Processing Large-Scale PlanetScope Data
Project description
plaknit
Processing Large-Scale PlanetScope Data
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Planet data is phenomenal for tracking change, but the current acquisition strategy sprays dozens of narrow strips across a scene. Without careful masking and mosaicking, even "cloud free" searches still include haze, seams, and nodata gaps.
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PlanetScope scenes are also huge. Building clean, analysis-ready products requires an automated workflow that can run on laptops or HPC clusters where GDAL, rasterio, and Orfeo Toolbox are already available.
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plaknitpackages the masking + mosaicking flow I rely on for regional mapping so the Planet community can stitch together reliable time series without copying shell scripts from old notebooks. -
Free software: MIT License
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Documentation: https://dzfinch.github.io/plaknit
Features
- GDAL-powered parallel masking of Planet strips with their UDM rasters.
- Tuned Orfeo Toolbox mosaicking pipeline with RAM hints for large jobs.
- CLI + Python API that scale from local experimentation to HPC batch runs.
- Raster analysis helpers (e.g., normalized difference indices) built on rasterio.
- Random Forest training + inference utilities for classifying Planet stacks.
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