Mercurial > repos > public > sbplib
view +time/SBPInTimeSecondOrderForm.m @ 774:66eb4a2bbb72 feature/grids
Remove default scaling of the system.
The scaling doens't seem to help actual solutions. One example that fails in the flexural code.
With large timesteps the solutions seems to blow up. One particular example is profilePresentation
on the tdb_presentation_figures branch with k = 0.0005
author | Jonatan Werpers <jonatan@werpers.com> |
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date | Wed, 18 Jul 2018 15:42:52 -0700 |
parents | c92d2f8319c2 |
children | b5e5b195da1e |
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classdef SBPInTimeSecondOrderForm < time.Timestepper properties A,B,C M, f n t k firstOrderTimeStepper end methods % Solves u_tt = Au + Bu_t + C % A, B can either both be constants or both be function handles, % They can also be omitted by setting them equal to the empty matrix. function obj = SBPInTimeSecondOrderForm(A, B, C, k, t0, v0, v0t, TYPE, order, blockSize) default_arg('TYPE', []); default_arg('order', []); default_arg('blockSize',[]); m = length(v0); default_arg('A', sparse(m, m)); default_arg('B', sparse(m, m)); default_arg('C', sparse(m, 1)); I = speye(m); O = sparse(m,m); obj.M = [ O, I; A, B; ]; obj.f = @(t)[ sparse(m,1); C; ]; w0 = [v0; v0t]; obj.k = k; obj.t = t0; obj.n = 0; obj.firstOrderTimeStepper = time.SBPInTime(obj.M, obj.f, obj.k, obj.t, w0, TYPE, order, blockSize); end function [v,t] = getV(obj) w = obj.firstOrderTimeStepper.getV(); v = w(1:end/2); t = obj.t; end function [vt,t] = getVt(obj) w = obj.firstOrderTimeStepper.getV(); vt = w(end/2+1:end); t = obj.t; end function obj = step(obj) obj.firstOrderTimeStepper.step(); obj.t = obj.firstOrderTimeStepper.t; obj.n = obj.firstOrderTimeStepper.n; end end end