SHOCK - Solar and Heliospheric Collisionless Kinetics

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Kinetic Instabilities | ExpFire1

ExpFire1 2D expanding box hybrid simulation of fire hose instabilities (Hellinger et al., 2003, Hellinger and Travnicek, 2008). Available products: B, B_x, B_y, B_z, Density, P, P_par, P_per, U, U_x, U_y, U_z
Coordinates X axis parallel to the ambient magnetic field and the radial direction. Expansion in Y and Z directions.	Initial conditions Initialization with a homogeneous plasma with beta_p=2.4 and Tper/Tpar=0.7	Parameters Grid: Nx=1024, Ny=512 (subgrid of 2048x1024); Time step: dt=0.05/Omega_p. Initial cell size: dx=dy=d_p (twice that one used in the simulation); NB the system expands in the Y direction.
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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