Improve shadow normal bias calculation (#9734)

The previous code used the max of the texel's width or height footprint
in world space to compute the offset; this could both overestimate or
underestimate the bias causing some peter panning or acne.

The new code replaces a sqrt with a dot, but is otherwise similar.
This commit is contained in:
Mathias Agopian
2026-02-25 12:16:13 -08:00
committed by GitHub
parent 07a7c6003a
commit 81c71fbbb9
8 changed files with 66 additions and 29 deletions

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@@ -6,3 +6,6 @@
appropriate header in [RELEASE_NOTES.md](./RELEASE_NOTES.md).
## Release notes for next branch cut
- engine: fix crash when using variance shadow maps
- materials: better shadow normal-bias calculations [⚠️ **New Material Version**]

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@@ -1117,16 +1117,16 @@ bool ShadowMap::intersectSegmentWithPlanarQuad(float3& UTILS_RESTRICT p,
return hit;
}
float ShadowMap::texelSizeWorldSpace(const mat3f& clipFromWorld, uint16_t shadowDimension) noexcept {
float2 ShadowMap::texelSizeWorldSpace(const mat3f& clipFromWorld, uint16_t shadowDimension) noexcept {
// The Jacobian of the transformation from texture-to-world is the matrix itself for
// orthographic projections. We just need to inverse shadowMapFromWorld,
// which is guaranteed to be orthographic.
// The two first columns give us how a texel maps in world-space.
float const oneTexel = 2.0f / float(shadowDimension);
const mat3f worldFromClip(inverse(clipFromWorld));
const float3 Jx = worldFromClip[0];
const float3 Jy = worldFromClip[1];
const float s = std::max(length(Jx), length(Jy)) * oneTexel;
mat3f const worldFromClip(inverse(clipFromWorld));
float3 const Jx = worldFromClip[0];
float3 const Jy = worldFromClip[1];
float2 const s = float2{ length(Jx), length(Jy) } * oneTexel;
return s;
}
@@ -1171,13 +1171,13 @@ static mat3f jacobian(mat4f const& M, float3 const& p) noexcept {
return (M_sub - t_cross_w / T.w) / T.w;
}
float ShadowMap::texelSizeWorldSpace(mat4f const& S, uint16_t const shadowDimension) noexcept {
float2 ShadowMap::texelSizeWorldSpace(mat4f const& S, uint16_t const shadowDimension) noexcept {
// The Jacobian is not constant, so we evaluate it in the center of the shadow-map texture.
// It might be better to do this computation in the vertex shader.
float3 const p = { 0.0f, 0.0f, 0.0f }; // clip-space
float const oneTexel = 2.0f / float(shadowDimension);
mat3f const J = jacobian(inverse(S), p);
const float s = std::max(length(J[0]), length(J[1])) * oneTexel;
float2 const s = float2{ length(J[0]), length(J[1]) } * oneTexel;
return s;
}

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@@ -135,7 +135,7 @@ public:
math::mat4f lightSpace{};
math::float4 lightFromWorldZ{};
math::float4 scissorNormalized{};
float texelSizeAtOneMeterWs{};
math::float2 texelSizeAtOneMeterWs{};
};
// Call once per frame if the light, scene (or visible layers) or camera changes.
@@ -319,8 +319,8 @@ private:
math::float4 getClampToEdgeCoords(ShadowMapInfo const& shadowMapInfo) const noexcept;
static float texelSizeWorldSpace(const math::mat3f& clipFromWorld, uint16_t shadowDimension) noexcept;
static float texelSizeWorldSpace(const math::mat4f& clipFromWorld, uint16_t shadowDimension) noexcept;
static math::float2 texelSizeWorldSpace(const math::mat3f& clipFromWorld, uint16_t shadowDimension) noexcept;
static math::float2 texelSizeWorldSpace(const math::mat4f& clipFromWorld, uint16_t shadowDimension) noexcept;
static constexpr Segment sBoxSegments[12] = {
{ 0, 1 }, { 1, 3 }, { 3, 2 }, { 2, 0 },

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@@ -742,17 +742,16 @@ ShadowMapManager::ShadowTechnique ShadowMapManager::updateCascadeShadowMaps(FEng
// Texel size is constant for directional light (although that's not true when LISPSM
// is used, but in that case we're pretending it is).
const float wsTexelSize = shaderParameters.texelSizeAtOneMeterWs;
float2 const wsTexelSize = shaderParameters.texelSizeAtOneMeterWs;
auto& s = mShadowUb.edit();
s.shadows[shadowIndex].layer = shadowMap.getLayer();
s.shadows[shadowIndex].lightFromWorldMatrix = shaderParameters.lightSpace;
s.shadows[shadowIndex].scissorNormalized = shaderParameters.scissorNormalized;
s.shadows[shadowIndex].normalBias = normalBias * wsTexelSize;
s.shadows[shadowIndex].texelSizeAtOneMeter = wsTexelSize;
s.shadows[shadowIndex].normalBias = wsTexelSize * normalBias;
s.shadows[shadowIndex].elvsm = options.vsm.elvsm;
s.shadows[shadowIndex].bulbRadiusLs =
mSoftShadowOptions.penumbraScale * options.shadowBulbRadius / wsTexelSize;
mSoftShadowOptions.penumbraScale * options.shadowBulbRadius / length(wsTexelSize);
shadowTechnique |= ShadowTechnique::SHADOW_MAP;
cascadeHasVisibleShadows |= 0x1u << i;
@@ -833,7 +832,7 @@ void ShadowMapManager::prepareSpotShadowMap(ShadowMap& shadowMap, FEngine& engin
// and if we need to generate it, update all the UBO data
if (shadowMap.hasVisibleShadows()) {
const size_t shadowIndex = shadowMap.getShadowIndex();
const float wsTexelSizeAtOneMeter = shaderParameters.texelSizeAtOneMeterWs;
const float2 wsTexelSizeAtOneMeter = shaderParameters.texelSizeAtOneMeterWs;
// note: normalBias is set to zero for VSM
const float normalBias = shadowMapInfo.vsm ? 0.0f : options->normalBias;
@@ -845,12 +844,11 @@ void ShadowMapManager::prepareSpotShadowMap(ShadowMap& shadowMap, FEngine& engin
s.shadows[shadowIndex].scissorNormalized = shaderParameters.scissorNormalized;
s.shadows[shadowIndex].normalBias = normalBias * wsTexelSizeAtOneMeter;
s.shadows[shadowIndex].lightFromWorldZ = shaderParameters.lightFromWorldZ;
s.shadows[shadowIndex].texelSizeAtOneMeter = wsTexelSizeAtOneMeter;
s.shadows[shadowIndex].nearOverFarMinusNear = float(n / (f - n));
s.shadows[shadowIndex].elvsm = options->vsm.elvsm;
s.shadows[shadowIndex].bulbRadiusLs =
mSoftShadowOptions.penumbraScale * options->shadowBulbRadius
/ wsTexelSizeAtOneMeter;
/ length(wsTexelSizeAtOneMeter);
}
}
@@ -926,7 +924,7 @@ void ShadowMapManager::preparePointShadowMap(ShadowMap& shadowMap,
// and if we need to generate it, update all the UBO data
if (shadowMap.hasVisibleShadows()) {
const size_t shadowIndex = shadowMap.getShadowIndex();
const float wsTexelSizeAtOneMeter = shaderParameters.texelSizeAtOneMeterWs;
const float2 wsTexelSizeAtOneMeter = shaderParameters.texelSizeAtOneMeterWs;
// note: normalBias is set to zero for VSM
const float normalBias = shadowMapInfo.vsm ? 0.0f : options->normalBias;
@@ -938,12 +936,11 @@ void ShadowMapManager::preparePointShadowMap(ShadowMap& shadowMap,
s.shadows[shadowIndex].scissorNormalized = shaderParameters.scissorNormalized;
s.shadows[shadowIndex].normalBias = normalBias * wsTexelSizeAtOneMeter;
s.shadows[shadowIndex].lightFromWorldZ = shaderParameters.lightFromWorldZ;
s.shadows[shadowIndex].texelSizeAtOneMeter = wsTexelSizeAtOneMeter;
s.shadows[shadowIndex].nearOverFarMinusNear = float(n / (f - n));
s.shadows[shadowIndex].elvsm = options->vsm.elvsm;
s.shadows[shadowIndex].bulbRadiusLs =
mSoftShadowOptions.penumbraScale * options->shadowBulbRadius
/ wsTexelSizeAtOneMeter;
/ length(wsTexelSizeAtOneMeter);
}
}

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@@ -299,10 +299,9 @@ struct ShadowUib { // NOLINT(cppcoreguidelines-pro-type-member-init)
math::mat4f lightFromWorldMatrix; // 64
math::float4 lightFromWorldZ; // 16
math::float4 scissorNormalized; // 16
float texelSizeAtOneMeter; // 4
float bulbRadiusLs; // 4
float nearOverFarMinusNear; // 4
float normalBias; // 4
math::float2 normalBias; // 4
bool elvsm; // 4
uint32_t layer; // 4
uint32_t reserved1; // 4

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@@ -111,7 +111,7 @@ highp vec4 getSpotLightSpacePosition(int index, highp vec3 dir, highp float zLig
highp mat4 lightFromWorldMatrix = shadowUniforms.shadows[index].lightFromWorldMatrix;
// for spotlights, the bias depends on z
float bias = shadowUniforms.shadows[index].normalBias * zLight;
highp vec2 bias = shadowUniforms.shadows[index].normalBias * zLight;
return computeLightSpacePosition(getWorldPosition(), getWorldGeometricNormalVector(),
dir, bias, lightFromWorldMatrix);

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@@ -12,12 +12,51 @@
*/
highp vec4 computeLightSpacePosition(highp vec3 p, const highp vec3 n,
const highp vec3 dir, const float b, highp_mat4 lightFromWorldMatrix) {
const highp vec3 dir, const highp vec2 b, highp_mat4 lightFromWorldMatrix) {
#if !defined(VARIANT_HAS_VSM)
highp float cosTheta = saturate(dot(n, dir));
highp float sinTheta = sqrt(1.0 - cosTheta * cosTheta);
p += n * (sinTheta * b);
// --------------------------------------------------------------------------------------
// Anisotropic Normal Bias for Shadow Mapping
// --------------------------------------------------------------------------------------
// To prevent shadow acne, we must push the geometry along its normal to clear the
// quantization steps of the shadow map's discrete depth grid. The exact physical depth
// error we must clear is proportional to the shadow texel's world-space dimensions.
//
// This implementation computes the exact geometric projection of the rectangular
// shadow map texel onto the surface normal.
//
// 1. Coordinate Space Transition:
// We project the world-space normal onto the light's X and Y basis vectors (L_right,
// L_up). This gives us the lateral components of the normal in Light Space (n_Lx, n_Ly).
//
// 2. The Implicit sin(theta) Slope Scale:
// Because the normal is a unit vector, the magnitude of its lateral components in
// light space inherently equals sin(theta), where theta is the angle of incidence.
// This perfectly and automatically scales the bias from 0.0 (top-down, flat surface)
// to maximum (grazing angle).
//
// 3. Exact Anisotropic Footprint (The L1 Norm):
// Shadow texels are rarely perfectly square due to Cascaded Shadow Maps (CSM) or
// Light Space Perspective Shadow Maps (LiSPSM). Jx and Jy are the physical world-space
// dimensions of the texel.
// By evaluating `abs(n_Lx * Jx) + abs(n_Ly * Jy)`, we compute the exact scalar
// projection of the rectangular texel footprint.
// - It is superior to `max(Jx, Jy)` which assumes a massive square and causes Peter Panning.
// - It is superior to `length()` which assumes an ellipse and under-biases the corners.
// --------------------------------------------------------------------------------------
// Extract the first row (Light's Right vector in World Space)
highp vec3 L_right = vec3(lightFromWorldMatrix[0][0], lightFromWorldMatrix[1][0], lightFromWorldMatrix[2][0]);
// Extract the second row (Light's Up vector in World Space)
highp vec3 L_up = vec3(lightFromWorldMatrix[0][1], lightFromWorldMatrix[1][1], lightFromWorldMatrix[2][1]);
// Project the world normal onto the shadow map's 2D grid
highp float n_Lx = dot(n, L_right);
highp float n_Ly = dot(n, L_up);
// Apply the anisotropic normal bias
p += n * (abs(n_Lx * b.x) + abs(n_Ly * b.y));
#endif
return mulMat4x4Float3(lightFromWorldMatrix, p);

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@@ -5,10 +5,9 @@ struct ShadowData {
highp mat4 lightFromWorldMatrix;
highp vec4 lightFromWorldZ;
highp vec4 scissorNormalized;
mediump float texelSizeAtOneMeter;
mediump float bulbRadiusLs;
mediump float nearOverFarMinusNear;
mediump float normalBias;
highp vec2 normalBias;
bool elvsm;
mediump uint layer;
mediump uint reserved1;