Detailed descriptionNumerical simulations of kinetic instabilities driven by non Maxwellian distribution functions.

Projects 
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} 

CoordinatesX axis parallel to the ambient magnetic field. 
Initial conditionsInitialization with a homogeneous plasma with beta_e=10 and Tper_e/Tpar_e=1.52 
ParametersGrid: Nx=1024x1024 (subgrid of 2048x2048), Time step: dt=0.025/Omega_e. Cell size: dx=dy=2*Lamda_e 
Simulation presets

Products in simulation


EOF2 Oblique Resonant Electron Fire Hose Driven by the Electron Parallel Temperature Anisotropy (Hellinger et al. 2014). 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} 

CoordinatesX axis parallel to the ambient magnetic field. 
Initial conditionsInitialization with a homogeneous plasma with beta_e=2 and Tper_e/Tpar_e=0.216 
ParametersGrid: Nx=2048x1024, Time step: dt=0.025/Omega_e. Cell size: dx=dy=Lamda_e 
Simulation presets

Products in simulation


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} 

CoordinatesX axis parallel to the ambient magnetic field and the radial direction. Expansion in Y and Z directions. 
Initial conditionsInitialization with a homogeneous plasma with beta_p=2.4 and Tper/Tpar=0.7 
ParametersGrid: 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

Products in simulation

