Nonlinear mirror mode structures

Details Nonlinear mirror mode structures Nonlinear mirror mode structures

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sf2a.conf..611s&link_type=abstract

SF2A-2007: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics held in Grenoble, France, July

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a brief survey of recent direct numerical simulations and asymptotic or phenomenological models, aimed to understand the formation and time evolution of pressure-balanced coherent structures observed in the solar wind or in planetary magnetosheaths, and usually viewed as nonlinear mirror modes. Special attention is paid to the conditions for the generation of magnetic holes or humps, and to the dynamical role of kinetic and hydrodynamic effects.

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