NVIDIA REAL-TIME DENOISERS v4.3.6 (NRD)

For quick starting see NRD sample project.

OVERVIEW

NVIDIA Real-Time Denoisers (NRD) is a spatio-temporal API agnostic denoising library. The library has been designed to work with low rpp (ray per pixel) signals. NRD is a fast solution that slightly depends on input signals and environment conditions.

NRD includes the following denoisers:

REBLUR - recurrent blur based denoiser
RELAX - SVGF based denoiser using clamping to fast history to minimize temporal lag, has been designed for RTXDI (RTX Direct Illumination). It uses 30% more memory and 20% slower than REBLUR
SIGMA - shadow-only denoiser

Supported signal types:

RELAX:
- Diffuse & specular radiance
REBLUR:
- Diffuse & specular radiance
- Diffuse (ambient) & specular occlusion (OCCLUSION variants)
- Diffuse (ambient) directional occlusion (DIRECTIONAL_OCCLUSION variant)
- Diffuse & specular radiance in spherical harmonics (spherical gaussians) (SH variants)
SIGMA:
- Shadows from an infinite light source (sun, moon)
- Shadows from a local light source (omni, spot)
- Shadows from multiple sources (experimental).

For diffuse and specular signals de-modulated irradiance (i.e. irradiance with "removed" materials) can be used instead of radiance (see "Recommendations and Best Practices" section).

NRD is distributed as a source as well with a “ready-to-use” library (if used in a precompiled form). It can be integrated into any DX12, VULKAN or DX11 engine using two variants:

Native implementation of the NRD API using engine capabilities
Integration via an abstraction layer. In this case, the engine should expose native Graphics API pointers for certain types of objects. The integration layer, provided as a part of SDK, can be used to simplify this kind of integration.

HOW TO BUILD?

Install Cmake 3.15+
Install on
- Windows: latest WindowsSDK (22000+), VulkanSDK (1.3.216+)
- Linux (x86-64): latest VulkanSDK
- Linux (aarch64): find a precompiled binary for DXC or disable shader compilation NRD_EMBEDS_SPIRV_SHADERS=OFF
Build (variant 1) - using Git and CMake explicitly
- Clone project and init submodules
- Generate and build the project using CMake
Build (variant 2) - by running scripts:
- Run 1-Deploy
- Run 2-Build

CMake options:

NRD_SHADERS_PATH - shader output path override
NRD_STATIC_LIBRARY - build static library (OFF by default)
NRD_DXC_CUSTOM_PATH - custom DXC to use if Vulkan SDK is not installed
NRD_NORMAL_ENCODING - normal encoding for the entire library
NRD_ROUGHNESS_ENCODING - roughness encoding for the entire library
NRD_EMBEDS_DXBC_SHADERS - NRD compiles and embeds DXBC shaders (ON by default on Windows)
NRD_EMBEDS_DXIL_SHADERS - NRD compiles and embeds DXIL shaders (ON by default on Windows)
NRD_EMBEDS_SPIRV_SHADERS - NRD compiles and embeds SPIRV shaders (ON by default)
NRD_DISABLE_SHADER_COMPILATION - disable shader compilation on the NRD side, NRD assumes that shaders are already compiled externally and have been put into NRD_SHADERS_PATH folder

NRD_NORMAL_ENCODING and NRD_ROUGHNESS_ENCODING can be defined only once during project deployment. These settings are dumped in NRDEncoding.hlsli file, which needs to be included on the application side prior NRD.hlsli inclusion to deliver encoding settings matching NRD settings. LibraryDesc includes encoding settings too. It can be used to verify that the library meets the application expectations.

Tested platforms:

OS	Architectures	Compilers
Windows	AMD64	MSVC, Clang
Linux	AMD64, ARM64	GCC, Clang

SDK packaging:

Compile the solution (Debug / Release or both, depending on what you want to get in NRD package)
Run 3-Prepare NRD SDK
Grab generated in the root directory _NRD_SDK and _NRI_SDK (if needed) folders and use them in your project

HOW TO UPDATE?

Clone latest with all dependencies
Run 4-Clean.bat
Run 1-Deploy
Run 2-Build

HOW TO REPORT ISSUES?

NRD sample has TESTS section in the bottom of the UI, a new test can be added if needed. The following procedure is recommended:

Try to reproduce a problem in the NRD sample first
- if reproducible
  - add a test (by pressing Add button)
  - describe the issue and steps to reproduce on GitHub
  - attach depending on the selected scene .bin file from the Tests folder
- if not
  - verify the integration
If nothing helps
- describe the issue, attach a video and steps to reproduce

Additionally, for any information, suggestions or general requests please feel free to contact us at [email protected]

API

Terminology:

Denoiser - a denoiser to use (for example: Denoiser::REBLUR_DIFFUSE)
Instance - a set of denoisers aggregated into a monolithic entity (the library is free to rearrange passes without dependencies). Each denoiser in the instance has an associated Identifier
Resource - an input, output or internal resource (currently can only be a texture)
Texture pool (or pool) - a texture pool that stores permanent or transient resources needed for denoising. Textures from the permanent pool are dedicated to NRD and can not be reused by the application (history buffers are stored here). Textures from the transient pool can be reused by the application right after denoising. NRD doesn’t allocate anything. NRD provides resource descriptions, but resource creations are done on the application side.

Flow:

GetLibraryDesc - contains general NRD library information (supported denoisers, SPIRV binding offsets). This call can be skipped if this information is known in advance (for example, is diffuse denoiser available?), but it can’t be skipped if SPIRV binding offsets are needed for VULKAN
CreateInstance - creates an instance for requested denoisers
GetInstanceDesc - returns descriptions for pipelines, samplers, texture pools, constant buffer and descriptor set. All this stuff is needed during the initialization step
SetCommonSettings - sets common (shared) per frame parameters
SetDenoiserSettings - can be called to change parameters dynamically before applying the denoiser on each new frame / denoiser call
GetComputeDispatches - returns per-dispatch data for the list of denoisers (bound subresources with required state, constant buffer data). Returned memory is owned by the instance and gets overwritten by the next GetComputeDispatches call
DestroyInstance - destroys an instance

NRD doesn't make any graphics API calls. The application is supposed to invoke a set of compute Dispatch calls to actually denoise input signals. Please, refer to NrdIntegration::Denoise() and NrdIntegration::Dispatch() calls in NRDIntegration.hpp file as an example of an integration using low level RHI.

NRD doesn’t have a "resize" functionality. On resolution change the old denoiser needs to be destroyed and a new one needs to be created with new parameters. But NRD supports dynamic resolution scaling via CommonSettings::resolutionScale.

Some textures can be requested as inputs or outputs for a method (see the next section). Required resources are specified near a denoiser declaration inside the Denoiser enum class. Also NRD.hlsli has a comment near each front-end or back-end function, clarifying which resources this function is for.

NON-NOISY INPUTS

Commons inputs for primary hits (if PSR is not used, common use case) or for secondary hits (if PSR is used, valid only for 0-roughness):

IN_MV - non-jittered surface motion (old = new + MV)

Modes:
- 2D screen-space motion - 2D motion doesn't provide information about movement along the view direction. NRD can reject history on dynamic objects in this case
- 2.5D screen-space motion (recommended) - similar to the 2D screen-space motion, but .z = viewZprev - viewZ
- 3D world-space motion - camera motion should not be included (it's already in the matrices). In other words, if there are no moving objects, all motion vectors must be 0 even if the camera is moving
Motion vector scaling can be provided via CommonSettings::motionVectorScale. NRD expectations:
- Use CommonSettings::isMotionVectorInWorldSpace = true for 3D world-space motion
- Use CommonSettings::isMotionVectorInWorldSpace = false and CommonSettings::motionVectorScale[2] == 0 for 2D screen-space motion
- Use CommonSettings::isMotionVectorInWorldSpace = false and CommonSettings::motionVectorScale[2] != 0 for 2.5D screen-space motion
IN_NORMAL_ROUGHNESS - surface world-space normal and linear roughness

Normal and roughness encoding must be controlled via Cmake parameters NRD_NORMAL_ENCODING and NRD_ROUGHNESS_ENCODING. Optional NRDEncoding.hlsli file is generated during project deployment, which can be included prior NRD.hlsli to make encoding macro definitions visible in shaders (if NRD_NORMAL_ENCODING and NRD_ROUGHNESS_ENCODING are not defined in another way by the application). Encoding settings can be known at runtime by accessing GetLibraryDesc().normalEncoding and GetLibraryDesc().roghnessEncoding respectively. NormalEncoding and RoughnessEncoding enums briefly describe encoding variants. It's recommended to use NRD_FrontEnd_PackNormalAndRoughness from NRD.hlsli to match decoding.

NRD computes local curvature using provided normals. Less accurate normals can lead to banding in curvature and local flatness. RGBA8 normals is a good baseline, but R10G10B10A10 oct-packed normals improve curvature calculations and specular tracking as the result.

If materialID is provided and supported by encoding, NRD diffuse and specular denoisers won't mix up surfaces with different material IDs.
IN_VIEWZ - .x - view-space Z coordinate of primary hits (linearized g-buffer depth)

Positive and negative values are supported. Z values in all pixels must be in the same space, matching space defined by matrices passed to NRD. If, for example, the protagonist's hands are rendered using special matrices, Z values should be computed as:
- reconstruct world position using special matrices for "hands"
- project on screen using matrices passed to NRD
- .w component is positive view Z (or just transform world-space position to main view space and take .z component)

All textures should be NaN free at each pixel, even at pixels outside of denoising range.

The illustration below shows expected inputs for primary hits:

hitDistance = length( B - A ); // hitT for 1st bounce (recommended baseline)

IN_VIEWZ = TransformToViewSpace( A ).z;
IN_NORMAL_ROUGHNESS = GetNormalAndRoughnessAt( A );
IN_MV = GetMotionAt( A );

See NRDDescs.h for more details and descriptions of other inputs and outputs.

NOISY INPUTS

NRD sample is a good start to familiarize yourself with input requirements and best practices, but main requirements can be summarized to:

Since NRD denoisers accumulate signals for a limited number of frames, the input signal must converge reasonably well for this number of frames. REFERENCE denoiser can be used to estimate temporal signal quality
Since NRD denoisers process signals spatially, high-energy fireflies in the input signal should be avoided. Most of them can be removed by enabling anti-firefly filter in NRD, but it will only work if the "background" signal is confident. The worst case is having a single pixel with high energy divided by a very small PDF to represent the lack of energy in neighboring non-representative (black) pixels
Radiance must be separated into diffuse and specular at primary hit (or secondary hit in case of PSR)
hitT can't be negative
hitT must not include primary hit distance
hitT for the first bounce after the primary hit or PSR must be provided "as is"
hitT for subsequent bounces and for bounces before PSR must be adjusted by curvature and lobe energy dissipation on the application side
- Do not pass sum of lengths of all segments as hitT. A solid baseline is to use hit distance for the 1st bounce only, it works well for diffuse and specular signals
- NRD sample uses more complex approach for accumulating hitT along the path, which takes into account energy dissipation due to lobe spread and curvature at the current hit
For rays pointing inside the surface (VNDF sampling can easily produce those), hitT must be set to 0 (but better to not cast such rays)
Noise in hit distances must follow a diffuse or specular lobe. It implies that hitT for roughness = 0 must be clean (if probabilistic sampling is not in use)
In case of probabilistic diffuse / specular selection at the primary hit, provided hitT must follow the following rules:
- Should not be divided by PDF
- If diffuse or specular sampling is skipped, hitT must be set to 0 for corresponding signal type
- hitDistanceReconstructionMode must be set to something other than OFF, but bear in mind that the search area is limited to 3x3 or 5x5. In other words, it's the application's responsibility to guarantee a valid sample in this area. It can be achieved by clamping probabilities and using Bayer-like dithering (see the sample for more details)
- Pre-pass must be enabled (i.e. diffusePrepassBlurRadius and specularPrepassBlurRadius must be set to 20-70 pixels) to compensate entropy increase, since radiance in valid samples is divided by probability to compensate 0 values in some neighbors
Probabilistic sampling for 2nd+ bounces is absolutely acceptable

See NRDDescs.h for more details and descriptions of other inputs and outputs.

IMPROVING OUTPUT QUALITY

The temporal part of NRD naturally suppresses jitter, which is essential for upscaling techniques. If an SH denoiser is in use, a high quality resolve can be applied to the final output to regain back macro details, micro details and per-pixel jittering. As an example, the image below demonstrates the results after and before resolve with active DLSS (quality mode).

The resolve process takes place on the application side and has the following modular structure:

construct an SG (spherical gaussian) light
apply diffuse or specular resolve function to reconstruct macro details
apply re-jittering to reconstruct micro details
(optionally) or just extract unresolved color (fully matches the output of a corresponding non-SH denoiser)

Shader code:

// Diffuse
float4 diff = gIn_Diff.SampleLevel( gLinearSampler, pixelUv, 0 );
float4 diff1 = gIn_DiffSh.SampleLevel( gLinearSampler, pixelUv, 0 );
NRD_SG diffSg = REBLUR_BackEnd_UnpackSh( diff, diff1 );

// Specular
float4 spec = gIn_Spec.SampleLevel( gLinearSampler, pixelUv, 0 );
float4 spec1 = gIn_SpecSh.SampleLevel( gLinearSampler, pixelUv, 0 );
NRD_SG specSg = REBLUR_BackEnd_UnpackSh( spec, spec1 );

// ( Optional ) AO / SO ( available only for REBLUR )
diff.w = diffSg.normHitDist;
spec.w = specSg.normHitDist;

if( gResolve )
{
    // ( Optional ) replace "roughness" with "roughnessAA"
    roughness = NRD_SG_ExtractRoughnessAA( specSg );

    // Regain macro-details
    diff.xyz = NRD_SG_ResolveDiffuse( diffSg, N ); // or NRD_SH_ResolveDiffuse( sg, N )
    spec.xyz = NRD_SG_ResolveSpecular( specSg, N, V, roughness );

    // Regain micro-details & jittering // TODO: preload N and Z into SMEM
    float3 Ne = NRD_FrontEnd_UnpackNormalAndRoughness( gIn_Normal_Roughness[ pixelPos + int2( 1, 0 ) ] ).xyz;
    float3 Nw = NRD_FrontEnd_UnpackNormalAndRoughness( gIn_Normal_Roughness[ pixelPos + int2( -1, 0 ) ] ).xyz;
    float3 Nn = NRD_FrontEnd_UnpackNormalAndRoughness( gIn_Normal_Roughness[ pixelPos + int2( 0, 1 ) ] ).xyz;
    float3 Ns = NRD_FrontEnd_UnpackNormalAndRoughness( gIn_Normal_Roughness[ pixelPos + int2( 0, -1 ) ] ).xyz;

    float Ze = gIn_ViewZ[ pixelPos + int2( 1, 0 ) ];
    float Zw = gIn_ViewZ[ pixelPos + int2( -1, 0 ) ];
    float Zn = gIn_ViewZ[ pixelPos + int2( 0, 1 ) ];
    float Zs = gIn_ViewZ[ pixelPos + int2( 0, -1 ) ];

    float2 scale = NRD_SG_ReJitter( diffSg, specSg, Rf0, V, roughness, viewZ, Ze, Zw, Zn, Zs, N, Ne, Nw, Nn, Ns );

    diff.xyz *= scale.x;
    spec.xyz *= scale.y;
}
else
{
    // ( Optional ) Unresolved color matching the non-SH version of the denoiser
    diff.xyz = NRD_SG_ExtractColor( diffSg );
    spec.xyz = NRD_SG_ExtractColor( specSg );
}

Re-jittering math with minorly modified inputs can also be used with RESTIR produced sampling without involving SH denoisers. You only need to get light direction in the current pixel from RESTIR. Despite that RESTIR produces noisy light selections, its low variations can be easily handled by DLSS or other upscaling techs.

VALIDATION LAYER

If CommonSettings::enableValidation = true REBLUR & RELAX denoisers render debug information into OUT_VALIDATION output. Alpha channel contains layer transparency to allow easy mix with the final image on the application side. Currently the following viewport layout is used on the screen:

0	1	2	3
4	5	6	7
8	9	10	11
12	13	14	15

where:

Viewport 0 - world-space normals
Viewport 1 - linear roughness
Viewport 2 - linear viewZ
- green = +
- blue = -
- red = out of denoising range
Viewport 3 - difference between MVs, coming from IN_MV, and expected MVs, assuming that the scene is static
- blue = out of screen
- pixels with moving objects have non-0 values
Viewport 4 - world-space grid & camera jitter:
- 1 cube = 1 unit
- the square in the bottom-right corner represents a pixel with accumulated samples
- the red boundary of the square marks jittering outside of the pixel area

REBLUR specific:

Viewport 7 - amount of virtual history
Viewport 8 - number of accumulated frames for diffuse signal (red = history reset)
Viewport 11 - number of accumulated frames for specular signal (red = history reset)
Viewport 12 - input normalized hitT for diffuse signal (ambient occlusion, AO)
Viewport 15 - input normalized hitT for specular signal (specular occlusion, SO)

MEMORY REQUIREMENTS

The Persistent column (matches NRD Permanent pool) indicates how much of the Working set is required to be left intact for subsequent frames of the application. This memory stores the history resources consumed by NRD. The Aliasable column (matches NRD Transient pool) shows how much of the Working set may be aliased by textures or other resources used by the application outside of the operating boundaries of NRD.

Resolution	Denoiser	Working set (Mb)	Persistent (Mb)	Aliasable (Mb)
1080p	REBLUR_DIFFUSE	86.69	42.25	44.44
	REBLUR_DIFFUSE_OCCLUSION	42.44	25.38	17.06
	REBLUR_DIFFUSE_SH	137.31	59.12	78.19
	REBLUR_SPECULAR	105.75	50.75	55.00
	REBLUR_SPECULAR_OCCLUSION	50.94	33.88	17.06
	REBLUR_SPECULAR_SH	156.38	67.62	88.75
	REBLUR_DIFFUSE_SPECULAR	169.06	71.88	97.19
	REBLUR_DIFFUSE_SPECULAR_OCCLUSION	72.12	38.12	34.00
	REBLUR_DIFFUSE_SPECULAR_SH	270.31	105.62	164.69
	REBLUR_DIFFUSE_DIRECTIONAL_OCCLUSION	86.69	42.25	44.44
	SIGMA_SHADOW	23.38	0.00	23.38
	SIGMA_SHADOW_TRANSLUCENCY	42.31	0.00	42.31
	RELAX_DIFFUSE	99.25	63.31	35.94
	RELAX_DIFFUSE_SH	158.31	88.62	69.69
	RELAX_SPECULAR	101.44	63.38	38.06
	RELAX_SPECULAR_SH	168.94	97.12	71.81
	RELAX_DIFFUSE_SPECULAR	168.94	97.12	71.81
	RELAX_DIFFUSE_SPECULAR_SH	303.94	164.62	139.31
	REFERENCE	33.75	33.75	0.00

1440p	REBLUR_DIFFUSE	153.81	75.00	78.81
	REBLUR_DIFFUSE_OCCLUSION	75.06	45.00	30.06
	REBLUR_DIFFUSE_SH	243.81	105.00	138.81
	REBLUR_SPECULAR	187.56	90.00	97.56
	REBLUR_SPECULAR_OCCLUSION	90.06	60.00	30.06
	REBLUR_SPECULAR_SH	277.56	120.00	157.56
	REBLUR_DIFFUSE_SPECULAR	300.06	127.50	172.56
	REBLUR_DIFFUSE_SPECULAR_OCCLUSION	127.56	67.50	60.06
	REBLUR_DIFFUSE_SPECULAR_SH	480.06	187.50	292.56
	REBLUR_DIFFUSE_DIRECTIONAL_OCCLUSION	153.81	75.00	78.81
	SIGMA_SHADOW	41.38	0.00	41.38
	SIGMA_SHADOW_TRANSLUCENCY	75.12	0.00	75.12
	RELAX_DIFFUSE	176.31	112.50	63.81
	RELAX_DIFFUSE_SH	281.31	157.50	123.81
	RELAX_SPECULAR	180.06	112.50	67.56
	RELAX_SPECULAR_SH	300.06	172.50	127.56
	RELAX_DIFFUSE_SPECULAR	300.06	172.50	127.56
	RELAX_DIFFUSE_SPECULAR_SH	540.06	292.50	247.56
	REFERENCE	60.00	60.00	0.00

2160p	REBLUR_DIFFUSE	326.81	159.38	167.44
	REBLUR_DIFFUSE_OCCLUSION	159.44	95.62	63.81
	REBLUR_DIFFUSE_SH	518.06	223.12	294.94
	REBLUR_SPECULAR	398.50	191.25	207.25
	REBLUR_SPECULAR_OCCLUSION	191.31	127.50	63.81
	REBLUR_SPECULAR_SH	589.75	255.00	334.75
	REBLUR_DIFFUSE_SPECULAR	637.56	270.94	366.62
	REBLUR_DIFFUSE_SPECULAR_OCCLUSION	271.00	143.44	127.56
	REBLUR_DIFFUSE_SPECULAR_SH	1020.06	398.44	621.62
	REBLUR_DIFFUSE_DIRECTIONAL_OCCLUSION	326.81	159.38	167.44
	SIGMA_SHADOW	88.06	0.00	88.06
	SIGMA_SHADOW_TRANSLUCENCY	159.69	0.00	159.69
	RELAX_DIFFUSE	374.69	239.12	135.56
	RELAX_DIFFUSE_SH	597.81	334.75	263.06
	RELAX_SPECULAR	382.69	239.12	143.56
	RELAX_SPECULAR_SH	637.69	366.62	271.06
	RELAX_DIFFUSE_SPECULAR	637.69	366.62	271.06
	RELAX_DIFFUSE_SPECULAR_SH	1147.69	621.62	526.06
	REFERENCE	127.50	127.50	0.00

INTEGRATION VARIANTS

VARIANT 1: Black-box library (using the application-side Render Hardware Interface)

RHI must have the ability to do the following:

Create shaders from precompiled binary blobs
Create an SRV for a specific range of subresources
Create and bind 4 predefined samplers
Invoke a Dispatch call (no raster, no VS/PS)
Create 2D textures with SRV / UAV access

VARIANT 2: White-box library (using the application-side Render Hardware Interface)

Logically it's close to the Method 1, but the integration takes place in the full source code (only the NRD project is needed). In this case NRD shaders are handled by the application shader compilation pipeline. The application should still use NRD via NRD API to preserve forward compatibility. This variant suits best for compilation on other platforms (consoles, ARM), unlocks NRD modification on the application side and increases portability.

VARIANT 3: Black-box library (using native API pointers)

If Graphics API's native pointers are retrievable from the RHI, the standard NRD integration layer can be used to greatly simplify the integration. In this case, the application should only wrap up native pointers for the Device, CommandList and some input / output Resources into entities, compatible with an API abstraction layer (NRI), and all work with NRD library will be hidden inside the integration layer:

Engine or App → native objects → NRD integration layer → NRI → NRD

NRI = NVIDIA Rendering Interface - an abstraction layer on top of Graphics APIs: DX11, DX12 and VULKAN. NRI has been designed to provide low overhead access to the Graphics APIs and simplify development of DX12 and VULKAN applications. NRI API has been influenced by VULKAN as the common denominator among these 3 APIs.

NRI and NRD are ready-to-use products. The application must expose native pointers only for Device, Resource and CommandList entities (no SRVs and UAVs - they are not needed, everything will be created internally). Native resource pointers are needed only for the denoiser inputs and outputs (all intermediate textures will be handled internally). Descriptor heap will be changed to an internal one, so the application needs to bind its original descriptor heap after invoking the denoiser.

In rare cases, when the integration via the engine’s RHI is not possible and the integration using native pointers is complicated, a "DoDenoising" call can be added explicitly to the application-side RHI. It helps to avoid increasing code entropy.

The pseudo code below demonstrates how NRD integration and NRI can be used to wrap native Graphics API pointers into NRI objects to establish connection between the application and NRD:

//=======================================================================================================
// INITIALIZATION - DECLARATIONS
//=======================================================================================================

#include "NRIDescs.hpp"
#include "Extensions/NRIWrapperD3D12.h"
#include "Extensions/NRIHelper.h"

#include "NRD.h"
#include "NRDIntegration.hpp"

NrdIntegration NRD = NrdIntegration(maxNumberOfFramesInFlight);

struct NriInterface
    : public nri::CoreInterface
    , public nri::HelperInterface
    , public nri::WrapperD3D12Interface
{};
NriInterface NRI;

//=======================================================================================================
// INITIALIZATION - WRAP NATIVE DEVICE
//=======================================================================================================

// Wrap the device
nri::DeviceCreationD3D12Desc deviceDesc = {};
deviceDesc.d3d12Device = ...;
deviceDesc.d3d12PhysicalAdapter = ...;
deviceDesc.d3d12GraphicsQueue = ...;
deviceDesc.enableNRIValidation = false;

nri::Device* nriDevice = nullptr;
nri::Result nriResult = nri::CreateDeviceFromD3D12Device(deviceDesc, nriDevice);

// Get core functionality
nriResult = nri::GetInterface(*nriDevice,
  NRI_INTERFACE(nri::CoreInterface), (nri::CoreInterface*)&NRI);

nriResult = nri::GetInterface(*nriDevice,
  NRI_INTERFACE(nri::HelperInterface), (nri::HelperInterface*)&NRI);

// Get appropriate "wrapper" extension (XXX - can be D3D11, D3D12 or VULKAN)
nriResult = nri::GetInterface(*nriDevice,
  NRI_INTERFACE(nri::WrapperXXXInterface), (nri::WrapperXXXInterface*)&NRI);

//=======================================================================================================
// INITIALIZATION - INITIALIZE NRD
//=======================================================================================================

const nrd::DenoiserDesc denoiserDescs[] =
{
    // Put neeeded denoisers here, like:
    { identifier1, nrd::Denoiser::XXX, renderResolution.x, renderResolution.y },
    { identifier2, nrd::Denoiser::YYY, renderResolution.x, renderResolution.y },
};

nrd::InstanceCreationDesc instanceCreationDesc = {};
instanceCreationDesc.denoisers = denoiserDescs;
instanceCreationDesc.denoisersNum = GetCountOf(denoiserDescs);

bool result = NRD.Initialize(*nriDevice, NRI, NRI, instanceCreationDesc);

//=======================================================================================================
// INITIALIZATION or RENDER - WRAP NATIVE POINTERS
//=======================================================================================================

// Wrap the command buffer
nri::CommandBufferD3D12Desc commandBufferDesc = {};
commandBufferDesc.d3d12CommandList = (ID3D12GraphicsCommandList*)d3d12CommandList;

// Not needed for NRD integration layer, but needed for NRI validation layer
commandBufferDesc.d3d12CommandAllocator = (ID3D12CommandAllocator*)d3d12CommandAllocatorOrJustNonNull;

nri::CommandBuffer* nriCommandBuffer = nullptr;
NRI.CreateCommandBufferD3D12(*nriDevice, commandBufferDesc, nriCommandBuffer);

// Wrap required textures (better do it only once on initialization)
nri::TextureTransitionBarrierDesc entryDescs[N] = {};
nri::Format entryFormat[N] = {};

for (uint32_t i = 0; i < N; i++)
{
    nri::TextureTransitionBarrierDesc& entryDesc = entryDescs[i];
    const MyResource& myResource = GetMyResource(i);

    nri::TextureD3D12Desc textureDesc = {};
    textureDesc.d3d12Resource = myResource->GetNativePointer();
    NRI.CreateTextureD3D12(*nriDevice, textureDesc, (nri::Texture*&)entryDesc.texture );

    // You need to specify the current state of the resource here, after denoising NRD can modify
    // this state. Application must continue state tracking from this point.
    // Useful information:
    //    SRV = nri::AccessBits::SHADER_RESOURCE, nri::TextureLayout::SHADER_RESOURCE
    //    UAV = nri::AccessBits::SHADER_RESOURCE_STORAGE, nri::TextureLayout::GENERAL
    entryDesc.nextAccess = ConvertResourceStateToAccessBits( myResource->GetCurrentState() );
    entryDesc.nextLayout = ConvertResourceStateToLayout( myResource->GetCurrentState() );
}

//=======================================================================================================
// RENDER - DENOISE
//=======================================================================================================

// Set common settings
//  - for the first time use defaults
//  - currently NRD supports only the following view space: X - right, Y - top, Z - forward or backward
nrd::CommonSettings commonSettings = {};
PopulateCommonSettings(commonSettings);

NRD.SetCommonSettings(commonSettings);

// Set settings for each method in the NRD instance
nrd::XxxSettings settings1 = {};
PopulateXxxSettings(settings1);

NRD.SetDenoiserSettings(identifier1, &settings1);

nrd::YyySettings settings2 = {};
PopulateYyySettings(settings2);

NRD.SetDenoiserSettings(identifier2, &settings2);

// Fill up the user pool
NrdUserPool userPool = {};
{
    // Fill only required "in-use" inputs and outputs in appropriate slots using entryDescs & entryFormat,
    // applying remapping if necessary. Unused slots will be {nullptr, nri::Format::UNKNOWN}
    NrdIntegration_SetResource(userPool, ...);
    ...
    NrdIntegration_SetResource(userPool, ...);
};

// Better use "true" if resources are not changing between frames (i.e. are not suballocated from a heap)
bool enableDescriptorCaching = true;

const nrd::Identifier denoisers[] = {identifier1, identifier2};
NRD.Denoise(denoisers, helper::GetCountOf(denoisers), *nriCommandBuffer, userPool, enableDescriptorCaching);

// IMPORTANT: NRD integration binds own descriptor pool, don't forget to re-bind back your pool (heap)

//=======================================================================================================
// SHUTDOWN or RENDER - CLEANUP
//=======================================================================================================

// Better do it only once on shutdown
for (uint32_t i = 0; i < N; i++)
    NRI.DestroyTexture(entryDescs[i].texture);

NRI.DestroyCommandBuffer(*nriCommandBuffer);

//=======================================================================================================
// SHUTDOWN - DESTROY
//=======================================================================================================

// Release wrapped device
NRI.DestroyDevice(*nriDevice);

// Also NRD needs to be recreated on "resize"
NRD.Destroy();

Shader part:

#if 1
    #include "NRDEncoding.hlsli"
#else
    // Or define NRD encoding in Cmake and deliver macro definitions to shader compilation command line
#endif

#include "NRD.hlsli"

// Call corresponding "front end" function to encode data for NRD (NRD.hlsli indicates which function
// needs to be used for a specific input for a specific denoiser). For example:

float4 nrdIn = RELAX_FrontEnd_PackRadianceAndHitDist(radiance, hitDistance);

// Call corresponding "back end" function to decode data produced by NRD. For example:

float4 nrdOut = RELAX_BackEnd_UnpackRadiance(nrdOutEncoded);

RECOMMENDATIONS AND BEST PRACTICES: GREATER TIPS

Denoising is not a panacea or miracle. Denoising works best with ray tracing results produced by a suitable form of importance sampling. Additionally, NRD has its own restrictions. The following suggestions should help to achieve best image quality:

MATERIAL DE-MODULATION (IRRADIANCE → RADIANCE)

NRD has been designed to work with pure radiance coming from a particular direction. This means that data in the form "something / probability" should be avoided if possible because overall entropy of the input signal will be increased (but it doesn't mean that denoising won't work). Additionally, it means that materials needs to be decoupled from the input signal, i.e. irradiance, typically produced by a path tracer, needs to be transformed into radiance, i.e. BRDF should be applied after denoising. This is achieved by using "demodulation" trick:

// Diffuse
Denoising( diffuseRadiance * albedo ) → NRD( diffuseRadiance / albedo ) * albedo

// Specular
float3 preintegratedBRDF = PreintegratedBRDF( Rf0, N, V, roughness )
Denoising( specularRadiance * BRDF ) → NRD( specularRadiance * BRDF / preintegratedBRDF ) * preintegratedBRDF

A good approximation for pre-integrated specular BRDF can be found here.

COMBINED DENOISING OF DIRECT AND INDIRECT LIGHTING

For specular signal use indirect hitT for both direct and indirect lighting

The reason is that the denoiser uses hitT mostly for calculating motion vectors for reflections. For that purpose, the denoiser expects to see hitT from surfaces that are in the specular reflection lobe. When calculating direct lighting (NEE/RTXDI), we select a light per pixel, and the distance to that light becomes the hitT for both diffuse and specular channels. In many cases, the light is selected for a surface because of its diffuse contribution, not specular, which makes the specular channel contain the hitT of a diffuse light. That confuses the denoiser and breaks reprojection. On the other hand, the indirect specular hitT is always computed by tracing rays in the specular lobe.

For diffuse signal hitT can be further adjusted by mixing hitT from direct and indirect rays to get sharper shadows

Use first bounce hit distance for the indirect in the pseudo-code below:

float hitDistContribution = directDiffuseLuminance / ( directDiffuseLuminance + indirectDiffuseLuminance + EPS );

float maxContribution = 0.5; // 0.65 works good as well
float directHitDistContribution = min(directHitDistContribution, maxContribution); // avoid over-sharpening

hitDist = lerp(indirectDiffuseHitDist, directDiffuseHitDist, directHitTContribution);

INTERACTION WITH PRIMARY SURFACE REPLACEMENTS (PSR)

When denoising reflections in pure mirrors, some advantages can be reached if NRD "sees" the first "non-pure mirror" point after a series of pure mirror bounces (delta events). This point is called Primary Surface Replacement.

Primary Surface Replacement (PSR) can be used with NRD.

Notes, requirements and restrictions:

the primary hit (0th bounce) gets replaced with the first "non-pure mirror" hit in the bounce chain - this hit becomes PSR
all associated data in the g-buffer gets replaced by PSR data
the camera "sees" PSRs like the mirror surfaces in-between don't exist. This space is called virtual world space
- virtual space position lies on the same view vector as the primary hit position, but the position is elongated. Elongation depends on hitT and curvature at bounces, starting from the primary hit
- virtual space normal is the normal at PSR hit mirrored several times in the reversed order until the primary hit is reached
PSR data is NOT always data at the PSR hit!
- material properties (albedo, metalness, roughness etc.) are from PSR hit
- IN_VIEWZ contains viewZ of the virtual position
- IN_MV contains motion of the virtual position
- IN_NORMAL_ROUGHNESS contains normal at virtual world space and roughness at PSR
- accumulated hitT for NRD starts at the PSR hit. Curvature must be taken into account on the application side only for 2nd+ bounces starting from this hit (similarly to hitT requirements in Noisy Inputs section)
- ray direction for NRD must be transformed into virtual space

In case of PSR NRD disocclusion logic doesn't take curvature at primary hit into account, because data for primary hits is replaced. This can lead to more intense disocclusions on bumpy surfaces due to significant ray divergence. To mitigate this problem 2x-10x larger disocclusionThreshold can be used. This is an applicable solution if the denoiser is used to denoise surfaces with PSR only (glass only, for example). In a general case, when PSR and normal surfaces are mixed on the screen, higher disocclusion thresholds are needed only for pixels with PSR. This can be achieved by using IN_DISOCCLUSION_THRESHOLD_MIX input to smoothly mix baseline disocclusionThreshold into bigger disocclusionThresholdAlternate from CommonSettings. Most likely the increased disocclusion threshold is needed only for pixels with normal details at primary hits (local curvature is not zero).

The illustration below shows expected inputs for secondary hits:

hitDistance = length( C - B ); // hitT for 2nd bounce, but it's 1st bounce in the reflected world
Bvirtual = A + viewVector * length( B - A );

IN_VIEWZ = TransformToViewSpace( Bvirtual ).z;
IN_NORMAL_ROUGHNESS = GetVirtualSpaceNormalAndRoughnessAt( B );
IN_MV = GetMotionAt( B );

INTERACTION WITH FRAME GENERATION TECHNIQUES

Frame generation (FG) techniques boost FPS by interpolating between 2 last available frames. NRD works better when framerate increases, because it gets more data per second. It's not the case for FG, because all rendering pipeline underlying passes (like, denoising) continue to work on the original non-boosted framerate.

RECOMMENDATIONS AND BEST PRACTICES: LESSER TIPS

[NRD] The NRD API has been designed to support integration into native VULKAN apps. If the RHI you work with is DX11-like, not all provided data will be needed.

[NRD] Read all comments in NRDDescs.h, NRDSettings.h and NRD.hlsli.

[NRD] If you are unsure of which parameters to use - use defaults via {} construction. It helps to improve compatibility with future versions and offers optimal IQ, because default settings are always adjusted by recent algorithmic changes.

[NRD] NRD requires linear roughness and world-space normals. See NRD.hlsli for more details and supported customizations.

[NRD] NRD requires non-jittered matrices.

[NRD] Most of denoisers do not write into output pixels outside of CommonSettings::denoisingRange.

[NRD] When upgrading to the latest version keep an eye on ResourceType enumeration. The order of the input slots can be changed or something can be added, you need to adjust the inputs accordingly to match the mapping. Or use NRD integration to simplify the process.

[NRD] All pixels in floating point textures should be INF / NAN free to avoid propagation, because such values are used in weight calculations and accumulation of a weighted sum. Functions XXX_FrontEnd_PackRadianceAndHitDist perform optional NAN / INF clearing of the input signal. There is a boolean to skip these checks.

[NRD] All denoisers work with positive RGB inputs (some denoisers can change color space in front end functions). For better image quality, HDR color inputs need to be in a sane range [0; 250], because the internal pipeline uses FP16 and RELAX tracks second moments of the input signal, i.e. x^2 must fit into FP16 range. If the color input is in a wider range, any form of non-aggressive color compression can be applied (linear scaling, pow-based or log-based methods). REBLUR supports wider HDR ranges, because it doesn't track second moments. Passing pre-exposured colors (i.e. color * exposure) is not recommended, because a significant momentary change in exposure is hard to react to in this case.

[NRD] NRD can track camera motion internally. For the first time pass all MVs set to 0 (you can use CommonSettings::motionVectorScale = {0} for this) and set CommonSettings::isMotionVectorInWorldSpace = true, it will allow you to simplify the initial integration. Enable application-provided MVs after getting denoising working on static objects.

[NRD] Using 2D MVs can lead to massive history reset on moving objects, because 2D motion provides information only about pixel screen position but not about real 3D world position. Consider using 2.5D or 3D MVs instead. 2.5D motion, which is 2D motion with additionally provided viewZ delta (i.e. viewZprev = viewZ + MV.z), is even better, because it has the same benefits as 3D motion, but doesn't suffer from imprecision problems caused by world-space delta rounding to FP16 during MV patching on the NRD side.

[NRD] Firstly, try to get a working reprojection on a diffuse signal for camera rotations only (without camera motion).

[NRD] Diffuse and specular signals must be separated at primary hit (or at secondary hit in case of PSR).

[NRD] Denoising logic is driven by provided hit distances. For indirect lighting denoising passing hit distance for the 1st bounce only is a good baseline. For direct lighting a distance to an occluder or a light source is needed. Primary hit distance must be excluded in any case.

[NRD] Importance sampling is recommended to achieve good results in case of complex lighting environments. Consider using:

Cosine distribution for diffuse from non-local light sources
VNDF sampling for specular
Custom importance sampling for local light sources (RTXDI).

[NRD] Additionally the quality of the input signal can be increased by re-using already denoised information from the current or the previous frame.

[NRD] Hit distances should come from an importance sampling method. But if denoising of AO/SO is needed, AO/SO can come from cos-weighted (or VNDF) sampling in a tradeoff of IQ.

[NRD] Low discrepancy sampling (blue noise) helps to have more stable output in 0.5-1 rpp mode. It's a must for REBLUR-based Ambient and Specular Occlusion denoisers and SIGMA.

[NRD] It's recommended to set CommonSettings::accumulationMode to RESET for a single frame, if a history reset is needed. If history buffers are recreated or contain garbage, it's recommended to use CLEAR_AND_RESET for a single frame. CLEAR_AND_RESET is not free because clearing is done in a compute shader. Render target clears on the application side should be prioritized over this solution.

[NRD] If there are areas (besides sky), which don't require denoising (for example, casting a specular ray only if roughness is less than some threshold), providing viewZ > CommonSettings::denoisingRange in IN_VIEWZ texture for such pixels will effectively skip denoising. Additionally, the data in such areas won't contribute to the final result.

[NRD] If there are areas (besides sky), which don't require denoising (for example, skipped diffuse rays for true metals). materialID and materialMask can be used to drive spatial passes.

[NRD] Input signal quality can be improved by enabling pre-pass via setting diffusePrepassBlurRadius and specularPrepassBlurRadius to a non-zero value. Pre-pass is needed more for specular and less for diffuse, because pre-pass outputs optimal hit distance for specular tracking (see the sample for more details).

[NRD] In case of probabilistic diffuse / specular split at the primary hit, hit distance reconstruction pass must be enabled, if exposed in the denoiser (see HitDistanceReconstructionMode).

[NRD] In case of probabilistic diffuse / specular split at the primary hit, pre-pass must be enabled, if exposed in the denoiser (see diffusePrepassBlurRadius and specularPrepassBlurRadius).

[NRD] Maximum number of accumulated frames can be FPS dependent. The following formula can be used on the application side to adjust maxAccumulatedFrameNum, maxFastAccumulatedFrameNum and potentially historyFixFrameNum too:

maxAccumulatedFrameNum = accumulationPeriodInSeconds * FPS

[NRD] The number of accumulated frames in the fast history needs to be carefully tuned to avoid introducing significant bias and dirt. Initial integration should be done by setting maxFastAccumulatedFrameNum to maxAccumulatedFrameNum. Bare in mind the following recommendation:

maxAccumulatedFrameNum > maxFastAccumulatedFrameNum > historyFixFrameNum

[NRD] In case of quarter resolution tracing and denoising use pixelPos / 2 as texture coordinates. Using a "rotated grid" approach (when a pixel gets selected from 2x2 footprint one by one) is not recommended because it significantly bumps entropy of non-noisy inputs, leading to more disocclusions. In case of REBLUR it's recommended to increase sigmaScale in antilag settings. "Nearest Z" upsampling works best for upscaling of the denoised output. Code, as well as upsampling function, can be found in NRD sample releases before 3.10.

[NRD] SH denoisers can use more relaxed lobeAngleFraction. It can help to improve stability, while details will be reconstructed back by SG resolve.

[REBLUR] If more performance is needed, consider using enablePerformanceMode = true.

[REBLUR] REBLUR expects hit distances in a normalized form. To avoid mismatching, REBLUR_FrontEnd_GetNormHitDist must be used for normalization. Normalization parameters should be passed into NRD as HitDistanceParameters for internal hit distance denormalization. Some tweaking can be needed here, but in most cases default HitDistanceParameters works well. REBLUR outputs denoised normalized hit distance, which can be used by the application as ambient or specular occlusion (AO & SO) (see unpacking functions from NRD.hlsli).

[REBLUR] Intensity antilag parameters need to be carefully tuned. The defaults are good but AntilagIntensitySettings::sensitivityToDarkness needs to be tuned for a given HDR range. Initial integration should work with intensity antilag turned off.

[REBLUR] Even if antilag is off, it's recommended to tune AntilagIntensitySettings::sensitivityToDarkness, because it is used for error estimation.

[RELAX] RELAX works well with signals produced by RTXDI or very clean high RPP signals. The Sweet Home of RELAX is RTXDI sample. Please, consider getting familiar with this application.

[SIGMA] Using "blue" noise can help to avoid shadow shimmering, it works best if the pattern is static on the screen. Additionally, blurRadiusScale can be set to 2-4 to mitigate such problems in complicated cases.

[SIGMA] SIGMA_TRANSLUCENT_SHADOW can be used for shadow denoising from multiple light sources:

L[i] - unshadowed analytical lighting from a single light source (not noisy)
S[i] - stochastically sampled light visibility for L[i] (noisy)
Σ( L[i] ) - unshadowed analytical lighting, typically a result of tiled lighting (HDR, not in range [0; 1])
Σ( L[i] × S[i] ) - final lighting (what we need to get)

The idea:
L1 × S1 + L2 × S2 + L3 × S3 = ( L1 + L2 + L3 ) × [ ( L1 × S1 + L2 × S2 + L3 × S3 ) / ( L1 + L2 + L3 ) ]

Or:
Σ( L[i] × S[i] ) = Σ( L[i] ) × [ Σ( L[i] × S[i] ) / Σ( L[i] ) ]
Σ( L[i] × S[i] ) / Σ( L[i] ) - normalized weighted sum, i.e. pseudo translucency (LDR, in range [0; 1])

Input data preparation example:

float3 Lsum = 0;
float2x3 multiLightShadowData = SIGMA_FrontEnd_MultiLightStart( );

for( uint i = 0; i < N; i++ )
{
    float3 L = ComputeLighting( i );
    Lsum += L;

    // "distanceToOccluder" should respect rules described in NRD.hlsli in "INPUT PARAMETERS" section
    float distanceToOccluder = SampleShadow( i );

    // The weight should be zero if a pixel is not in the penumbra, but it is not trivial to compute...
    float weight = ...;

    SIGMA_FrontEnd_MultiLightUpdate( L, distanceToOccluder, tanOfLightAngularRadius, weight, multiLightShadowData );
}

float4 shadowTranslucency;
float2 shadowData = SIGMA_FrontEnd_MultiLightEnd( viewZ, multiLightShadowData, Lsum, shadowTranslucency );

After denoising the final result can be computed as:

Σ( L[i] × S[i] ) = Σ( L[i] ) × OUT_SHADOW_TRANSLUCENCY.yzw

Is this a biased solution? If spatial filtering is off - no, because we just reorganized the math equation. If spatial filtering is on - yes, because denoising will be driven by most important light in a given pixel.

This solution is limited and hard to use:

obviously, can be used "as is" if shadows don't overlap (weight = 1)
if shadows overlap, a separate pass is needed to analyze noisy input and classify pixels as umbra - penumbra (and optionally empty space). Raster shadow maps can be used for this if available
it is not recommended to mix 1 cd and 100000 cd lights, since FP32 texture will be needed for a weighted sum. In this case, it's better to process the sun and other bright light sources separately.

Name		Name	Last commit message	Last commit date
Latest commit History 79 Commits
.github/workflows		.github/workflows
External		External
Images		Images
Include		Include
Integration		Integration
Resources		Resources
Shaders		Shaders
Source		Source
.gitignore		.gitignore
.gitmodules		.gitmodules
1-Deploy.bat		1-Deploy.bat
1-Deploy.sh		1-Deploy.sh
2-Build.bat		2-Build.bat
2-Build.sh		2-Build.sh
3-Prepare NRD SDK.bat		3-Prepare NRD SDK.bat
3-Prepare NRD SDK.sh		3-Prepare NRD SDK.sh
4-Clean.bat		4-Clean.bat
4-Clean.sh		4-Clean.sh
CLA.txt		CLA.txt
CMakeLists.txt		CMakeLists.txt
LICENSE.txt		LICENSE.txt
README.md		README.md
Shaders.cfg		Shaders.cfg
UPDATE.md		UPDATE.md

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NVIDIA REAL-TIME DENOISERS v4.3.6 (NRD)

OVERVIEW

HOW TO BUILD?

HOW TO UPDATE?

HOW TO REPORT ISSUES?

API

NON-NOISY INPUTS

NOISY INPUTS

IMPROVING OUTPUT QUALITY

VALIDATION LAYER

MEMORY REQUIREMENTS

INTEGRATION VARIANTS

VARIANT 1: Black-box library (using the application-side Render Hardware Interface)

VARIANT 2: White-box library (using the application-side Render Hardware Interface)

VARIANT 3: Black-box library (using native API pointers)

RECOMMENDATIONS AND BEST PRACTICES: GREATER TIPS

MATERIAL DE-MODULATION (IRRADIANCE → RADIANCE)

COMBINED DENOISING OF DIRECT AND INDIRECT LIGHTING

INTERACTION WITH PRIMARY SURFACE REPLACEMENTS (PSR)

INTERACTION WITH FRAME GENERATION TECHNIQUES

RECOMMENDATIONS AND BEST PRACTICES: LESSER TIPS

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NVIDIA REAL-TIME DENOISERS v4.3.6 (NRD)

OVERVIEW

HOW TO BUILD?

HOW TO UPDATE?

HOW TO REPORT ISSUES?

API

NON-NOISY INPUTS

NOISY INPUTS

IMPROVING OUTPUT QUALITY

VALIDATION LAYER

MEMORY REQUIREMENTS

INTEGRATION VARIANTS

VARIANT 1: Black-box library (using the application-side Render Hardware Interface)

VARIANT 2: White-box library (using the application-side Render Hardware Interface)

VARIANT 3: Black-box library (using native API pointers)

RECOMMENDATIONS AND BEST PRACTICES: GREATER TIPS

MATERIAL DE-MODULATION (IRRADIANCE → RADIANCE)

COMBINED DENOISING OF DIRECT AND INDIRECT LIGHTING

INTERACTION WITH PRIMARY SURFACE REPLACEMENTS (PSR)

INTERACTION WITH FRAME GENERATION TECHNIQUES

RECOMMENDATIONS AND BEST PRACTICES: LESSER TIPS

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