Building a weak shockwave from linear modes
Abstract
In shockwave theory, the density, velocity and pressure jumps are derived from the conservation equations. Here, we address the physics of a weak shock the other way around. We first show that the density profile of a weak shockwave in a fluid can be expressed as a sum of linear acoustic modes. The shock so built propagates at the speed of sound and matter is exactly conserved at the front crossing. Yet, momentum and energy are only conserved up to order 0 in powers of the shock amplitude. The density, velocity and pressure jumps are similar to those of a fluid shock, and an equivalent Mach number can be defined. A similar process is possible in magnetohydrodynamics. Yet, such a decomposition is found impossible for collisionless shocks due to the dispersive nature of ion acoustic waves. Weakly nonlinear corrections to their frequency do not solve the problem. Weak collisionless shocks could be inherently nonlinear, non-amenable to any linear superposition. Or they could be non-existent, as hinted by recent works.
- Publication:
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Journal of Plasma Physics
- Pub Date:
- February 2022
- DOI:
- arXiv:
- arXiv:2111.10190
- Bibcode:
- 2022JPlPh..88a9008B
- Keywords:
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- astrophysical plasmas;
- plasma nonlinear phenomena;
- space plasma physics;
- Physics - Plasma Physics;
- Physics - Classical Physics;
- Physics - Fluid Dynamics
- E-Print:
- 8 pages, 2 figures, to appear in Journal of Plasma Physics