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Commit a67434b8 authored by Antoine Cyril David Hoffmann's avatar Antoine Cyril David Hoffmann
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added kr parameter for MOLI

parent 0eaffa97
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%% Run MOLI for a scan in kperp
%% Move to MOLI workspace
cd ../../MoliSolver/MOLI/workspace/
%% Add paths
......@@ -91,7 +92,8 @@ params.nu = MODEL.nu; % electron/ion collision frequency ... on
params.nuoveromegapemax = inf; % Maximum ratio between electron/ion collision frequency and electron plasma frequency [See Banks et al. (2017)]. Set to inf if not desired !!!
params.mu = MODEL.sigma_e; % sqrt(m_e/m_i)
params.kpar = 0.0; % normalized parallel wave number to the major radius
params.kperp = GRID.kzmin; % normalized perpendicular wave number to the soundLarmor radius. Note: If ions ==0 (e.g. EPW), kperp --> b
params.kperp = GRID.kzmin; % normalized perpendicular toroidal wave number to the soundLarmor radius. Note: If ions ==0 (e.g. EPW), kperp --> b
params.kr = GRID.krmin; % Radial component of perpendicular vector
params.alphaD = 0.0; % (k*Debye length)^2
params.Rn = MODEL.eta_n; % Major Radius / Background density gradient length
params.RTe = MODEL.eta_T; % Major Radius * normalized kperp / Background electron temperature gradient length
......
%% Run MOLI for a time evolution of the moments at a given kperp
%% Move to MOLI workspace
cd ../../MoliSolver/MOLI/workspace/
%% Add paths
......@@ -91,7 +92,8 @@ params.nu = MODEL.nu; % electron/ion collision frequency ... on
params.nuoveromegapemax = inf; % Maximum ratio between electron/ion collision frequency and electron plasma frequency [See Banks et al. (2017)]. Set to inf if not desired !!!
params.mu = MODEL.sigma_e; % sqrt(m_e/m_i)
params.kpar = 0.0; % normalized parallel wave number to the major radius
params.kperp = GRID.kzmin; % normalized perpendicular wave number to the soundLarmor radius. Note: If ions ==0 (e.g. EPW), kperp --> b
params.kperp = GRID.kzmin; % normalized perpendicular toroidal wave number to the soundLarmor radius. Note: If ions ==0 (e.g. EPW), kperp --> b
params.kr = GRID.krmin; % Radial component of perpendicular vector
params.alphaD = 0.0; % (k*Debye length)^2
params.Rn = MODEL.eta_n; % Major Radius / Background density gradient length
params.RTe = MODEL.eta_T; % Major Radius * normalized kperp / Background electron temperature gradient length
......
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