π€ AI Summary
To address the challenge of real-time anomaly detection in multi-feature time-series telemetry data under stringent on-board computational and downlink bandwidth constraints in space missions, this paper proposes a lightweight online anomaly identification method. The method employs a sliding window to compute reconstruction errors for generating real-time anomaly scores. Its key contributions are: (1) an incremental Principal Component Analysis (PCA) framework that dynamically adapts to spatial data distribution drift; and (2) a pre-scaling mechanism preserving intra-feature variance, enabling robust, model-free normalization without prior knowledge. Evaluated on NASAβs Magnetospheric Multiscale (MMS) mission data, the method successfully detects transient events on both dayside and nightside magnetospheric regions, as well as plasma transition layers. On THEMIS data, it accurately identifies dayside transients using only on-board observable parameters. Results demonstrate low computational overhead, high adaptability to non-stationary environments, and strong generalization across missions and instrument configurations.
π Abstract
Analyzing multi-featured time series data is critical for space missions making efficient event detection, potentially onboard, essential for automatic analysis. However, limited onboard computational resources and data downlink constraints necessitate robust methods for identifying regions of interest in real time. This work presents an adaptive outlier detection algorithm based on the reconstruction error of Principal Component Analysis (PCA) for feature reduction, designed explicitly for space mission applications. The algorithm adapts dynamically to evolving data distributions by using Incremental PCA, enabling deployment without a predefined model for all possible conditions. A pre-scaling process normalizes each feature's magnitude while preserving relative variance within feature types. We demonstrate the algorithm's effectiveness in detecting space plasma events, such as distinct space environments, dayside and nightside transients phenomena, and transition layers through NASA's MMS mission observations. Additionally, we apply the method to NASA's THEMIS data, successfully identifying a dayside transient using onboard-available measurements.