Mercurial > hg > octave-nkf
view scripts/plot/comet.m @ 17122:eaab03308c0b
doc: Rewrite docstrings for most plot functions.
Emphasize clarity, use common "voice", and increase density of seealso links.
* doc/interpreter/plot.txi: Add @findex entries that were in xlim.m
* scripts/miscellaneous/getappdata.m scripts/miscellaneous/setappdata.m,
scripts/plot/allchild.m, scripts/plot/ancestor.m, scripts/plot/area.m,
scripts/plot/axes.m, scripts/plot/axis.m, scripts/plot/bar.m,
scripts/plot/barh.m, scripts/plot/box.m, scripts/plot/caxis.m,
scripts/plot/cla.m, scripts/plot/clabel.m, scripts/plot/clf.m,
scripts/plot/close.m, scripts/plot/closereq.m, scripts/plot/colorbar.m,
scripts/plot/comet.m, scripts/plot/comet3.m, scripts/plot/compass.m,
scripts/plot/contour.m, scripts/plot/contour3.m, scripts/plot/contourc.m,
scripts/plot/contourf.m, scripts/plot/copyobj.m, scripts/plot/cylinder.m,
scripts/plot/daspect.m, scripts/plot/diffuse.m, scripts/plot/ellipsoid.m,
scripts/plot/errorbar.m, scripts/plot/ezcontour.m, scripts/plot/ezcontourf.m,
scripts/plot/ezmesh.m, scripts/plot/ezmeshc.m, scripts/plot/ezplot.m,
scripts/plot/ezplot3.m, scripts/plot/ezpolar.m, scripts/plot/ezsurf.m,
scripts/plot/ezsurfc.m, scripts/plot/feather.m, scripts/plot/figure.m,
scripts/plot/fill.m, scripts/plot/findall.m, scripts/plot/findobj.m,
scripts/plot/fplot.m, scripts/plot/gca.m, scripts/plot/gcbf.m,
scripts/plot/gcbo.m, scripts/plot/gcf.m, scripts/plot/gco.m,
scripts/plot/ginput.m, scripts/plot/graphics_toolkit.m, scripts/plot/grid.m,
scripts/plot/gtext.m, scripts/plot/guidata.m, scripts/plot/guihandles.m,
scripts/plot/hdl2struct.m, scripts/plot/hggroup.m, scripts/plot/hidden.m,
scripts/plot/hist.m, scripts/plot/hold.m, scripts/plot/ishghandle.m,
scripts/plot/ishold.m, scripts/plot/isocolors.m, scripts/plot/isprop.m,
scripts/plot/legend.m, scripts/plot/line.m, scripts/plot/linkprop.m,
scripts/plot/loglog.m, scripts/plot/loglogerr.m, scripts/plot/mesh.m,
scripts/plot/meshc.m, scripts/plot/meshgrid.m, scripts/plot/meshz.m,
scripts/plot/newplot.m, scripts/plot/orient.m, scripts/plot/pareto.m,
scripts/plot/patch.m, scripts/plot/pcolor.m, scripts/plot/peaks.m,
scripts/plot/pie.m, scripts/plot/pie3.m, scripts/plot/plot.m,
scripts/plot/plot3.m, scripts/plot/plotmatrix.m, scripts/plot/plotyy.m,
scripts/plot/polar.m, scripts/plot/print.m, scripts/plot/quiver.m,
scripts/plot/quiver3.m, scripts/plot/rectangle.m, scripts/plot/refresh.m,
scripts/plot/refreshdata.m, scripts/plot/ribbon.m, scripts/plot/rose.m,
scripts/plot/saveas.m, scripts/plot/scatter.m, scripts/plot/scatter3.m,
scripts/plot/semilogx.m, scripts/plot/semilogxerr.m, scripts/plot/semilogy.m,
scripts/plot/semilogyerr.m, scripts/plot/shading.m, scripts/plot/shg.m,
scripts/plot/shrinkfaces.m, scripts/plot/slice.m, scripts/plot/specular.m,
scripts/plot/sphere.m, scripts/plot/stairs.m, scripts/plot/stem.m,
scripts/plot/stem3.m, scripts/plot/struct2hdl.m, scripts/plot/subplot.m,
scripts/plot/surf.m, scripts/plot/surface.m, scripts/plot/surfc.m,
scripts/plot/surfl.m, scripts/plot/tetramesh.m, scripts/plot/text.m,
scripts/plot/title.m, scripts/plot/trimesh.m, scripts/plot/triplot.m,
scripts/plot/trisurf.m, scripts/plot/view.m, scripts/plot/waitbar.m,
scripts/plot/waitforbuttonpress.m, scripts/plot/waterfall.m,
scripts/plot/whitebg.m, scripts/plot/xlabel.m, scripts/plot/xlim.m,
scripts/plot/ylabel.m, scripts/plot/ylim.m, scripts/plot/zlabel.m,
scripts/plot/zlim.m: Rewrite docstrings for most plot functions.
Emphasize clarity, use common "voice", and increase density of seealso links.
author | Rik <rik@octave.org> |
---|---|
date | Wed, 31 Jul 2013 13:53:30 -0700 |
parents | 2d17dbdf6b7d |
children | 26589abbc78d |
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## Copyright (C) 2008-2012 Ben Abbott ## ## 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/>. ## -*- texinfo -*- ## @deftypefn {Function File} {} comet (@var{y}) ## @deftypefnx {Function File} {} comet (@var{x}, @var{y}) ## @deftypefnx {Function File} {} comet (@var{x}, @var{y}, @var{p}) ## @deftypefnx {Function File} {} comet (@var{hax}, @dots{}) ## Produce a simple comet style animation along the trajectory provided by ## the input coordinate vectors (@var{x}, @var{y}). If @var{x} is not ## specified it defaults to the indices of @var{y}. ## ## The speed of the comet may be controlled by @var{p}, which represents the ## time each point is displayed before moving to the next one. The default for ## @var{p} is 0.1 seconds. ## ## If the first argument @var{hax} is an axes handle, then plot into this axis, ## rather than the current axes returned by @code{gca}. ## @seealso{comet3} ## @end deftypefn ## Author: Ben Abbott bpabbott@mac.com ## Created: 2008-09-21 function comet (varargin) [hax, varargin, nargin] = __plt_get_axis_arg__ ("comet", varargin{:}); if (nargin == 0) print_usage (); elseif (nargin == 1) y = varargin{1}; x = 1:numel (y); p = 0.1; elseif (nargin == 2) x = varargin{1}; y = varargin{2}; p = 0.1; elseif (nargin == 3) x = varargin{1}; y = varargin{2}; p = varargin{3}; endif oldfig = ifelse (isempty (hax), [], get (0, "currentfigure")); unwind_protect hax = newplot (hax); limits = [min(x), max(x), min(y), max(y)]; num = numel (y); dn = round (num/10); for n = 1:(num+dn); m = n - dn; m = max ([m, 1]); k = min ([n, num]); plot (hax, x(1:m), y(1:m), "r", x(m:k), y(m:k), "g", x(k), y(k), "ob"); axis (hax, limits); drawnow (); pause (p); endfor unwind_protect_cleanup if (! isempty (oldfig)) set (0, "currentfigure", oldfig); endif end_unwind_protect endfunction %!demo %! clf; %! t = 0:.1:2*pi; %! x = cos (2*t) .* (cos (t).^2); %! y = sin (2*t) .* (sin (t).^2); %! comet (x, y);