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[bibtex]@InProceedings{Ekim_2025_CVPR, author = {Ekim, Burak and Tadesse, Girmaw Abebe and Robinson, Caleb and Hacheme, Gilles and Schmitt, Michael and Dodhia, Rahul and Ferres, Juan M. Lavista}, title = {Distribution Shifts at Scale: Out-of-distribution Detection in Earth Observation}, booktitle = {Proceedings of the Computer Vision and Pattern Recognition Conference (CVPR) Workshops}, month = {June}, year = {2025}, pages = {2265-2274} }
Distribution Shifts at Scale: Out-of-distribution Detection in Earth Observation
Abstract
Training robust deep learning models is crucial in Earth Observation, where globally deployed models often face distribution shifts that degrade performance, especially in low-data regions. Out-of-distribution (OOD) detection addresses this by identifying inputs that deviate from in-distribution (ID) data. However, existing methods either assume access to OOD data or compromise primary task performance, limiting real-world use. We introduce TARDIS, a post-hoc OOD detection method designed for scalable geospatial deployment. Our core innovation lies in generating surrogate distribution labels by leveraging ID data within the feature space. TARDIS takes a pre-trained model, ID data, and data from an unknown distribution (WILD), separates WILD into surrogate ID and OOD labels based on internal activations, and trains a binary classifier to detect distribution shifts. We validate on EuroSAT and xBD across 17 setups covering covariate and semantic shifts, showing near-upper-bound surrogate labeling performance in 13 cases and matching the performance of top post-hoc activation- and scoring-based methods. Finally, deploying TARDIS on Fields of the World reveals actionable insights into pre-trained model behavior at scale. The code is available at https://github.com/microsoft/geospatial-ood-detection
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