(luke)¶
LUKE solves the bounce-averaged Fokker-Planck equation in one spatial dimension and two momentum dimensions.
Summary of options¶
Option | Description |
luke interptype |
Interpolation method to use. |
dream logarithmize |
Whether or not to interpolate in the logarithm of the distribution function. |
luke name |
Name of file containing distribution function. |
Example configuration¶
File layout¶
The file containing the LUKE distribution function must contain the variables listed in the table below:
Variable | Description |
betath_ref |
Reference normalized thermal speed \(\beta_\mathrm{th,ref}\) (for de-normalization). |
f |
Distribution function \(f(\psi,\xi,p)\). |
mhu |
Pitch grid in the variable \(\xi = \cos\theta_{\mathrm{p}}\). |
pn |
Momentum grid, with momentum normalized to \(\beta_{\mathrm{th,ref}}\). |
xrhoG |
Radial grid in the variable \(\psi/\psi_a\), i.e. normalized poloidal flux. |
All options¶
-
interptype
¶
Default value: cubic
Allowed values: cubic
orlinear
SOFT interpolates in the given distribution function to evaluate it at arbitrary points on the phase space grid. A linear interpolation scheme is always used to interpolate in the radial coordinate, but interpolation in the momentum coordinates (\(p\) and \(\xi\)) can either be done using bi-linear or bi-cubic splines.
-
logarithmize
¶
Default value: no
Allowed values: yes
orno
If
yes
, interpolates in the logarithm of the distribution function instead of in the distribution function directly. This can aid in fitting sharply decaying ditsribution functions.
-
name
¶
Default value: Nothing Allowed values: Any valid file name Name of the file containing the distribution function.