New type of soliton in bi-ion plasmas and possible implications

被引:64
作者
Sauer, K
Dubinin, E
McKenzie, JF
机构
[1] Max Planck Inst Aeron, D-37191 Katlenburg Duhm, Germany
[2] Univ Natal, Sch Pure & Appl Phys, ZA-4001 Durban, South Africa
关键词
D O I
10.1029/2001GL013047
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
It is well known that the addition of a second ion population into a proton-electron plasma gives rise to new low-frequency wave modes. Here we investigate stationary structures streaming with sub-fast speed in such a bi-ion plasma. It is shown that a new type of stationary structure occurs as result of mode splitting effects caused by the second ion population. These so-called 'oscillitons' are characterized by an oscillating spatial structure superimposed on the spatial growth or decay associated with the usual single-ion solitons. Examples of the solution of the full non-linear equations describing stationary bi-ion flows are given which show that 'oscillitons' may contribute to a better understanding of diverse low-frequency phenomena observed in the mass loaded plasma environments of Mars, Jupiter and comets.
引用
收藏
页码:3589 / 3592
页数:4
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