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path: root/source/blender/nodes/NOD_static_types.h
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2018-07-18Cycles: add Principled Hair BSDF.L. E. Segovia
This is a physically-based, easy-to-use shader for rendering hair and fur, with controls for melanin, roughness and randomization. Based on the paper "A Practical and Controllable Hair and Fur Model for Production Path Tracing". Implemented by Leonardo E. Segovia and Lukas Stockner, part of Google Summer of Code 2018.
2018-07-18Compositor: Cryptomatte compositing node.Stefan Werner
This patch adds a new matte node that implements the Cryptomatte specification. It also incluces a custom eye dropper that works outside of a color picker. Cryptomatte export for the Cycles render engine will be in a separate patch. Reviewers: brecht Reviewed By: brecht Subscribers: brecht Tags: #compositing Differential Revision: https://developer.blender.org/D3531
2018-06-15Cycles: change Ambient Occlusion shader to output colors.Lukas Stockner
This means the shader can now be used for procedural texturing. New settings on the node are Samples, Inside, Local Only and Distance. Original patch by Lukas with further changes by Brecht. Differential Revision: https://developer.blender.org/D3479
2018-05-27Cycles: Add Support for IES files as textures for light strengthLukas Stockner
This patch adds support for IES files, a file format that is commonly used to store the directional intensity distribution of light sources. The new IES node is supposed to be plugged into the Strength input of the Emission node of the lamp. Since people generating IES files do not really seem to care about the standard, the parser is flexible enough to accept all test files I have tried. Some common weirdnesses are distributing values over multiple lines that should go into one line, using commas instead of spaces as delimiters and adding various useless stuff at the end of the file. The user interface of the node is similar to the script node, the user can either select an internal Text or load a file. Internally, IES files are handled similar to Image textures: They are stored in slots by the LightManager and each unique IES is assigned to one slot. The local coordinate system of the lamp is used, so that the direction of the light can be changed. For UI reasons, it's usually best to add an area light, rotate it and then change its type, since especially the point light does not immediately show its local coordinate system in the viewport. Reviewers: #cycles, dingto, sergey, brecht Reviewed By: #cycles, dingto, brecht Subscribers: OgDEV, crazyrobinhood, secundar, cardboard, pisuke, intrah, swerner, micah_denn, harvester, gottfried, disnel, campbellbarton, duarteframos, Lapineige, brecht, juicyfruit, dingto, marek, rickyblender, bliblubli, lockal, sergey Differential Revision: https://developer.blender.org/D1543
2018-02-23Cycles: add Principled Volume shader.Brecht Van Lommel
Similar to the Principled BSDF, this should make it easier to set up volume materials. Smoke and fire can be rendererd with just a single principled volume node, the appropriate attributes will be used when available. The node also works for simpler homogeneous volumes like water or mist. Differential Revision: https://developer.blender.org/D3033
2018-02-03Cycles: add Vector Displacement node and extend Displacement node.Brecht Van Lommel
This adds midlevel and object/world space for displacement, and a vector displacement node with tangent/object/world space, midlevel and scale. Note that tangent space vector displacement still is not exactly compatible with maps created by other software, this will require changes to the tangent computation. Differential Revision: https://developer.blender.org/D1734
2018-01-23Cycles: add Displacement node.Brecht Van Lommel
This converts object space height to world space displacement, to be linked to the new vector displacement material output. Differential Revision: https://developer.blender.org/D3015
2017-11-08Cycles: add bevel shader, for raytrace based rounded edges.Brecht Van Lommel
The algorithm averages normals from nearby surfaces. It uses the same sampling strategy as BSSRDFs, casting rays along the normal and two orthogonal axes, and combining the samples with MIS. The main concern here is that we are introducing raytracing inside shader evaluation, which could be quite bad for GPU performance and stack memory usage. In practice it doesn't seem so bad though. Note that using this feature can easily slow down renders 20%, and that if you care about performance then it's better to use a bevel modifier. Mainly this is useful for baking, and for cases where the mesh topology makes it difficult for the bevel modifier to work well. Differential Revision: https://developer.blender.org/D2803
2017-05-22Fix T51308: Bright/Contrast Doesn't respect Pre-multiplied AlphaSergey Sharybin
Brightness/contrast node was changing color but did not modify alpha or ensured colors are premultiplied on the output. This was giving artifacts later on unless alpha was manually converted. Compositor is supposed to work in premultiplied alpha (except of some really corner cases) so it makes sense to ensure premultiplied alpha after brightness/contrast node. This is now done as an option enabled by default, so we: (a) Keep compatibility with old files. (b) Have correct behavior for newly created files. Later on we can get rid of this option.
2017-04-18Squashed commit of the following:Pascal Schoen
commit 90778901c9ea1e16d5907981e91bceba25ff207d Merge: 76eebd9 3bf0026 Author: Schoen <schoepas@deher1m1598.emea.adsint.biz> Date: Mon Apr 3 07:52:05 2017 +0200 Merge branch 'master' into cycles_disney_brdf commit 76eebd9379a5dad519ff01cf215fbe3db6de931e Author: Schoen <schoepas@deher1m1598.emea.adsint.biz> Date: Thu Mar 30 15:34:20 2017 +0200 Updated copyright for the new files. commit 013f4a152a3898946ba5c616141c6e44d928ccfd Author: Schoen <schoepas@deher1m1598.emea.adsint.biz> Date: Thu Mar 30 15:32:55 2017 +0200 Switched from multiplication of base and subsurface color to blending between them using the subsurface parameter. commit 482ec5d1f20ceabc9cbda4838d4ae37d1d673458 Author: Schoen <schoepas@deher1m1598.emea.adsint.biz> Date: Mon Mar 13 15:47:12 2017 +0100 Fixed a bug that caused an additional white diffuse closure call when using path tracing. commit 26e906d162a6a8d67f2ebc8880993fcbab69559e Merge: 0593b8c 223aff9 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Feb 6 11:32:31 2017 +0100 Merge branch 'master' into cycles_disney_brdf commit 0593b8c51bf7db0ed5ca92ed6f68d0d984dad0dd Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Feb 6 11:30:36 2017 +0100 Fixed the broken GLSL shader and implemented the Disney BRDF in the real-time view port. commit 8c7e11423be640dc44b1807912058480710e51f4 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Feb 3 14:24:05 2017 +0100 Fix to comply strict compiler flags and some code cleanup commit 17724e9d2dbffb1aaa61401224ecbf2349c1dac3 Merge: 379ba34 520afa2 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jan 24 09:59:58 2017 +0100 Merge branch 'master' into cycles_disney_brdf commit 379ba346b0acd1ea779365b940fcd01f5ba1165f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jan 24 09:28:56 2017 +0100 Renamed the Disney BSDF to Principled BSDF. commit f80dcb4f34f1dc41841ced5965787fc26ace22a2 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Dec 2 13:55:12 2016 +0100 Removed reflection call when roughness is low because of artifacts. commit 732db8a57f6d4e5d6f44bbad176c15fd55377f0a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Nov 16 09:22:25 2016 +0100 Indication if to use fresnel is now handled via the type of the BSDF. commit 0103659f5e705b314cde98b0e4a01c14c55acd5e Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Nov 11 13:04:11 2016 +0100 Fixed an error in the clearcoat where it appeared too bright for default light sources (like directional lights) commit 0aa68f533529c9fd197a3ab0427f9e41a15456b9 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Nov 7 12:04:38 2016 +0100 Resolved inconsistencies in using tabs and spaces commit f5897a9494e352de274b99e7bee971336c0dc386 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Nov 7 08:13:41 2016 +0100 Improved the clearcoat part by using GTR1 instead of GTR2 commit 3dfc240e61b3d4d0e7c476989792e4ada869ce91 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Oct 31 11:31:36 2016 +0100 Use reflection BSDF for glossy reflections when roughness is 0.0 to reduce computational expense and some code cleanup Code cleanup includes: - Code style cleanup and removed unused code - Consolidated code in the bsdf_microfacet_multi_impl.h to reduce some computational expense commit a2dd0c5fafdabe1573299170fb3be98a3e46d17a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Oct 26 08:51:10 2016 +0200 Fixed glossy reflections and refractions for low roughness values and cleaned up the code. For low roughness values, the reflections had some strange behavior. commit 981737591231a1a5a1c85950950580b65d029505 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Oct 25 12:37:40 2016 +0200 Removed default values in setup functions and added extra functions for GGX with fresnel. commit bbc5d9d4527346a74155cf17be21fb02ee3e0779 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Oct 25 11:09:36 2016 +0200 Switched from uniform to cosine hemisphere sampling for the diffuse and the sheen part. commit d52d8f2813d64363713f11160a6c725d4cafbcfa Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Oct 24 16:17:13 2016 +0200 Removed the color parameters from the diffuse and sheen shader and use them as closure weights instead. commit 8f3d92738532ad867a0a3543c00393626ab8f6ec Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Oct 24 09:57:06 2016 +0200 Fixed the issue with artifacts when using anisotropy without linking the tangent input to a tangent node. commit d93f680db9acaaade0354b34857a3ccaf348557f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Oct 24 09:14:51 2016 +0200 Added subsurface radius parameter to control the per color channel effection radius of the subsurface scattering. commit c708c3e53b323773fc852bdc239bc51e157dcaef Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Oct 24 08:14:10 2016 +0200 Rearranged the inputs of the shader. commit dfbfff9c389074d3e5c1f49dd38a95e9b317eb1f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Oct 21 09:27:05 2016 +0200 Put spaces in the parameter names of the shader node commit e5a748ced17c8f59e5e73309096adeea3ba95e04 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Oct 21 08:51:20 2016 +0200 Removed code that isn't in use anymore commit 75992bebc128c8b44cab4f0d8855603787f57260 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Oct 21 08:50:07 2016 +0200 Code style cleanup commit 4dfcf455f7769752044e051b399fb6a5dfcd0e22 Merge: 243a0e3 2cd6a89 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Thu Oct 20 10:41:50 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit 243a0e3eb80ef82704d5ea2657384c3a4b9fb497 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Thu Oct 20 10:01:45 2016 +0200 Switching between OSL and SVM is more consistant now when using Disney BSDF. There were some minor differences in the OSL implementation, e.g. the refraction roughness was missing. commit 2a5ac509223c838285a00c4c12775567666e7154 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 27 09:17:57 2016 +0200 Fixed a bug that caused transparency to be always white when using OSL and selecting GGX as distribution of the Disney BSDF commit e1fa8623915407cea942a07fd0a106b04e113c09 Merge: d0530a8 7f76f6f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 27 08:59:32 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit d0530a8af0e076c0aca4c9a61b0a64cada45ac4d Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 27 08:53:18 2016 +0200 Cleanup the Disney BSDF implementation and removing unneeded files. commit 3f4fc826bd9c1f47c694c0f6b2947daf5b524b1a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 27 08:36:07 2016 +0200 Unified the OSL implementation of the Disney clearcoat as a simple microfacet shader like it was previously done in SVM commit 4d3a0032ecea99031979f342bfd5f66ea5a8625a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Sep 26 12:35:36 2016 +0200 Enhanced performance for Disney materials without subsurface scattering commit 3cd5eb56cf5c9006837f111c8866e4c6e1c2a6fd Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Sep 16 08:47:56 2016 +0200 Fixed a bug in the Disney BSDF that caused specular reflections to be too bright and diffuse is now reacting to the roughness again - A normalization for the fresnel was missing which caused the specular reflections to become too bright for the single-scatter GGX - The roughness value for the diffuse BSSRDF part has always been overwritten and thus always 0 - Also the performance for refractive materials with roughness=0.0 has been improved commit 7cb37d711938e5626651db21f20da50edd96abaf Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Thu Sep 8 12:24:43 2016 +0200 Added selection field to the Disney BSDF node for switching between "Multiscatter GGX" and "GGX" In the "GGX" mode there is an additional parameter for changing the refraction roughness for materials with smooth surfaces and rough interns (e.g. honey). With the "Multiscatter GGX" this effect can't be produced at the moment and so here will be no separation of the two roughness values. commit cdd29d06bb86672ed0779eefb8eee95796b8f939 Merge: 02c315a b40d1c1 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 6 15:59:05 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit 02c315aeb0f0d7bb429d4396912e03dbb8a77340 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Sep 6 15:16:09 2016 +0200 Implemented the OSL part of the Disney shader commit 5f880293aeeacf269032824248b46d613691a36c Merge: 630b80e b399a6d Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Sep 2 10:53:36 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit 630b80e08b6acf83834bc95264af4ccdbbc5f82c Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Sep 2 10:52:13 2016 +0200 Fresnel in the microfacet multiscatter implementation improved commit 0d9f4d7acb2de65d1c98d425cea4bf364795c155 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Aug 26 11:11:05 2016 +0200 Fixed refraction roughness problem (refractions were always 100% rough) and set IOR of clearcoat to 1.5 commit 9eed34c7d980e1b998df457c4f76021162c80f78 Merge: ef29aae ae475e3 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Aug 16 15:22:32 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit ef29aaee1af8074e0228c480d962700e97ea5b36 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Aug 16 15:17:12 2016 +0200 Implemented the fresnel in the multi-scatter GGX for the Disney BSDF - The specular/metallic part uses the multi-scatter GGX - The fresnel of the metallic part is controlled by the specular value - The color of the reflection part when using transparency can be controlled by the specularTint value commit 88567af085ac94119b98c95246b6d6f63161bc01 Merge: cc267e5 285e082 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Aug 3 15:05:09 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit cc267e52f20d036a66aeeff127ee1c856f7c651b Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Aug 3 15:00:25 2016 +0200 Implemented the Disney clearcoat as a variation of the microfacet bsdf, removed the transparency roughness again and added an input for anisotropic rotations commit 81f6c06b1f53180bf32a5c11ac1fa64e2b6abf52 Merge: ece5a08 7065022 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Aug 3 11:42:02 2016 +0200 Merge branch 'master' into cycles_disney_brdf commit ece5a08e0d6e51a83c223ea87346134216e5b34e Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jul 26 16:29:21 2016 +0200 Base color now applied again to the refraction of transparent Disney materials commit e3aff6849e06853c56da7bd610210dcab70e6070 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jul 26 16:05:19 2016 +0200 Added subsurface color parameter to the Disney shader commit b3ca6d8a2f4f866b323fc2df0a3beff577218c27 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jul 26 12:30:25 2016 +0200 Improvement of the SSS in the Disney shader * Now the bump normal is correctly used for the SSS. * SSS in Disney uses the Disney diffuse shader commit d68729300ee557e90a8e7e4be6eb8ef98db80fe2 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jul 26 12:23:13 2016 +0200 Better calculation of the Disney diffuse part Now the values for NdotL und NdotV are clamped to 0.0f for a better look when using normal maps commit cb6e500b12e7bce884d3db19ee138c975c215f2d Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Jul 25 16:26:42 2016 +0200 Now one can disable specular reflactions again by setting specular and metallic to 0 (cracked this in the previous commit) commit bfb9cb11b548103369de2a46ce18b4ddf661362c Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Jul 25 16:11:07 2016 +0200 fixed the Disney SSS and cleaned the initialization of the Disney shaders commit 642c0fdad12548c1a2ccbf595bae3a995d3022f7 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Jul 25 16:09:55 2016 +0200 fixed an error that was caused by the missing LABEL_REFLECT in the Disney diffuse shader commit c10b484dcad3412c34455736e9656cd38716bcb0 Author: Jens Verwiebe <info@jensverwiebe.de> Date: Fri Jul 22 01:15:21 2016 +0200 Rollback attempt to fix sss crashing, it prevented crash by disabling sss completely, thus useless commit 462bba3f97fcc41834e0e20cc806a7958e5106f5 Author: Jens Verwiebe <info@jensverwiebe.de> Date: Thu Jul 21 23:11:59 2016 +0200 Add an undef for sc_next for safety commit 32d348577d69be251aa04110c5f6156cd2645f48 Author: Jens Verwiebe <info@jensverwiebe.de> Date: Thu Jul 21 00:15:48 2016 +0200 Attempt to fix Disney SSS commit dbad91ca6d46f5a4a6f2ba7ed4c811ffa723942f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed Jul 20 11:13:00 2016 +0200 Added a roughness parameter for refractions (for scattering of the rays within an object) With this, one can create a translucent material with a smooth surface and with a milky look. The final refraction roughness has to be calculated using the surface roughness and the refraction roughness because those two are correlated for refractions. If a ray hits a rough surface of a translucent material, it is scattered while entering the surface. Then it is scattered further within the object. The calculation I'm using is the following: RefrRoughnessFinal = 1.0 - (1.0 - Roughness) * (1.0 - RefrRoughness) commit 50ea5e3e34394a727e3cceb6203adb48834a9ab7 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue Jun 7 10:24:50 2016 +0200 Disney BSDF is now supporting CUDA commit 10974cc826a4bfa8fb3ef59177abf0b0dc441065 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 31 11:18:07 2016 +0200 Added parameters IOR and Transparency for refractions With this, the Disney BRDF/BSSRDF is extended by the BTDF part. commit 218202c0905a4ec93ee19850360d1a39966d2c25 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon May 30 15:08:18 2016 +0200 Added an additional normal for the clearcoat With this normal one can simulate a thin layer of clearcoat by applying a smoother normal map than the original to this input commit dd139ead7e04aa87a894ccf3732cfce711258ff1 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon May 30 12:40:56 2016 +0200 Switched to the improved subsurface scattering from Christensen and Burley commit 11160fa4e1c32230119d4506e7e9fd3da2ab37f2 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon May 30 10:16:30 2016 +0200 Added Disney Sheen shader as a preparation to get to a BSSRDF commit cee4fe0cc94515ee60d4afa4d4e10c41003f1579 Merge: 4f955d0 6b5bab6 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon May 30 09:08:09 2016 +0200 Merge branch 'cycles_disney_brdf' of git.blender.org:blender into cycles_disney_brdf Conflicts: intern/cycles/kernel/closure/bsdf_disney_clearcoat.h intern/cycles/kernel/closure/bsdf_disney_diffuse.h intern/cycles/kernel/closure/bsdf_disney_specular.h intern/cycles/kernel/closure/bsdf_util.h intern/cycles/kernel/osl/CMakeLists.txt intern/cycles/kernel/osl/bsdf_disney_clearcoat.cpp intern/cycles/kernel/osl/bsdf_disney_diffuse.cpp intern/cycles/kernel/osl/bsdf_disney_specular.cpp intern/cycles/kernel/osl/osl_closures.h intern/cycles/kernel/shaders/node_disney_bsdf.osl intern/cycles/render/nodes.cpp intern/cycles/render/nodes.h commit 4f955d052358206209454decf2c3539e6a21b42f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 24 16:38:23 2016 +0200 SVM and OSL are both working for the simple version of the Disney BRDF commit 1f5c41874b01ad297eb8a6bad9985296c6c0a6e1 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 24 09:58:50 2016 +0200 Disney node can be used without SVM and started to cleanup the OSL implementation There is still some wrong behavior for SVM for the Schlick Fresnel part at the specular and clearcoat commit d4b814e9304ebb44cc7c291cd83f7b7cdebcd152 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 18 10:22:29 2016 +0200 Switched from a parameter struct for Disney parameters to ShaderClosure params commit b86a1f5ba5019c7818153cb70b49f5f7a0bc52a0 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 18 10:19:57 2016 +0200 Added additional variables for storing parameters in the ShaderClosure struct commit 585b88623695fa07dfca9c9909d6d9184c3519c8 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 17 12:03:17 2016 +0200 added output parameter to the DisneyBsdfNode That has been forgotten after removing the inheritance of BsdfNode commit f91a28639884cbda7804715b910d64abba0718ef Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 17 10:40:48 2016 +0200 removed BsdfNode class inheritance for DisneyBsdfNode That's due to a naming difference. The Disney BSDF uses the name 'Base Color' while the BsdfNode had a 'Color' input. That caused a text message to be printed while rendering. commit 30da91c9c51d8cbc6a7564c7aaa61c9efe2ab654 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 4 16:08:10 2016 +0200 disney implementation cleaned commit 30d41da0f0352fad29375a395ffcb9cb7891eeb1 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 4 13:23:07 2016 +0200 added the disney brdf as a shader node commit 1f099fce249cb35e949cc629f7cca2167fca881a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 3 16:54:49 2016 +0200 added clearcoat implementation commit 00a1378b98e435e9cdbfbac86eb974c19b2a8151 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Apr 29 22:56:49 2016 +0200 disney diffuse und specular implemented commit 6baa7a7eb787638661cddad0c4e7f78bd3a8fa5c Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Apr 18 15:21:32 2016 +0200 disney diffuse is working correctly commit d8fa169bf3caf71c40a124101b33dee6c510188e Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Apr 18 08:41:53 2016 +0200 added vessel for disney diffuse shader commit 6b5bab6cecde153122625cf8dc10e4209ed1eb0f Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 18 10:22:29 2016 +0200 Switched from a parameter struct for Disney parameters to ShaderClosure params commit f6499c2676e074a36033627ffc7540107777630d Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 18 10:19:57 2016 +0200 Added additional variables for storing parameters in the ShaderClosure struct commit 7100640b65c2ff5447a18c01fc4e93594b4f486a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 17 12:03:17 2016 +0200 added output parameter to the DisneyBsdfNode That has been forgotten after removing the inheritance of BsdfNode commit 419ee5441100a906b4b3fd8373cb768a71bfdfe6 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 17 10:40:48 2016 +0200 removed BsdfNode class inheritance for DisneyBsdfNode That's due to a naming difference. The Disney BSDF uses the name 'Base Color' while the BsdfNode had a 'Color' input. That caused a text message to be printed while rendering. commit 6006f91e8730f78df5874f808690d3908db103ab Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 4 16:08:10 2016 +0200 disney implementation cleaned commit 0ed08959141fc7c5f8c6e37c6552ecb9fcc5749c Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Wed May 4 13:23:07 2016 +0200 added the disney brdf as a shader node commit 0630b742d71c658915575a4a71a325094a0fc313 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Tue May 3 16:54:49 2016 +0200 added clearcoat implementation commit 9f3d39744b85619750c79c901f678b8c07fe0ee2 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Fri Apr 29 22:56:49 2016 +0200 disney diffuse und specular implemented commit 9b262063767d6b05a617891c967d887d21bfb177 Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Apr 18 15:21:32 2016 +0200 disney diffuse is working correctly commit 4711a3927dfcadaa1c36de0ba78fc304fac1dc8a Author: Pascal Schoen <pascal_schoen@gmx.net> Date: Mon Apr 18 08:41:53 2016 +0200 added vessel for disney diffuse shader Differential Revision: https://developer.blender.org/D2313
2017-01-26Compositor: Make HSV node inputs a real socketsSergey Sharybin
This is much more flexible solution which will allow doing some more procedural features. Reviewers: brecht, dfelinto, mont29 Reviewed By: mont29 Subscribers: Severin Differential Revision: https://developer.blender.org/D2403
2016-06-23Cycles: Add multi-scattering, energy-conserving GGX as an option to the ↵Lukas Stockner
Glossy, Anisotropic and Glass BSDFs This commit adds a new distribution to the Glossy, Anisotropic and Glass BSDFs that implements the multiple-scattering microfacet model described in the paper "Multiple-Scattering Microfacet BSDFs with the Smith Model". Essentially, the improvement is that unlike classical GGX, which only models single scattering and assumes the contribution of multiple bounces to be zero, this new model performs a random walk on the microsurface until the ray leaves it again, which ensures perfect energy conservation. In practise, this means that the "darkening problem" - GGX materials becoming darker with increasing roughness - is solved in a physically correct and efficient way. The downside of this model is that it has no (known) analytic expression for evalation. However, it can be evaluated stochastically, and although the correct PDF isn't known either, the properties of MIS and the balance heuristic guarantee an unbiased result at the cost of slightly higher noise. Reviewers: dingto, #cycles, brecht Reviewed By: dingto, #cycles, brecht Subscribers: bliblubli, ace_dragon, gregzaal, brecht, harvester, dingto, marcog, swerner, jtheninja, Blendify, nutel Differential Revision: https://developer.blender.org/D2002
2015-07-18Cycles: Point density texture supportSergey Sharybin
This commit implements point density texture for Cycles shading nodes. It's done via creating voxel texture at shader compilation time, Not totally memory efficient, but avoids adding sampling code to kernel (which keeps render time as low as possible), In the future this will be compensated by using OpenVDB for more efficient storage of sparse volume data. Sampling of the voxel texture is happening at blender side and the same code is used as for Blender Internal's renderer. This texture is controlled by only object, particle system and radius. Linear falloff is used and there's no turbulence. This is because falloff is expected to happen using Curve Mapping node. Turbulence will be done as a distortion on the input coordinate. It's already possible to fake it using nose textures and in the future we can add more proper turbulence distortion node, which then could also be used for 2D texture mapping. Particle color support is done by Lukas, thanks!
2015-04-06Multi-View and Stereo 3DDalai Felinto
Official Documentation: http://www.blender.org/manual/render/workflows/multiview.html Implemented Features ==================== Builtin Stereo Camera * Convergence Mode * Interocular Distance * Convergence Distance * Pivot Mode Viewport * Cameras * Plane * Volume Compositor * View Switch Node * Image Node Multi-View OpenEXR support Sequencer * Image/Movie Strips 'Use Multiview' UV/Image Editor * Option to see Multi-View images in Stereo-3D or its individual images * Save/Open Multi-View (OpenEXR, Stereo3D, individual views) images I/O * Save/Open Multi-View (OpenEXR, Stereo3D, individual views) images Scene Render Views * Ability to have an arbitrary number of views in the scene Missing Bits ============ First rule of Multi-View bug report: If something is not working as it should *when Views is off* this is a severe bug, do mention this in the report. Second rule is, if something works *when Views is off* but doesn't (or crashes) when *Views is on*, this is a important bug. Do mention this in the report. Everything else is likely small todos, and may wait until we are sure none of the above is happening. Apart from that there are those known issues: * Compositor Image Node poorly working for Multi-View OpenEXR (this was working prefectly before the 'Use Multi-View' functionality) * Selecting camera from Multi-View when looking from camera is problematic * Animation Playback (ctrl+F11) doesn't support stereo formats * Wrong filepath when trying to play back animated scene * Viewport Rendering doesn't support Multi-View * Overscan Rendering * Fullscreen display modes need to warn the user * Object copy should be aware of views suffix Acknowledgments =============== * Francesco Siddi for the help with the original feature specs and design * Brecht Van Lommel for the original review of the code and design early on * Blender Foundation for the Development Fund to support the project wrap up Final patch reviewers: * Antony Riakiotakis (psy-fi) * Campbell Barton (ideasman42) * Julian Eisel (Severin) * Sergey Sharybin (nazgul) * Thomas Dinged (dingto) Code contributors of the original branch in github: * Alexey Akishin * Gabriel Caraballo
2015-03-25minor cleanup: alignmentMike Erwin
2014-08-12Freestyle: Added new UV Along Stroke shader node.Tamito Kajiyama
2014-08-12Freestyle: Added "blend_type" and "use_clamp" options to the Output Line ↵Tamito Kajiyama
Style shader node.
2014-08-12Added new Output Line Style shader node for defining a node-based line material.Tamito Kajiyama
2014-07-26New compositor node "Sun Beams"Lukas Tönne
This allows adding a "fake" sun beam effect, simulating crepuscular rays from light being scattered in a medium like the atmosphere or deep water. Such effects can be created also by renderers using volumetric lighting, but the compositor feature is a lot cheaper and is independent from 3D rendering. This makes it ideally suited for motion graphics. The implementation uses am optimized accumulation method for gathering color values along a line segment. The inner buffer loop uses fixed offset increments to avoid unnecessary multiplications and avoids variables by using compile-time specialization (see inline comments for further details).
2014-06-14Cycles: Don't show "Sharp" distribution in the Anisotropic node.Thomas Dinges
2014-06-14Cycles: glossy and anisotropic BSDF changesBrecht Van Lommel
* Anisotropic BSDF now supports GGX and Beckmann distributions, Ward has been removed because other distributions are superior. * GGX is now the default distribution for all glossy and anisotropic nodes, since it looks good, has low noise and is fast to evaluate. * Ashikhmin-Shirley is now available in the Glossy BSDF.
2014-06-14Cycles: Ashikhmin-Shirley anisotropic BSDFKarsten Schwenk
* Ashikhmin-Shirley anisotropic BSDF was added as closure * Anisotropic BSDF node now has two distributions Reviewers: brecht, dingto Differential Revision: https://developer.blender.org/D549
2014-06-13Cycles: Add dedicated nodes to split/combine vectors.Thomas Dinges
This was already possible via the RGB nodes, but that seems weird.
2014-04-02Cycles: add dedicated UV Map node, easier to find and has convenient auto ↵Kevin Dietrich
complete. Fixes T37954. Reviewed By: brecht, dingto Differential Revision: https://developer.blender.org/D230
2014-03-11New Corner Pin node: uses explicit corner values for a plane warp ↵Lukas Tönne
transformation. This was suggested by Christopher Barrett (terrachild). Corner pin is a common feature in compositing. The corners for the plane warping can be defined by using vector node inputs to allow using perspective plane transformations without having to go via the MovieClip editor tracking data. Uses the same math as the PlaneTrack node, but without the link to MovieClip and Object. {F78199} The code for PlaneTrack operations has been restructured a bit to share it with the CornerPin node. * PlaneDistortCommonOperation.h/.cpp: Shared generic code for warping images based on 4 plane corners and a perspective matrix generated from these. Contains operation base classes for both the WarpImage and Mask operations. * PlaneTrackOperation.h/.cpp: Current plane track node operations, based on the common code above. These add pointers to MovieClip and Object which define the track data from wich to read the corners. * PlaneCornerPinOperation.h/.cpp: New corner pin variant, using explicit input sockets for the plane corners. One downside of the current compositor design is that there is no concept of invariables (constants) that don't vary over the image space. This has already been an issue for Blur nodes (size input is usually constant except when "variable size" is enabled) and a few others. For the corner pin node it is necessary that the corner input sockets are also invariant. They have to be evaluated for each tile now, otherwise the data is not available. This in turn makes it necessary to make the operation "complex" and request full input buffers, which adds unnecessary overhead.
2014-01-20Fix T37978: cycles nodes with multiple Material Output nodes not predictable.Brecht Van Lommel
Now it uses the last activated node like compositing does. This should have no effect on existing files until you activate another output node there.
2013-12-28Cycles Volume Render: work on nodes and closures.Brecht Van Lommel
* Henyey-Greenstein scattering closure implementation. * Rename transparent to absorption node and isotropic to scatter node. * Volume density is folded into the closure weights. * OSL support for volume closures and nodes. * This commit has no user visible changes, there is no volume render code yet. This is work by "storm", Stuart Broadfoot, Thomas Dinges and myself.
2013-11-25Blender Internal: Add "Lamp Data" shader node that allows shaders to acquire ↵IRIE Shinsuke
information such as light vector from specified Lamp. For now this provides the following outputs: - Color - Light Vector - Distance - Shadow - Visibility Factor Note: Color output is multiplied by the lamp energy. Multiplication of color*max(dot(light_vector,normal_vector),0)*shadow*visibility_factor produces the exact same result as the Lambert shader. Many thanks to Brecht for code review and discussion!
2013-09-24modifiers_isCorrectableDeformed now checks a modifier is enabled before ↵Campbell Barton
returning true, also check deformMatricesEM callback for modifier_isCorrectableDeformed() rather then checking modifier types.
2013-09-16Cycles Hair: Two basic bair shaders addedStuart Broadfoot
A new hair bsdf node, with two closure options, is added. These closures allow the generation of the reflective and transmission components of hair. The node allows control of the highlight colour, roughness and angular shift. Llimitations include: -No glint or fresnel adjustments. -The 'offset' is un-used when triangle primitives are used.
2013-09-12Fix #36706: Added complementary API functions for the FileOutput node so ↵Lukas Toenne
file/layer slots (input sockets) can be added without using the operator. Instead of adding sockets to these node using the node.inputs collection, the node.file_slots or node.layer_slots collections should be used. Both of them work, they just provide slightly different properties for use with simple files or multi-layer EXR. The FileOutput node design is cumbersome and should be considered broken. It should eventually be replaced, the problem with that is backward/forward compatibility.
2013-08-18Cycles: Subsurface ScatteringBrecht Van Lommel
New features: * Bump mapping now works with SSS * Texture Blur factor for SSS, see the documentation for details: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/Shaders#Subsurface_Scattering Work in progress for feedback: Initial implementation of the "BSSRDF Importance Sampling" paper, which uses a different importance sampling method. It gives better quality results in many ways, with the availability of both Cubic and Gaussian falloff functions, but also tends to be more noisy when using the progressive integrator and does not give great results with some geometry. It works quite well for the non-progressive integrator and is often less noisy there. This code may still change a lot, so unless you're testing it may be best to stick to the Compatible falloff function. Skin test render and file that takes advantage of the gaussian falloff: http://www.pasteall.org/pic/show.php?id=57661 http://www.pasteall.org/pic/show.php?id=57662 http://www.pasteall.org/blend/23501
2013-08-16Merge plane track feature from tomato branchSergey Sharybin
This commit includes all the changes made for plane tracker in tomato branch. Movie clip editor changes: - Artist might create a plane track out of multiple point tracks which belongs to the same track (minimum amount of point tracks is 4, maximum is not actually limited). When new plane track is added, it's getting "tracked" across all point tracks, which makes it stick to the same plane point tracks belong to. - After plane track was added, it need to be manually adjusted in a way it covers feature one might to mask/replace. General transform tools (G, R, S) or sliding corners with a mouse could be sued for this. Plane corner which corresponds to left bottom image corner has got X/Y axis on it (red is for X axis, green for Y). - Re-adjusting plane corners makes plane to be "re-tracked" for the frames sequence between current frame and next and previous keyframes. - Kayframes might be removed from the plane, using Shit-X (Marker Delete) operator. However, currently manual re-adjustment or "re-track" trigger is needed. Compositor changes: - Added new node called Plane Track Deform. - User selects which plane track to use (for this he need to select movie clip datablock, object and track names). - Node gets an image input, which need to be warped into the plane. - Node outputs: * Input image warped into the plane. * Plane, rasterized to a mask. Masking changes: - Mask points might be parented to a plane track, which makes this point deforming in a way as if it belongs to the tracked plane. Some video tutorials are available: - Coder video: http://www.youtube.com/watch?v=vISEwqNHqe4 - Artist video: https://vimeo.com/71727578 This is mine and Keir's holiday code project :)
2013-08-01Cycles / HSV Separator and Combine node:Thomas Dinges
* Added nodes to separate and combine hsv colors. Part of my GSoC 2013 project, SVN merge of r57981.
2013-08-01Cycles / Vector Transform node:Thomas Dinges
* Add a note to convert a Vector, Point or Normal between World <=> Camera <=> Object coordinate space. Documentation: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/More#Vector_Transform Part of my GSoC 2013 project, SVN merge of r57599, r57670, r57918, r57919, r58245 and r58775.
2013-08-01Cycles / Blackbody to RGB node:Thomas Dinges
* Added a node to convert a temperature in Kelvin to an RGB color. This can be used e.g. for lights, to easily find the right color temperature. = Some common temperatures = Candle light: 1500 Kelvin Sunset/Sunrise: 1850 Kelvin Studio lamps: 3200 Kelvin Horizon daylight: 5000 Kelvin Documentation: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/More#Blackbody Thanks to Philipp Oeser (lichtwerk), who essentially contributed to this with a patch! :) This is part of my GSoC 2013 project. SVN merge of r57424, r57487, r57507, r57525, r58253 and r58774
2013-07-19Nodes / UI:Thomas Dinges
* Change UI string for LayerWeight node to "Layer Weight" (with the gap in between), for consistency with other nodes.
2013-07-04Cycles:Thomas Dinges
* Added 2 new nodes to combine and separate HSV colors. Screenshot: http://www.pasteall.org/pic/show.php?id=54828
2013-06-20Cycles / Vector Transform Node:Thomas Dinges
* First step towards a new vector transform node, to convert Points/Vectors between World/Object/Camera space. This only contains the Blender UI, RNA... code, no Cycles integration yet.
2013-06-13Cycles / Blackbody node:Thomas Dinges
* First step towards a Blackbody to RGB converter. You can specify a color in Kelvin inside the node. * Only implemented for OSL atm, SVM will follow.
2013-06-10Cycles / Wavelength to RGB node:Thomas Dinges
* Added a node to convert wavelength (in nanometer, from 380nm to 780nm) to RGB values. This can be useful to match real world colors easier. Example render: http://www.pasteall.org/pic/show.php?id=53202 ToDo: * Move some functions into an util file, maybe a common util_color.h or so. * Test GPU, unfortunately sm_21 doesn't work for me yet.
2013-05-23Cycles / Toon BSDF:Thomas Dinges
* Added a toon bsdf node to Cycles. This was already available as OSL only closure, but is now available inside the SVM backed as well, for CPU and GPU rendering. * There are 2 variations available, diffuse and glossy toon, selectable via a menu inside the node. Documentation: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/Shaders#Toon Example render & blend file: http://www.pasteall.org/pic/show.php?id=51970 http://www.pasteall.org/blend/21579
2013-05-20Cycles / Wireframe node:Thomas Dinges
* Added a wireframe node (Input category) to get access to Mesh wireframe data. The thickness can be controlled via a "Size" parameter, and is available in world units (default) and screen pixel size. * Only the triangulated mesh is available now, quads is for later. Documentation: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/More#Wireframe Render and Example file: http://www.pasteall.org/pic/show.php?id=51731 http://www.pasteall.org/blend/21510
2013-05-10Cycles: bump node changes to add a Distance input that controls the overall ↵Brecht Van Lommel
displacement distance, and an Invert option to invert the bump effect.
2013-05-05correction for uv template, also some doxygen comment corrections. Campbell Barton
2013-04-02Cycles: initial subsurface multiple scattering support. It's not working asBrecht Van Lommel
well as I would like, but it works, just add a subsurface scattering node and you can use it like any other BSDF. It is using fully raytraced sampling compatible with progressive rendering and other more advanced rendering algorithms we might used in the future, and it uses no extra memory so it's suitable for complex scenes. Disadvantage is that it can be quite noisy and slow. Two limitations that will be solved are that it does not work with bump mapping yet, and that the falloff function used is a simple cubic function, it's not using the real BSSRDF falloff function yet. The node has a color input, along with a scattering radius for each RGB color channel along with an overall scale factor for the radii. There is also no GPU support yet, will test if I can get that working later. Node Documentation: http://wiki.blender.org/index.php/Doc:2.6/Manual/Render/Cycles/Nodes/Shaders#BSSRDF Implementation notes: http://wiki.blender.org/index.php/Dev:2.6/Source/Render/Cycles/Subsurface_Scattering
2013-03-18Merge of the PyNodes branch (aka "custom nodes") into trunk.Lukas Toenne
PyNodes opens up the node system in Blender to scripters and adds a number of UI-level improvements. === Dynamic node type registration === Node types can now be added at runtime, using the RNA registration mechanism from python. This enables addons such as render engines to create a complete user interface with nodes. Examples of how such nodes can be defined can be found in my personal wiki docs atm [1] and as a script template in release/scripts/templates_py/custom_nodes.py [2]. === Node group improvements === Each node editor now has a tree history of edited node groups, which allows opening and editing nested node groups. The node editor also supports pinning now, so that different spaces can be used to edit different node groups simultaneously. For more ramblings and rationale see (really old) blog post on code.blender.org [3]. The interface of node groups has been overhauled. Sockets of a node group are no longer displayed in columns on either side, but instead special input/output nodes are used to mirror group sockets inside a node tree. This solves the problem of long node lines in groups and allows more adaptable node layout. Internal sockets can be exposed from a group by either connecting to the extension sockets in input/output nodes (shown as empty circle) or by adding sockets from the node property bar in the "Interface" panel. Further details such as the socket name can also be changed there. [1] http://wiki.blender.org/index.php/User:Phonybone/Python_Nodes [2] http://projects.blender.org/scm/viewvc.php/trunk/blender/release/scripts/templates_py/custom_nodes.py?view=markup&root=bf-blender [3] http://code.blender.org/index.php/2012/01/improving-node-group-interface-editing/
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