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https://github.com/Nexoniarz/Fry3DX.git
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f3e8eca87b
Shapes with live settings, shape editing, knife and hole tools, drawing shapes onto other objects, combining objects (add / subtract / overlap), copies, thickness, painting with stickers and layers, a Layout tab, a Print tab with checks, packed .fry files with autosave, export to GLB, glTF, FBX, OBJ, 3MF, STL and PLY, folders in Layers, its own crash screen, and a website for GitHub Pages in docs/. Co-Authored-By: Claude Opus 5.5 <noreply@anthropic.com> Claude-Session: https://claude.ai/code/session_01NMSrd5oe1GpUD7E6d825KP
63 lines
3.4 KiB
GLSL
63 lines
3.4 KiB
GLSL
#version 460
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// Ambient occlusion from the depth buffer alone (Alchemy-style, half resolution): for each
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// pixel, view-space points around it in a spiral; those above the surface's plane and close
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// enough darken it. Rows are the depth buffer's own (uv from gl_FragCoord), on both backends.
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#define KEEL_POST // screen-space: render targets, sampled clamped
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#include "backend.glsl"
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PUSH_BLOCK {
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uint depth; // scene depth slot
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uint w, h; // its size
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uint outW, outH; // this target's
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float radius; // world units
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float strength;
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float pad;
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vec4 proj; // tan(half fov x), tan(half fov y), near, far
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} pc;
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layout(location = 0) out vec4 o_ao;
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// The point seen at uv: its depth from the pixel there, and its place across the screen from
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// that same pixel's centre (not uv itself: on a slanted wall the two would disagree by a part of
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// a pixel, in a pattern that depends on how the window's size halves; stripes on walls).
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vec3 viewPos(vec2 uv) {
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ivec2 p = clamp(ivec2(uv * vec2(pc.w, pc.h)), ivec2(0), ivec2(pc.w - 1, pc.h - 1));
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float d = fetchTex(pc.depth, p).r;
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float z = pc.proj.z * pc.proj.w / (pc.proj.w - d * (pc.proj.w - pc.proj.z));
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vec2 at = (vec2(p) + 0.5) / vec2(pc.w, pc.h);
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return vec3((at * 2.0 - 1.0) * pc.proj.xy * z, z);
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}
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void main() {
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vec2 uv = gl_FragCoord.xy / vec2(pc.outW, pc.outH);
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ivec2 full = clamp(ivec2(uv * vec2(pc.w, pc.h)), ivec2(0), ivec2(pc.w - 1, pc.h - 1));
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if (fetchTex(pc.depth, full).r >= 1.0) { o_ao = vec4(1.0); return; } // sky
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vec3 p = viewPos(uv);
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// The surface normal from neighbouring depths (the smaller step on each axis, so edges hold).
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vec2 texel = 1.0 / vec2(pc.outW, pc.outH);
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vec3 px1 = viewPos(uv + vec2(texel.x, 0)) - p, px2 = p - viewPos(uv - vec2(texel.x, 0));
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vec3 py1 = viewPos(uv + vec2(0, texel.y)) - p, py2 = p - viewPos(uv - vec2(0, texel.y));
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// The smaller step, but never one off the screen's edge (there it clamps onto this pixel,
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// a zero step, and the normal goes wrong: a dark line along the border).
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bool right = uv.x + texel.x < 1.0, left = uv.x - texel.x > 0.0, down = uv.y + texel.y < 1.0, up = uv.y - texel.y > 0.0;
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vec3 dx = !right ? px2 : !left ? px1 : dot(px1, px1) < dot(px2, px2) ? px1 : px2;
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vec3 dy = !down ? py2 : !up ? py1 : dot(py1, py1) < dot(py2, py2) ? py1 : py2;
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vec3 n = normalize(cross(dx, dy));
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if (dot(n, p) > 0.0) n = -n; // towards the camera
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// Interleaved gradient noise turns the spiral per pixel; the blur evens it out.
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float noise = fract(52.9829189 * fract(dot(gl_FragCoord.xy, vec2(0.06711056, 0.00583715))));
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const int kSamples = 12;
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float occlusion = 0.0;
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for (int i = 0; i < kSamples; ++i) {
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float t = (float(i) + noise) / float(kSamples);
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float a = (float(i) * 2.39996 + noise * 6.2831853);
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float r = pc.radius * t;
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vec2 off = vec2(cos(a), sin(a)) * r / (p.z * pc.proj.xy * 2.0);
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vec2 q = uv + off;
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if (any(lessThan(q, vec2(0.0))) || any(greaterThan(q, vec2(1.0)))) continue; // off screen: nothing known there
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vec3 v = viewPos(q) - p;
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float vv = dot(v, v);
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float falloff = max(0.0, 1.0 - vv / (pc.radius * pc.radius));
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occlusion += max(0.0, dot(v, n) - 0.01 * p.z) / (vv + 1.0) * falloff;
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}
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float ao = max(0.0, 1.0 - 2.0 * occlusion / float(kSamples) * pc.radius * 0.6);
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o_ao = vec4(mix(1.0, ao * ao, pc.strength));
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}
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