Skip to main content

Premium desktop workstation for Earth observation segmentation.

Project description

SpectraForge

A premium desktop workstation for Earth observation processing and visualization across sensors. Unsupervised segmentation and uncertainty are optional modules inside a much broader EO workflow. Built to run locally on Windows/macOS/Linux.

Why it exists

  • Multi-sensor preprocessing (Sentinel‑1/2/3, Landsat, ERA5, ENMAP, hyperspectral, PlanetScope, UAV)
  • Band management and index generation for fast EO analysis
  • Interactive ROI labeling for ground‑truthing and validation
  • Optional unsupervised segmentation with probability maps and uncertainty
  • Designed for patent-ready workflows (keep private until filing)

Features (v1)

  • Clean, modern studio UI (not a QGIS clone)
  • GeoTIFF, NetCDF, ENVI (hyperspectral), Sentinel‑2 folder support
  • Sensor presets (Sentinel‑1/2/3, Landsat, PlanetScope, UAV, ERA5, ENMAP, hyperspectral)
  • Auto feature selection across multi-band data
  • Unsupervised segmentation with probability maps and entropy-based uncertainty (optional)
  • Index Builder with curated indices per sensor + custom JSON/YAML recipes
  • ROI selection + cluster labeling workflow
  • Run history saved to runs/
  • Copernicus + Planet API panels (offline stub in this build)

Install

From PyPI:

python -m pip install spectraforce

From source:

python -m pip install -r requirements.txt

Run

spectraforge

Alternative:

python -m spectraforge

Data formats

  • GeoTIFF: .tif, .tiff
  • NetCDF: .nc (ERA5 and other gridded products)
  • ENVI: .hdr + .img (hyperspectral)
  • Sentinel‑2: SAFE folder with .jp2 band files
  • NumPy: .npy arrays (2D or 3D)
  • Tabular: .csv, .xlsx

Indices

SpectraForge ships with curated indices (NDVI, NDWI, etc.) per sensor. You can add your own:

  • JSON/YAML recipe files (see samples/ for examples)
  • Index layers appear in the layer stack like any other band Example custom indices file: samples/indices_example.json

NPY export

Export data to .npy directly from the UI:

  • All bands in one file
  • Selected bands in one file
  • Individual band files
  • Optional index layer exports

Offline samples

Synthetic samples live in samples/ so the repo runs without downloads. Real cropped samples live in samples/real/. Manipur example outputs live in samples/manipur/.

API keys (stored locally)

API keys are stored in ~/.spectraforge/config.json on your machine.

Connectors (step by step)

The Connectors tab provides a guided workflow for sensor platform access (Copernicus and PlanetScope). This build ships with an offline stub so the UI and local key storage can be tested without network access. The steps below describe the full workflow, and the current offline behavior is noted where relevant.

What the Connectors tab does

  • Collects and stores API keys locally
  • Lets a dataset browser query sensors (S1/S2/S3 and PlanetScope)
  • Builds a download queue with a save location

Step-by-step workflow

  1. Open the Connectors tab in the right‑hand inspector.
  2. Choose a provider in the left panel.
  3. Paste the API key and click Save.
  4. If a Test or Validate button is shown, click it.
  5. Open the Dataset Browser section.
  6. Pick a sensor family (for example: Sentinel‑2).
  7. Set a bounding box or choose a saved ROI.
  8. Set a date range and cloud filter.
  9. Click Search to list scenes.
  10. Select one or more scenes and click Add to Queue.
  11. Set the Save Location.
  12. Click Start Download.

Example

  1. Provider: Copernicus.
  2. Sensor: Sentinel‑2.
  3. AOI: a polygon ROI drawn in the map.
  4. Date range: 2025-01-01 to 2025-02-01.
  5. Cloud filter: 0–20%.
  6. Action: search, add two scenes to queue, save to samples/downloads/.
  7. Result: queued items appear in the download list with size, sensor, and target path.

Offline stub behavior in this build

  • Keys are saved locally and shown as “stored”.
  • Searches and downloads are disabled to keep the build offline.
  • The UI still displays the full workflow so it can be demonstrated end‑to‑end.

Why SpectraForge Helps

SpectraForge provides a fast, repeatable path from raw EO images to clean indices, analysis layers, and exportable outputs. Custom scripts do not need to be rebuilt for every dataset. The same workflow can be applied across sensors for consistent results. A typical workflow can be done by loading a folder, letting the app auto detect bands, choosing indices, and optionally running unsupervised segmentation with ROI labeling.

UI Demo (Auto NPY Detection)

When a .npy dataset is opened, SpectraForge can automatically detect the sensor, load the bands, and populate the band list. If the sensor cannot be detected, it can be selected manually and the workflow can continue without restarting.

Auto NPY Detection Demo

Step by Step Outputs for Manipur Sentinel‑2

The full pipeline was run on real Sentinel‑2 data from Manipur, and the outputs were saved below.

Step 1 — Load bands and true color

Manipur True Color

Step 2 — NDVI and NDWI indices

Manipur NDVI
NDVI
Manipur NDWI
NDWI

Step 3 — Unsupervised segmentation with 8 clusters

Manipur Segmentation Labels

Step 4 — ROI selection and labeling

Manipur ROI Overlay
ROI overlay
Manipur ROI Labels
ROI labels

Step 5 — Uncertainty and confidence The same color rule is used for both maps: blue means low, red means high.
For uncertainty, blue means low uncertainty and red means high uncertainty.
For confidence, blue means low confidence and red means high confidence.

Manipur Segmentation Uncertainty
Uncertainty
Manipur Segmentation Confidence
Confidence

Saved outputs full resolution

  • samples/manipur_full/manipur_full_stack.npy
  • samples/manipur_full/manipur_full_stack_preview.tif
  • samples/manipur_full/manipur_full_<index>.npy
  • samples/manipur_full/manipur_full_<index>.tif

Color Legend for segmentation labels

Clusters are unsupervised. Colors map to cluster IDs in order:

  • 0 → maroon #800000
  • 1 → darkblue #00008B
  • 2 → darkgreen #006400
  • 3 → cyan #00FFFF
  • 4 → darkcyan #008B8B
  • 5 → magenta #FF00FF
  • 6 → indigo #4B0082
  • 7 → grey #808080
  • 8 → peru #CD853F
  • 9 → slateblue #6A5ACD
  • 10 → mediumspringgreen #00FA9A
  • 11 → orangered #FF4500

If you run fewer than 12 clusters, only the first N colors are used.

Color Notes for indices

Index quicklooks use a viridis scale: brighter colors indicate higher values.

Uncertainty calibration made easy

  • Run segmentation → get probability maps (predict_proba)
  • Use entropy + confidence to visualize uncertain regions
  • Assign labels with ROI selections (no labeled data required)

Segmentation engine

If your environment has scientific stack conflicts, switch the engine to Safe mode in the UI.
Fast mode uses scikit‑learn when available.

SpectraForge vs QGIS (Pros & Cons)

Aspect SpectraForge QGIS
Focus EO segmentation + indices + uncertainty Full GIS for all domains
Setup One command local run Heavier install + plugins
Unsupervised segmentation + uncertainty Built‑in, turnkey Requires plugins/workflows
Indices Curated EO indices + custom recipes Many tools, but more manual setup
UI style Modern studio layout (not QGIS style) Traditional GIS layout
Extensibility Focused feature set Huge plugin ecosystem
Geoprocessing breadth Focused EO analytics Broad GIS toolbox
Best for Fast EO segmentation + research demos Full GIS analysis & cartography

Pros of SpectraForge: fast EO‑first workflow, built‑in uncertainty, simple NPY export, easy to demo.
Cons vs QGIS: fewer GIS tools, smaller plugin ecosystem, less advanced cartography.

Contributions

See CONTRIBUTING.md and CODE_OF_CONDUCT.md.

Credits

Arnab Bhowmik

How to cite

If you use SpectraForge in academic work, please cite it like this:

Arnab Bhowmik. SpectraForge: Earth Observation Processing and Visualization Toolkit. Version 0.16, 2026. https://github.com/ArnaBannonymus/SpectraForge

BibTeX:

@software{spectraforge_2026,
  author = {Bhowmik, Arnab},
  title = {SpectraForge: Earth Observation Processing and Visualization Toolkit},
  year = {2026},
  version = {0.16},
  url = {https://github.com/ArnaBannonymus/SpectraForge}
}

Privacy note

Runs locally. No data leaves your machine.

License

Proprietary (permission required for any use)

Project details


Download files

Download the file for your platform. If you're not sure which to choose, learn more about installing packages.

Source Distribution

spectraforce-0.16.tar.gz (32.9 kB view details)

Uploaded Source

Built Distribution

If you're not sure about the file name format, learn more about wheel file names.

spectraforce-0.16-py3-none-any.whl (36.8 kB view details)

Uploaded Python 3

File details

Details for the file spectraforce-0.16.tar.gz.

File metadata

  • Download URL: spectraforce-0.16.tar.gz
  • Upload date:
  • Size: 32.9 kB
  • Tags: Source
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/6.1.0 CPython/3.13.7

File hashes

Hashes for spectraforce-0.16.tar.gz
Algorithm Hash digest
SHA256 2159de2a2e6f0b49a352c46467dd328dc678abef9b91813f6fe164506e9fff5d
MD5 763c28519abab7a1691c59ff2067a126
BLAKE2b-256 776e51fc349e23644864c7fbb00e3d871bfd2431ecb98c25403d166472c3cd29

See more details on using hashes here.

File details

Details for the file spectraforce-0.16-py3-none-any.whl.

File metadata

  • Download URL: spectraforce-0.16-py3-none-any.whl
  • Upload date:
  • Size: 36.8 kB
  • Tags: Python 3
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/6.1.0 CPython/3.13.7

File hashes

Hashes for spectraforce-0.16-py3-none-any.whl
Algorithm Hash digest
SHA256 b23519122c36ae861110dd5d3bb5283a62873c86cbe1c74b8f6180bbb0f98421
MD5 7aa2001accf8b8cb964b51403d4feaa2
BLAKE2b-256 9d4e736d650316c6faf3084d4a1091835cb150f9409b3cf1714e7eb79ed86165

See more details on using hashes here.

Supported by

AWS Cloud computing and Security Sponsor Datadog Monitoring Depot Continuous Integration Fastly CDN Google Download Analytics Pingdom Monitoring Sentry Error logging StatusPage Status page