view scripts/plot/comet.m @ 14237:11949c9795a0

Revamp %!demos in m-files to use Octave coding conventions on spacing, etc. Add clf() to all demos using plot features to get reproducibility. Use 64 as input to all colormaps (jet (64)) to get reproducibility. * bicubic.m, cell2mat.m, celldisp.m, cplxpair.m, interp1.m, interp2.m, interpft.m, interpn.m, profile.m, profshow.m, convhull.m, delaunay.m, griddata.m, inpolygon.m, voronoi.m, autumn.m, bone.m, contrast.m, cool.m, copper.m, flag.m, gmap40.m, gray.m, hot.m, hsv.m, image.m, imshow.m, jet.m, ocean.m, pink.m, prism.m, rainbow.m, spring.m, summer.m, white.m, winter.m, condest.m, onenormest.m, axis.m, clabel.m, colorbar.m, comet.m, comet3.m, compass.m, contour.m, contour3.m, contourf.m, cylinder.m, daspect.m, ellipsoid.m, errorbar.m, ezcontour.m, ezcontourf.m, ezmesh.m, ezmeshc.m, ezplot.m, ezplot3.m, ezpolar.m, ezsurf.m, ezsurfc.m, feather.m, fill.m, fplot.m, grid.m, hold.m, isosurface.m, legend.m, loglog.m, loglogerr.m, pareto.m, patch.m, pbaspect.m, pcolor.m, pie.m, pie3.m, plot3.m, plotmatrix.m, plotyy.m, polar.m, quiver.m, quiver3.m, rectangle.m, refreshdata.m, ribbon.m, rose.m, scatter.m, scatter3.m, semilogx.m, semilogxerr.m, semilogy.m, semilogyerr.m, shading.m, slice.m, sombrero.m, stairs.m, stem.m, stem3.m, subplot.m, surf.m, surfc.m, surfl.m, surfnorm.m, text.m, title.m, trimesh.m, triplot.m, trisurf.m, uigetdir.m, uigetfile.m, uimenu.m, uiputfile.m, waitbar.m, xlim.m, ylim.m, zlim.m, mkpp.m, pchip.m, polyaffine.m, spline.m, bicgstab.m, cgs.m, gplot.m, pcg.m, pcr.m, treeplot.m, strtok.m, demo.m, example.m, rundemos.m, speed.m, test.m, calendar.m, datestr.m, datetick.m, weekday.m: Revamp %!demos to use Octave coding conventions on spacing, etc.
author Rik <octave@nomad.inbox5.com>
date Fri, 20 Jan 2012 12:59:53 -0800
parents 72c96de7a403
children 4506eade9f04
line wrap: on
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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{ax}, @dots{})
## Produce a simple comet style animation along the trajectory provided by
## the input coordinate vectors (@var{x}, @var{y}), where @var{x} will default
## to the indices of @var{y}.
##
## The speed of the comet may be controlled by @var{p}, which represents the
## time which passes as the animation passes from one point to the next.  The
## default for @var{p} is 0.1 seconds.
##
## If @var{ax} is specified the animation is produced in that axis rather than
## the @code{gca}.
## @end deftypefn

## Author: Ben Abbott bpabbott@mac.com
## Created: 2008-09-21

function comet (varargin)

  [h, 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

  oldh = gca ();
  unwind_protect
    axes (h);
    newplot ();
    theaxis = [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]);
      h = plot (x(1:m), y(1:m), "r", x(m:k), y(m:k), "g", x(k), y(k), "ob");
      axis (theaxis);
      drawnow ();
      pause (p);
    endfor
  unwind_protect_cleanup
    axes (oldh);
  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);