Mercurial > hg > octave-lyh
annotate scripts/plot/surfl.m @ 14868:5d3a684236b0
maint: Use Octave coding conventions for cuddling parentheses in scripts directory
* lin2mu.m, loadaudio.m, wavread.m, accumarray.m, bicubic.m, celldisp.m,
colon.m, cplxpair.m, dblquad.m, divergence.m, genvarname.m, gradient.m,
int2str.m, interp1.m, interp1q.m, interp2.m, interpn.m, loadobj.m, nthargout.m,
__isequal__.m, __splinen__.m, quadgk.m, quadl.m, quadv.m, rat.m, rot90.m,
rotdim.m, saveobj.m, subsindex.m, triplequad.m, delaunay3.m, griddata.m,
inpolygon.m, tsearchn.m, voronoi.m, get_first_help_sentence.m, which.m,
gray2ind.m, pink.m, dlmwrite.m, strread.m, textread.m, textscan.m, housh.m,
ishermitian.m, issymmetric.m, krylov.m, logm.m, null.m, rref.m,
compare_versions.m, copyfile.m, dump_prefs.m, edit.m, fileparts.m,
getappdata.m, isappdata.m, movefile.m, orderfields.m, parseparams.m,
__xzip__.m, rmappdata.m, setappdata.m, swapbytes.m, unpack.m, ver.m, fminbnd.m,
fminunc.m, fsolve.m, glpk.m, lsqnonneg.m, qp.m, sqp.m, configure_make.m,
copy_files.m, describe.m, get_description.m, get_forge_pkg.m, install.m,
installed_packages.m, is_architecture_dependent.m, load_package_dirs.m,
print_package_description.m, rebuild.m, repackage.m, save_order.m, shell.m,
allchild.m, ancestor.m, area.m, axes.m, axis.m, clabel.m, close.m, colorbar.m,
comet.m, comet3.m, contour.m, cylinder.m, ezmesh.m, ezsurf.m, findobj.m,
fplot.m, hist.m, isocolors.m, isonormals.m, isosurface.m, isprop.m, legend.m,
mesh.m, meshz.m, pareto.m, pcolor.m, peaks.m, plot3.m, plotmatrix.m, plotyy.m,
polar.m, print.m, __add_datasource__.m, __add_default_menu__.m,
__axes_limits__.m, __bar__.m, __clabel__.m, __contour__.m, __errcomm__.m,
__errplot__.m, __ezplot__.m, __file_filter__.m, __fltk_print__.m,
__ghostscript__.m, __gnuplot_print__.m, __go_draw_axes__.m,
__go_draw_figure__.m, __interp_cube__.m, __marching_cube__.m, __patch__.m,
__pie__.m, __plt__.m, __print_parse_opts__.m, __quiver__.m, __scatter__.m,
__stem__.m, __tight_eps_bbox__.m, __uigetdir_fltk__.m, __uigetfile_fltk__.m,
__uiputfile_fltk__.m, quiver.m, quiver3.m, rectangle.m, refreshdata.m,
ribbon.m, scatter.m, semilogy.m, shading.m, slice.m, subplot.m, surface.m,
surfl.m, surfnorm.m, text.m, uigetfile.m, uiputfile.m, whitebg.m, deconv.m,
mkpp.m, pchip.m, polyaffine.m, polyder.m, polygcd.m, polyout.m, polyval.m,
ppint.m, ppjumps.m, ppval.m, residue.m, roots.m, spline.m, splinefit.m,
addpref.m, getpref.m, setpref.m, ismember.m, setxor.m, arch_fit.m, arch_rnd.m,
arch_test.m, autoreg_matrix.m, diffpara.m, fftconv.m, filter2.m, hanning.m,
hurst.m, periodogram.m, triangle_sw.m, sinc.m, spectral_xdf.m, spencer.m,
stft.m, synthesis.m, unwrap.m, yulewalker.m, bicgstab.m, gmres.m, pcg.m, pcr.m,
__sprand_impl__.m, speye.m, spfun.m, sprandn.m, spstats.m, svds.m,
treelayout.m, treeplot.m, bessel.m, factor.m, legendre.m, perms.m, primes.m,
magic.m, toeplitz.m, corr.m, cov.m, mean.m, median.m, mode.m, qqplot.m,
quantile.m, ranks.m, zscore.m, logistic_regression_likelihood.m,
bartlett_test.m, chisquare_test_homogeneity.m, chisquare_test_independence.m,
kolmogorov_smirnov_test.m, run_test.m, u_test.m, wilcoxon_test.m, z_test.m,
z_test_2.m, bin2dec.m, dec2base.m, mat2str.m, strcat.m, strchr.m, strjust.m,
strtok.m, substr.m, untabify.m, assert.m, demo.m, example.m, fail.m, speed.m,
test.m, now.m: Use Octave coding conventions for cuddling parentheses in
scripts directory.
author | Rik <octave@nomad.inbox5.com> |
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date | Tue, 17 Jul 2012 07:08:39 -0700 |
parents | ce2b59a6d0e5 |
children | 022dba56de1e |
rev | line source |
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1 ## Copyright (C) 2009-2012 Kai Habel |
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2 ## |
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3 ## This file is part of Octave. |
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4 ## |
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5 ## Octave is free software; you can redistribute it and/or modify it |
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6 ## under the terms of the GNU General Public License as published by |
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7 ## the Free Software Foundation; either version 3 of the License, or (at |
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8 ## your option) any later version. |
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9 ## |
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10 ## Octave is distributed in the hope that it will be useful, but |
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11 ## WITHOUT ANY WARRANTY; without even the implied warranty of |
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12 ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU |
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13 ## General Public License for more details. |
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14 ## |
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15 ## You should have received a copy of the GNU General Public License |
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16 ## along with Octave; see the file COPYING. If not, see |
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17 ## <http://www.gnu.org/licenses/>. |
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18 |
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19 ## -*- texinfo -*- |
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20 ## @deftypefn {Function File} {} surfl (@var{x}, @var{y}, @var{z}) |
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21 ## @deftypefnx {Function File} {} surfl (@var{z}) |
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22 ## @deftypefnx {Function File} {} surfl (@var{x}, @var{y}, @var{z}, @var{L}) |
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23 ## @deftypefnx {Function File} {} surfl (@var{x}, @var{y}, @var{z}, @var{L}, @var{P}) |
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24 ## @deftypefnx {Function File} {} surfl (@dots{}, "light") |
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25 ## Plot a lighted surface given matrices @var{x}, and @var{y} from |
14248 | 26 ## @code{meshgrid} and a matrix @var{z} corresponding to the @var{x} and |
27 ## @var{y} coordinates of the mesh. If @var{x} and @var{y} are vectors, then | |
28 ## a typical vertex is (@var{x}(j), @var{y}(i), @var{z}(i,j)). Thus, columns | |
29 ## of @var{z} correspond to different @var{x} values and rows of @var{z} | |
30 ## correspond to different @var{y} values. | |
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31 ## |
14248 | 32 ## The light direction can be specified using @var{L}. It can be given as a |
33 ## 2-element vector [azimuth, elevation] in degrees or as a 3-element vector | |
34 ## [lx, ly, lz]. The default value is rotated 45 degrees counterclockwise | |
35 ## from the current view. | |
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36 ## |
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37 ## The material properties of the surface can specified using a 4-element vector |
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38 ## @var{P} = [@var{AM} @var{D} @var{SP} @var{exp}] which defaults to |
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39 ## @var{p} = [0.55 0.6 0.4 10]. |
14248 | 40 ## |
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41 ## @table @asis |
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42 ## @item "AM" strength of ambient light |
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43 ## |
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44 ## @item "D" strength of diffuse reflection |
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45 ## |
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46 ## @item "SP" strength of specular reflection |
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47 ## |
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48 ## @item "EXP" specular exponent |
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49 ## @end table |
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50 ## |
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51 ## The default lighting mode "cdata", changes the cdata property to give the |
14248 | 52 ## impression of a lighted surface. Please note: the alternative "light" |
53 ## mode, which creates a light object to illuminate the surface is not | |
54 ## implemented (yet). | |
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55 ## |
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56 ## Example: |
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57 ## |
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58 ## @example |
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59 ## @group |
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60 ## colormap (bone (64)); |
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61 ## surfl (peaks); |
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62 ## shading interp; |
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63 ## @end group |
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64 ## @end example |
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65 ## @seealso{surf, diffuse, specular, surface} |
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66 ## @end deftypefn |
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67 |
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68 ## Author: Kai Habel <kai.habel@gmx.de> |
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69 |
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70 function retval = surfl (varargin) |
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71 |
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72 [h, varargin] = __plt_get_axis_arg__ ("surfl", varargin{:}); |
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73 |
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74 oldh = gca (); |
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75 unwind_protect |
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76 axes (h); |
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77 newplot (); |
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78 |
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79 ## Check for lighting type. |
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80 use_cdata = true; |
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81 if (ischar (varargin{end})) |
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82 lstr = tolower (varargin{end}); |
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83 if (strncmp (lstr, "light", 5)) |
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84 warning ("light method not supported (yet), using cdata method instead"); |
10549 | 85 ## This can be implemented when light objects are supported. |
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86 use_cdata = false; |
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87 elseif (strncmp (lstr, "cdata", 5)) |
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88 use_cdata = true; |
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89 else |
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90 error ("surfl: unknown lighting method"); |
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91 endif |
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92 varargin(end) = []; |
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93 endif |
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94 |
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95 ## Check for reflection properties argument. |
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96 ## |
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97 ## r = [ambient light strength, |
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98 ## diffuse reflection strength, |
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99 ## specular reflection strength, |
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100 ## specular shine] |
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101 if (length (varargin{end}) == 4 && isnumeric (varargin{end})) |
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102 r = varargin{end}; |
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103 varargin(end) = []; |
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104 else |
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105 ## Default values. |
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106 r = [0.55, 0.6, 0.4, 10]; |
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107 endif |
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108 |
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109 ## Check for light vector (lv) argument. |
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110 have_lv = false; |
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111 if (isnumeric (varargin{end})) |
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112 len = numel (varargin{end}); |
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113 lastarg = varargin{end}; |
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114 if (len == 3) |
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115 lv = lastarg; |
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116 varargin(end) = []; |
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117 have_lv = true; |
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118 elseif (len == 2) |
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119 [lv(1), lv(2), lv(3)] = sph2cart ((lastarg(1) - 90) * pi/180, lastarg(2) * pi/180, 1.0); |
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120 varargin(end) = []; |
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121 have_lv = true; |
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122 endif |
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123 endif |
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124 |
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125 htmp = surface (varargin{:}); |
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126 if (! ishold ()) |
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127 set (h, "view", [-37.5, 30], |
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129 endif |
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130 |
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131 ## Get view vector (vv). |
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132 a = axis; |
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133 [az, el] = view; |
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134 [vv(1), vv(2), vv(3)] = sph2cart ((az - 90) * pi/180.0, el * pi/180.0, 1.0); |
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135 vv /= norm (vv); |
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136 |
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137 if (!have_lv) |
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138 ## Calculate light vector (lv) from view vector. |
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139 Phi = 45.0 / 180.0 * pi; |
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140 R = [cos(Phi), -sin(Phi), 0; |
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141 sin(Phi), cos(Phi), 0; |
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142 0, 0, 1]; |
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143 lv = (R * vv.').'; |
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144 endif |
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145 |
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146 vn = get (htmp, "vertexnormals"); |
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147 dar = get (h, "plotboxaspectratio"); |
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148 vn(:,:,1) *= dar(1); |
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149 vn(:,:,2) *= dar(2); |
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150 vn(:,:,3) *= dar(3); |
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151 |
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152 ## Normalize vn. |
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153 vn = vn ./ repmat (sqrt (sumsq (vn, 3)), [1, 1, 3]); |
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154 [nr, nc] = size (get (htmp, "zdata")); |
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155 |
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156 ## Ambient, diffuse, and specular term. |
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157 cdata = (r(1) * ones (nr, nc) |
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158 + r(2) * diffuse (vn(:,:,1), vn(:,:,2), vn(:,:,3), lv) |
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159 + r(3) * specular (vn(:,:,1), vn(:,:,2), vn(:,:,3), lv, vv, r(4))); |
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160 |
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161 set (htmp, "cdata", cdata ./ sum (r(1:3))); |
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162 |
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163 unwind_protect_cleanup |
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164 axes (oldh); |
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165 end_unwind_protect |
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166 |
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167 if (nargout > 0) |
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168 retval = htmp; |
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169 endif |
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170 |
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171 endfunction |
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172 |
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173 |
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174 %!demo |
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175 %! clf; |
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176 %! [X,Y,Z] = sombrero (); |
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177 %! colormap (copper (64)); |
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178 %! surfl (X,Y,Z); |
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179 %! shading interp; |
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180 |
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181 %!demo |
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182 %! clf; |
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183 %! [X,Y,Z] = sombrero (); |
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184 %! colormap (copper (64)); |
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185 %! [az, el] = view (); |
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186 %! surfl (X,Y,Z, [az+225,el], [0.2 0.6 0.4 25]); |
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187 %! shading interp; |
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188 |