Mirror structures above and below the linear instability threshold: Cluster observations, fluid model and hybrid simulations

Vincent Génot (1) , E. Budnik (1) , P. Hellinger (2) , T. Passot (3) , G. Belmont (4) , P. M. Trávnícek (2) , P.-L. Sulem (3) , E. Lucek (5) , I. Dandouras (1)

1 CESR - Centre d'étude spatiale des rayonnements
2 IAP - Institute of Atmospheric Physics [Prague]
3 CASSIOPEE - Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides
4 CETP - Centre d'étude des environnements terrestre et planétaires
5 Blackett Laboratory

Using 5 years of Cluster data, we present a detailed statistical analysis of magnetic fluctuations associated with mirror structures in the magnetosheath. We especially focus on the shape of these fluctuations which, in addition to quasi-sinusoidal forms, also display deep holes and high peaks. The occurrence frequency and the most probable location of the various types of structures is discussed, together with their relation to local plasma parameters. While these properties have previously been correlated to the ? of the plasma, we emphasize here the influence of the distance to the linear mirror instability threshold. This enables us to interpret the observations of mirror structures in a stable plasma in terms of bistability and subcritical bifurcation. The data analysis is supplemented by the prediction of a quasi-static anisotropic MHD model and hybrid numerical simulations in an expanding box aimed at mimicking the magnetosheath plasma. This leads us to suggest a scenario for the formation and evolution of mirror structures.

Domains: Earth and Planetary Astrophysics [astro-ph.EP]; Earth and Planetary Astrophysics [astro-ph.EP]

Vincent Génot, E. Budnik, P. Hellinger, T. Passot, G. Belmont, et al.. Mirror structures above and below the linear instability threshold: Cluster observations, fluid model and hybrid simulations. Annales Geophysicae, 2009, 27, pp.601-615. ⟨hal-00362805⟩