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| EPoS Contribution |
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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 | |
| Collaborators: P.J. Malinen, FSU, US P. Myers, CfA, US B. Burkhart, CfA, US |
Key publication
Suggested Session: Filaments |