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Multi-ion oscillitons - origin of magnetospheric EMIC waves and further implications
  • Konrad Sauer,
  • Eduard Dubinin
Konrad Sauer
Retired from MPI for Solar System Research

Corresponding Author:[email protected]

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Eduard Dubinin
Max-Planck-Institute for Solar System Research
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Abstract

The recent spacecraft observations by MMS and Van Allen Probes associated with electromagnetic ion cyclotron waves (EMIC) in the Earth magnetosphere emphasize the important role of multi-ion plasma composition for generation and characteristics of these emissions. We show that the main properties of EMIC waves can be explained with the concept of ‘multi-ion oscillitons’ (Sauer et al., 2001). In a plasma with two types of ions of different masses (e.g. protons and oxygen ions), oscillitons arise from the exchange of momentum and energy between the two ion components, with the electromagnetic field acting as a mediator. At frequencies near cross-over frequencies of different wave modes in the multi-ion plasma the nonlinear resonance which strongly amplifies the seed unstable mode can be excited. A small phase difference in oscillations of different ion species leads to a nonlinear wave beating and generation of wave packets. The ‘resonance ‘ frequency is characterized by a local maximum of the phase velocity and the coincidence of phase and group velocity. The generation of coherent waves by oscillitons is of a general nature and may contribute to understand the manifold of phenomena in other space plasma environments in which the dynamics of minor ion admixtures cannot be neglected, as alpha particles in the solar wind and heavy ions around active comets. The concept of oscillitons also applies to the momentum exchange between different particle groups of the same mass. On this way, whistler oscillitons may arise in two-temperature electron plasmas.