1) disturbed interplanetary magnetic field
行星际扰动场
3) interplanetary disturbance structure
行星际扰动结构
1.
The response of the morphological category of geomagnetic storms to interplanetary disturbance structures is analyzed, which includes the shock, the high density structure and the strong magnetic field structure, as well as the high-speed stream.
本文介绍对日地系统扰动作多层次综合研究所取得的最新成果;分析了磁暴形态类型对行星际扰动结构,包括激波、高密度结构、强磁场结构、高速流等的响应特征;讨论了磁暴主相形成、延迟和消隐,及初相形成的条件;发现了行星际强磁场膨胀结构的动力学效应,及新的亚阿尔文波速流事例。
4) Interplanetary combinative structure
行星际扰动组合结构
5) Interplanetary Magnetic Field (IMF)
行星际磁场
1.
The statistic study have been performed on the relationship between the formation of the magnetic flux ropes and Interplanetary Magnetic Field (IMF).
收集了Cluster卫星在2001-2005年间观测到的磁尾磁通量绳事件,并对磁通量绳(magnetic flux rope)形成及其内部磁场结构与行星际磁场(IMF)的关系作了统计研究。
6) IMF
[英][,aɪ em 'ef] [美]['aɪ 'ɛm 'ɛf]
行星际磁场
1.
The response of high-latitude ionospheric convection during a southward IMF turning event;
一次行星际磁场南向突变的高纬电离层对流响应特征
2.
DEPENDENCE OF THE POSTNOON AURORAL INTENSITY UPON THE IMF;
午后极光强度与行星际磁场的相关
3.
A GLOBAL MODEL OF MAGNETIC RECONNECTION AT MAGNETOPAUSE FOR NORTHWARD IMF;
行星际磁场北向时磁层顶区磁场重联的全球模式
补充资料：行星和行星际探测器
见空间探测器。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条