| 行星际磁场北向时磁层顶区磁场重联的全球模式 |
| |
| 引用本文： | 张洪,刘振兴.行星际磁场北向时磁层顶区磁场重联的全球模式[J].空间科学学报,1996,16(4):274-281. |
| |
| 作者姓名： | 张洪 刘振兴 |
| |
| 作者单位： | 中国科学院空间科学与应用研究中心, 北京 100080 |
| |
| 摘 要： | 在对背阳面磁层顶区局域磁场重联模拟的基础上提出了一个行星际磁场北向时磁层顶磁场重联的全球模式。行星际磁场北向时碰层顶磁场重联导致近地尾瓣的能量被输送到远磁尾,太阳风能量不在磁尾储存,向阳面磁层顶变厚,磁层受到一系列扰动。
|
| 关 键 词： | 行星际磁场 磁层顶 磁场重联 磁流体力学数值模拟 |
| 收稿时间： | 1995-06-29 |
A GLOBAL MODEL OF MAGNETIC RECONNECTION AT MAGNETOPAUSE FOR NORTHWARD IMF |
| |
| Zhang Hong, Liu Zhen-xing.A GLOBAL MODEL OF MAGNETIC RECONNECTION AT MAGNETOPAUSE FOR NORTHWARD IMF[J].Chinese Journal of Space Science,1996,16(4):274-281. |
| |
| Authors: | Zhang Hong Liu Zhen-xing |
| |
| Institution: | Center for Space Science and aApplied Research, Academia Sinica, Beijing 100080 |
| |
| Abstract: | A 2D compressible model is used to simulate the local magnetic reconnection at the nightside magnetopause for northward IMF. Based on the simulation result, a globe magnetic reconnection model for northward IMF is proposed. As results of magnetic reconnection at magnetopause for northward IMF, the magnetic energy in tail lobe is transported to far magnetotail, dayside magnetopause become thicker, and the magnetosphere is disturbed. |
| |
| Keywords: | IMF Magnetopause Magnetic reconnection MHD simulation |
| 本文献已被 CNKI 维普 等数据库收录！ |
| 点击此处可从《空间科学学报》浏览原始摘要信息 |
| 点击此处可从《空间科学学报》下载免费的PDF全文 |
|
