conference on Numerical Modeling of Space Plasma Flows (ASTRONUM-2008), June 8-13, 2008, St. John, U.S.V.I