List of input parameters

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phys_module

parameter default description 180 183 199 600 710 711 712 750
eta 1.d-5 Resistivity at plasma cener (normalized) x x x x x x x x
eta_ohmic 0. Resistivity at core for the Ohmic heating term x x x x x x x x
eta_T_dependent .true. Resistivity dependent on temperature? Otherwise constant x x x x x x x x
eta_coul_log_dep .true. Resistivity dependent on variations of the Coulomb logarithm?       x       x
T_max_eta 1.d99 Temperature above which the resistivity is truncated (use with care; only for numerical reasons)       x        
T_max_eta_ohm 1.d99 Temperature above which the resistivity used in the Ohmic heating term is truncated (use with care; only for numerical reasons)       x        
T_max_visco 1.d99 Temperature above which the viscosity is truncated; It is aimed for keeping the Prandtl number constant when T_max_eta is activated.       x        
visco 1.d-5 Viscosity at plasma center (normalized) x x x x x x x x
visco_heating 0. Viscosity used in the perpendicular viscous heating term       x        
visco_T_dependent .true. Viscosity dependent on temperature? Otherwise constant. x x x x x x x x
visco_old_setup .false. If true, the old perp. viscosity treatment is used for compatibility (old visco depends on R^2)       x        
visco_par 1.d-5 Cross B-field viscosity acting on parallel flow (normalized) x x x x x x x x
visco_par_par 0. B-field Parallel viscosity acting on parallel flow (normalized)   x   x        
visco_par_heating 0. Parallel viscosity used in the parallel viscous heating term (normalized)       x        
TiTe_ratio 0.5 ratio to set ion and electron temperature from T (in model 180): Ti=TiTe_ratioT; Te=(1.0-TiTe_ratio)T x              
F0 10. Determines fixed toroidal magnetic field: $ B_\phi = F_0/R $ x x x x x x x x
central_density 1. particle density at the magnetic axis (in units of $10^{20} m^{-3}$) x x x x x x x x
central_mass 2.01410177811 average ion mass in atomic mass units (constant in time and space, including electron mass) x x x x x x x x
gamma 5. / 3. ratio of specific heat (typically 5/3)         x x x x
tauIC 0. Scaling factor for diamagnetic terms (see [[diamag|diamagnetic]]) x x x x x x x x
Wdia .false. Include diamagnetic flows in viscosity terms? (see [[wdia|here]])       x        
gamma_sheath 4.5 sheath boundary condition on open fieldlines (JOREK units); you can also provide gamma_stangeby in normal units instead! x x x x x x x x
gamma_stangeby -1.d99 Sheath tranmission coefficient given by P. Stangeby in (The plasma boundary of magnetic fusion devices)       x x x x x
gamma_sheath_e 3.00 sheath boundary condition on open fieldlines (JOREK units); you can also provide gamma_stangeby in normal units instead!       x   x x x
gamma_e_stangeby -1.d99 Sheath tranmission coefficient given by P. Stangeby in (The plasma boundary of magnetic fusion devices)       x        
gamma_sheath_i -1.11d-1 sheath boundary condition on open fieldlines (JOREK units); you can also provide gamma_stangeby in normal units instead!       x   x x x
gamma_i_stangeby -1.d99 Sheath tranmission coefficient given by P. Stangeby in (The plasma boundary of magnetic fusion devices)       x        
density_reflection 0. density reflection coeefficient on open fieldlines x x x x        
neutral_reflection 0. reflection coefficient of ions into neutrals (model500)       x     x x
loop_voltage 0. Apply a loop voltage at the boundary of the computational domain (in V; works only for fixed boundary)       x        
old_deuterium_atomic .false. use old fit to calculate atomic coefficients for D (ionization, recombination, radiation), otherwise a better fit is used       x        
deuterium_adas .false. use OPEN ADAS to calculate ionization, recombination and radiation coeffients for deuterium       x        
deuterium_adas_1e20 .false. use OPEN ADAS with fixed density=1e20 to calculate ionization, recombination and radiation coeffients for deuterium       x        
mach_one_bnd_integral .false.         x        
vpar_smoothing .false. apply a smoothing function to smooth jumps in Vpar at B.n=0       x        
vpar_smoothing_coef 0.01, 0., 0. coefficients for the smoothing profile of the parallel velocity       x        
min_sheath_angle 1. For sheath boundary conditions: Minimum incident angle for heat and particle fluxes (in degrees)       x        
mode   Toroidal mode number corresponding to the JOREK modes, e.g., for n_period=8 and n_tor=3, mode(:)=0,8,8 x x x x x x x x
nout 9999999 Output a restart file every nout timesteps x x x x x x x x
nout_projection -1 Output particle projection every nout_projection timesteps (only for diagnostics)       x x x x x
xcase LOWER_XPOINT 1->LowerXpoint. 2->UpperXpoint. 3->doubleNull x x x x x x x x
forceSDN .false. Force a symmetric double null, within the accuracy of SDN_threshold     x x x x x x
SDN_threshold 1.d-4 threshold, in absolute psi, for a symmetric-double-null grid construction x x x x x x x x
rst_format 0 0 == old format, 1 == new format for restart file x x x x        
restart .false. Restart a code run from the restart file jorek_restart.h5? x x x x x x x x
regrid .false. Re-generate the flux-aligned grid (does not work currently)? x x x x x x x x
regrid_from_rz .false. Re-generate the flux-aligned grid from an rz equilibrium x x x x x x x x
xpoint .false. X-point plasma or not? see also xcase x x x x x x x x
Z_xpoint_limit -0.4 0.4 Search the lower X-point in the region Z < Z_xpoint_limit(1) and the upper X-point in the region Z > Z_xpoint_limit(2)       x x x x x
xpoint_search_tries 500 The number of candidate elements to check for being the element containing the upper or lower X-point.     x x x x x x
bootstrap .false. Evolve the Bootstrap current consistently with time? x x x x        
bootstrap_psin_cutoff 0.9995   x x x x        
refinement .false. Use mesh refinement? (not presently available) x x x x x x x x
force_central_node .true. Force all nodes in the center to have the same values in flux aligned grids or independent values? x x x x x     x
fix_axis_nodes .false. Fix t-derivative and cross st-derivative on axis to avoid noise x x x x x x x x
treat_axis .false. > Flag for chosing grid axis treatment (see grids/mod_axis_treatment.f90) x x x x x x x x
bc_natural_flux .false. boundary conditions for flux surface boundaries (2 and 3)         x x x x
bc_natural_open .false. use natural boundary conditions on the open fieldlines x x x x x x x x
produce_live_data .true. Write data 'macroscopic_vars.dat' during the code run allowing to use plot_live_data.sh? x x x x x x x x
grid_to_wall .false. extend the grid to a physical wall x x x x x x x x
RZ_grid_inside_wall .false. build the rectangular grid inside first wall       x x x x x
RZ_grid_jump_thres 0.85 threshold to change R-resolution as RZ-grid gets sqeezed by limiter contour       x x x x x
manipulate_psi_map 0. 99. 99. 0.1 0.1 Option to manipulate Psi_boundary for the initial grid x x x x x x x x
adaptive_time .false. (presently not useful) x x x x x x x x
equil .true. compute equilibrium x x x x x x x x
no_mach1_bc .false. Never apply Mach-1 BCs       x x x x x
Mach1_openBC .true. Full-MHD: Apply Mach-1 BCs inside mod_boundary_matrix_open.f90 (or mod_boundary_conditions.f90)         x x x x
Mach1_fix_B .true. Full-MHD: Use the initial magnetic field for Mach1 BCs on targets, ie. without AR and AZ variations         x     x
export_polar_boundary .false. Option to export boundary.txt even in the case of a polar boundary.       x        
eta_ARAZ_const 0. Use uniform resistivity for AR and AZ equations, used only if eta_ARAZ_on=.false.         x x x x
eta_ARAZ_on .true. Full-MHD: to switch on/off resistive terms for AR and AZ equations         x x x x
eta_ARAZ_simple .false. Full-MHD: remove the Fprof dependence of Bphi in the resistive terms for AR and AZ (which should be compensated by current source anyway)         x x x x
tauIC_ARAZ_on .true. Full-MHD: to switch on/off diamagnetic terms for AR and AZ equations         x x x x
bench_without_plot .false. if .true., do not produce certain output plots (e.g., for benchmarking) x x x x x x x x
gmres   Use iterative GMRES solver x x x x x x x x
gmres_max_iter 200 Maximum number of GMRES iterations x x x x x x x x
keep_n0_const .false. Perform a linear run where the equilibrium quantities (i_tor=1) do not change with time?     x x x x x x
linear_run .false. Same as keep_n0_const, to be replaced soon by true linear run where modes are independent     x x x x x x
export_for_nemec .false. Export equilibrium information for the NEMEC code? x x x x x x x x
export_aux_node_list .true. Include the aux_node_list for particle projections in the restart files     x x x x x x
use_murge .false. (Deprecated, Cannot be used any more) x x x x x x x x
use_murge_element .false. (Deprecated, Cannot be used any more) x x x x x x x x
use_BLR_compression .false. Use Block-Low-Rank (BLR) compression in MUMPS / PaStiX 6 solvers x x x x x x x x
epsilon_BLR 0. Accuracy of BLR compression x x x x x x x x
just_in_time_BLR .true. Use Just-in-time strategy for BLR compression (speed optimized) x x x x x x x x
write_ps .true. Write postscript file at the end of the run x x x x x x x x
use_mumps .false. Use Mumps solver x x x x x x x x
use_pastix .false. Use Pastix solver x x x x x x x x
use_strumpack .true. Use Strumpack solver x x x x x x x x
use_mumps_eq .false. Use Mumps equilibrium solver x x x x x x x x
use_pastix_eq .false. Use Pastix equilibrium solver x x x x x x x x
use_strumpack_eq .false. Use Strumpack equilibrium solver x x x x x x x x
use_mumps_prj .true. Use Mumps projection solver x x x x x x x x
use_pastix_prj .false. Use Pastix projection solver x x x x x x x x
use_strumpack_prj .false. Use Strumpack projection solver x x x x x x x x
use_wsmp .false. Use WSMP solver x x x x        
centralize_harm_mat .true. Centralize harmonic matrices on toridal master ranks; switch for STRUMPACK solver x x x x x x x x
mumps_ordering 7 MUMPS ordering option (7:automatic, 3:Scotch, 4:PORD, 5:METIS), default: 7 x x x x x x x x
pastix_maxthrd 1024 maximum number of threads used by pastix solver (could be beneficial to use the reduced number) x x x x x x x x
pastix_pivot   Pastix epsilon for magnitude control (pivot threshold) x x x x        
use_newton .false. Use inexact Newton method     x x x x x  
maxNewton 20 maximum number of Newton iterations     x x x x x  
gamma_Newton 0.5 Newton gamma-parameter: gmres_tol = gamma_Newton*(normRHScurrent/normRHSprevious)**alpha_Newton     x x x x x  
alpha_Newton 2. Newton alpha-parameter: gmres_tol = gamma_Newton*(normRHScurrent/normRHSprevious)**alpha_Newton     x x x x x  
strumpack_matching .false. Perform maximum-diagonal-product reordering algorithm in STRUMPACK solver (improves direct solver, but use matrix centralization)     x x x x x x
bcs see its wiki page                  
n_limiter 0 Number of limiter points x x x x x x x x
R_limiter 0. R-positions of the limiter points x x x x x x x x
Z_limiter 0. Z-positions of the limiter points x x x x x x x x
first_target_point     x x x x x x x x
last_target_point     x x x x x x x x
gvec_grid_import .false. Generate grid fourier representation with GVEC x x x          
extended_boundary .false. Choose if extended boundary conditions (Biot-Savart version) should be used, default (false) is grad_chi with Dommaschk potentials x              
j_cutoff_rcoord 99.0 Radial location from which the current is set to zero as it approaches the boundary - rcoord corresponds to the normalised toroidal flux x              
j_cutoff_sig 0.025 Radial width over which the current is ramped down to zero towards the boundary x              
eqdsk_psi_fact 1. multiply eqdsk psi by factor for grid_inside_wall       x x x x x
extend_existing_grid .false. Add patches to existing grid from restart file       x x x x x
n_wall_blocks 0 Number of blocks       x x x x x
corner_block 0 =1 for a corner block ("left" side will also be wall-aligned)       x x x x x
n_ext_block 0 Number of 'radial' grid points from the outermost flux surface to wall)       x x x x x
n_ext_equidistant .false. if true, radial spacing of grid points will be equidistant (not adapted)       x x x x x
n_block_points_left 0 Number of points on left side of block       x x x x x
R_block_points_left 0. R-positions of points on left side of block       x x x x x
Z_block_points_left 0. Z-positions of points on left side of block       x x x x x
n_block_points_right 0 Number of points on left side of block       x x x x x
R_block_points_right 0. R-positions of points on left side of block       x x x x x
Z_block_points_right 0. Z-positions of points on left side of block       x x x x x
use_simple_bnd_types .false. convert Stan's bnd_types to Guido's bnd_types       x x x x x
xampl 0. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
xwidth 0. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
xsig 1. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
xtheta 0. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
xshift 0. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
xleft 0. Allows to construct simple X-point cases by coefficients (modifies Psi boundary condition) x x x x x x x x
particlesource 1.e-5 Particle source amplitude x x x x x x x x
particlesource_psin 1.0 Position around which the source is ramped down x x x x x x x x
particlesource_sig 0.1 Width over which the source is ramped down x x x x x x x x
particlesource_gauss 0. Additional Gaussian particle source amplitude x x x x x x x x
particlesource_gauss_psin 0.9 Position around which Gaussian source is set x x x x x x x x
particlesource_gauss_sig 0.1 Width over which Gaussian source is set x x x x x x x x
edgeparticlesource 0. Edge particle source amplitude x x x x x x x x
edgeparticlesource_psin 0.98 Position around which the edge particle source is located x x x x x x x x
edgeparticlesource_sig 0.01 Width over which edge particle source extends x x x x x x x x
neutral_line_source 0. neutral inflow source       x     x x
neutral_line_R_start 1.d20 neutral inflow source (starting point of line source)       x     x x
neutral_line_Z_start 1.d20 neutral inflow source       x     x x
neutral_line_R_end 2.d20 neutral inflow source (end point of line source)       x     x x
neutral_line_Z_end 2.d20 neutral inflow source       x     x x
heatsource 1.e-7 Heat source amplitude x x x x x x x x
heatsource_e 0.5e-7 Electron heat source amplitude x x   x   x x x
heatsource_i 0.5e-7 Ion heat source amplitude x x   x   x x x
heatsource_psin 1.0 Position around which the source is ramped down x x x x x x x x
heatsource_sig 0.1 Width over which the source is ramped down x x x x x x x x
heatsource_e_psin 1.0 Position around which the electron source is ramped down x     x        
heatsource_e_sig 0.1 Width over which the electron source is ramped down x     x        
heatsource_i_psin 1.0 Position around which the ion source is ramped down x     x        
heatsource_i_sig 0.1 Width over which the ion source is ramped down x     x        
heatsource_gauss 0. Additional Gaussian heat source amplitude x x x x x x x x
heatsource_gauss_psin 0.9 Position around which Gaussian source is located x x x x x x x x
heatsource_gauss_sig 0.1 Width over which Gaussian source extends x x x x x x x x
heatsource_gauss_e 0. Gaussian heat source for electrons x x   x   x x x
heatsource_gauss_i 0. Gaussian heat source for ions x x   x   x x x
heatsource_gauss_e_psin 0.9 Position around which electrons Gaussian source is located x x   x        
heatsource_gauss_e_sig 0.1 Width over which electrons Gaussian source extends x x   x        
heatsource_gauss_i_psin 0.9 Position around which ions Gaussian source is located x x   x        
heatsource_gauss_i_sig 0.1 Width over which ions Gaussian source extends x x   x        
constant_imp_source 0. Adds a constant impurity source       x        
eta_num 0.   x x x x x x x x
visco_num 0.   x x x x x x x x
visco_par_num 0.   x x x x x x x x
Dn_perp_num 0.         x     x x
maintain_profiles .false. Add artificial sources to maintain initial rho and T profiles   x            
use_sc .false. Use shock-capturing stabilization       x       x
D_perp_sc_num 0.         x       x
D_par_sc_num 0.         x       x
Dn_pol_sc_num 0.         x       x
Dn_p_sc_num 0.         x       x
D_perp_imp_sc_num 0.         x       x
D_par_imp_sc_num 0.         x       x
ZK_perp_sc_num 0.         x       x
ZK_par_sc_num 0.         x       x
ZK_i_perp_sc_num 0.         x       x
ZK_i_par_sc_num 0.         x       x
ZK_e_perp_sc_num 0.         x       x
ZK_e_par_sc_num 0.         x       x
visco_sc_num 0.         x       x
visco_par_sc_num 0.         x       x
eta_num_T_dependent .false. Hyper-resistivity dependent on temperature? Otherwise constant.       x        
eta_num_psin_dependent .false. Give profile for Hyper-resistivity as function of \psi_N? Useful for 2D current flattening       x        
eta_num_prof 0. 0.8 0.03 Coefficients to specify \psi_N profile for hyper-resistivity       x        
visco_num_T_dependent .false.         x        
add_sources_in_sc .false. Whether to add effect of sources in shock-capturing stabilization or not       x       x
use_vms .false. Use VMS stabilization in model 750 only               x
vms_coeff_AR 0.                 x
vms_coeff_AZ 0.                 x
vms_coeff_A3 0.                 x
vms_coeff_UR 0.                 x
vms_coeff_UZ 0.                 x
vms_coeff_Up 0.                 x
vms_coeff_T 0.                 x
vms_coeff_Te 0.                 x
vms_coeff_Ti 0.                 x
vms_coeff_rho 0.                 x
vms_coeff_rhon 0.                 x
vms_coeff_rhoimp 0.                 x
tstep 1. Size of the timesteps ($ \Delta t $) x x x x x x x x
tstep_n 1. Alternative to tstep: Up to ten values may be given x x x x x x x x
nstep 0 Number of timesteps to perform x x x x x x x x
nstep_n 0 Alternative to nstep: Up to ten values may be given x x x x x x x x
time_evol_scheme 'Crank-Nicholson' Time evolution scheme to use (see [[time-integration|time_integration]]) x x x x x x x x
time_evol_theta   Time evolution parameter theta (see [[time-integration|time_integration]])         x x x x
time_evol_zeta   Time evolution parameter zeta (see [[time-integration|time_integration]])         x x x x
rst_hdf5 1 Write hdf5 restart files if set to 1 x x x x x x x x
rst_hdf5_version   Write which version of hdf5 files? x x x x x x x x
tokamak_device 'none' Name of the tokamak device we are simulating x x x x x x x x
amin 1. Minor radius for polar grid construction, set to 1 if boundary is specified with R,Z points x x x x x x x x
ellip 1. Ellipticity of polar grid (see analytical definition in phys_module.f90) x x x x x x x x
tria_u 0. Upper triangularity of polar grid (see analytical definition in phys_module.f90) x x x x x x x x
tria_l 0. Lower triangularity of polar grid (see analytical definition in phys_module.f90) x x x x x x x x
quad_u 0. Upper quadrangularity of polar grid (see analytical definition in phys_module.f90) x x x x x x x x
quad_l 0. Lower quadrangularity of polar grid (see analytical definition in phys_module.f90) x x x x x x x x
mf 2 Number of entries in fbnd and fpsi x x x x x x x x
fbnd 0.; fbnd(1) = 2. Fourier expansion of boundary x x x x x x x x
fpsi   Fourier expansion of the poloidal flux at the boundary x x x x x x x x
n_boundary 0 Number of points in R_boundary, Z_boundary, psi_boundary. x x x x x x x x
R_boundary 0. Numerical R values defining the boundary x x x x x x x x
Z_boundary 0. Numerical Z values defining the boundary x x x x x x x x
psi_boundary 0. Numerical values giving the poloidal flux at the boundary x x x x x x x x
n_pfc 0 Number of coils, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
Rmin_pfc 0. Minimum R of coil, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
Rmax_pfc 0. Maximum R of coil, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
Zmin_pfc 0. Minimum Z of coil, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
Zmax_pfc 0. Maximum Z of coil, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
current_pfc 0. Current density in the coil, (OLD. for MAST…) use JOREK-STARWALL for coils instead [[jorek-starwall|JOREK-STARWALL]] x x x x        
n_jropes 0 Number of ropes,       x        
R_jropes 0. R centre of rope       x        
Z_jropes 0. Z centre of rope       x        
w_jropes 0. width of rope       x        
current_jropes 0. Current inside the rope       x        
pellet_amplitude 0. amplitude of density source (when pellet modelled as density source) x x x x x x x x
pellet_R 3.8 major radius position pellet x x x x x x x x
pellet_Z 0.0 Z position pellet x x x x x x x x
pellet_phi 1.57 width of the pellet cloud (density source) in toroidal angle x x x x x x x x
pellet_ellipse 5. the ellipticity of the pellet source x x x x        
pellet_radius 0.08 radius of the simulation pellet x x x x x x x x
pellet_sig 0.02 width of smoothing of density source (arctan( (r-pellet_radius)/pellet_sig) ) x x x x x x x x
pellet_length 0.785 width of smoothing of density source in toroidal angle x x x x x x x x
pellet_theta 0. orientation of the pellet ellipse x x x x        
pellet_psi 1.0 pellet_width in poloidal flux x x x x x x x x
pellet_delta_psi 999. width of smoothing in poloidal flux x x x x x x x x
pellet_velocity_R 0. pellet velocity component radial direction x x x x        
pellet_velocity_Z 0. pellet velocity component Z direction x x x x        
pellet_density 5.985d8 pellet atom number density (in units $10^{20} m^{-3}$) x x x x       x
pellet_density_bg 5.958d8 background species pellet atom number density (in units $10^{20} m^{-3}$)       x       x
pellet_particles 0. the number of particles in the pellet (in units of $10^{20}$) x x x x     x x
use_pellet .false.   x x x x     x x
t_ns 2.d3 MGI onset time (JOREK units)       x     x x
ns_amplitude 0. Amplitude of gas source       x     x x
ns_R 3.2 R position of gas source       x     x x
ns_Z 1.5 Z position of gas source       x     x x
ns_phi 1.57 Phi position of gas source       x     x x
ns_radius 0.08 Poloidal radius of gas source       x     x x
ns_deltaphi 0.5 Toroidal extension of gas source       x     x x
ns_delta_minor_rad 0. Extension of gas source in the minor radial direction (if greater than 0.)       x     x x
drift_distance 0. Shift the R position of the neutral deposition outward by drift_distance (in meters) for plasmoid drift       x     x x
energy_teleported 0. Energy (in eV) teleported per atom to consider plasmoid drift effects       x     x x
imp_type ' ' Type of injected material or background impurity species: Argon, neon, …       x       x
use_imp_adas .true. Use open adas to calculate ionization, recombination and radiation coeffients for impurities       x        
JET_MGI .false. Switch to use a JET-like MGI       x     x x
ASDEX_MGI .false. Switch to use an ASDEX-like MGI       x     x x
V_Dmv 9.75d-4 Volume of the DMV reservoir       x     x x
P_Dmv   Pressure in the DMV reservoir (bar)       x     x x
A_Dmv 1.77d-2 Cross sectional area of DMV (Disruption mitigation valve) pipe       x     x x
K_Dmv 4.d-2 Correction parameter describing the gas expansion near the pipe orifice       x     x x
L_tube 0. Pipe length       x     x x
ksi_ion 1.84d-24 Energy cost of each ionization, ksi_ion / mu_0 / (gamma-1) / e = 13.7 eV       x     x x
delta_n_convection 0 Switch to activate the convection term for neutrals (at the plasma velocity)       x     x x
nimp_bg 0. Density of background impurities (in $m^{-3}$)       x     x x
index_main_imp 0 Index of the main impurity species (in imp_type and nimp_bg) solved with continuity equation       x       x
using_spi .false. This determines whether to use SPI or traditional MGI; see [[spi_tutorial|SPI Tutorial]]       x     x x
spi_Vel_Rref 0.0 Reference velocity of pellet center along R upon injection       x     x x
spi_Vel_Zref 0.0 Reference velocity of pellet center along Z upon injection       x     x x
spi_Vel_RxZref 0.0 Reference velocity of pellet center along RxZ direction upon injection       x     x x
spi_quantity 0.0 Total injected atom number for impurity SPI       x     x x
spi_quantity_bg 0.0 Total injected atom number for background species SPI       x       x
ns_radius_ratio 1.4 We are assuming a constant ratio between the radius of NG clouds       x     x x
spi_Vel_diff 0.0 The velocity difference from the reference velocity       x     x x
spi_angle 0.0 The vertex angle of spi spreading in terms of rad       x     x x
spi_L_inj 0.25 Distance between SPI nozzle and ns_R, ns_Z, ns_phi       x     x x
spi_L_inj_diff 0.0 The position difference with respect to the point (ns_R, ns_Z, ns_phi)       x     x x
tor_frequency 0.0 The rigid body rotation frequency       x     x x
ns_radius_min 8.d-2 This defines the minimum radius of neutral cloud for numerical reasons (in m)       x     x x
spi_abl_history_old .false. If this is .t., convert the old spi_abl_history format to the new one upon restart.       x        
n_spi 0 1 Number of shattered fragment injected for each injection       x     x x
n_inj 1 Number of injections       x     x x
spi_abl_model -1 Determine which type of ablation model is used.       x     x x
spi_rnd_seed 0 Random seed array used for the generation of the SPI velocity spread       x     x x
spi_shard_file 'none' The name of the shard size file       x       x
spi_plume_file 'none' The name of the shard information datafile (array)       x       x
spi_plume_hdf5 .false. if 'spi_plume_file' is in HDF5format?       x        
spi_abl_mag_reduction .false. Whether to use the magnetic reduction effect described in Eq.(27) of Nucl. Fusion 60 066027       x        
n_adas 1 Number of species to be traced by ADAS       x       x
spi_tor_rot .false. Flag to turn on a rigid body toroidal plasma rotation for SPI       x     x x
spi_num_vol .true. Flag to turn on numerical integration of the gas source volumes from SPI       x     x x
adas_dir ' ' The directory of ADAS data file to be read       x       x
output_prad_phi .false. Output Prad(phi) into a file using integrals_3D       x       x
amix 0. Mix Poisson solution with previous one with a given factor x x x x x x x x
equil_accuracy 1.d-6 Tolerance of the convergence for the fix-boundary equilibrium x x x x x x x x
axis_srch_radius 99. Magnetic axis will be searched inside a circle with this radius x x x x x x x x
delta_psi_GS 10000. Expected psi_bnd - psi_axis for the final equilibrium     x x x x x x
newton_GS_fixbnd .false. Newton instead of Picard iterations for fixed-boundary equilibria?     x x x x x x
newton_GS_freebnd .true. Newton instead of Picard iterations for free-boundary equilibria?     x x x x x x
freeboundary_equil .false. use a free or fixed boundary equilibrium? ([[jorek-starwall|JOREK-STARWALL]]) x x x x x x x x
freeboundary .false. use free or fixed boundary conditions in time-evolution? ([[jorek-starwall|JOREK-STARWALL]]) x x x x x x x x
resistive_wall .false. use a resistive or ideal wall? ([[jorek-starwall|JOREK-STARWALL]]) x x x x x x x x
freeb_equil_iterate_area .false. iterate to a target area during freeboundary equilibrium limiter cases [[jorek-starwall-faqs|jorek_starwall]] x x x x x x x x
amix_freeb 0.85 choose amix for freeboundary equilibrium x x x x x x x x
equil_accuracy_freeb 1.d-6 Tolerance of the convergence for the freeboundary equilibrium x x x x x x x x
freeb_change_indices .true. Exchange grid node indices to parallelize boundary integral x x x x x x x x
n_R 0 Number of grid points in R-direction (for rectangular grid) (see also [[grids#tutorials|here]]) x x x x x x x x
n_Z 0 Number of grid points in Z-direction (for rectangular grid) x x x x x x x x
R_begin -0.1 Left boundary of grid in R-direction (for rectangular grid) x x x x x x x x
R_end 0.1 Right boundary of grid in R-direction (for rectangular grid) x x x x x x x x
Z_begin -0.1 Lower boundary of grid in Z-direction (for rectangular grid) x x x x x x x x
Z_end 0.1 Upper boundary of grid in Z-direction (for rectangular grid) x x x x x x x x
rect_grid_vac_psi 0. Use a vacuum psi-bnd condition for squared-grid, ie. (rect_grid_vac_psi * R**2)       x        
force_horizontal_Xline .false. Force the grid line through Xpoint to be horizontal (instead of perp. to line between Xpoint and axis) x x x x x x x x
n_radial 11 Number of radial grid points (for polar grid) (see also [[grids|here]]) x x x x x x x x
n_pol 16 Number of poloidal grid points (for polar grid) x x x x x x x x
R_geo 10. Center of the grid (for polar grid) x x x x x x x x
Z_geo 0. Center of the grid (for polar grid) x x x x x x x x
psi_axis_init -0.1 Initial guess for Psi at the magnetic axis (for polar grid) x x x x x x x x
XR_r 999. Psi_N position of radial grid accumulation (two positions) (for polar grid) (also used for R-position in square-grid) x x x x x x x x
SIG_r 999. Width of grid accumulation (two positions) (for polar grid) (also used for R-width in square-grid) x x x x x x x x
XR_tht 999. Position of poloidal grid accumulation (0…1, two positions) (for polar grid) x x x x x x x x
SIG_tht 999. Width of grid accumulation (two positions) (for polar grid) x x x x x x x x
XR_z 999. Z-position of square grid accumulation (two positions) (for square grid)       x        
SIG_z 999. Z-Width of grid accumulation (two positions) (for square grid)       x        
bgf_r 0.7         x        
bgf_z 0.7 Background for meshac distribution for R-Z accumulation       x        
bgf_rpolar 0.6       x x x x x x
bgf_tht 0.6 Background for meshac distribution for R-theta accumulation     x x x x x x
n_flux 11 Number of radial grid points (for flux-aligned grid) (see also [[grids#tutorials|here]]) x x x x x x x x
n_tht 16 Number of poloidal grid points (for flux-aligned grid) x x x x x x x x
xr1 9999. Grid accumulation parameter (for flux-aligned grid) x x x x x x x x
xr2 99999. Grid accumulation parameter (for flux-aligned grid) x x x x x x x x
sig1 9999. Grid accumulation parameter (for flux-aligned grid) x x x x x x x x
sig2 99999. Grid accumulation parameter (for flux-aligned grid) x x x x x x x x
m_pol_bc 1 Number of poloidal modes for Psi boundary condition in stellarator x              
i_plane_rtree 1 The poloidal plane in a stellarator on which the RTree is to be built (RZ_minmax refers to this plane) x x            
n_open 5 Number of 'radial' grid points in the open flux region - between the two separatrices if double-null x x x x x x x x
n_outer 0 Number of 'radial' grid points in the open flux region on the outer side (LFS) if double-null x x x x x x x x
n_inner 0 Number of 'radial' grid points in the open flux region on the inner side (HFS) if double-null x x x x x x x x
n_private 5 Number of 'radial' grid points in the private flux region at the bottom x x x x x x x x
n_leg 5 Number of 'poloidal' grid points along the divertor legs at the bottom x x x x x x x x
n_leg_out 0 Number of 'poloidal' grid points along the divertor legs at the bottom on the LFS       x x x x x
n_up_priv 0 Number of 'radial' grid points in the private flux region at the top (upper Xpoint or double-null) x x x x x x x x
n_up_leg 0 Number of 'poloidal' grid points along the divertor legs at the top (upper Xpoint or double-null) x x x x x x x x
n_up_leg_out 0 Number of 'poloidal' grid points along the divertor legs on the top on the LFS (upper Xpoint or double-null)       x x x x x
n_ext 0 Number of 'radial' grid points from the outermost flux surface to wall) x x x x x x x x
n_tht_equidistant .false. switch on to get an equidistant poloidal distribution of elements in the core of the grid (psi<0.5)       x x x x x
xr_closed 1.0, 9999., 9999. Location for grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_closed 0.1, 9999., 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_open 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_outer 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_inner 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_private 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_up_priv 0.1 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_theta 0.03 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_theta_up 999. Width with grid accumulation (for flux-aligned grid; only valid for double-null)     x x x x x x
SIG_leg_0 0.05 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_leg_1 0.2 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_up_leg_0 0.05 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
SIG_up_leg_1 0.2 Width with grid accumulation (for flux-aligned grid) x x x x x x x x
dPSI_open 0.11 Delta Psi grid extends into the open flux region (for flux-aligned grid) x x x x x x x x
dPSI_outer 0.11 Delta Psi grid extends into the open flux region (for flux-aligned grid) x x x x x x x x
dPSI_inner 0.11 Delta Psi grid extends into the open flux region (for flux-aligned grid) x x x x x x x x
dPSI_private 0.03 Delta Psi grid extends into the private flux region (for flux-aligned grid) x x x x x x x x
dPSI_up_priv 0.03 Delta Psi grid extends into the private flux region (for flux-aligned grid) x x x x x x x x
D_perp 1.d-5, 0., 0., 99., 99. Coefficients for perpendicular particle diffusion profile x x x x x x x x
D_par 0. Parallel particle diffusion (usually not useful) x x x x x x x x
V_pinch_gauss 0. Amplitude of Gaussian inward pinch velocity profile for background fluid (rho only).       x        
V_pinch_psin 0. Centre of V_pinch Gaussian in normalised poloidal flux (psin).       x        
V_pinch_sig 1. Width (sigma) of V_pinch Gaussian in psin units.       x        
D_perp_imp 1.d-5, 0., 0., 99., 99. Coefficients for perpendicular imp particle diffusion profile       x       x
D_par_imp 0. Parallel impurity particle diffusion (usually not useful)       x       x
ZK_perp 1.d-5, 0., 0., 99., 99. Coefficients for perpendicular heat diffusion profile x x x x x x x x
ZK_par 1. Parallel heat diffusion value in the plasma center x x x x x x x x
ZK_par_max 1.d20 Do not use larger parallel heat diffusion values for numerical reasons x x x x x x x x
T_min_ZKpar -1.d12 Do not use smaller parallel heat diffusion values below this MHD temperature (Ti+Te); JOREK units       x        
Ti_min_ZKpar -1.d12 Do not use smaller parallel heat diffusion values below Ti; JOREK units       x        
Te_min_ZKpar -1.d12 Do not use smaller parallel heat diffusion values below Te; JOREK units       x        
ZK_i_perp 1.d-5, 0., 0., 99., 99. Coefficients for perpendicular ion heat diffusion profile   x   x   x x x
ZK_e_perp 1.d-5, 0., 0., 99., 99. Coefficients for perpendicular electron heat diffusion profile   x   x   x x x
ZK_i_par 1. Ion parallel heat diffusion coefficient in the plasma center   x   x   x x x
ZK_e_par 1. Electron parallel heat diffusion coefficient in the plasma center   x   x   x x x
D_neutral_x 1.d-5 Neutral particle diffusivity in R-direction       x     x x
D_neutral_y 1.d-5 Neutral particle diffusivity in Z-direction       x     x x
D_neutral_p 1.d-5 Neutral particle diffusivity in phi-direction       x     x x
ZKpar_T_dependent .true. Use a temperature dependent parallel heat diffusivity x x x x x x x x
d_perp_file 'none' ASCII file with perpendicular particle diffusion profile x x x x        
zk_perp_file 'none' ASCII file with perpendicular heat diffusion profile x x x x        
zk_e_perp_file 'none' ASCII file with perpendicular electron heat diffusion profile       x        
zk_i_perp_file 'none' ASCII file wtih perpendicular ion heat diffusion profile       x        
v_pinch_file 'none' ASCII file with inward pinch velocity profile (psin, V_pinch columns)       x        
rho_0 1. Central normalized density (usually 1) x x x x x x x x
rho_1 1. SOL normalized density x x x x x x x x
rho_coef 0.; rho_coef(1) = 0. Density profile coefficients x x x x x x x x
rho_file 'none' ASCII file the density profile is read from. x x x x x x x x
T_0 1.d-6 Central normalized temperature x x x x x x x x
T_1 1.d-8 SOL normalized temperature x x x x x x x x
T_coef 0.; T_coef(1) = -1. Temperature profile coefficients x x x x x x x x
Ti_0 5.d-7 Central ion normalized temperature x x   x   x x x
Ti_1 5.d-9 SOL ion normalized temperature x x   x   x x x
Ti_coef 0.; Ti_coef(1) = -1. Ion temperature profile coefficients x x   x   x x x
Te_0 5.d-7 Central ion normalized temperature x x   x   x x x
Te_1 5.d-9 SOL ion normalized temperature x x   x   x x x
Te_coef 0.; Te_coef(1) = -1. Ion temperature profile coefficients x x   x   x x x
T_file 'none' ASCII file the temperature profile is read from. x x x x x x x x
Ti_file 'none' ASCII file the ion temperature profile is read from.       x   x x x
Te_file 'none' ASCII file the electron temperature profile is read from.       x   x x x
rhon_0 0. Central value for the initial normalized neutral density       x        
rhon_1 0. SOL value for the initial normalized neutral density       x        
rhon_coef 0. 0.01 0.01 Coefficients for the intitial neutral density profile       x        
Fprofile_file 'none' ASCII file the Fprofile is read from.         x x x x
phi_0 0. Central background potential; (usually 1) x x            
phi_1 0. Edge background potential x x            
phi_coef 0.; phi_coef(1) = 0.; phi_coef(4) = 1. potential profile coefficients x x            
phi_file 'none' ASCII file the potential profile is read from. x x            
nu_phi_source 0. Friction coefficient of the n=0 background potential profile source term (>~ visco)   x            
FF_0 1. FF' value in the plasma center x x x x x x x x
FF_1 0. FF' value in the SOL x x x x x x x x
FF_coef 0.; FF_coef(1) = -1. Coefficients for FF' profile x x x x x x x x
ffprime_file 'none' ASCII file the FF' profile is read from. x x x x x x x x
NEO .false. If .true. neoclassical effects are considered, (see [[neo|here]]) x x x x x x x x
neo_file 'none' ASCII file the aki and amu profiles is read from. x x x x x x x x
aki_neo_const 0. if ( (NEO) .and. (neo_file=='none') ), this constant value is used for aki_neo x x x x x x x x
amu_neo_const 0. if ( (NEO) .and. (neo_file=='none') ), this constant value is used for amu_neo x x x x x x x x
output_bnd_elements .false. If .true., writes bnd nodes and bnd elements in files 'boundary_nodes.dat' and 'boundary_elements.dat' x x x x x x x x
RMP_on .false. Activates RMPs on boundary if .true. (the old version without STARWALL) x x x x        
RMP_psi_cos_file 'none' ASCII file the profiles of psi_RMP_cos and derivatives are read from x x x x        
RMP_psi_sin_file 'none' ASCII file the profiles of psi_RMP_sin and derivatives are read from x x x x        
RMP_growth_rate 0.011   x x x x        
RMP_ramp_up_time 1000 parameters for time dependence of psi_RMP: Sigmoid f(t)= 1/ (1 + exp(-RMP_growth_rate*(t-RMP_ramp_up_time/2) )) x x x x        
RMP_har_cos 2   x x x x        
RMP_har_sin 3   x x x x        
Number_RMP_harmonics 1 Number_RMP_harmonics < N_RMP_max. If only one harmonic, Number_RMP_harmonics=1, by default it's =1 in models/preset_parameters.f90       x        
RMP_har_cos_spectrum RMP_har_cos If only one harmonic,by default RMP_har_cos_spectrum(1)=RMP_har_cos;       x        
RMP_har_sin_spectrum RMP_har_sin If only one harmonic,by default RMP_har_sin_spectrum(1)=RMP_har_sin       x        
V_0 0. analytical parallel rotation profile -- central value x x x x x x x x
V_1 0. analytical parallel rotation profile -- SOL value x x x x x x x x
V_coef 0., 0., 0., 0.1, 1.0 analytical parallel rotation profile -- coefficients x x x x x x x x
R_Z_psi_bnd_file 'none' ASCII file for R_boundary,Z_boundary, psi_boundary, with n_boundary size. x x x x x x x x
wall_file 'wall.txt' ASCII file for external wall geometry, if n_ext is greater than zero. x x x x x x x x
rot_file 'none' ASCII file the parallel rotation profile is read from (see normalized_velocity_profile) x x x x        
normalized_velocity_profile .true. if true, reads the normalized velocity profile as flux function, else Omega_tor is read as flux function. x x x x        
domm_file 'none' Namelist file containing the coefficients for Dommaschk potentials x x            
iter_precon 10 whenever the number of gmres iterations exceeds iter_precon, the preconditioning matrix is updated x x x x x x x x
max_steps_noUpdate 10000000 whenever the steps without preconditioning matrix update exceeds max_steps_noUpdate, the preconditioning matrix is updated x x x x x x x x
gmres_m 20 gmres restart parameter (dimension) x x x x x x x x
gmres_4 1.d3 see gmres manual (error ratio between preconditioned and non-preconditioned error) x x x x x x x x
gmres_tol 1.d-8 the tolerance for the gmres iterations to be seen as converged x x x x x x x x
tgnum 0. Coefficients for Taylor Galerkin stabilization for each equation separately x x x          
tgnum_psi 0. Same as previous line, but avoiding equation indexing for model families       x        
tgnum_u 0.         x        
tgnum_zj 0.         x        
tgnum_w 0.         x        
tgnum_rho 0.         x        
tgnum_T 0.         x        
tgnum_Ti 0.         x        
tgnum_Te 0.         x        
tgnum_vpar 0.         x        
tgnum_rhon 0.         x        
tgnum_rhoimp 0.         x        
tgnum_nre 0.         x        
tgnum_AR 0.         x        
tgnum_AZ 0.         x        
tgnum_A3 0.         x        
keep_current_prof .true. Artificial current source to approximately keep the initial current profile, i.e., $\eta(j-j0)$? x x x x x x x x
init_current_prof .false. Initialize the current source from the current profile present x x            
D_prof_neg 1.d-5 Particle diffusion coefficient in regions with negative background species density x x x x        
D_prof_neg_thresh 0. D_prof_neg becomes effective if r0-rimp0 < D_prof_neg_thresh x x x x        
D_prof_imp_neg_thresh -1.d3 D_prof_neg becomes effective if rimp0 < D_prof_imp_neg_thresh       x        
D_prof_tot_neg_thresh 0. D_prof_neg becomes effective if r0 < D_prof_tot_neg_thresh       x        
ZK_prof_neg 1.d-5 Perp. heat diffusion coefficient in regions with negative temperature x x x x        
ZK_par_neg 1.d-3 Parallel diffusion coefficient in regions with negative temperature       x        
ZK_prof_neg_thresh 0. ZK_prof_neg becomes effective if T < ZK_prof_neg_thresh x x x x        
ZK_par_neg_thresh 0. ZK_par_neg becomes effective if T < ZK_par_neg_thresh       x        
ZK_e_prof_neg 1.d-5 Perp. heat diffusion coefficient in regions with negative temperature       x        
ZK_e_par_neg 1.d-3 Parallel diffusion coefficient in regions with negative temperature       x        
ZK_e_prof_neg_thresh 0. ZK_e_prof_neg becomes effective if T < ZK_e_prof_neg_thresh       x        
ZK_e_par_neg_thresh 0. ZK_e_par_neg becomes effective if T < ZK_e_par_neg_thresh       x        
ZK_i_prof_neg 1.d-5 Perp. heat diffusion coefficient in regions with negative temperature       x        
ZK_i_par_neg 1.d-3 Parallel diffusion coefficient in regions with negative temperature       x        
ZK_i_prof_neg_thresh 0. ZK_i_prof_neg becomes effective if T < ZK_i_prof_neg_thresh       x        
ZK_i_par_neg_thresh 0. ZK_i_par_neg becomes effective if T < ZK_i_par_neg_thresh       x        
D_imp_extra_neg_thresh -1.d3 D_imp_extra_neg becomes effective if rho_imp < D_imp_extra_neg_thresh       x        
T_min 1.0d-20 minimum temperature (limits on the temperature dependence of resistivity etc.) value in jorek units: 2.01d-5central_densityTmin_ev (preset central_density = 1, 20 eV) x x x x x x x x
rho_min 1.0d-20 minimum density     x x x x x x
ne_SI_min 1.d18 minimum e density (in SI unit) below which we cut-off the radiation loss       x        
Te_eV_min 5. minimum temperature (in eV) below which we cut-off the radiation loss       x       x
rn0_min 1.d-8 minimum impurity density (in JU) for radiation loss cut-off       x        
T_min_neg -1.d12 minimum temperature,used for correcting negative values,in jorek units: 2.01d-5central_densityTmin_ev (preset central_density = 1, 20 eV)     x x x x x x
rho_min_neg -1.d12 minimum density, used for correcting negative values     x x x x x x
implicit_heat_source 0. Choose = 1.d0 to fully switch on the implicit heat source for numerical stabilization       x        
n_tor_fft_thresh 2 If n_tor >= n_tor_fft_thresh, element_matrix_fft will be used x x x x x x x x
corr_neg_temp_coef 0.5, 0.5 Parameters used in models/corr_neg.f90 x x x x x x x x
corr_neg_dens_coef 0.5, 0.5 Parameters used in models/corr_neg.f90 x x x x x x x x
thermalization .true. If true turns on the ion-electron thermalization term       x   x x x
zjz_0 0.1173   x x x x x x x x
zjz_1 0.0   x x x x x x x x
zj_coef 0.; zj_coef(1) = -1.   x x x x x x x x

vacuum

parameter default description 180 183 199 600 710 711 712 750
CARIDDI_mode .false. CARIDDI or STARWALL;True if CARIDDI input file     x x x x x x
vacuum_min .false. Mode to minimalize memory consumption     x x x x x x
wall_resistivity_fact 1. Scaling factor for the wall and coil resistivities specified in STARWALL x x x x        
wall_resistivity 0. Resistivity of the external wall x x x x        
n_pf_coils 0 number of poloidal field coils x x x x x x x x
starwall_equil_coils .false. specify wheter the equilibrium PF coils will be given by STARWALL or not x x x x x x x x
find_pf_coil_currents .false. search for optimal pf_coil currents to build a free-bnd equil? [[jorek-starwall-faqs|fbnd_eq_FAQs]] x x x x x x x x
psi_offset_freeb 0. Allows to shift the value of psi by a global constant for freeb_equil (improves convergence) x x x x x x x x
current_ref 1.d22 Target total plasma current Ip for the feedback (FB) [[jorek-starwall-faqs|fbnd_eq_FAQs]] x x x x x x x x
FB_Ip_position 0.2 Amplification factor for Ip feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
FB_Ip_integral 0.01 Amplification factor for Ip feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
Z_axis_ref 1.d22 Target magnetic axis vertical position (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
R_axis_ref -99. Optional target magnetic axis radial position (see [[jorek-starwall-faqs|fbnd_eq_FAQs]])     x x x x x x
FB_Zaxis_position 1. Amplification factor for Zaxis feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
FB_Zaxis_derivative 0. Amplification factor for Zaxis feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
FB_Zaxis_integral 0. Amplification factor for Zaxis feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
cte_current_FB_fact -1d99 Constant factor that scales FF'& T profiles before freebnd GS iterations (switches off current FB)     x x x x x x
start_VFB 10 Iteration for starting vertical feedback (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
n_feedback_current 2 Feedback will be performed each n_… iterations (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
n_feedback_vertical 1 Feedback will be performed each n_… iterations (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
n_iter_freeb 900 Number of iterations for freeboundary equilibirum (see [[jorek-starwall-faqs|fbnd_eq_FAQs]]) x x x x x x x x
diag_coils   see [[jorek-starwall-faqs|jorek_starwall_FAQs]] x x x x x x x x
rmp_coils   see [[jorek-starwall-faqs|jorek_starwall_FAQs]] x x x x x x x x
voltage_coils   not ready yet (see [[jorek-starwall-faqs|jorek_starwall_FAQs]]) x x x x x x x x
pf_coils 0 see [[jorek-starwall-faqs|jorek_starwall_FAQs]] x x x x x x x x
vert_FB_amp   Tune direction and magnitude of vert feedback for each poloidal field coil ([[jorek-starwall-faqs|eq_FAQs]]) x x x x x x x x
rad_FB_amp   Tune direction and magnitude of vert feedback for each poloidal field coil ([[jorek-starwall-faqs|eq_FAQs]])     x x x x x x
vert_pos_file     x x x x x      
start_VFB_ts 0. start time of active VFB during simulation ([JOREK units]) x x x x x      
vert_FB_amp_ts 0. Amplitude and sign of vert feedback for each coil ([[jorek-starwall-faqs|eq_FAQs]]);amplification factor (of PF coil) x x x x x      
I_coils_max 1.d99 Current limit of each coil ([Ampere]);Maximum absolute value for coils x x x x x      
vert_FB_gain 0. Gain parameters for vertical feedback controller;Proportional, derivative, integral gain of VFB controller x x x x x      
vert_FB_tact 1.d-9 Time interval between two controller actions ([JOREK units]);Tact of VFB controller x x x x x