The Modeling of Pickup Ion or Energetic Particle Mediated Plasmas

10th International Conference on Numerical Modeling of Space Plasma Flows: ASTRONUM-2015

Zank, G.P.^1,2 ; Mostafavi, P.^1,2 ; Hunana, P.^1,2

Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville

AL

35805, United States^1

Department of Space Science, University of Alabama in Huntsville, Huntsville

AL

35805, United States^2

关键词: Chapman-Enskog expansion;    Energetic particles;    Local interstellar medium;    Outer heliosphere;    Scalar pressure;    Solar energetic particles;    Suprathermal particles;    System of equations;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/719/1/012014/pdf
DOI  :  10.1088/1742-6596/719/1/012014

来源: IOP

【 摘 要 】

Suprathermal energetic particles, such as solar energetic particles (SEPs) in the inner heliosphere and pickup ions (PUIs) in the outer heliosphere and the very local interstellar medium, often form a thermodynamically dominant component in their various environments. In the supersonic solar wind beyond > 10 AU, in the inner heliosheath (IHS), and in the very local interstellar medium (VLISM), PUIs do not equilibrate collisionally with the background plasma. Similarly, SEPs do not equilibrate collisionally with the background solar wind in the inner heliosphere. In the absence of equilibration between plasma components, a separate coupled plasma description for the energetic particles is necessary. Using a collisionless Chapman-Enskog expansion, we derive a closed system of multi-component equations for a plasma comprised of thermal protons and electrons, and suprathermal particles (SEPs, PUIs). The energetic particles contribute an isotropic scalar pressure to leading order, a collisionless heat flux at the next order, and a collisionless stress tensor at the second-order. The collisionless heat conduction and viscosity in the multi-fluid description results from a nonisotropic energetic particle distribution. A simpler single-fluid MHD-like system of equations with distinct equations of state for both the background plasma and the suprathermal particles is derived. We note briefly potential pitfalls that can emerge in the numerical modeling of collisionless plasma flows that contain a dynamically important energetic particle component.