TY - JOUR
T1 - Bridging the gap between collisional and collisionless shock waves
AU - Bret, Antoine
AU - Pe'er, Asaf
N1 - Publisher Copyright: © The Author(s), 2021. Published by Cambridge University Press.
PY - 2021/3/9
Y1 - 2021/3/9
N2 - While the front of a fluid shock is a few mean-free-paths thick, the front of a collisionless shock can be orders of magnitude thinner. By bridging between a collisional and a collisionless formalism, we assess the transition between these two regimes. We consider non-relativistic, non-magnetized, planar shocks in electron-ion plasmas. In addition, our treatment of the collisionless regime is restricted to high-Mach-number electrostatic shocks. We find that the transition can be parameterized by the upstream plasma parameter which measures the coupling of the upstream medium. For, the upstream is collisional, i.e. strongly coupled, and the strong shock front is about thick, where and are the upstream mean free path and Mach number, respectively. A transition occurs for beyond which the front is thick for. Considering that can reach billions in astrophysical settings, this allows an understanding of how the front of a collisionless shock can be orders of magnitude smaller than the mean free path, and how physics transitions continuously between these two extremes.
AB - While the front of a fluid shock is a few mean-free-paths thick, the front of a collisionless shock can be orders of magnitude thinner. By bridging between a collisional and a collisionless formalism, we assess the transition between these two regimes. We consider non-relativistic, non-magnetized, planar shocks in electron-ion plasmas. In addition, our treatment of the collisionless regime is restricted to high-Mach-number electrostatic shocks. We find that the transition can be parameterized by the upstream plasma parameter which measures the coupling of the upstream medium. For, the upstream is collisional, i.e. strongly coupled, and the strong shock front is about thick, where and are the upstream mean free path and Mach number, respectively. A transition occurs for beyond which the front is thick for. Considering that can reach billions in astrophysical settings, this allows an understanding of how the front of a collisionless shock can be orders of magnitude smaller than the mean free path, and how physics transitions continuously between these two extremes.
KW - astrophysical plasmas
KW - plasma nonlinear phenomena
KW - space plasma physics
UR - http://www.scopus.com/inward/record.url?scp=85102335066&partnerID=8YFLogxK
U2 - https://doi.org/10.1017/S002237782100012X
DO - https://doi.org/10.1017/S002237782100012X
M3 - مقالة
SN - 0022-3778
JO - Journal of Plasma Physics
JF - Journal of Plasma Physics
M1 - 905870204
ER -