Magnetic Alfvén-Cyclotron Fluctuations of Anisotropic Non-Thermal Plasmas

Thursday, 18 December 2014
Roberto Navarro1, Victor Munoz1, Jaime A Araneda2, Adolfo F. Vinas3, Pablo S Moya3 and Juan Alejandro Valdivia1, (1)University of Chile, Santiago, Chile, (2)Univ. Concepcion, Concepcion, Chile, (3)NASA Goddard Space Flight Center, Heliophysics Division, Geospace Physics Laboratory, Mail Code 673, Greenbelt, MD, United States
Remote and in situ observations in the solar wind show that ion and electron velocity distributions persistently present deviations from thermal equilibrium. Ion anisotropies seem to be constrained by instability thresholds which are in agreement with linear kinetic theory. For plasma states below these instability thresholds, the quasi-stable solar wind plasma sustains a small but detectable level of magnetic fluctuation power. These fluctuations may be related to spontaneous electromagnetic fluctuations arising from the discreteness of charged particles. Here, we study electromagnetic fluctuations propagating along a background magnetic field in a plasma composed of thermal and suprathermal protons and electrons via the fluctuation-dissipation theorem. The total fluctuating magnetic power is estimated in a proton temperature anisotropy-beta diagram for three different families of proton distribution functions, which can be compared to a number of recent measurements in the solar wind.