Mercurial > repos > public > sbplib
view +time/CdiffTimeDep.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 | 151ab2b5a686 |
children | 8894e9c49e40 |
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classdef CdiffTimeDep < time.Timestepper properties D E S k t v v_prev n end methods % Solves u_tt = Du + E(t)u_t + S(t) % D, E, S can either all be constants or all be function handles, % They can also be omitted by setting them equal to the empty matrix. % CdiffTimeDep(D, E, S, k, t0, n0, v, v_prev) function obj = CdiffTimeDep(D, E, S, k, t0, n0, v, v_prev) m = length(v); default_arg('E', @(t)sparse(m,m)); default_arg('S', @(t)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) [obj.v, obj.v_prev] = time.cdiff.cdiff(obj.v, obj.v_prev, obj.k, obj.D, obj.E(obj.t), obj.S(obj.t)); obj.t = obj.t + obj.k; obj.n = obj.n + 1; end end end