Going Beyond the MHD Approximation: Physics-based Numerical Solution of the CGL Equations

We present a new numerical model for solving the Chew–Goldberger–Low system of equations describing a bi-Maxwellian plasma in a magnetic field. Heliospheric and geospace environments are often observed to be in an anisotropic state with distinctly different parallel and perpendicular pressure compon...

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Veröffentlicht in:	The Astrophysical journal 2024-08, Vol.970 (2), p.154
Hauptverfasser:	Bhoriya, Deepak, Balsara, Dinshaw, Florinski, Vladimir, Kumar, Harish
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Anisotropy Computational astronomy Computational methods Field strength Hyperbolic functions Magnetic fields Magnetohydrodynamics Magnetospheres Mathematical models Numerical models Physics Pitch (inclination) Plasma astrophysics Space plasmas
Online-Zugang:	Volltext
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