The inner magnetosphere : physics and modeling
The inner magnetosphere : physics and modeling
复制标题
内部磁层：物理和建模
DOI：
10.1029/gm155
复制
发表时间：
2005
期刊：
影响因子：
--
通讯作者：
R. Friedel
中科院分区：
文献类型：
--
作者：
T. Pulkkinen;N. Tsyganenko;R. Friedel
由美国地球物理学联合会出版，作为地球物理学专著系列第155卷的一部分。随着我们成为航天文化，越来越需要可靠的方法来预测地球空间环境中的电磁场，热等离子体和高能粒子的动态，因为所有这些因素都会影响星载系统。另一方面，从电动力学的观点来看，内磁层是日地过程连接链中的一个关键要素。最值得注意的是，这是一个区域，其中很大一部分来自太阳风的风暴能量输入被储存和消散。
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 155. As we become a space-faring culture, there is an increasing need for reliable methods to forecast the dynamics of electromagnetic fields, thermal plasma, and energetic particles in the geospace environment, as all these factors affect satellite-borne systems. From the electrodynamics viewpoint, on the other hand, the inner magnetosphere is a key element in the Sun-Earth connection chain of processes. Most notably, it is a region where a significant part of the storm-time energy input from the solar wind is deposited and dissipated.