节点文献
磁层亚暴与磁层暴(Ⅱ):太阳风参数对Dst的影响机制研究
MAGNETOSPHERIC STORM AND SUBSTORMS (Ⅱ): THE MECHANISM OF THE EFFECT OF THE SOLAR-WIND PARAMETERS ON Dst
【摘要】 为了研究地磁活动指数Dst受太阳风参数影响,包括行星际磁场(IMF)南向分量Bst、太阳风速度V?和太阳风-磁层发电机电动势U调制的机制,应用太阳风-磁层-电离层输入-输出[I(t)-O(t)]电网络模型,对磁层亚暴与磁层暴过程中,Bz(t)-Dst、V-a(t)-Dst和U(t)—Dst的激励-响应特性进行模拟。研究表明,Bz是形成亚暴与磁层暴的前提条件,Vst是形成亚暴与磁层暴的充分条件,二者统一于电动势Ust研究结果与观测结果一致。
【Abstract】 In order to study the modulating mechanism of the Dst index versus solar wind parameters, including the intherplanetary magnetic field (IMF), Bz, the solas wind speed, Vs, and the electromotive fore (EMF), U, we simulate the input-output characteristics of Bz-Dst,Vs-Dst,U-Dst with the input-output network model of the system of solar wind-magnetosphere-ionosphere. The model predicts that Bz is the preroquisite for substorms and storm, and Vs, is the additional condition for them. Bz and Vs, are integrated to EMF, U(t). The results are well-accordant with the observed results.
【Key words】 Solar wind; Substorms and storm; Geomagnetic activities; Network; Simulation.;
- 【文献出处】 地球物理学报 ,Chinese Journal of Geophysics , 编辑部邮箱 ,1999年S1期
- 【分类号】P353
- 【被引频次】4
- 【下载频次】134