Commit e0e299e6 authored by Laurent Belcour's avatar Laurent Belcour
Browse files

Adding script files for the Gray.

parents 3fa25081 84d25f6b
<?xml version="1.0"?>
<alta>
<!-- This script file compute the fitting of the retro-reflecting materials
present in the ALTA library. This script file should be executed in
the sources directory of repository as all directories are relative.
It is also necessary to create a results/3d/retro directory to store
the resulting fits and exports to BRDF-explorer and matlab.
-->
<configuration>
<parameter name="lib-dir" value="./build" />
</configuration>
<!-- Fitting the lobe using a back parametrization:
The ABC model uses the dot product between the back and the
normal vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_abc_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_abc">
<parameter name="param" value="COS_TK" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_abc_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_abc">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
<parameter name="param" value="COS_TK" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_abc_back.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_abc_back.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_abc_back.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<!-- Fitting the lobe using a retro parametrization:
The ABC model uses the dot product between the light and the
view vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_abc_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_abc">
<parameter name="param" value="COS_TLV" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_abc_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_abc">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
<parameter name="param" value="COS_TLV" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_abc_retro.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_abc_retro.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_abc_retro.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
</alta>
<?xml version="1.0"?>
<alta>
<!-- This script file compute the fitting of the retro-reflecting materials
present in the ALTA library. This script file should be executed in
the sources directory of repository as all directories are relative.
It is also necessary to create a results/3d/retro directory to store
the resulting fits and exports to BRDF-explorer and matlab.
-->
<configuration>
<parameter name="lib-dir" value="./build" />
</configuration>
<!-- Fitting the lobe using a back parametrization:
The ABC model uses the dot product between the back and the
normal vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_beck_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retrobeckmann">
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_beck_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retrobeckmann">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_beck_back.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_beck_back.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_beck_back.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<!-- Fitting the lobe using a retro parametrization:
The ABC model uses the dot product between the light and the
view vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_beck_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retrobeckmann">
<parameter name="retro" value="" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_beck_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retrobeckmann">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
<parameter name="retro" value="" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_beck_retro.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_beck_retro.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_beck_retro.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
</alta>
<?xml version="1.0"?>
<alta>
<!-- This script file compute the fitting of the retro-reflecting materials
present in the ALTA library. This script file should be executed in
the sources directory of repository as all directories are relative.
It is also necessary to create a results/3d/retro directory to store
the resulting fits and exports to BRDF-explorer and matlab.
-->
<configuration>
<parameter name="lib-dir" value="./build" />
</configuration>
<!-- Fitting the lobe using a back parametrization:
The ABC model uses the dot product between the back and the
normal vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retroblinn">
<parameter name="param" value="COS_TK" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retroblinn">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
<parameter name="param" value="COS_TK" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_blinn_back.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_blinn_back.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_back.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<!-- Fitting the lobe using a retro parametrization:
The ABC model uses the dot product between the light and the
view vectors.
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retroblinn">
<parameter name="param" value="COS_TLV" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_retro.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_retroblinn">
<parameter name="fresnel" value="./build/libnonlinear_fresnel_retroschlick.so"/>
<parameter name="param" value="COS_TLV" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
<parameter name="bootstrap" value="./results/3d/retro/half/Bande_fluo_blinn_retro.brdf" />
</action>
<!-- Export the fit -->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_blinn_retro.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_blinn_retro.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
</alta>
<?xml version="1.0"?>
<alta>
<!-- This script file compute the fitting of the retro-reflecting materials
present in the ALTA library. This script file should be executed in
the sources directory of repository as all directories are relative.
It is also necessary to create a results/3d/retro directory to store
the resulting fits and exports to BRDF-explorer and matlab.
-->
<configuration>
<parameter name="lib-dir" value="./build" />
</configuration>
<!-- Fitting the lobe using the Lafortune model
-->
<action name="data2brdf">
<!-- Input and output arguments of the action -->
<input name="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<output name="./results/3d/retro/half/Bande_fluo_laf_back.brdf" />
<!-- Define the function to use -->
<function name="nonlinear_function_diffuse" />
<function name="nonlinear_function_lafortune">
<parameter name="lobes" value="1" />
</function>
<!-- Define the ftting procedure to use -->
<plugin type="fitter" name="nonlinear_fitter_ceres" />
<!-- Parameters -->
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
<!-- Export the fit
-->
<action name="brdf2gnuplot">
<!-- Input and output arguments of the action -->
<input name="./results/3d/retro/half/Bande_fluo_laf_back.brdf" />
<output name="./results/3d/retro/half/Bande_fluo_laf_back.dat" />
<parameter name="data" value="../papers/retro/mesures/original/Bande_fluo_grise/3d/633nm/Fichiers\ definitifs/densityHelmholtz/Bande_grise_3D+3DS+3DR__BRDF_min_retro_lobe_dense.alta" />
<parameter name="min" value="[0.1, -2, -2]" />
<parameter name="max" value="[1.7, 2, 2]" />
</action>
</alta>
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