On a user level this fixes configuration when a spot light is
linked to an object, and a sun light is not linked to anything.
It used to be making non-linked receivers to be very noisy.
This is because the distant light did not update the node's
light linking settings when they are added to the node.
A simple demo file will be added to the tests suit as
light_link_distant_tree.blend.
Pull Request: https://projects.blender.org/blender/blender/pulls/108311
Similar to objects, store the name of Blender's side light name
on the Cycles side. This allows to have readable logs where a
name and property is logged (while previously in the logs all
lights will be called lamp).
There is no user-measurable change.
Pull Request: https://projects.blender.org/blender/blender/pulls/108310
The original names were `...update_position()`, but no update in
position is performed in these functions, rather, the entries in
`LightSample` are updated. Also make clear that the functions are used
by MNEE.
This patch fixes an undefined behaviour where we were trying to use linked functions with binary archives. This isn't supported yet. At best this will fail silently, but this is not guaranteed in future. To fix this we simply disable binary archives if any linked functions are involved. The impact of this is that the `SHADE_SURFACE_RAYTRACE` and `SHADE_SURFACE_MNEE` kernels will fall back to the file system cache when MetalRT is enabled. The file system cache will occasionally be purged due to factors beyond Blender's control.
Pull Request: https://projects.blender.org/blender/blender/pulls/108176
Only Embree CPU BVH was built in the multi-device case. However, one
Embree GPU BVH is needed per GPU, so we now reuse the same logic as in
the other backends.
Pull Request: https://projects.blender.org/blender/blender/pulls/107992
Hardware Raytracing wasn't properly disabled or enabled in the
subdevices of the multi-device.
This construct:
foreach ( DeviceInfo &info,
(device.multi_devices.size() != 0 ?
device.multi_devices : vector<DeviceInfo>({device}))
)
was a nice trap - it was giving a copy to iterate on.
Pull Request: https://projects.blender.org/blender/blender/pulls/107989
Used to be https://archive.blender.org/developer/D17123.
Internally these are already using the same code path anyways, there's no point in maintaining two distinct nodes.
The obvious approach would be to add Anisotropy controls to the Glossy BSDF node and remove the Anisotropic BSDF node. However, that would break forward compability, since older Blender versions don't know how to handle the Anisotropy input on the Glossy BSDF node.
Therefore, this commit technically removes the Glossy BSDF node, uses versioning to replace them with an Anisotropic BSDF node, and renames that node to "Glossy BSDF".
That way, when you open a new file in an older version, all the nodes show up as Anisotropic BSDF nodes and render correctly.
This is a bit ugly internally since we need to preserve the old `idname` which now no longer matches the UI name, but that's not too bad.
Also removes the "Sharp" distribution option and replaces it with GGX, sets Roughness to zero and disconnects any input to the Roughness socket.
Pull Request: https://projects.blender.org/blender/blender/pulls/104445
NanoVDB headers have unused code using "double" type, which is not supported on Arc GPUs.
Recent DPC++ changes enforced runtime verifications:
7663dc201d
which prevents execution when such type has been present even if unused.
This is a solution to avoid double to be compiled at all, similar as how it is done for Metal.
Area light sampling use special techniques to reduce noise with small
spread angles; the change in sampled area was not taken into
consideration when computing the pdf in MNEE.
Pull Request: https://projects.blender.org/blender/blender/pulls/107897
After the removal of the Shadow pass this no longer worked. Now it works by
marking the object as a shadow catcher and returning the Shadow Catcher pass.
The result is different than before, since it also takes into account indirect
light now and uses a different method to weight the contribution of lights that
is adaptive to the light strength.
