Combining dust polarization angle dispersion with Zeeman-based line-of-sight Alfvén Mach number can classify simulated molecular clouds as sub-, trans-, or super-Alfvénic.
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Tracing 3-D Magnetic Field Structure Using Dust Polarization and the Zeeman Effect
Combining dust polarization angle dispersion with Zeeman-based line-of-sight Alfvén Mach number can classify simulated molecular clouds as sub-, trans-, or super-Alfvénic.