SHOCK - Solar and Heliospheric Collisionless Kinetics

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Turbulence | ExpTurb3D

ExpTurb3D 3D hybrid expanding box simulation of plasma turbulence and fire hose instabilities, see Hellinger et al. (ApJ, 2019). Available products: B, B_x, B_y, B_z, Density, P, P_par, P_per, U, U_x, U_y, U_z
Coordinates X and Y axes perpendicular to the ambient magnetic field.	Initial conditions Initialization with balanced large-scale Alvenic modes with dB_rms=0.25 B_0.	Parameters Grid: Nx=Ny=Nz=256 (subgrid of 512x512x256); Time step: dt=0.05/Omega_p. Cell size: dx=dy=dz=0.5 d_p (dx and dy are double of 0.25 d_p used in the simulation)
Simulation presets (no presets available for this simulation)	Products in simulation B - Magnitude of the magnetic field B_x - X component of the magnetic field B_y - Y component of the magnetic field B_z - Z component of the magnetic field Density - Proton number density P - Total proton pressure P_par - Parallel proton pressure P_per - Perpendicular proton pressure U - Magnitude of the proton bulk velocity U_x - X component of the proton bulk velocity U_y - Y component of the proton bulk velocity U_z - Z component of the proton bulk velocity

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Author of the data: SHOCK Team | The portal is created under the SHOCK Project of the FP7 (EC)

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