Speaker
Koen Kemel
Description
A reduction of total mean turbulent pressure due to the
presence of magnetic fields was previously shown to be a
measurable effect in direct numerical simulations. However,
in the studied parameter regime the formation of large-scale
structures, as anticipated from earlier mean-field
simulations, was not found. An analysis of the relevant
mean-field parameter dependency and the parameter domain of
interest is conducted in order to clarify this apparent
discrepancy.