3D data snapshot from a radiative particle-in-cell simulation of plasma turbulence
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2024-07-15, 2024-07-15
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Description
A full 3D data snapshot of plasma turbulence as simulated by the Runko particle-in-cell code. The data is visualized in Fig. 3 of Nättilä 2024. The simulation models the magnetized corona around black-hole accretion flows.
The dataset includes the simulation snapshot (flds_2500.h5) and the corresponding runko configuration file (x16.ini). The turbulence is excited with a Langevin antenna and has a guide field along the z-axis. See the paper for other physical and technical details.
The flds_2500.h5 HDF5 file includes 10 datasets with a 640^3 resolution:
ex, ey, ez for electric field x, y, and z components
bx, by, bz for magnetic field components
jx, jy, jz for current density components
rho for plasma density