Magnetohydrodynamic simulations show a well - defined jet that extracts energy from a black hole.
Not exact matches
«Three dimensional numerical
simulations, taking into account the
magnetohydrodynamic properties and the relativistic velocities, predict the appearance and the propagation of instabilities in the jet, which then distort it» explains Acosta.
Also expected to benefit are physicist Weixing Wang, who seeks advanced visualization of the data from turbulence
simulation runs, and physicists Josh Breslau and Steve Jardin, who use animated visualizations to help interpret the output of their
magnetohydrodynamic codes, which treat plasma as a magnetic fluid.
Also selected to participate in Cori's NERSC Exascale Science Applications Program (NESAP) is the PPPL - led M3D - CI, an extended
magnetohydrodynamics (MHD) code focused on
simulation of plasma disruptions led by physicist Stephen Jardin, with support from physicists Joshua Breslau, Nate Ferraro and Jin Chen.
Among the numerous star - planet interaction (SPI) models that have been developed,
magnetohydrodynamic (MHD)
simulations combine state of the art numerical models of cool star magnetospheres with simplified models of planets.
The
simulations resolve the flow in the upper atmospheres of the giant planets, with implicit links to the (convective) flow, mean meridional circulations and (likely
magnetohydrodynamic) dissipation mechanisms at depth.