SHOCK - Solar and Heliospheric Collisionless Kinetics

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Kinetic Instabilities | Electron Whistler and Mirror Instabilities

Electron Whistler and Mirror Instabilities Electron whistler and mirror instabilities by the electron perpendicular temperature anisotropy (Hellinger and Stverak, 2018). Available products: B, B_x, B_y, B_z, Electron Density, Proton Density, U_e, U_p, U_xe, U_xp, U_ye, U_yp, U_ze, U_zp
Coordinates X axis parallel to the ambient magnetic field.	Initial conditions Initialization with a homogeneous plasma with beta_e=10 and Tper_e/Tpar_e=1.52	Parameters Grid: Nx=1024x1024 (subgrid of 2048x2048), Time step: dt=0.025/Omega_e. Cell size: dx=dy=2*Lamda_e
Simulation presets (no presets available for this simulation)	Products in simulation B - Magnitude of the magnetic field B_x - Magnetic field component Bx B_y - Magnetic field component By B_z - Magnetic field component Bz Electron Density - Electron number density Proton Density - Proton bulk velocity component Dnp U_e - Magnitude of the electron bulk velocity U_p - Magnitude of the proton bulk velocity U_xe - Electron bulk velocity component Uxe U_xp - Proton bulk velocity component Uxp U_ye - Electron bulk velocity component Uye U_yp - Proton bulk velocity component Uyp U_ze - Electron bulk velocity component Uze U_zp - Proton bulk velocity component Uzp

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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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