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			15 Commits
		
	
	
	| Author | SHA1 | Message | Date | |
|---|---|---|---|---|
|  JMS55 | aa626e4f0b | Per-meshlet compressed vertex data (#15643) # Objective - Prepare for streaming by storing vertex data per-meshlet, rather than per-mesh (this means duplicating vertices per-meshlet) - Compress vertex data to reduce the cost of this ## Solution The important parts are in from_mesh.rs, the changes to the Meshlet type in asset.rs, and the changes in meshlet_bindings.wgsl. Everything else is pretty secondary/boilerplate/straightforward changes. - Positions are quantized in centimeters with a user-provided power of 2 factor (ideally auto-determined, but that's a TODO for the future), encoded as an offset relative to the minimum value within the meshlet, and then stored as a packed list of bits using the minimum number of bits needed for each vertex position channel for that meshlet - E.g. quantize positions (lossly, throws away precision that's not needed leading to using less bits in the bitstream encoding) - Get the min/max quantized value of each X/Y/Z channel of the quantized positions within a meshlet - Encode values relative to the min value of the meshlet. E.g. convert from [min, max] to [0, max - min] - The new max value in the meshlet is (max - min), which only takes N bits, so we only need N bits to store each channel within the meshlet (lossless) - We can store the min value and that it takes N bits per channel in the meshlet metadata, and reconstruct the position from the bitstream - Normals are octahedral encoded and than snorm2x16 packed and stored as a single u32. - Would be better to implement the precise variant of octhedral encoding for extra precision (no extra decode cost), but decided to keep it simple for now and leave that as a followup - Tried doing a quantizing and bitstream encoding scheme like I did for positions, but struggled to get it smaller. Decided to go with this for simplicity for now - UVs are uncompressed and take a full 64bits per vertex which is expensive - In the future this should be improved - Tangents, as of the previous PR, are not explicitly stored and are instead derived from screen space gradients - While I'm here, split up MeshletMeshSaverLoader into two separate types Other future changes include implementing a smaller encoding of triangle data (3 u8 indices = 24 bits per triangle currently), and more disk-oriented compression schemes. References: * "A Deep Dive into UE5's Nanite Virtualized Geometry" https://advances.realtimerendering.com/s2021/Karis_Nanite_SIGGRAPH_Advances_2021_final.pdf#page=128 (also available on youtube) * "Towards Practical Meshlet Compression" https://arxiv.org/pdf/2404.06359 * "Vertex quantization in Omniforce Game Engine" https://daniilvinn.github.io/2024/05/04/omniforce-vertex-quantization.html ## Testing - Did you test these changes? If so, how? - Converted the stanford bunny, and rendered it with a debug material showing normals, and confirmed that it's identical to what's on main. EDIT: See additional testing in the comments below. - Are there any parts that need more testing? - Could use some more size comparisons on various meshes, and testing different quantization factors. Not sure if 4 is a good default. EDIT: See additional testing in the comments below. - Also did not test runtime performance of the shaders. EDIT: See additional testing in the comments below. - How can other people (reviewers) test your changes? Is there anything specific they need to know? - Use my unholy script, replacing the meshlet example https://paste.rs/7xQHk.rs (must make MeshletMesh fields pub instead of pub crate, must add lz4_flex as a dev-dependency) (must compile with meshlet and meshlet_processor features, mesh must have only positions, normals, and UVs, no vertex colors or tangents) --- ## Migration Guide - TBD by JMS55 at the end of the release | ||
|  arcashka | 6027890a11 | move wgsl color operations from bevy_pbr to bevy_render (#13209) # Objective `bevy_pbr/utils.wgsl` shader file contains mathematical constants and color conversion functions. Both of those should be accessible without enabling `bevy_pbr` feature. For example, tonemapping can be done in non pbr scenario, and it uses color conversion functions. Fixes #13207 ## Solution * Move mathematical constants (such as PI, E) from `bevy_pbr/src/render/utils.wgsl` into `bevy_render/src/maths.wgsl` * Move color conversion functions from `bevy_pbr/src/render/utils.wgsl` into new file `bevy_render/src/color_operations.wgsl` ## Testing Ran multiple examples, checked they are working: * tonemapping * color_grading * 3d_scene * animated_material * deferred_rendering * 3d_shapes * fog * irradiance_volumes * meshlet * parallax_mapping * pbr * reflection_probes * shadow_biases * 2d_gizmos * light_gizmos --- ## Changelog * Moved mathematical constants (such as PI, E) from `bevy_pbr/src/render/utils.wgsl` into `bevy_render/src/maths.wgsl` * Moved color conversion functions from `bevy_pbr/src/render/utils.wgsl` into new file `bevy_render/src/color_operations.wgsl` ## Migration Guide In user's shader code replace usage of mathematical constants from `bevy_pbr::utils` to the usage of the same constants from `bevy_render::maths`. | ||
|  Patrick Walton | 961b24deaf | Implement filmic color grading. (#13121) This commit expands Bevy's existing tonemapping feature to a complete set of filmic color grading tools, matching those of engines like Unity, Unreal, and Godot. The following features are supported: * White point adjustment. This is inspired by Unity's implementation of the feature, but simplified and optimized. *Temperature* and *tint* control the adjustments to the *x* and *y* chromaticity values of [CIE 1931]. Following Unity, the adjustments are made relative to the [D65 standard illuminant] in the [LMS color space]. * Hue rotation. This simply converts the RGB value to [HSV], alters the hue, and converts back. * Color correction. This allows the *gamma*, *gain*, and *lift* values to be adjusted according to the standard [ASC CDL combined function]. * Separate color correction for shadows, midtones, and highlights. Blender's source code was used as a reference for the implementation of this. The midtone ranges can be adjusted by the user. To avoid abrupt color changes, a small crossfade is used between the different sections of the image, again following Blender's formulas. A new example, `color_grading`, has been added, offering a GUI to change all the color grading settings. It uses the same test scene as the existing `tonemapping` example, which has been factored out into a shared glTF scene. [CIE 1931]: https://en.wikipedia.org/wiki/CIE_1931_color_space [D65 standard illuminant]: https://en.wikipedia.org/wiki/Standard_illuminant#Illuminant_series_D [LMS color space]: https://en.wikipedia.org/wiki/LMS_color_space [HSV]: https://en.wikipedia.org/wiki/HSL_and_HSV [ASC CDL combined function]: https://en.wikipedia.org/wiki/ASC_CDL#Combined_Function ## Changelog ### Added * Many new filmic color grading options have been added to the `ColorGrading` component. ## Migration Guide * `ColorGrading::gamma` and `ColorGrading::pre_saturation` are now set separately for the `shadows`, `midtones`, and `highlights` sections. You can migrate code with the `ColorGrading::all_sections` and `ColorGrading::all_sections_mut` functions, which access and/or update all sections at once. * `ColorGrading::post_saturation` and `ColorGrading::exposure` are now fields of `ColorGrading::global`. ## Screenshots   | ||
|  JMS55 | 40bfce556a | Add random shader utils, fix cluster_debug_visualization (#11956) # Objective - Partially addresses https://github.com/bevyengine/bevy/issues/11470 (I'd like to add Spatiotemporal Blue Noise in the future, but that's a bit more controversial). - Fix cluster_debug_visualization which has not compiled for a while --- ## Changelog - Added random white noise shader functions to `bevy_pbr::utils` ## Migration Guide - The `bevy_pbr::utils::random1D` shader function has been replaced by the similar `bevy_pbr::utils::rand_f`. | ||
|  Elabajaba | 70a592f31a | Update to wgpu 0.18 (#10266) # Objective Keep up to date with wgpu. ## Solution Update the wgpu version. Currently blocked on naga_oil updating to naga 0.14 and releasing a new version. 3d scenes (or maybe any scene with lighting?) currently don't render anything due to ``` error: naga_oil bug, please file a report: composer failed to build a valid header: Type [2] '' is invalid = Capability Capabilities(CUBE_ARRAY_TEXTURES) is required ``` I'm not sure what should be passed in for `wgpu::InstanceFlags`, or if we want to make the gles3minorversion configurable (might be useful for debugging?) Currently blocked on https://github.com/bevyengine/naga_oil/pull/63, and https://github.com/gfx-rs/wgpu/issues/4569 to be fixed upstream in wgpu first. ## Known issues Amd+windows+vulkan has issues with texture_binding_arrays (see the image [here](https://github.com/bevyengine/bevy/pull/10266#issuecomment-1819946278)), but that'll be fixed in the next wgpu/naga version, and you can just use dx12 as a workaround for now (Amd+linux mesa+vulkan texture_binding_arrays are fixed though). --- ## Changelog Updated wgpu to 0.18, naga to 0.14.2, and naga_oil to 0.11. - Windows desktop GL should now be less painful as it no longer requires Angle. - You can now toggle shader validation and debug information for debug and release builds using `WgpuSettings.instance_flags` and [InstanceFlags](https://docs.rs/wgpu/0.18.0/wgpu/struct.InstanceFlags.html) ## Migration Guide - `RenderPassDescriptor` `color_attachments` (as well as `RenderPassColorAttachment`, and `RenderPassDepthStencilAttachment`) now use `StoreOp::Store` or `StoreOp::Discard` instead of a `boolean` to declare whether or not they should be stored. - `RenderPassDescriptor` now have `timestamp_writes` and `occlusion_query_set` fields. These can safely be set to `None`. - `ComputePassDescriptor` now have a `timestamp_writes` field. This can be set to `None` for now. - See the [wgpu changelog](https://github.com/gfx-rs/wgpu/blob/trunk/CHANGELOG.md#v0180-2023-10-25) for additional details | ||
|  Marco Buono | 44928e0df4 | StandardMaterialLight Transmission (#8015)# Objective
<img width="1920" alt="Screenshot 2023-04-26 at 01 07 34"
src="https://user-images.githubusercontent.com/418473/234467578-0f34187b-5863-4ea1-88e9-7a6bb8ce8da3.png">
This PR adds both diffuse and specular light transmission capabilities
to the `StandardMaterial`, with support for screen space refractions.
This enables realistically representing a wide range of real-world
materials, such as:
  - Glass; (Including frosted glass)
  - Transparent and translucent plastics;
  - Various liquids and gels;
  - Gemstones;
  - Marble;
  - Wax;
  - Paper;
  - Leaves;
  - Porcelain.
Unlike existing support for transparency, light transmission does not
rely on fixed function alpha blending, and therefore works with both
`AlphaMode::Opaque` and `AlphaMode::Mask` materials.
## Solution
- Introduces a number of transmission related fields in the
`StandardMaterial`;
- For specular transmission:
- Adds logic to take a view main texture snapshot after the opaque
phase; (in order to perform screen space refractions)
- Introduces a new `Transmissive3d` phase to the renderer, to which all
meshes with `transmission > 0.0` materials are sent.
- Calculates a light exit point (of the approximate mesh volume) using
`ior` and `thickness` properties
- Samples the snapshot texture with an adaptive number of taps across a
`roughness`-controlled radius enabling “blurry” refractions
- For diffuse transmission:
- Approximates transmitted diffuse light by using a second, flipped +
displaced, diffuse-only Lambertian lobe for each light source.
## To Do
- [x] Figure out where `fresnel_mix()` is taking place, if at all, and
where `dielectric_specular` is being calculated, if at all, and update
them to use the `ior` value (Not a blocker, just a nice-to-have for more
correct BSDF)
- To the _best of my knowledge, this is now taking place, after
 | ||
|  Griffin | a15d152635 | Deferred Renderer (#9258) # Objective - Add a [Deferred Renderer](https://en.wikipedia.org/wiki/Deferred_shading) to Bevy. - This allows subsequent passes to access per pixel material information before/during shading. - Accessing this per pixel material information is needed for some features, like GI. It also makes other features (ex. Decals) simpler to implement and/or improves their capability. There are multiple approaches to accomplishing this. The deferred shading approach works well given the limitations of WebGPU and WebGL2. Motivation: [I'm working on a GI solution for Bevy](https://youtu.be/eH1AkL-mwhI) # Solution - The deferred renderer is implemented with a prepass and a deferred lighting pass. - The prepass renders opaque objects into the Gbuffer attachment (`Rgba32Uint`). The PBR shader generates a `PbrInput` in mostly the same way as the forward implementation and then [packs it into the Gbuffer]( | ||
|  JMS55 | af9c945f40 | Screen Space Ambient Occlusion (SSAO) MVP (#7402) 
# Objective
- Add Screen space ambient occlusion (SSAO). SSAO approximates
small-scale, local occlusion of _indirect_ diffuse light between
objects. SSAO does not apply to direct lighting, such as point or
directional lights.
- This darkens creases, e.g. on staircases, and gives nice contact
shadows where objects meet, giving entities a more "grounded" feel.
- Closes https://github.com/bevyengine/bevy/issues/3632.
## Solution
- Implement the GTAO algorithm.
-
https://www.activision.com/cdn/research/Practical_Real_Time_Strategies_for_Accurate_Indirect_Occlusion_NEW%20VERSION_COLOR.pdf
-
https://blog.selfshadow.com/publications/s2016-shading-course/activision/s2016_pbs_activision_occlusion.pdf
- Source code heavily based on [Intel's
XeGTAO]( | ||
|  Marco Buono | 292e069bb5 | Apply codebase changes in preparation for StandardMaterialtransmission (#8704)# Objective - Make #8015 easier to review; ## Solution - This commit contains changes not directly related to transmission required by #8015, in easier-to-review, one-change-per-commit form. --- ## Changelog ### Fixed - Clear motion vector prepass using `0.0` instead of `1.0`, to avoid TAA artifacts on transparent objects against the background; ### Added - The `E` mathematical constant is now available for use in shaders, exposed under `bevy_pbr::utils`; - A new `TAA` shader def is now available, for conditionally enabling shader logic via `#ifdef` when TAA is enabled; (e.g. for jittering texture samples) - A new `FallbackImageZero` resource is introduced, for when a fallback image filled with zeroes is required; - A new `RenderPhase<I>::render_range()` method is introduced, for render phases that need to render their items in multiple parceled out “steps”; ### Changed - The `MainTargetTextures` struct now holds both `Texture` and `TextureViews` for the main textures; - The fog shader functions under `bevy_pbr::fog` now take the a `Fog` structure as their first argument, instead of relying on the global `fog` uniform; - The main textures can now be used as copy sources; ## Migration Guide - `ViewTarget::main_texture()` and `ViewTarget::main_texture_other()` now return `&Texture` instead of `&TextureView`. If you were relying on these methods, replace your usage with `ViewTarget::main_texture_view()`and `ViewTarget::main_texture_other_view()`, respectively; - `ViewTarget::sampled_main_texture()` now returns `Option<&Texture>` instead of a `Option<&TextureView>`. If you were relying on this method, replace your usage with `ViewTarget::sampled_main_texture_view()`; - The `apply_fog()`, `linear_fog()`, `exponential_fog()`, `exponential_squared_fog()` and `atmospheric_fog()` functions now take a configurable `Fog` struct. If you were relying on them, update your usage by adding the global `fog` uniform as their first argument; | ||
|  Elabajaba | bfd1d4b0a7 | Wgpu 0.15 (#7356) # Objective Update Bevy to wgpu 0.15. ## Changelog - Update to wgpu 0.15, wgpu-hal 0.15.1, and naga 0.11 - Users can now use the [DirectX Shader Compiler](https://github.com/microsoft/DirectXShaderCompiler) (DXC) on Windows with DX12 for faster shader compilation and ShaderModel 6.0+ support (requires `dxcompiler.dll` and `dxil.dll`, which are included in DXC downloads from [here](https://github.com/microsoft/DirectXShaderCompiler/releases/latest)) ## Migration Guide ### WGSL Top-Level `let` is now `const` All top level constants are now declared with `const`, catching up with the wgsl spec. `let` is no longer allowed at the global scope, only within functions. ```diff -let SOME_CONSTANT = 12.0; +const SOME_CONSTANT = 12.0; ``` #### `TextureDescriptor` and `SurfaceConfiguration` now requires a `view_formats` field The new `view_formats` field in the `TextureDescriptor` is used to specify a list of formats the texture can be re-interpreted to in a texture view. Currently only changing srgb-ness is allowed (ex. `Rgba8Unorm` <=> `Rgba8UnormSrgb`). You should set `view_formats` to `&[]` (empty) unless you have a specific reason not to. #### The DirectX Shader Compiler (DXC) is now supported on DX12 DXC is now the default shader compiler when using the DX12 backend. DXC is Microsoft's replacement for their legacy FXC compiler, and is faster, less buggy, and allows for modern shader features to be used (ShaderModel 6.0+). DXC requires `dxcompiler.dll` and `dxil.dll` to be available, otherwise it will log a warning and fall back to FXC. You can get `dxcompiler.dll` and `dxil.dll` by downloading the latest release from [Microsoft's DirectXShaderCompiler github repo](https://github.com/microsoft/DirectXShaderCompiler/releases/latest) and copying them into your project's root directory. These must be included when you distribute your Bevy game/app/etc if you plan on supporting the DX12 backend and are using DXC. `WgpuSettings` now has a `dx12_shader_compiler` field which can be used to choose between either FXC or DXC (if you pass None for the paths for DXC, it will check for the .dlls in the working directory). | ||
|  IceSentry | 3c63c0dab7 | Move prepass functions to prepass_utils (#7354) # Objective - The functions added to utils.wgsl by the prepass assume that mesh_view_bindings are present, which isn't always the case - Fixes https://github.com/bevyengine/bevy/issues/7353 ## Solution - Move these functions to their own `prepass_utils.wgsl` file Co-authored-by: IceSentry <IceSentry@users.noreply.github.com> | ||
|  IceSentry | b3224e135b | Add depth and normal prepass  (#6284) # Objective - Add a configurable prepass - A depth prepass is useful for various shader effects and to reduce overdraw. It can be expansive depending on the scene so it's important to be able to disable it if you don't need any effects that uses it or don't suffer from excessive overdraw. - The goal is to eventually use it for things like TAA, Ambient Occlusion, SSR and various other techniques that can benefit from having a prepass. ## Solution The prepass node is inserted before the main pass. It runs for each `Camera3d` with a prepass component (`DepthPrepass`, `NormalPrepass`). The presence of one of those components is used to determine which textures are generated in the prepass. When any prepass is enabled, the depth buffer generated will be used by the main pass to reduce overdraw. The prepass runs for each `Material` created with the `MaterialPlugin::prepass_enabled` option set to `true`. You can overload the shader used by the prepass by using `Material::prepass_vertex_shader()` and/or `Material::prepass_fragment_shader()`. It will also use the `Material::specialize()` for more advanced use cases. It is enabled by default on all materials. The prepass works on opaque materials and materials using an alpha mask. Transparent materials are ignored. The `StandardMaterial` overloads the prepass fragment shader to support alpha mask and normal maps. --- ## Changelog - Add a new `PrepassNode` that runs before the main pass - Add a `PrepassPlugin` to extract/prepare/queue the necessary data - Add a `DepthPrepass` and `NormalPrepass` component to control which textures will be created by the prepass and available in later passes. - Add a new `prepass_enabled` flag to the `MaterialPlugin` that will control if a material uses the prepass or not. - Add a new `prepass_enabled` flag to the `PbrPlugin` to control if the StandardMaterial uses the prepass. Currently defaults to false. - Add `Material::prepass_vertex_shader()` and `Material::prepass_fragment_shader()` to control the prepass from the `Material` ## Notes In bevy's sample 3d scene, the performance is actually worse when enabling the prepass, but on more complex scenes the performance is generally better. I would like more testing on this, but @DGriffin91 has reported a very noticeable improvements in some scenes. The prepass is also used by @JMS55 for TAA and GTAO discord thread: <https://discord.com/channels/691052431525675048/1011624228627419187> This PR was built on top of the work of multiple people Co-Authored-By: @superdump Co-Authored-By: @robtfm Co-Authored-By: @JMS55 Co-authored-by: Charles <IceSentry@users.noreply.github.com> Co-authored-by: JMS55 <47158642+JMS55@users.noreply.github.com> | ||
|  Torstein Grindvik | cb5e2d84be | Use wgsl saturate (#6318) # Objective Use saturate wgsl function now implemented in naga (version 0.10.0). There is now no need for one in utils.wgsl. naga's version allows usage for not only scalars but vectors as well. ## Solution Remove the utils.wgsl saturate function. ## Changelog Remove saturate function from utils.wgsl in favor of saturate in naga v0.10.0. | ||
|  robtfm | 503c2a9677 | adjust cluster index for viewport origin (#5947) # Objective fixes #5946 ## Solution adjust cluster index calculation for viewport origin. from reading point 2 of the rasterization algorithm description in https://gpuweb.github.io/gpuweb/#rasterization, it looks like framebuffer space (and so @bulitin(position)) is not meant to be adjusted for viewport origin, so we need to subtract that to get the right cluster index. - add viewport origin to rust `ExtractedView` and wgsl `View` structs - subtract from frag coord for cluster index calculation | ||
|  Robert Swain | c6222f1acc | Separate out PBR lighting, shadows, clustered forward, and utils from pbr.wgsl (#4938) # Objective - Builds on top of #4901 - Separate out PBR lighting, shadows, clustered forward, and utils from `pbr.wgsl` as part of making the PBR code more reusable and extensible. - See #3969 for details. ## Solution - Add `bevy_pbr::utils`, `bevy_pbr::clustered_forward`, `bevy_pbr::lighting`, `bevy_pbr::shadows` shader imports exposing many shader functions for external use - Split `PI`, `saturate()`, `hsv2rgb()`, and `random1D()` into `bevy_pbr::utils` - Split clustered-forward-specific functions into `bevy_pbr::clustered_forward`, including moving the debug visualization code into a `cluster_debug_visualization()` function in that import - Split PBR lighting functions into `bevy_pbr::lighting` - Split shadow functions into `bevy_pbr::shadows` --- ## Changelog - Added: `bevy_pbr::utils`, `bevy_pbr::clustered_forward`, `bevy_pbr::lighting`, `bevy_pbr::shadows` shader imports exposing many shader functions for external use - Split `PI`, `saturate()`, `hsv2rgb()`, and `random1D()` into `bevy_pbr::utils` - Split clustered-forward-specific functions into `bevy_pbr::clustered_forward`, including moving the debug visualization code into a `cluster_debug_visualization()` function in that import - Split PBR lighting functions into `bevy_pbr::lighting` - Split shadow functions into `bevy_pbr::shadows` |