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.
write newline
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2025 2roles
background 1polarities
background 1representative citing papers
A review summarizing pitfalls in older CR-MHD models and progress toward more rigorous treatments that connect microphysical CR scales to galactic dynamics.
citing papers explorer
-
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.
-
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.