Bridging the gap between collisional and collisionless shock waves
Abstract
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 $\varLambda$ which measures the coupling of the upstream medium. For $\varLambda \lesssim 1.12$, the upstream is collisional, i.e. strongly coupled, and the strong shock front is about $M_1 λ _{mfp,1}$ thick, where $λ _{mfp,1}$ and $M_1$ are the upstream mean free path and Mach number, respectively. A transition occurs for $\varLambda ∼ 1.12$ beyond which the front is $∼ M_1λ _{mfp,1}\ln \varLambda /\varLambda$ thick for $\varLambda \gtrsim 1.12$. Considering that $\varLambda$ 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.
- Publication:
-
Journal of Plasma Physics
- Pub Date:
- March 2021
- DOI:
- 10.1017/S002237782100012X
- arXiv:
- arXiv:2101.09130
- Bibcode:
- 2021JPlPh..87b9004B
- Keywords:
-
- astrophysical plasmas;
- plasma nonlinear phenomena;
- space plasma physics;
- Physics - Plasma Physics;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Solar and Stellar Astrophysics;
- Physics - Space Physics
- E-Print:
- 13 pages, 4 figures, Under consideration for publication in J. Plasma Phys