Four-field model for dispersive field-line resonances: Effects of coupling between shear-Alfven and slow modes

被引:17
作者
Bhattacharjee, A [1 ]
Kletzing, CA [1 ]
Ma, ZW [1 ]
Ng, CS [1 ]
Otani, NF [1 ]
Wang, X [1 ]
机构
[1] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
关键词
D O I
10.1029/1999GL003628
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A new theoretical model is proposed far dispersive field-line resonances in collisionless magnetospheric plasmas on the basis of reduced four-field equations. The model improves upon the predictive capabilities of earlier two-field models. In particular, due to the coupling of the shear-Alfven mode to the slow mode in the four-field system, it is now possible to account for the observed low frequencies of field-line resonances. Furthermore, parallel electric fields can be large without requiring the field-aligned current density to be unrealistically large. Qualitative implications for recent FAST and ground-based observations are discussed.
引用
收藏
页码:3281 / 3284
页数:4
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