Mercurial > repos > public > sbplib
view +time/SBPInTimeSecondOrderFormImplicit.m @ 1198:2924b3a9b921 feature/d2_compatible
Add OpSet for fully compatible D2Variable, created from regular D2Variable by replacing d1 by first row of D1. Formal reduction by one order of accuracy at the boundary point.
author | Martin Almquist <malmquist@stanford.edu> |
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date | Fri, 16 Aug 2019 14:30:28 -0700 |
parents | 66eb4a2bbb72 |
children | 8894e9c49e40 |
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classdef SBPInTimeSecondOrderFormImplicit < time.Timestepper properties A, B, C, f AA, BB, ff n t k firstOrderTimeStepper end methods % Solves A*u_tt + B*u_t + C*u = f(t) % 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 = SBPInTimeSecondOrderFormImplicit(A, B, C, f, k, t0, v0, v0t, do_scaling, TYPE, order, blockSize) default_arg('f', []); default_arg('TYPE', []); default_arg('order', []); default_arg('blockSize',[]); default_arg('do_scaling', false); m = length(v0); default_arg('A', speye(m, m)); default_arg('B', sparse(m, m)); default_arg('C', sparse(m, m)); I = speye(m); O = sparse(m,m); % Rewrite to % AA*w_t = BB*w + ff(t); obj.AA = [ I, O; O, A; ]; obj.BB = [ O, I; -C, -B; ]; if ~isempty(f) obj.ff = @(t)[ sparse(m,1); f(t); ]; else obj.ff = @(t) sparse(2*m,1); end w0 = [v0; v0t]; obj.k = k; obj.t = t0; obj.n = 0; if do_scaling scaling = [ones(m,1); sqrt(diag(C))]; obj.firstOrderTimeStepper = time.SBPInTimeScaled(obj.AA, obj.BB, obj.ff, obj.k, obj.t, w0, scaling, TYPE, order, blockSize); else obj.firstOrderTimeStepper = time.SBPInTimeImplicitFormulation(obj.AA, obj.BB, obj.ff, obj.k, obj.t, w0, TYPE, order, blockSize); end 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