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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all
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}
} catch(__e) { console.warn('[Userscript:Add Copy Buttons to Code Blocks]', __e); }
})();
(function(){
try {
var __m = "github.com";
var __re = new RegExp('^' + "github\\.com" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

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Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Force GitHub README to respect dark mode\n(function() {\n var style = document.createElement('style');\n style.textContent = '\n .markdown-body {\n color-scheme: dark light;\n }\n .markdown-body pre { background: #161b22 !important; }\n .markdown-body code { background: rgba(110, 118, 129, 0.4) !important; }\n .markdown-body table th, .markdown-body table td { border-color: #30363d !important; }\n .markdown-body img { background: #0d1117; }\n .markdown-body blockquote { border-left-color: #8b949e; }\n .markdown-body hr { border-color: #30363d; }\n ';\n document.head.appendChild(style);\n})();", "GitHub Dark Mode README Fix"); } } catch(__e) { console.warn('[Userscript:GitHub Dark Mode README Fix]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Highlight search terms from Google/DuckDuckGo/Bing referrer\n(function() {\n var ref = document.referrer;\n var terms = [];\n \n if (ref.includes('google.com') || ref.includes('duckduckgo.com') || ref.includes('bing.com')) {\n var url = new URL(ref);\n var q = url.searchParams.get('q') || url.searchParams.get('p');\n if (q) {\n terms = q.split(/\\s+/).filter(function(t) { return t.length > 2; });\n }\n }\n \n if (terms.length === 0) return;\n \n var style = document.createElement('style');\n style.textContent = '.userscript-highlight { background: #fbbf24; color: #1a1a2e; padding: 1px 3px; border-radius: 2px; }';\n document.head.appendChild(style);\n \n function highlight(node) {\n if (node.nodeType === 3) { // text node\n var text = node.textContent;\n var found = false;\n terms.forEach(function(term) {\n var regex = new RegExp('(' + term.replace(/[.*+?^${}()|[\\]\\\\]/g, '\\\\') + ')', 'gi');\n if (regex.test(text)) {\n found = true;\n var frag = document.createDocumentFragment();\n var parts = text.split(regex);\n parts.forEach(function(part, i) {\n if (i % 2 === 0) {\n frag.appendChild(document.createTextNode(part));\n } else {\n var span = document.createElement('span');\n span.className = 'userscript-highlight';\n span.textContent = part;\n frag.appendChild(span);\n }\n });\n node.parentNode.replaceChild(frag, node);\n }\n });\n } else if (node.nodeType === 1 && node.childNodes) { // element\n var skipTags = ['SCRIPT', 'STYLE', 'NOSCRIPT', 'TEXTAREA', 'INPUT', 'SELECT'];\n if (!skipTags.includes(node.tagName)) {\n Array.from(node.childNodes).forEach(highlight);\n }\n }\n }\n \n highlight(document.body);\n \n // Re-highlight on dynamic content\n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1 || node.nodeType === 3) highlight(node);\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Highlight Search Terms"); } } catch(__e) { console.warn('[Userscript:Highlight Search Terms]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Strip utm_, fbclid, gclid, etc. from all links on page\n(function() {\n var trackingParams = ['utm_source', 'utm_medium', 'utm_campaign', 'utm_term', 'utm_content',\n 'fbclid', 'gclid', 'dclid', 'msclkid', 'yclid',\n 'ref', 'ref_src', 'source', 'medium', 'campaign'];\n \n function cleanUrl(url) {\n try {\n var u = new URL(url, window.location.origin);\n var changed = false;\n trackingParams.forEach(function(p) {\n if (u.searchParams.has(p)) {\n u.searchParams.delete(p);\n changed = true;\n }\n });\n return changed ? u.toString() : url;\n } catch (e) {\n return url;\n }\n }\n \n function cleanLinks() {\n document.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n \n cleanLinks();\n \n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1) {\n if (node.tagName === 'A') cleanLinks();\n node.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Remove Tracking Parameters from Links"); } } catch(__e) { console.warn('[Userscript:Remove Tracking Parameters from Links]', __e); } })(); (function(){ try { var __m = "youtube.com"; var __re = new RegExp('^' + "youtube\\.com" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

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0 watching

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Auto-enable theater mode on YouTube\n(function() {\n function tryTheater() {\n var btn = document.querySelector('button[aria-label=\"Theater mode\"], ytd-player #player button[title=\"Theater mode\"]');\n if (btn && !btn.classList.contains('activated')) {\n btn.click();\n }\n }\n \n // Try immediately\n tryTheater();\n \n // Try after navigation (SPA)\n var lastUrl = location.href;\n setInterval(function() {\n if (location.href !== lastUrl) {\n lastUrl = location.href;\n setTimeout(tryTheater, 500);\n }\n }, 1000);\n \n // Also try on player load\n var observer = new MutationObserver(tryTheater);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "YouTube Theater Mode Default"); } } catch(__e) { console.warn('[Userscript:YouTube Theater Mode Default]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Remove or un-stick sticky/fixed headers that block content\n(function() {\n function unstick() {\n document.querySelectorAll('header, nav, [role=\"banner\"], .header, .navbar, .sticky, .fixed-top, [style*=\"position: fixed\"], [style*=\"position:sticky\"]').forEach(function(el) {\n if (el.style.position === 'fixed' || el.style.position === 'sticky' || \n getComputedStyle(el).position === 'fixed' || getComputedStyle(el).position === 'sticky') {\n el.style.position = 'static';\n el.style.top = 'auto';\n el.style.zIndex = 'auto';\n }\n });\n }\n \n unstick();\n \n var observer = new MutationObserver(unstick);\n observer.observe(document.body, { childList: true, subtree: true, attributes: true, attributeFilter: ['style', 'class'] });\n})();", "Kill Sticky Headers"); } } catch(__e) { console.warn('[Userscript:Kill Sticky Headers]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Universal Dark Mode - works on any site\n(function() {\n var enabled = true;\n \n function applyDarkMode() {\n if (!enabled) return;\n \n // Create style element if it doesn't exist\n var style = document.getElementById('universal-dark-mode-style');\n if (!style) {\n style = document.createElement('style');\n style.id = 'universal-dark-mode-style';\n document.head.appendChild(style);\n }\n \n // Dark mode CSS - inverts colors but preserves images/video\n style.textContent = '\n /* Invert everything except media */\n html {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #1a1a2e !important;\n }\n \n /* Restore images, videos, iframes, canvas */\n img, video, iframe, canvas, svg, picture, [style*=\"background-image\"] {\n filter: invert(1) hue-rotate(180deg) !important;\n }\n \n /* Preserve specific elements that should not be inverted */\n .no-dark-mode, .no-dark-mode *,\n [data-theme=\"light\"], [data-theme=\"light\"],\n .ace_editor, .ace_editor *,\n .CodeMirror, .CodeMirror *,\n .monaco-editor, .monaco-editor *,\n .markdown-body pre, .markdown-body pre *,\n .highlight, .highlight *,\n pre code, pre code * {\n filter: none !important;\n }\n \n /* Fix common UI elements */\n .modal, .popup, .dropdown-menu, .tooltip, .popover {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #2d2d44 !important;\n border-color: #444 !important;\n }\n \n /* Scrollbars */\n ::-webkit-scrollbar { background: #1a1a2e !important; }\n ::-webkit-scrollbar-thumb { background: #444 !important; }\n ::-webkit-scrollbar-thumb:hover { background: #555 !important; }\n \n /* Selection */\n ::selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ::-moz-selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ';\n }\n \n function removeDarkMode() {\n var style = document.getElementById('universal-dark-mode-style');\n if (style) style.remove();\n }\n \n // Toggle with Alt+Shift+D\n document.addEventListener('keydown', function(e) {\n if (e.altKey && e.shiftKey && e.key === 'D') {\n e.preventDefault();\n enabled = !enabled;\n if (enabled) {\n applyDarkMode();\n console.log('[Universal Dark Mode] Enabled');\n } else {\n removeDarkMode();\n console.log('[Universal Dark Mode] Disabled');\n }\n }\n });\n \n // Apply on load\n applyDarkMode();\n \n // Re-apply on dynamic content\n var observer = new MutationObserver(function(mutations) {\n if (enabled && !document.getElementById('universal-dark-mode-style')) {\n applyDarkMode();\n }\n });\n observer.observe(document.head, { childList: true });\n \n console.log('[Universal Dark Mode] Loaded - Press Alt+Shift+D to toggle');\n})();", "Universal Dark Mode"); } } catch(__e) { console.warn('[Userscript:Universal Dark Mode]', __e); } })(); })();
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STMapExtension

A Nuke tool for uncropping ST maps — extending UV values past their original bbox by extrapolating the gradient outward.

When an ST map gets cropped (so its data window no longer covers full 0..1 in U and V), downstream STMap nodes can't sample beyond the bbox edges. This tool reconstructs plausible UV values for the padded region by fitting per-axis functions to the outermost trusted pixels and projecting them outward, with smoothing to suppress noise amplification.

preview

Features

  • BlinkScript GPU implementation, runs at viewer speed
  • Four extrapolation modes: clamp, linear, zero, fade
  • Linear or quadratic order — handles real lens distortion curvature, not just constant gradients
  • Edge trim with uniform, per-edge override, and auto-detect modes — replace unreliable edge pixels with synthetic values
  • Edge smoothing knob to suppress noise streaks
  • Auto-centering of source within target canvas
  • Reads source bbox from src.bounds — no manual size sync needed
  • Self-contained Group node, no external dependencies

Installation

Quick start

  1. Clone this repo:
    git clone https://github.com/bratgot/STMapExtension.git
  2. In Nuke's Script Editor:
    exec(open('/path/to/STMapExtension/install.py').read())

The first run writes the kernel to ~/.nuke/STMapOverscan_kernel.rpp and creates a new STMapOverscan1 group node.

Persistent menu install

Copy install/menu.py.example into your ~/.nuke/menu.py, edit STMAP_INSTALL_PATH to point at your clone, and you'll get a menu entry plus an Shift+O hotkey.

Usage

  1. Connect a cropped ST map to the input
  2. Set width / height on the Output Format section to the target uncropped size
  3. Pick an extrapolation mode (default: linear)
  4. Pick an order: 1 (linear) for clean gradients, 2 (quadratic) for curving lens distortion
  5. Adjust edge smoothing if you see streak artifacts (default: 8, sweet spot: 816)
  6. If the input has bad edges (black bleeds, ringing), set edge trim values or click Auto-Analyze Edges

How it works

For each output pixel:

  1. Find the corresponding source-space coordinate (subtract pad offset)
  2. If inside the trusted region → sample directly
  3. If outside → walk to the nearest edge of the trusted region, fit a function from a smoothing-pixel baseline averaged along the tangent, project it outward
  4. Order 1 fits a straight line (first-order Taylor); order 2 fits a parabola (second-order Taylor)

The tangent-direction averaging is the key to clean output. A slope built from just two pixels turns per-pixel noise in the source into multi-thousand-pixel streaks across the padded region; averaging the edge samples first keeps the estimate stable.

The kernel reads src.bounds in init() so the data window is auto-detected at every cook — no manual size knobs to keep in sync.

See docs/HOW_IT_WORKS.md for the math walkthrough.

Modes

ModeBehavior
clampRepeat edge values into the padded region
linearExtrapolate using order 1 (line) or order 2 (parabola)
zeroFill padding with black
fadeSoft falloff from edge values to black

Order

OrderDescriptionBest for
1First-order Taylor (straight line)Linear gradients, mild distortion
2Second-order Taylor (parabola)Wide-angle, fisheye, anamorphic distortion

Order 2 is exact for quadratic fields and a good approximation for general curving fields. The trade-off is sensitivity to noise — quadratic curvature gets amplified by Δ², so quadratic mode benefits from smoothing ≥ 4.

Edge Trim

Many real ST maps have unreliable outermost pixels — black borders from incomplete renders, anti-aliasing softness, or upstream interpolation artifacts. The trim controls let you replace those pixels with synthetic edge values:

  • Uniform trim: trim N pixels from all four edges
  • Per-edge override: enable to set independent trim for left/right/top/bottom
  • Auto-Analyze Edges: samples the input, fits a linear trend to interior values, identifies where the outer pixels deviate from that trend, and sets per-edge trim automatically

Trimmed pixels behave the same as out-of-bbox pixels — they get extrapolated from the trusted interior.

Files

STMapExtension/
├── install.py # main installer (run in Nuke)
├── kernel/
│ └── STMapOverscan_kernel.rpp # standalone BlinkScript kernel
├── install/
│ └── menu.py.example # menu.py snippet for studio install
├── examples/
│ └── STMapCropped.exr # test ST map (linear unit gradient)
├── docs/
│ ├── HOW_IT_WORKS.md
│ └── images/
├── LICENSE
├── CHANGELOG.md
└── README.md

Caveats

Quadratic extrapolation is exact for quadratic fields and approximates higher-order distortion well for moderate distances. For very strong distortion projected very far past the bbox, errors still grow — the curvature itself isn't constant in real lenses, so even a parabola eventually drifts. Cubic order would be the next upgrade if needed.

The auto-analyze edge detection is heuristic. It works well for obvious cases (visible black borders, abrupt gradient breaks) but can miss subtle edge softness. Manual trim values are always available as a fallback.

Compatibility

Tested on Nuke 14.1+. Should work on any Nuke with BlinkScript GPU support.

License

MIT — see LICENSE.

Credit

Built by Marten Blumen.

About

No description, website, or topics provided.

Resources

Stars

4 stars

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages