EPoS Contribution
EPoS Contribution
Time and Magnetic Field Evolution of Filaments in AMR simulations

David Collins
FSU, Tallahassee, US
I will be presenting magnetic field morphology and time evolution from AMR MHD simulations of turbulent clouds. It is found that filaments evolve in substantially less than a mean free-fall time, and that measurements of magnetic field morphology is strongly subject to line-of-sight confusion. We will also discuss resolution effects in the study, which indicates that filament width is strongly connected to sampling resolution
P.J. Malinen, FSU, US
P. Myers, CfA, US
B. Burkhart, CfA, US
Key publication

Suggested Session: Filaments