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🛰️ SatCLIP - A Global, General-Purpose Geographic Location Encoder
Overview of the pretraining and deployment pipeline for SatCLIP.
Approach
SatCLIP trains location and image encoders via contrastive learning, by matching images to their corresponding locations. This is analogous to the CLIP approach, which matches images to their corresponding text. Through this process, the location encoder learns characteristics of a location, as represented by satellite imagery. For more details, check out our paper.
Overview
Usage of SatCLIP is simple:
from model import *
from location_encoder import *
model = SatCLIP(
embed_dim=512,
image_resolution=224, in_channels=13, vision_layers=4, vision_width=768, vision_patch_size=32, # Image encoder
le_type='sphericalharmonics', pe_type='siren', legendre_polys=10, frequency_num=16, max_radius=360, min_radius=1, harmonics_calculation='analytic' # Location encoder
)
img_batch = torch.randn(32, 13, 224, 224) # Represents a batch of 32 images
loc_batch = torch.randn(32, 2) # Represents the corresponding 32 locations (lon/lat)
with torch.no_grad():
logits_per_image, logits_per_coord = model(img_batch, loc_batch)
probs = logits_per_image.softmax(dim=-1).detach().cpu().numpy()
Training
You first need to download the S2-100k dataset in /data/s2
. First, download the index file:
cd data/s2
wget https://satclip.z13.web.core.windows.net/satclip/index.csv
Within /data/s2
, navigate to /images
, download all images and unpack them:
cd images
wget https://satclip.z13.web.core.windows.net/satclip/satclip.tar
tar -xf satclip.tar
Now, to train SatCLIP models, set the paths correctly, adapt training configs in satclip/configs/default.yaml
and train SatCLIP by running:
cd satclip
python main.py
Use of the S2-100K dataset
The S2-100K dataset is a dataset of 100,000 multi-spectral satellite images sampled from Sentinel-2 via the Microsoft Planetary Computer. Copernicus Sentinel data is captured between Jan 1, 2021 and May 17, 2023. The dataset is sampled approximately uniformly over landmass and only includes images without cloud coverage. The dataset is available for research purposes only. If you use the dataset, please cite our paper. More information on the dataset can be found in our paper.
Pretrained Models
Visualization of embeddings obtained by different location encoders for locations around the globe.
We provide six pretrained SatCLIP models, trained with different vision encoders and spatial resolution hyperparameters $L$ (these indicate the number of Legendre polynomials used for spherical harmonics location encoding. Please refer to our paper for more details). The pretrained models can be downloaded as follows:
- SatCLIP-ResNet18-L10:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-resnet18-l10.ckpt
- SatCLIP-ResNet18-L40:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-resnet18-l40.ckpt
- SatCLIP-ResNet50-L10:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-resnet50-l10.ckpt
- SatCLIP-ResNet50-L40:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-resnet50-l40.ckpt
- SatCLIP-ViT16-L10:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-vit16-l10.ckpt
- SatCLIP-ViT16-L40:
wget https://satclip.z13.web.core.windows.net/satclip/satclip-vit16-l40.ckpt
Usage of pretrained models is simple:
from load import get_satclip
device = 'cuda'
c = torch.randn(32, 2) # Represents a batch of 32 locations (lon/lat)
model = get_satclip('path_to_satclip', device=device) #Only loads location encoder by default
model.eval()
with torch.no_grad():
emb = model(c.double().to(device)).detach().cpu()
You can also access SatCLIP model weights directly via Hugging Face.
Examples
Examples on how to obtain and use pretrained SatCLIP embeddings can be found in the notebooks
folder. We provide notebooks (optimized for use with Google Colab) for the following use cases.
Setup:
Example use cases:
Use baseline pretrained location encoders:
Citation
@article{klemmer2023satclip,
title={SatCLIP: Global, General-Purpose Location Embeddings with Satellite Imagery},
author={Klemmer, Konstantin and Rolf, Esther and Robinson, Caleb and Mackey, Lester and Ru{\ss}wurm, Marc},
journal={arXiv preprint arXiv:2311.17179},
year={2023}
}
Contributing
This project welcomes contributions and suggestions. Most contributions require you to agree to a Contributor License Agreement (CLA) declaring that you have the right to, and actually do, grant us the rights to use your contribution. For details, visit https://cla.opensource.microsoft.com.
When you submit a pull request, a CLA bot will automatically determine whether you need to provide a CLA and decorate the PR appropriately (e.g., status check, comment). Simply follow the instructions provided by the bot. You will only need to do this once across all repos using our CLA.
This project has adopted the Microsoft Open Source Code of Conduct. For more information see the Code of Conduct FAQ or contact opencode@microsoft.com with any additional questions or comments.
Trademarks
This project may contain trademarks or logos for projects, products, or services. Authorized use of Microsoft trademarks or logos is subject to and must follow Microsoft's Trademark & Brand Guidelines. Use of Microsoft trademarks or logos in modified versions of this project must not cause confusion or imply Microsoft sponsorship. Any use of third-party trademarks or logos are subject to those third-party's policies.