aiqbench analysis
This research presents a novel unsupervised framework for detecting anomalies in spacecraft telemetry, eliminating the need for labeled historical data or extended warm-up periods. By integrating incremental retraining with adaptive Extreme Value Theory (EVT), the method achieves high performance on ESA datasets while maintaining strict chronological evaluation standards. The approach offers a practical solution for real-time fault detection in space missions where prior fault knowledge is unavailable.
Structure-Aware Unsupervised Anomaly Detection for Spacecraft Telemetry with Adaptive EVT Thresholding
arXiv:2609.10017v1 Announce Type: new Abstract: Operational anomaly detection in spacecraft telemetry typically requires labeled historical anomalies or extended warm-up periods. These requirements are rarely met in practice. We propose an unsupervised, deployment-ready framework that produces predictions from the second month of operation without any labels, prior fault knowledge, or mission-specific tuning. The approach combines incremental monthly retraining, statistical model selection, and adaptive Extreme Value Theory (EVT) thresholding for false alarm control. On the ESA Anomalies Dataset (ESA-AD), it achieves $F_{0.5}=0.700$ on Mission~1 and $F_{0.5}=0.698$ on Mission~2 under strict chronological evaluation.
Abstract:Operational anomaly detection in spacecraft telemetry typically requires labeled historical anomalies or extended warm-up periods. These requirements are rarely met in practice. We propose an unsupervised, deployment-ready framework that produces predictions from the second month of operation without any labels, prior fault knowledge, or mission-specific tuning. The approach combines incremental monthly retraining, statistical model selection, and adaptive Extreme Value Theory (EVT) thresholding for false alarm control. On the ESA Anomalies Dataset (ESA-AD), it achieves $F_{0.5}=0.700$ on Mission~1 and $F_{0.5}=0.698$ on Mission~2 under strict chronological evaluation.
5 pages, 4 figures. Accepted as a poster at SPAICE 2026
Machine Learning (cs.LG)
arXiv:2609.10017 [cs.LG]
(or arXiv:2609.10017v1 [cs.LG] for this version)
https://doi.org/10.48550/arXiv.2609.10017 Focus to learn more arXiv-issued DOI via DataCite (pending registration)
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Full text under the publisher's open licence · 190 words
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