12/2008
3D MHD simulations of counter-helicity spheromak merging.
Re-run of 2005 10V RCC case. Initial conditions from M. Schaffer file "fort_CtrGun10V.41". Normalized resistivity eta=1e-3, normalized viscosity mu=2e-3. Grid size nz=129, nr=65, nphi=32, number of time frames=36.
Pressure file (Compressed 20M, use Unix 'uncompress' command)
Data format: nz,nr,nphi,nt, z(nz),r(nr),phi(nphi),time(nt), p(nz,nr,nphi,nt)
Magnetic field file(Compressed 100M)
Data format: nz,nr,nphi,nt, z(nz),r(nr),phi(nphi),time(nt), v1(nz,nr,nphi,nt), v2(nz,nr,nphi,nt), v3(nz,nr,nphi,nt)
09/2013
S*=8 Equilibrium file (Assumes V_i=0, T_e=0, mirror ratio=1)
07/2014
B is normalized to B0, V is normalized to V_A, density to n_0, t_a=15.5 [1/omega_ci]
3D M.field file t=400.[1/omega_ci]
Time evolution of n=0-4 Fourier harmonics
10/2014 using Python script with default n0 and B0
Case 1 with C2-like equilibrium and periodic BC; n=1 wobble mode most unstable
8/2015 SILO files for VisIt plots
Case 1 with rmirror=1 equilibrium and non-symmetric BC; n=1 wobble mode most unstable
Case 2 with C2-like equilibrium with strong beam and periodic BC; n=2 mode most unstable
Case 3 with rmirror=3 equilibrium no beam; n=1 wobble mode most unstable