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Using satellite imagery to identify shelterbelts and measure their impacts on agricultural productivity

Project description

shelterbelts

This repo is for using satellite imagery to map and categorise shelterbelts across Australia, in preparation for measuring impacts on agricultural productivity at scale.

Google Earth Engine App

You can visualise some results from the repo in this Earth Engine App:
https://christopher-bradley-phd.projects.earthengine.app/view/shelterbelts

Or a mobile friendly version at:
https://christopher-bradley-phd.projects.earthengine.app/view/shelterbelts-mobile

Notebook Examples

There are jupyter notebooks to demo the functionality of this repo in examples.

Documentation

View the published docs at:
https://christopherbradley.github.io/shelterbelts/index.html

Installation

pip install shelterbelts
View the pypi package at: https://pypi.org/project/shelterbelts

Current Methods

The tree predictions come from annual Sentinel-2 imagery largely following a method by Stewart et al. (2025), using a tree/no-tree training dataset provided by Nicolas Pucino.

After the predictions, pixels were categorised using the following method:

  • Assign trees from model confidence (50% threshold)
  • Assign scattered trees to small groups (< 20 pixels)
  • Assign core & buffers to big groups (> 3 pixels thick)
  • Assign sheltered vs unsheltered pixels based on percent cover within 100m (5% threshold) , or wind direction (20 pixels leeward, 10 pixels upwind)
  • Assign grassland, cropland, urban and water categories from WorldCover 2021
  • Assign riparian and roads trees (3 pixel buffer)
  • Assign linear vs non-linear patches by fitting an ellipse and skeleton to each group and applying length and width thresholds.

Upcoming Plans

  • Calculate summary statistics for different regions (IBRA, LGAs, GRDC agricultural zones)
  • Include 1m shelter categories for all of ACT & NSW
  • Analyse effects on productivity & potential future benefits
  • Add layers with opportunities for more trees.

Parameter Reference

The main parameters for categorising shelterbelts are below:

Parameter Default Low Threshold High Threshold Description
min_patch_size 20 15 25 Minimum area (pixels) to classify as a patch rather than scattered trees
min_core_size 1000 100 10000 Minimum patch size (pixels) to classify as a core area
edge_size 3 2 5 Distance (pixels) defining the edge region around patch cores
buffer_width 4 3 5 Number of pixels away from the feature that still counts as within the buffer
distance_threshold 20 10 30 Distance from trees that counts as sheltered
density_threshold 5 3 10 Percentage tree cover within distance_threshold that counts as sheltered
wind_threshold 20 15 25 Wind speed threshold in km/h
wind_method WINDWARD MOST_COMMON ANY Method to determine primary wind direction
min_shelterbelt_length 20 15 25 Minimum skeleton length (in pixels) to classify a cluster as linear
max_shelterbelt_width 6 5 7 Maximum skeleton width (in pixels) to classify a cluster as linear

Parameters can be modified when calling functions directly in Python or via command-line arguments. For example:

python -m shelterbelts.indices.tree_categories input.tif --min_patch_size 30 --edge_size 5

Setup

Local Setup

  1. Download and install Miniconda from https://www.anaconda.com/download/success
  2. Add the miniconda filepath to your ~/.zhrc, e.g. export PATH="/opt/miniconda3/bin:$PATH"
  3. git clone https://github.com/ChristopherBradley/shelterbelts.git
  4. cd shelterbelts
  5. conda env create -f environment.yml
  6. conda activate shelterbelts

Setup on gadi at the National Computing Infrastructure (NCI)

  1. Create an account and request access to the projects xe2 (Borevitz Lab), v10 (Digital Earth Australia modules), ka08 (Sentinel-2 Imagery), ob53 (BARRA Wind).
  2. ssh {username}@nci.org.au and enter the password used to create your account.
  3. git clone https://github.com/ChristopherBradley/shelterbelts.git
  4. There are examples usage of the environments in pbs_scripts
  5. (optional) I like to have git ignore the .ipynb files, so that images don't clog up the git history git ls-files "*.ipynb" | xargs git update-index --skip-worktree

Usage on NCI ARE (National Computing Infrastructure's Australian Research Environment)

  1. Login here: https://are.nci.org.au/
  2. Go to JupyterLab and create a session with 1 hour, queue normalbw, compute size small, project xe2, storage gdata/+gdata/xe2+gdata/v10+gdata/ka08+gdata/ob53, python environment base /g/data/xe2/cb8590/miniconda, conda environment /g/data/xe2/cb8590/miniconda/envs/shelterbelts. Except for demo_sentinel_nci.py, use Module Directories /g/data/v10/public/modules/modulefiles and Modules: dea/20231204.
  3. Right click any .py file and open as a jupyter notebook.

Testing

If on gadi: qsub -I -P xe2 -q copyq -l ncpus=1 -l mem=8GB -l walltime=02:00:00 -l storage=gdata/xe2+scratch/xe2+gdata/v10+gdata/ka08 -l wd

Then: conda activate shelterbelts pytest tests # everything should pass except test_sentinel_nci.py

Finally: module use /g/data/v10/public/modules/modulefiles module load dea/20231204 pytest tests/test_classifications/test_sentinel_nci.py

Generating the Documentation

Generate the html: make clean && make html

You can view the documenation locally in a browser by opening docs/build/index.html

Run the doctests: make doctest

Upload the html to github pages: ghp-import -n -p -f docs/build/html

Uploading to PyPI

  1. rm dist/*
  2. Update the version in pyproject.toml
  3. python3 -m build
  4. twine upload dist/*
  5. Enter the API token
  6. Check it out at https://pypi.org/project/shelterbelts

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