Mercurial > repos > public > sbplib
view +time/CdiffNonlin.m @ 577:e45c9b56d50d feature/grids
Add an Empty grid class
The need turned up for the flexural code when we may or may not have a grid for the open water and want to plot that solution.
In case there is no open water we need an empty grid to plot the empty gridfunction against to avoid errors.
author | Jonatan Werpers <jonatan@werpers.com> |
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date | Thu, 07 Sep 2017 09:16:12 +0200 |
parents | d1f9dd55a2b0 |
children | b5e5b195da1e |
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classdef CdiffNonlin < time.Timestepper properties D E S k t v v_prev n end methods function obj = CdiffNonlin(D, E, S, k, t0,n0, v, v_prev) m = size(D(v),1); default_arg('E',0); default_arg('S',0); if isnumeric(S) S = @(v,t)S; end if isnumeric(E) E = @(v)E; end % m = size(D,1); % default_arg('E',sparse(m,m)); % default_arg('S',sparse(m,1)); obj.D = D; obj.E = E; obj.S = S; obj.k = k; obj.t = t0; obj.n = n0; obj.v = v; obj.v_prev = v_prev; end function [v,t] = getV(obj) v = obj.v; t = obj.t; end function [vt,t] = getVt(obj) vt = (obj.v-obj.v_prev)/obj.k; % Could be improved using u_tt = f(u)) t = obj.t; end function obj = step(obj) D = obj.D(obj.v); E = obj.E(obj.v); S = obj.S(obj.v,obj.t); m = size(D,1); I = speye(m); %% Calculate for which indices we need to solve system of equations [rows,cols] = find(E); j = union(rows,cols); i = setdiff(1:m,j); %% Calculate matrices need for the timestep % Before optimization: A = 1/k^2 * I - 1/(2*k)*E; k = obj.k; Aj = 1/k^2 * I(j,j) - 1/(2*k)*E(j,j); B = 2/k^2 * I + D; C = -1/k^2 * I - 1/(2*k)*E; %% Take the timestep v = obj.v; v_prev = obj.v_prev; % Want to solve the seq A*v_next = b where b = (B*v + C*v_prev + S); % Before optimization: obj.v = A\b; obj.v(i) = k^2*b(i); obj.v(j) = Aj\b(j); obj.v_prev = v; %% Update state of the timestepper obj.t = obj.t + obj.k; obj.n = obj.n + 1; end end end