SplatTransform - 3D Gaussian Splat Converter

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SplatTransform is an open source library and CLI tool for converting and editing Gaussian splats. It can:

📥 Read PLY, Compressed PLY, SOG, SPZ, SPLAT, KSPLAT, LCC and LCC2 formats
📤 Write PLY, Compressed PLY, SOG, SPZ, GLB, CSV, HTML Viewer, LOD, Voxel and WebP image formats
📊 Generate statistical summaries for data analysis
🔗 Merge multiple splats
🔄 Apply transformations to input splats
🎛️ Filter out Gaussians or spherical harmonic bands
🔀 Reorder splats for improved spatial locality
⚙️ Procedurally generate splats using JavaScript generators

The library is platform-agnostic and can be used in both Node.js and browser environments.

Installation

Install or update to the latest version:

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npm install -g @playcanvas/splat-transform

For library usage, install as a dependency:

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npm install @playcanvas/splat-transform

For running on a backend with Docker (including GPU/Vulkan setup), see the Docker Backend Guide.

[!TIP]
For one-off conversions without installing anything, try SuperSplat Convert — a browser-based frontend to splat-transform. See the Convert page docs for details.

Guides

• Streamed SOG Guide — build a multi-LOD streamed SOG from a single PLY.
• LOD Streaming Guide — load and render streamed SOG output in a PlayCanvas app.
• Collision Mesh Guide — generate voxel/collision data from a splat scene.
• Docker Backend Guide — run splat-transform on a backend (incl. GPU/Vulkan setup).

Format Specifications

Format	Description
PLY	Industry-standard uncompressed format for source, editing and interchange
SOG	Super-compressed format for web delivery (meta.json + WebP textures, bundled or unbundled)
Streamed SOG	Multi-LOD chunked SOG for streaming very large scenes (lod-meta.json)
Voxel	Sparse voxel octree for collision detection (.voxel.json / .voxel.bin)

CLI Usage

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splat-transform [GLOBAL] input [ACTIONS]  ...  output [ACTIONS]

Key points:

• Input files become the working set; ACTIONS are applied in order
• The last file is the output; actions after it modify the final result
• Use null as output to discard file output

Supported Formats

Format	Input	Output	Description
.ply	✅	✅	Standard PLY format
.sog	✅	✅	Bundled super-compressed format (recommended)
meta.json	✅	✅	Unbundled super-compressed format (accompanied by .webp textures)
.compressed.ply	✅	✅	Compressed PLY format (auto-detected and decompressed on read)
.spz	✅	✅	Compressed splat format (Niantic format, v2–4)
.lcc	✅	❌	LCC file format (XGRIDS)
.lcc2	✅	❌	LCC2 file format (XGRIDS, octree)
.ksplat	✅	❌	Compressed splat format (mkkellogg format)
.splat	✅	❌	Compressed splat format (antimatter15 format)
.mjs	✅	❌	Generate a scene using an mjs script (Beta)
.glb	❌	✅	Binary glTF with KHR_gaussian_splatting extension
.csv	❌	✅	Comma-separated values spreadsheet
.html	❌	✅	HTML viewer app (single-page or unbundled) based on SOG
.voxel.json	❌	✅	Sparse voxel octree for collision detection
lod-meta.json	❌	✅	Streamed LOD data stored in SOG chunks
.webp	❌	✅	Lossless WebP image rendered from a camera view via GPU rasterizer
null	❌	✅	Discard output (useful with --summary for analysis-only runs)

Actions

Actions execute in the order specified and can be repeated. Any action may appear after any input or output file:

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-t, --translate        <x,y,z>          Translate Gaussians by (x, y, z)
-r, --rotate           <x,y,z>          Rotate Gaussians by Euler angles (x, y, z), in degrees
-s, --scale            <factor>         Uniformly scale Gaussians by factor
-H, --filter-harmonics <0|1|2|3>        Remove spherical harmonic bands > n
-N, --filter-nan                        Remove Gaussians with NaN values and most Inf values;
                                          retains +Infinity in opacity and -Infinity in scale_*
-B, --filter-box       <x,y,z,X,Y,Z>    Remove Gaussians outside box (min, max corners)
-S, --filter-sphere    <x,y,z,radius>   Remove Gaussians outside sphere (center, radius)
-V, --filter-value     <name,cmp,value> Keep Gaussians where <name> <cmp> <value>
                                          cmp ∈ {lt,lte,gt,gte,eq,neq}
                                          opacity, scale_*, f_dc_* use transformed values
                                          (linear opacity 0-1, linear scale, linear color 0-1).
                                          Append _raw for raw PLY values (e.g. opacity_raw).
-F, --decimate         <n|n%>           Simplify to n Gaussians via progressive pairwise merging
                                          Use n% to keep a percentage of Gaussians
-G, --filter-floaters  [size,op,min]    Remove Gaussians not contributing to any solid voxel.
                                          Evaluates each Gaussian at occupied voxel centers.
                                          Default: size=0.05, opacity=0.1, min=0.004 (1/255).
                                          Bare flag (no value) uses all defaults.
-D, --filter-cluster   [res,op,min]     Keep only the connected cluster at --seed-pos.
                                          GPU-voxelizes at coarse resolution (res world units/voxel).
                                          Default: res=1.0, opacity=0.999, min=0.1.
                                          Bare flag (no value) uses all defaults.
-p, --params           <key=val,...>    Pass parameters to .mjs generator script
-l, --lod              <n>              Tag the Gaussians with LOD level n (n >= 0)
-m, --summary                           Print per-column statistics to stdout
-M, --morton-order                      Reorder Gaussians by Morton code (Z-order curve)

General Options

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-h, --help                              Show this help and exit
-v, --version                           Show version and exit
-q, --quiet                             Suppress non-error output
    --verbose                           Show debug-level diagnostics
    --mem                               Show memory usage in progress output
    --tty                               Interactive bar rendering (default on a TTY; --no-tty to disable)
-w, --overwrite                         Overwrite output file if it exists

GPU Options

Used by SOG compression and GPU voxelization (--filter-cluster, --filter-floaters, .voxel.json output).

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-L, --list-gpus                         List available GPU adapters and exit
-g, --gpu              <n|cpu>          Device for GPU operations: GPU adapter index | 'cpu'
                                          ('cpu' disables GPU and is incompatible with
                                          GPU-only features like --filter-cluster)

SOG Compression Options

Apply when writing .sog, meta.json, lod-meta.json, or .html outputs.

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-i, --iterations       <n>              Iterations for SH compression (more=better). Default: 10

SPZ Output Options

Apply when writing .spz outputs.

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    --spz-version      <3|4>            The SPZ format version to write. Default: 4

HTML Viewer Output Options

Apply when writing .html outputs.

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-E, --viewer-settings  <settings.json>  HTML viewer settings JSON file
-U, --unbundled                         Generate unbundled HTML viewer with separate files

[!NOTE]
See the SuperSplat Viewer Settings Schema for details on how to pass data to the -E option.

LCC / LCC2 Input Options

Apply when reading .lcc and .lcc2 files.

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-O, --lod-select       <n,n,...>        Comma-separated LOD levels to read from LCC / LCC2 input

LOD Output Options

Apply when writing lod-meta.json (multi-LOD streaming SOG bundle).

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-C, --lod-chunk-count  <n>              Approximate number of Gaussians per LOD chunk in K. Default: 512
-X, --lod-chunk-extent <n>              Approximate size of an LOD chunk in world units (m). Default: 16

See Generating Streamed SOG for an end-to-end walkthrough.

Voxel Output Options

Apply when writing .voxel.json (sparse voxel octree for collision detection). See the Collision Mesh Guide for a deep dive on each step and tuning.

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    --voxel-params     [size,opacity]   Voxel size and opacity threshold. Default: 0.05,0.1
    --voxel-external-fill [size]        Seal exterior voxels via boundary flood fill (interior scenes).
                                          [size] (world units) is the dilation distance applied
                                          before the flood fill to bridge small wall gaps.
                                          --seed-pos is used to verify the volume is enclosed at
                                          the seed; the fill is skipped if the seed is reachable
                                          from outside.
                                          Default size: 1.6
    --voxel-floor-fill [size]           Fill each column upward from bottom until hitting solid (exterior scenes).
                                          Optional size (world units): only patch XZ areas surrounded by floor
                                          within 2*size; large empty exterior areas are left alone.
                                          Default size: 1.6
    --voxel-carve      [h,r]            Carve navigable space using capsule flood fill from seed.
                                          Default: height=1.6, radius=0.2
    --seed-pos         <x,y,z>          Seed position for voxel fill/carve and --filter-cluster.
                                          Default: 0,0,0
-K, --collision-mesh   [smooth|faces]   Generate collision mesh (.collision.glb). Default: smooth

Image Output Options

Apply when writing .webp (lossless WebP rendered via GPU rasterizer).

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    --projection       <pinhole|equirect>  Camera projection. Default: pinhole.
                                        equirect = 360°×180° panorama from --camera; --fov must be
                                        omitted; --resolution must be 2:1 (default 2048x1024).
    --camera           <x,y,z>          Camera position in world space. Default: 2,1,-2
    --look-at          <x,y,z>          Camera target point. Default: 0,0,0
    --up               <x,y,z>          World up vector. Default: 0,1,0
    --fov              <degrees>        Vertical field of view in degrees. Default: 60. Rejected with --projection equirect.
    --resolution       <WxH>            Output resolution, e.g. 1920x1080. Default: 1280x720 (pinhole) or 2048x1024 (equirect)
    --near             <n>              Near clip distance. Default: 0.2 (matches reference 3DGS)
    --background       <r,g,b[,a]>      Background color in [0,1]. Default: 0,0,0,1
    --f-stop           <N>              Aperture as a photographic f-stop (e.g. 2.8, 5.6, 11). Enables defocus blur;
                                        smaller = more blur. Pinhole only. Default: disabled (no defocus).
    --focus-distance   <n>              Camera-space Z of the focus plane (world units). Default: distance to --look-at.
                                        Pinhole only; only meaningful with --f-stop.
    --sensor-size      <n>              Vertical sensor height in world units. Gives --f-stop a physical meaning.
                                        Default: 0.024 (35mm full-frame, world units = meters). Scale to your world:
                                        world unit = decimeter → 0.24, world unit = millimeter → 24.
    --camera-end       <x,y,z>          End camera position. When set, enables camera motion blur: the renderer
                                        averages sub-frames with the camera interpolated from --camera (shutter open)
                                        to --camera-end (shutter close). Default: disabled (no motion blur).
    --look-at-end      <x,y,z>          End camera target. Default: same as --look-at. Only with --camera-end.
    --up-end           <x,y,z>          End up vector. Default: same as --up. Only with --camera-end.
    --shutter          <0..1>           Fraction of the start→end segment integrated, centered on the midpoint
                                        (1.0 = full motion; 0.5 = 180° shutter). Default: 1. Only with --camera-end.
    --motion-samples   <n>              Sub-frames to accumulate for motion blur. Cost is N× a single render.
                                        Default: 16. Only with --camera-end.

Examples

Basic Operations

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# Simple format conversion
splat-transform input.ply output.csv

# Convert from .splat format
splat-transform input.splat output.ply

# Convert from .ksplat format
splat-transform input.ksplat output.ply

# Convert to compressed PLY
splat-transform input.ply output.compressed.ply

# Uncompress a compressed PLY back to standard PLY
# (compressed .ply is detected automatically on read)
splat-transform input.compressed.ply output.ply

# Convert to SOG bundled format
splat-transform input.ply output.sog

# Convert to SOG unbundled format
splat-transform input.ply output/meta.json

# Convert from SOG (bundled) back to PLY
splat-transform scene.sog restored.ply

# Convert from SOG (unbundled folder) back to PLY
splat-transform output/meta.json restored.ply

# Convert to standalone HTML viewer (bundled, single file)
splat-transform input.ply output.html

# Convert to unbundled HTML viewer (separate CSS, JS, and SOG files)
splat-transform -U input.ply output.html

# Convert to HTML viewer with custom settings
splat-transform -E settings.json input.ply output.html

Transformations

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# Scale and translate
splat-transform bunny.ply -s 0.5 -t 0,0,10 bunny_scaled.ply

# Rotate by 90 degrees around Y axis
splat-transform input.ply -r 0,90,0 output.ply

# Chain multiple transformations
splat-transform input.ply -s 2 -t 1,0,0 -r 0,0,45 output.ply

Filtering

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# Remove entries containing NaN and Inf
splat-transform input.ply --filter-nan output.ply

# Filter by opacity values (keep only splats with opacity > 0.5)
splat-transform input.ply -V opacity,gt,0.5 output.ply

# Strip spherical harmonic bands higher than 2
splat-transform input.ply --filter-harmonics 2 output.ply

# Simplify to 50000 splats via progressive pairwise merging
splat-transform input.ply --decimate 50000 output.ply

# Simplify to 25% of original splat count
splat-transform input.ply -F 25% output.ply

Advanced Usage

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# Combine multiple files with different transforms
splat-transform -w cloudA.ply -r 0,90,0 cloudB.ply -s 2 merged.compressed.ply

# Apply final transformations to combined result
splat-transform input1.ply input2.ply output.ply -t 0,0,10 -s 0.5

Statistical Summary

Generate per-column statistics for data analysis or test validation:

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# Print summary, then write output
splat-transform input.ply --summary output.ply

# Print summary without writing a file (discard output)
splat-transform input.ply -m null

# Print summary before and after a transform
splat-transform input.ply --summary -s 0.5 --summary output.ply

The summary includes min, max, median, mean, stdDev, nanCount and infCount for each column in the data.

Generators (Beta)

Generator scripts can be used to synthesize gaussian splat data. See gen-grid.mjs for an example.

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splat-transform gen-grid.mjs -p width=10,height=10,scale=10,color=0.1 scenes/grid.ply -w

Voxel Format

The voxel format stores sparse voxel octree data for collision detection. It consists of two files: .voxel.json (metadata) and .voxel.bin (binary octree data). Pass -K to also emit a .collision.glb mesh derived from the voxel grid.

For a step-by-step walkthrough of each option (with illustrations), see the Collision Mesh Guide.

Recommended pipeline

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splat-transform input.ply \
    --filter-cluster --seed-pos x,y,z \
    [--voxel-external-fill | --voxel-floor-fill] [--voxel-carve] \
    [-K [smooth|faces]] \
    output.voxel.json

--filter-cluster isolates the central scene and discards stray floaters before voxelization. --seed-pos is shared by --filter-cluster and the voxel fill/carve passes — set it once to a known-walkable point inside the scene.

Interior scenes (rooms, indoor scans)

Use --voxel-external-fill to seal the void around the room interior, then --voxel-carve to hollow out the navigable space:

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splat-transform room.ply \
    --filter-cluster --seed-pos 0,1,0 \
    --voxel-external-fill --voxel-carve \
    -K room.voxel.json

Exterior scenes (outdoor objects, terrain)

Use --voxel-floor-fill to fill the ground beneath surfaces, optionally followed by --voxel-carve:

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splat-transform terrain.ply \
    --filter-cluster --seed-pos 0,0,0 \
    --voxel-floor-fill \
    -K terrain.voxel.json

Other examples

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# Voxelize with custom resolution and opacity threshold
splat-transform --voxel-params 0.1,0.3 input.ply output.voxel.json

# Custom carve capsule (height, radius)
splat-transform --seed-pos 1,0,0 --voxel-carve 2.0,0.3 input.ply output.voxel.json

# Watertight voxel-face collision mesh
splat-transform -K faces input.ply output.voxel.json

Image Rendering

Render a splat scene to a lossless WebP image from a given camera view. Rendering runs on the GPU.

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# Default 1280x720 render
splat-transform input.ply view.webp

# Custom camera and resolution
splat-transform input.ply view.webp \
    --camera 2,1,-2 --look-at 0,0,0 \
    --fov 50 --resolution 1920x1080

# Transparent background
splat-transform input.ply view.webp --background 0,0,0,0

# Defocus blur (focus on look-at, f/2.8 aperture)
splat-transform input.ply view.webp --f-stop 2.8

# Defocus with explicit focus distance and a smaller world scale
splat-transform input.ply view.webp \
    --f-stop 2.8 --focus-distance 3 --sensor-size 0.1

# 360° equirectangular panorama from camera position
splat-transform input.ply pano.webp \
    --projection equirect --camera 0,1,0 --look-at 0,1,1

# Camera motion blur (dolly from start to end pose over the shutter)
splat-transform input.ply view.webp \
    --camera 2,1,-2 --camera-end 3,1,-2 \
    --motion-samples 16 --shutter 1

Device Selection for SOG Compression

When compressing to SOG format, you can control which device (GPU or CPU) performs the compression:

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# List available GPU adapters
splat-transform --list-gpus

# Let WebGPU automatically choose the best GPU (default behavior)
splat-transform input.ply output.sog

# Explicitly select a GPU adapter by index
splat-transform -g 0 input.ply output.sog  # Use first listed adapter
splat-transform -g 1 input.ply output.sog  # Use second listed adapter

# Use CPU for compression instead (much slower but always available)
splat-transform -g cpu input.ply output.sog

[!NOTE]
When -g is not specified, WebGPU automatically selects the best available GPU. Use -L to list available adapters with their indices and names. The order and availability of adapters depends on your system and GPU drivers. Use -g <index> to select a specific adapter, or -g cpu to force CPU computation.

[!WARNING]
CPU compression can be significantly slower than GPU compression (often 5-10x slower). Use CPU mode only if GPU drivers are unavailable or problematic.

Getting Help

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# Show version
splat-transform --version

# Show help
splat-transform --help

---

Library Usage

SplatTransform exposes a programmatic API for reading, processing, and writing Gaussian splat data.

Basic Import

typescriptCopy
import {
    readFile,
    writeFile,
    getInputFormat,
    getOutputFormat,
    DataTable,
    processDataTable
} from '@playcanvas/splat-transform';

Key Exports

Export	Description
readFile	Read splat data from various formats
writeFile	Write splat data to various formats
getInputFormat	Detect input format from filename
getOutputFormat	Detect output format from filename
DataTable, Column	Core data structures for splat data
combine	Merge multiple DataTables into one
convertToSpace	Convert a DataTable between coordinate spaces
processDataTable	Apply a sequence of processing actions
computeSummary	Generate statistical summary of data
sortMortonOrder	Sort indices by Morton code for spatial locality
sortByVisibility	Sort indices by visibility score for filtering
writeVoxel	Write sparse voxel octree files
writeImage	Render a camera view to a lossless WebP image (requires GPU)
renderSplats	Lower-level renderer returning the raw RGBA byte buffer

File System Abstractions

The library uses abstract file system interfaces for maximum flexibility:

Reading:

• UrlReadFileSystem - Read from URLs (browser/Node.js)
• MemoryReadFileSystem - Read from in-memory buffers
• ZipReadFileSystem - Read from ZIP archives

Writing:

• MemoryFileSystem - Write to in-memory buffers
• ZipFileSystem - Write to ZIP archives

Example: Reading and Processing

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import { Vec3 } from 'playcanvas';
import {
    readFile,
    writeFile,
    getInputFormat,
    getOutputFormat,
    processDataTable,
    UrlReadFileSystem,
    MemoryFileSystem
} from '@playcanvas/splat-transform';

// Read a PLY file from URL
const fileSystem = new UrlReadFileSystem();
const inputFormat = getInputFormat('scene.ply');

const dataTables = await readFile({
    filename: 'https://example.com/scene.ply',
    inputFormat,
    options: { iterations: 10 },
    params: [],
    fileSystem
});

// Apply transformations
const processed = processDataTable(dataTables[0], [
    { kind: 'scale', value: 0.5 },
    { kind: 'translate', value: new Vec3(0, 1, 0) },
    { kind: 'filterNaN' }
]);

// Write to in-memory buffer
const memFs = new MemoryFileSystem();
const outputFormat = getOutputFormat('output.ply', {});

await writeFile({
    filename: 'output.ply',
    outputFormat,
    dataTable: processed,
    options: {}
}, memFs);

// Get the output data
const outputBuffer = memFs.files.get('output.ply');

Processing Actions

The processDataTable function accepts an array of actions:

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type ProcessAction =
    | { kind: 'translate'; value: Vec3 }
    | { kind: 'rotate'; value: Vec3 }       // Euler angles in degrees
    | { kind: 'scale'; value: number }
    | { kind: 'filterNaN' }
    | { kind: 'filterByValue'; columnName: string; comparator: 'lt'|'lte'|'gt'|'gte'|'eq'|'neq'; value: number }
    | { kind: 'filterBands'; value: 0|1|2|3 }
    | { kind: 'filterBox'; min: Vec3; max: Vec3 }
    | { kind: 'filterSphere'; center: Vec3; radius: number }
    | { kind: 'filterFloaters'; voxelResolution?: number; opacityCutoff?: number; minContribution?: number } // GPU
    | { kind: 'filterCluster'; voxelResolution?: number; seed?: Vec3; opacityCutoff?: number; minContribution?: number } // GPU
    | { kind: 'decimate'; count: number | null; percent: number | null }
    | { kind: 'param'; name: string; value: string }
    | { kind: 'lod'; value: number }
    | { kind: 'summary' }
    | { kind: 'mortonOrder' };

[!NOTE]
filterFloaters and filterCluster require a GPU device — pass createDevice via the ProcessOptions argument to processDataTable.

Custom Logging

Configure the logger for your environment:

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import { logger } from '@playcanvas/splat-transform';

logger.setLogger({
    log: console.log,
    warn: console.warn,
    error: console.error,
    debug: console.debug,
    progress: (text) => process.stdout.write(text),
    output: console.log
});

logger.setQuiet(true); // Suppress non-error output