SHOCK - Solar and Heliospheric Collisionless Kinetics

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Turbulence | ExpMir1

ExpMir1 2D expanding box hybrid simulation of mirror instability in the turbulent plasma (Hellinger et al. 2017). Available products: B, B_x, B_y, B_z, Density, P, P_par, P_per, U, U_x, U_y, U_z
Coordinates Z axis parallel to the ambient magnetic field, Y axis parallel to the radial direction. Expansion in X and Z directions.	Initial conditions Initialization with random-phase, Alfvenic fluctuations dB/B_0~0.25, parallel proton beta = 3 and the proton temperature anisotropy 1.2.	Parameters Grid: Nx=1024, Ny=1024 (subgrid of 2048x4096); Time step: dt=0.05/Omega_p. Initial cell size: dx=dy=0.5 d_p0 (twice that one 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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