球坐标系六片网格下三维定态行星际太阳风模拟
Three-dimensional Steady State Interplanetary Solar Wind Simulation in Spherical Coordinates with a Six-component Grid
查看参考文献41篇
文摘
|
采用二阶MacCormack差分格式,利用稳态的磁流体(MHD)方程组在球坐标系六片网格下模拟研究了行星际太阳风.六片网格系统能有效避免极区奇性和网格收敛性.迭代按径向方向推进求解,很大程度上减少了计算量,节约了计算时间.内边界条件根据太阳与行星际观测确定,比较测试了5种内边界条件,模拟给出了1922卡林顿周的背景太阳风结构.几种内边界条件所得模拟结果与行星际观测基本吻合.太阳风速度采用McGregor等的经验公式给出,磁场由水平电流片(HCCS)模型得到,密度和温度分别根据动量守恒和气压守恒得到,研究表明采用这样的边界条件模拟结果最佳. |
其他语种文摘
|
In this paper, the MacCormack scheme is applied to the time-independent Magneto-hydrodynamics (MHD) equations in spherical coordinates with a six-component grid for the three-dimensional interplanetary solar wind simulation. The use of six-component grid system can better body-fit the spherical shell domain of interplanetary space as well as avoid the singularity and the mesh convergence near the poles. The radial coordinate is treated as a time-like coordinate, thus can significantly reduce the computational time. The inner boundary distribution is determined by the empirical relations and observation. Five kinds of inner boundary conditions used formerly by MHD modelers are comparatively used to simulate the Carrington Rotation (CR) 1922 solar wind background. The numerical results show that all these boundary conditions can produce consistent large-scale solar wind structure with the observation, and better result in agreement with observations can be achieved when adopting the following inner boundary condition: the radial speed is obtained by the empirical relationship proposed by McGregor et al. in 2011,the magnetic field is obtained by Horizontal Current Current Sheet (HCCS) model, an assumption of constant momentum flux is used to derive number density, and temperature is chosen to assure that the total pressure is uniform at the inner boundary. |
来源
|
空间科学学报
,2014,34(6):773-784 【核心库】
|
关键词
|
MHD方程组
;
六片网格系统
;
行星际太阳风模拟
|
地址
|
中国科学院空间科学与应用研究中心, 空间天气学国家重点实验室, 北京, 100190
|
语种
|
中文 |
文献类型
|
研究性论文 |
ISSN
|
0254-6124 |
学科
|
地球物理学 |
基金
|
国家973计划
;
国家自然科学基金项目
;
中国科学院知识创新工程重大项目
;
国家重点实验室专项基金项目共同资助
|
文献收藏号
|
CSCD:5287945
|
参考文献 共
41
共3页
|
1.
Toth G. Space weather modeling framework: A new tool for the space science community.
J. Geophys. Res,2005,110:A12226
|
被引
13
次
|
|
|
|
2.
Odstrcil D. Numerical simulation of the 12 May 1997 interplanetary CME event.
J. Geophys. Res,2004,109:A02116
|
被引
3
次
|
|
|
|
3.
Feng Xueshang. Validation of the 3D AMR SIP-CESE solar wind model for four Carrington rotations.
Solar Phys,2012,279:207-229
|
被引
9
次
|
|
|
|
4.
Feng Xueshang. Numerical study of interplanetary solar storms.
Sci. China Earth Sci,2013,43:912-933
|
被引
1
次
|
|
|
|
5.
Feng X S. A hybrid solar wind model of the CESE+HLL method with a yin-yang overset grid and an AMR grid.
Astrophys. J,2011,734
|
被引
1
次
|
|
|
|
6.
Feng X S. GPU-accelerated computing of three-dimensional solar wind background.
Sci. China Earth Sci,2013,56:1864-1880
|
被引
8
次
|
|
|
|
7.
Han S M. A three-dimensional, timedependent numerical modeling of the super-sonic, super-alfvenic MHD flow.
Comp. Fluids,1988,16:81-103
|
被引
14
次
|
|
|
|
8.
Pizzo V J. Global quasi-steady dynamics of the distant solar wind 1 Origin of north-south flows in the outer heliosphere.
J. Geophys. Res,1994,99:4173-4183
|
被引
2
次
|
|
|
|
9.
Usmanov A V. The global structure of the solar wind in June 1991.
Solar Phys,1993,148:371-382
|
被引
1
次
|
|
|
|
10.
Usmanov A V. A global MHD solar wind model with WKB Alfve'n waves: Comparison with Ulysses data.
J. Geophys. Res,2000,105:12675-12695
|
被引
7
次
|
|
|
|
11.
Detman Thomas. A hybrid heliospheric modeling system: Background solar wind.
J. Geophys. Res,2006,111:A07102
|
被引
1
次
|
|
|
|
12.
Detman T R. The influence of pickup protons, from interstellar neutral hydrogen, on the propagation of interplanetary shocks from the Halloween 2003 solar events to ACE and Ulysses: A 3-D MHD modeling study.
J. Geophys. Res,2011,116:A03105
|
被引
2
次
|
|
|
|
13.
Hayashi K. An MHD simulation model of time-dependent co-rotating solar wind.
J. Geophys. Res,2012,117:A08105
|
被引
4
次
|
|
|
|
14.
Odstrcil D. Modeling 3D solar wind structure.
Adv. Space Res,2003,32:497-506
|
被引
12
次
|
|
|
|
15.
Arge C N. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates.
J. Geophys. Res,2000,105
|
被引
14
次
|
|
|
|
16.
Riley P. An empirically-driven global MHD model of the solar corona and inner heliosphere.
J. Geophys. Res,2001,106(A8):15889-15901
|
被引
8
次
|
|
|
|
17.
Wiengarten T. MHD simulation of the inner-heliospheric magnetic field.
J. Geophys. Res,2013,118:29-44
|
被引
4
次
|
|
|
|
18.
Van der Holst B. Modelling of solar wind, CME Initiation and CME propagation.
Space Sci. Rev,2005,121:91-104
|
被引
1
次
|
|
|
|
19.
Jiang J. Modeling the Sun's open magnetic flux and the heliospheric current sheet.
Astrophys. J,2010,709:301-307
|
被引
2
次
|
|
|
|
20.
Zhao X. Predicting the heliospheric magnetic field using the current sheet-source surface model.
Adv. Space Res,2005,16
|
被引
1
次
|
|
|
|
|