Mercurial > hg > octave-lyh
view doc/interpreter/interpimages.m @ 17489:0ad2f93fd83c
doc: Fix a typo in findobj docstring.
* scripts/plot/findobj.m: Use '3' instead of 'D' in findobj example of depth 3.
author | Rik <rik@octave.org> |
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date | Wed, 25 Sep 2013 08:13:30 -0700 |
parents | 333243133364 |
children |
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## Copyright (C) 2007-2012 David Bateman ## ## This file is part of Octave. ## ## Octave is free software; you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation; either version 3 of the License, or (at ## your option) any later version. ## ## Octave is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Octave; see the file COPYING. If not, see ## <http://www.gnu.org/licenses/>. function interpimages (nm, typ) graphics_toolkit ("gnuplot"); set_print_size (); hide_output (); if (strcmp (typ, "png")) set (0, "defaulttextfontname", "*"); endif if (strcmp (typ, "eps")) d_typ = "-depsc2"; else d_typ = ["-d", typ]; endif if (strcmp (typ, "txt")) image_as_txt (nm); elseif (strcmp (nm, "interpft")) t = 0 : 0.3 : pi; dt = t(2)-t(1); n = length (t); k = 100; ti = t(1) + [0 : k-1]*dt*n/k; y = sin (4*t + 0.3) .* cos (3*t - 0.1); yp = sin (4*ti + 0.3) .* cos (3*ti - 0.1); plot (ti, yp, 'g', ti, interp1(t, y, ti, 'spline'), 'b', ... ti, interpft (y, k), 'c', t, y, 'r+'); legend ('sin(4t+0.3)cos(3t-0.1)','spline','interpft','data'); print ([nm "." typ], d_typ); elseif (strcmp (nm, "interpn")) x = y = z = -1:1; f = @(x,y,z) x.^2 - y - z.^2; [xx, yy, zz] = meshgrid (x, y, z); v = f (xx,yy,zz); xi = yi = zi = -1:0.1:1; [xxi, yyi, zzi] = ndgrid (xi, yi, zi); vi = interpn(x, y, z, v, xxi, yyi, zzi, 'spline'); mesh (zi, yi, squeeze (vi(1,:,:))); print ([nm "." typ], d_typ); elseif (strcmp (nm, "interpderiv1")) t = -2:2; dt = 1; ti =-2:0.025:2; dti = 0.025; y = sign(t); ys = interp1(t,y,ti,'spline'); yp = interp1(t,y,ti,'pchip'); plot (ti, ys,'r-', ti, yp,'g-'); legend('spline','pchip', 4); print ([nm "." typ], d_typ); elseif (strcmp (nm, "interpderiv2")) t = -2:2; dt = 1; ti =-2:0.025:2; dti = 0.025; y = sign(t); ddys = diff(diff(interp1(t,y,ti,'spline'))./dti)./dti; ddyp = diff(diff(interp1(t,y,ti,'pchip'))./dti)./dti; plot (ti(2:end-1),ddys,'r*', ti(2:end-1),ddyp,'g+'); legend('spline','pchip'); print ([nm "." typ], d_typ); endif hide_output (); endfunction function set_print_size () image_size = [5.0, 3.5]; # in inches, 16:9 format border = 0; # For postscript use 50/72 set (0, "defaultfigurepapertype", "<custom>"); set (0, "defaultfigurepaperorientation", "landscape"); set (0, "defaultfigurepapersize", image_size + 2*border); set (0, "defaultfigurepaperposition", [border, border, image_size]); endfunction ## Use this function before plotting commands and after every call to ## print since print() resets output to stdout (unfortunately, gnpulot ## can't pop output as it can the terminal type). function hide_output () f = figure (1); set (f, "visible", "off"); endfunction ## generate something for the texinfo @image command to process function image_as_txt(nm) fid = fopen (sprintf ("%s.txt", nm), "wt"); fputs (fid, "\n"); fputs (fid, "+---------------------------------+\n"); fputs (fid, "| Image unavailable in text mode. |\n"); fputs (fid, "+---------------------------------+\n"); fclose (fid); endfunction