Layouts Arrays Parameters Grids Calculations
| Type | Intent | Optional | Attributes | Name | ||
|---|---|---|---|---|---|---|
| complex, | intent(in), | dimension(:, :, kxkyz_lo%llim_proc:) | :: | g | ||
| complex, | intent(inout), | dimension(:, :, -nzgrid:, :) | :: | phi | ||
| complex, | intent(inout), | dimension(:, :, -nzgrid:, :) | :: | apar | ||
| complex, | intent(inout), | dimension(:, :, -nzgrid:, :) | :: | bpar | ||
| character(len=*), | intent(in) | :: | dist |
If we are parallelising over (vpa,mu) then this subroutine is called
This is the more common version used compared with parallelising over
(kx,ky,z) and is the default for stella.
This advances the fields when Electromagnetic effects are included, so
we advance
| Type | Intent | Optional | Attributes | Name | ||
|---|---|---|---|---|---|---|
| complex, | intent(in), | dimension(:, :, -nzgrid:, :, vmu_lo%llim_proc:) | :: | g | ||
| complex, | intent(out), | dimension(:, :, -nzgrid:, :) | :: | phi | ||
| complex, | intent(out), | dimension(:, :, -nzgrid:, :) | :: | apar | ||
| complex, | intent(out), | dimension(:, :, -nzgrid:, :) | :: | bpar | ||
| character(len=*), | intent(in) | :: | dist |