| /* |
| # |
| # File : use_skeleton.cpp |
| # ( C++ source file ) |
| # |
| # Description : Example of use for the CImg plugin 'plugins/skeleton.h'. |
| # This file is a part of the CImg Library project. |
| # ( http://cimg.eu ) |
| # |
| # Copyright : Francois-Xavier Dupe |
| # ( http://www.greyc.ensicaen.fr/~fdupe/ ) |
| # |
| # License : CeCILL v2.0 |
| # ( http://www.cecill.info/licences/Licence_CeCILL_V2-en.html ) |
| # |
| # This software is governed by the CeCILL license under French law and |
| # abiding by the rules of distribution of free software. You can use, |
| # modify and/ or redistribute the software under the terms of the CeCILL |
| # license as circulated by CEA, CNRS and INRIA at the following URL |
| # "http://www.cecill.info". |
| # |
| # As a counterpart to the access to the source code and rights to copy, |
| # modify and redistribute granted by the license, users are provided only |
| # with a limited warranty and the software's author, the holder of the |
| # economic rights, and the successive licensors have only limited |
| # liability. |
| # |
| # In this respect, the user's attention is drawn to the risks associated |
| # with loading, using, modifying and/or developing or reproducing the |
| # software by the user in light of its specific status of free software, |
| # that may mean that it is complicated to manipulate, and that also |
| # therefore means that it is reserved for developers and experienced |
| # professionals having in-depth computer knowledge. Users are therefore |
| # encouraged to load and test the software's suitability as regards their |
| # requirements in conditions enabling the security of their systems and/or |
| # data to be ensured and, more generally, to use and operate it in the |
| # same conditions as regards security. |
| # |
| # The fact that you are presently reading this means that you have had |
| # knowledge of the CeCILL license and that you accept its terms. |
| # |
| */ |
| |
| #include <queue> |
| #define cimg_plugin "plugins/skeleton.h" |
| #include "CImg.h" |
| using namespace cimg_library; |
| #ifndef cimg_imagepath |
| #define cimg_imagepath "img/" |
| #endif |
| |
| // Main procedure |
| //---------------- |
| int main (int argc, char **argv) { |
| |
| cimg_usage("Compute the skeleton of a shape, using Hamilton-Jacobi equations"); |
| |
| // Read command line arguments |
| cimg_help("Input/Output options\n" |
| "--------------------"); |
| const char* file_i = cimg_option("-i",cimg_imagepath "milla.bmp","Input (black&white) image"); |
| const int median = cimg_option("-median",0,"Apply median filter"); |
| const bool invert = cimg_option("-inv",false,"Invert image values"); |
| const char* file_o = cimg_option("-o",(char*)0,"Output skeleton image"); |
| const bool display = cimg_option("-visu",true,"Display results"); |
| |
| cimg_help("Skeleton computation parameters\n" |
| "-------------------------------"); |
| const float thresh = cimg_option("-t",-0.3f,"Threshold"); |
| const bool curve = cimg_option("-curve",false,"Create medial curve"); |
| |
| cimg_help("Torsello correction parameters\n" |
| "------------------------------"); |
| const bool correction = cimg_option("-corr",false,"Torsello correction"); |
| const float dlt1 = 2; |
| const float dlt2 = cimg_option("-dlt",1.0f,"Discrete step"); |
| |
| // Load the image (forcing it to be scalar with 2 values { 0,1 }). |
| CImg<unsigned int> image0(file_i), image = image0.get_norm().quantize(2).normalize(0.0f,1.0f).round(); |
| if (median) image.blur_median(median); |
| if (invert) (image-=1)*=-1; |
| if (display) (image0.get_normalize(0,255),image.get_normalize(0,255)).display("Input image - Binary image"); |
| |
| // Compute distance map. |
| CImgList<float> visu; |
| CImg<float> distance = image.get_distance(0); |
| if (display) visu.insert(distance); |
| |
| // Compute the gradient of the distance function, and the flux (divergence) of the gradient field. |
| const CImgList<float> grad = distance.get_gradient("xyz"); |
| CImg<float> flux = image.get_flux(grad,1,1); |
| if (display) visu.insert(flux); |
| |
| // Use the Torsello correction of the flux if necessary. |
| if (correction) { |
| CImg<float> |
| logdensity = image.get_logdensity(distance,grad,flux,dlt1), |
| nflux = image.get_corrected_flux(logdensity,grad,flux,dlt2); |
| if (display) visu.insert(logdensity).insert(nflux); |
| flux = nflux; |
| } |
| |
| if (visu) { |
| cimglist_apply(visu,normalize)(0,255); |
| visu.display(visu.size()==2?"Distance function - Flux":"Distance function - Flux - Log-density - Corrected flux"); |
| } |
| |
| // Compute the skeleton |
| const CImg<unsigned int> skel = image.get_skeleton(flux,distance,curve,thresh); |
| if (display) { |
| (image0.resize(-100,-100,1,3)*=0.7f).get_shared_channel(1)|=skel*255.0; |
| image0.draw_image(0,0,0,0,image*255.0,0.5f).display("Image + Skeleton"); |
| } |
| |
| // Save output image if necessary. |
| if (file_o) skel.save(file_o); |
| |
| return 0; |
| } |