Open AccessDifferential ion streaming in the solar wind as an equilibrium state
Author(s) -
Dubinin E.,
Sauer K.,
McKenzie J. F.
Publication year - 2005
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2004ja010826
Subject(s) - physics , proton , magnetohydrodynamics , nonlinear system , ion , solar wind , atomic physics , thermodynamic equilibrium , alfvén wave , differential equation , beam (structure) , plasma , computational physics , classical mechanics , quantum electrodynamics , nuclear physics , quantum mechanics , optics
We analyze the nonlinear evolution of differential streaming between core protons and alpha particles (or any secondary minor protons) based on the analysis of fully nonlinear multifluid MHD equations. It is shown that such an ion beam‐plasma system possesses an equilibrium state with a remnant of differential streaming. The properties of this state are studied. The system through the action of nonlinear hydromagnetic waves can attain an equilibrium state which is characterized by a “gyrating” motion of both ion populations with a phase shift of π. The waves which bring about a such transition are either the Alfven or magnetosonic modes, depending upon the beam speed. It is shown that the equilibrium differential speed between the alphas and protons V α p lies between 0.8 and 1.5 V A but only in a certain regime of injection speeds of the alphas. A similar picture obtains for proton/proton configurations in which the number density of the secondary protons imposes a constraint on the injection speeds, 1.5 ≥ V p , p / V A ≥ 0.3 ( V A is a local Alfven speed). Nonlinear Alfven waves bring about a transition to equilibrium states with much higher differential velocities u α p ( u pp ), proportional to the injection speeds, than magnetosonic waves.