Electric fields and currents in solar-terrestrial plasmas
Yang, Zhongwei; Parks, George K.; Lee, Ensang
United States, South Korea, China
Abstract
This article will review many ideas and concepts originally suggested by Alfvén (Space Sci Rev 7:1940, 1967) and Fälthammar (Rev Geophys 15: 457, 1977) on the important roles electric fields and currents play in solar-terrestrial plasmas. Much of our understanding of planetary and solar plasmas has come primarily from treating plasmas as fluids. Fluid theory has emphasized bulk parameters and frozen-in magnetic field. This article, however, will focus on electric field, currents, and particles. This approach will give us a much broader perspective about space and solar plasma dynamics. We review relevant observations, theories, and models that will help us understand the basic physics. Our discussion includes the heliospheric current sheet formed by the solar wind (SW). All of the planets are immersed in this current sheet, and magnetospheres are formed by the interaction of the current sheet with planetary magnetic fields. We discuss how the electric fields induced by the evolving current sheets can accelerate particles to high energies pertinent for auroras and solar flares. The magnetic polarity across the current sheets can reverse directions over a distance of a few Larmor radii. We review the orbit trajectories resulting from inclusion of a