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A deep learning model detects dust storms in real time on satellites, improving monitoring efficiency and accuracy.
Dust storms evolve on 10 min time scales, yet satellite monitoring remains constrained by ground segment pipelines that delay actionable products by half-hour to hours. We present an on-orbit deep learning framework that executes dust storm detection and quantitative retrieval directly onboard the satellite, converting geostationary Himawari-8/9 observations into exposure-grade products within 5.62 min─an ∼80% latency reduction relative to conventional acquisition-to-product chains. A cascaded design couples a lightweight event gate with a multitask retriever for PM10 and PM2.5, optimized by a tail-aware loss that prioritizes fidelity at extreme concentrations. Compared to the baseline among LGBM, XGBoost, MLP, CNN, and LSTM, our system reduces the RMSE by 30% (from ∼32.25 to 20.54 μg/m3) for PM10 and by 25% (from ∼14.44 to 10.27 μg/m3) for PM2.5, markedly mitigating the underestimation of high-concentration values. To assess on-orbit feasibility, we simulate deployment on an NVIDIA Jetson AGX Orin platform, representative of resource-constrained satellite computing environments, where the model achieves a 3.60 s inference latency with a ∼10 W power draw and <3 GB memory footprint, confirming its viability for resource-constrained spacecraft environments. Case studies (May 19–20, 2023; April 15, 2025) show spatially coherent dust cores, sharper plume gradients, and minutes-scale fusion with population grids and vulnerable locations for real-time exposure assessment and early warning. This work integrates on-orbit inference, tailored retrieval, and demographic coupling to transform dust storm monitoring into minute-level, exposure-focused intelligence, providing a scalable model for other disaster aerosols.
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Peng et al. (2026) studied this question.
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