Affiliation:
1. Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA
Abstract
Recently, a method to achieve a “natural hot-ion mode” was suggested by utilizing ion viscous heating in a rotating plasma with a fixed boundary. We explore the steady-state solution to the Braginskii equations and find the parameter regime in which a significant temperature difference between ions and electrons can be sustained in a driven steady state. The threshold for this effect occurs at [Formula: see text]. An analytic, leading order low flow solution is obtained, and a numerical, moderate Mach number [Formula: see text] is investigated. The limitation is found to be at moderate Mach numbers.
Funder
National Nuclear Security Administration
National Science Foundation
Oak Ridge Institute for Science and Education