Lagrangian methods reproduce high-resolution Eulerian behavior for toroidally-magnetized disks and continue to lose flux at low resolution by following thin layers, unlike Eulerian methods that show no evolution.
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2 Pith papers cite this work. Polarity classification is still indexing.
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A review summarizing pitfalls in older CR-MHD models and progress toward more rigorous treatments that connect microphysical CR scales to galactic dynamics.
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Lagrangian versus Eulerian Methods for Toroidally-Magnetized Isothermal Disks
Lagrangian methods reproduce high-resolution Eulerian behavior for toroidally-magnetized disks and continue to lose flux at low resolution by following thin layers, unlike Eulerian methods that show no evolution.
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Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models
A review summarizing pitfalls in older CR-MHD models and progress toward more rigorous treatments that connect microphysical CR scales to galactic dynamics.