view scripts/plot/appearance/specular.m @ 20266:83792dd9bcc1

Use in-place operators in m-files where possible. * scripts/audio/@audioplayer/set.m, scripts/audio/@audiorecorder/set.m, scripts/audio/mu2lin.m, scripts/elfun/cosd.m, scripts/general/del2.m, scripts/general/profexplore.m, scripts/general/quadl.m, scripts/general/rat.m, scripts/general/rotdim.m, scripts/help/get_first_help_sentence.m, scripts/help/private/__strip_html_tags__.m, scripts/image/cubehelix.m, scripts/io/textread.m, scripts/linear-algebra/duplication_matrix.m, scripts/linear-algebra/housh.m, scripts/linear-algebra/krylov.m, scripts/linear-algebra/logm.m, scripts/linear-algebra/normest.m, scripts/linear-algebra/onenormest.m, scripts/optimization/fminsearch.m, scripts/optimization/lsqnonneg.m, scripts/optimization/qp.m, scripts/plot/appearance/annotation.m, scripts/plot/appearance/axis.m, scripts/plot/appearance/legend.m, scripts/plot/appearance/specular.m, scripts/plot/draw/colorbar.m, scripts/plot/draw/hist.m, scripts/plot/draw/plotmatrix.m, scripts/plot/draw/private/__stem__.m, scripts/plot/util/__actual_axis_position__.m, scripts/plot/util/__gnuplot_drawnow__.m, scripts/plot/util/findobj.m, scripts/plot/util/print.m, scripts/plot/util/private/__go_draw_axes__.m, scripts/plot/util/private/__print_parse_opts__.m, scripts/plot/util/rotate.m, scripts/polynomial/pchip.m, scripts/polynomial/polyaffine.m, scripts/polynomial/polyder.m, scripts/polynomial/private/__splinefit__.m, scripts/polynomial/residue.m, scripts/signal/arch_fit.m, scripts/signal/arch_rnd.m, scripts/signal/bartlett.m, scripts/signal/blackman.m, scripts/signal/freqz.m, scripts/signal/hamming.m, scripts/signal/hanning.m, scripts/signal/spectral_adf.m, scripts/signal/spectral_xdf.m, scripts/signal/stft.m, scripts/sparse/bicgstab.m, scripts/sparse/cgs.m, scripts/sparse/private/__sprand_impl__.m, scripts/sparse/qmr.m, scripts/sparse/sprandsym.m, scripts/sparse/svds.m, scripts/specfun/legendre.m, scripts/special-matrix/gallery.m, scripts/statistics/base/gls.m, scripts/statistics/models/logistic_regression.m, scripts/statistics/tests/kruskal_wallis_test.m, scripts/statistics/tests/manova.m, scripts/statistics/tests/wilcoxon_test.m, scripts/time/datevec.m: Use in-place operators in m-files where possible.
author Rik <rik@octave.org>
date Tue, 26 May 2015 21:07:42 -0700
parents 4197fc428c7d
children
line wrap: on
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## Copyright (C) 2009-2015 Kai Habel
##
## 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} {} specular (@var{sx}, @var{sy}, @var{sz}, @var{lv}, @var{vv})
## @deftypefnx {Function File} {} specular (@var{sx}, @var{sy}, @var{sz}, @var{lv}, @var{vv}, @var{se})
## Calculate the specular reflection strength of a surface defined by the
## normal vector elements @var{sx}, @var{sy}, @var{sz} using Phong's
## approximation.
##
## The light source location and viewer location vectors are specified using
## parameters @var{lv} and @var{vv} respectively.  The location vectors can
## given as 2-element vectors [azimuth, elevation] in degrees or as 3-element
## vectors [x, y, z].
##
## An optional sixth argument specifies the specular exponent (spread) @var{se}.
## If not given, @var{se} defaults to 10.
## @seealso{diffuse, surfl}
## @end deftypefn

## Author: Kai Habel <kai.habel@gmx.de>

function retval = specular (sx, sy, sz, lv, vv, se)

  if (nargin < 5 || nargin > 6)
    print_usage ();
  endif

  ## Check normal vectors
  if (! size_equal (sx, sy, sz))
    error ("specular: SX, SY, and SZ must be the same size");
  endif

  ## Check light vector (lv) argument
  if (! isvector (lv) || length (lv) < 2 || length (lv) > 3)
    error ("specular: light vector LV must be a 2- or 3-element vector");
  elseif (length (lv) == 2)
    [lv(1), lv(2), lv(3)] = sph2cart (lv(1) * pi/180, lv(2) * pi/180, 1.0);
  endif

  ## Check view vector (vv) argument
  if (! isvector (vv) || length (vv) < 2 || length (lv) > 3)
    error ("specular: view vector VV must be a 2- or 3-element vector");
  elseif (length (vv) == 2)
    [vv(1), vv(2), vv(3)] = sph2cart (vv(1) * pi / 180, vv(2) * pi / 180, 1.0);
  endif

  ## Check specular exponent (se) argument
  if (nargin < 6)
    se = 10;
  elseif (! (isnumeric (se) && numel (se) == 1 && se > 0))
    error ("specular: exponent SE must be a positive scalar");
  endif

  ## Normalize view and light vectors
  if (sum (abs (lv)) > 0)
    lv /= norm (lv);
  endif
  if (sum (abs (vv)) > 0)
    vv /= norm (vv);
  endif

  ## Calculate normal vector lengths and dot-products
  ns = sqrt (sx.^2 + sy.^2 + sz.^2);
  l_dot_n = (sx * lv(1) + sy * lv(2) + sz * lv(3)) ./ ns;
  v_dot_n = (sx * vv(1) + sy * vv(2) + sz * vv(3)) ./ ns;

  ## Calculate specular reflection using Phong's approximation
  retval = 2 * l_dot_n .* v_dot_n - dot (lv, vv);

  ## Set reflectance to zero if light is on the other side
  retval(l_dot_n < 0) = 0;

  ## Allow postive values only
  retval(retval < 0) = 0;
  retval .^= se;

endfunction