3D data snapshot from a radiative particle-in-cell simulation of plasma turbulence

dc.contributor.affiliationUniversity of Helsinki - Nättilä, Joonas
dc.contributor.authorNättilä, Joonas
dc.date.accessioned2025-03-24T15:17:25Z
dc.date.issued2024-07-15
dc.date.issued2024-07-15
dc.descriptionA 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
dc.identifierhttps://doi.org/10.5281/zenodo.12743684
dc.identifier.urihttps://hydatakatalogi-test-24.it.helsinki.fi/handle/123456789/10137
dc.rightsOpen
dc.rights.licensecc-by-4.0
dc.title3D data snapshot from a radiative particle-in-cell simulation of plasma turbulence
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