Abstract
We describe a new model for the study of weakly collisional, magnetised plasmas derived from exploiting the separation of the dynamics parallel and perpendicular to the magnetic field. This unique system of equations retains the particle dynamics parallel to the magnetic field while approximating the perpendicular dynamics through a spectral expansion in the perpendicular degrees of freedom, analogous to moment-based fluid approaches. In so doing, a hybrid approach is obtained that is computationally efficient enough to allow for larger-scale modelling of plasma systems while eliminating a source of difficulty in deriving fluid equations applicable to magnetised plasmas. We connect this system of equations to historical asymptotic models and discuss advantages and disadvantages of this approach, including the extension of this parallel-kinetic-perpendicular moment beyond the typical region of validity of these more traditional asymptotic models. This paper forms the first of a multi-part series on this new model, covering the theory and derivation, alongside demonstration benchmarks of this approach that include shocks and magnetic reconnection.
| Original language | English (US) |
|---|---|
| Article number | E129 |
| Journal | Journal of Plasma Physics |
| Volume | 91 |
| Issue number | 5 |
| DOIs | |
| State | Published - Sep 19 2025 |
All Science Journal Classification (ASJC) codes
- Condensed Matter Physics
Keywords
- astrophysical plasmas
- plasma simulation
- space plasma physics