Generalized Time-Series Analysis for In Situ Spacecraft Observations: Anomaly Detection and Data Prioritization Using Principal Components Analysis and Unsupervised Clustering

IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Matthew G. Finley, Miguel Martinez-Ledesma, William R. Paterson, Matthew R. Argall, David M. Miles, John C. Dorelli, Eftyhia Zesta
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Abstract

In situ spacecraft observations are critical to our study and understanding of the various phenomena that couple mass, momentum, and energy throughout near-Earth space and beyond. However, on-orbit telemetry constraints can severely limit the capability of spacecraft to transmit high-cadence data, and missions are often only able to telemeter a small percentage of their captured data at full rate. This presents a programmatic need to prioritize intervals with the highest probability of enabling the mission's science goals. Larger missions such as the Magnetospheric Multiscale mission (MMS) aim to solve this problem with a Scientist-In-The-Loop (SITL), where a domain expert flags intervals of time with potentially interesting data for high-cadence data downlink and subsequent study. Although suitable for some missions, the SITL solution is not always feasible, especially for low-cost missions such as CubeSats and NanoSats. This manuscript presents a generalizable method for the detection of anomalous data points in spacecraft observations, enabling rapid data prioritization without substantial computational overhead or the need for additional infrastructure on the ground. Specifically, Principal Components Analysis and One-Class Support Vector Machines are used to generate an alternative representation of the data and provide an indication, for each point, of the data's potential for scientific utility. The technique's performance and generalizability is demonstrated through application to intervals of observations, including magnetic field data and plasma moments, from the CASSIOPE e-POP/Swarm-Echo and MMS missions.

Abstract Image

航天器现场观测的广义时间序列分析:利用主成分分析和无监督聚类进行异常检测和数据优先排序
航天器的现场观测对于我们研究和了解整个近地空间及其他空间的质量、动量和能量耦合的各种现象至关重要。然而,在轨遥测制约因素会严重限制航天器传输高信度数据的能力,飞行任务通常只能全速遥测其捕获数据的一小部分。这就需要在计划中优先考虑最有可能实现飞行任务科学目标的时间间隔。磁层多尺度任务(MMS)等规模较大的任务旨在通过科学家在环(SITL)来解决这一问题,在该任务中,领域专家会标记具有潜在有趣数据的时间间隔,以便进行高信度数据下行和后续研究。虽然 SITL 解决方案适用于某些任务,但并不总是可行的,尤其是对于立方体卫星和纳米卫星等低成本任务。本手稿提出了一种可推广的方法,用于检测航天器观测数据中的异常数据点,从而在无需大量计算开销或地面额外基础设施的情况下快速确定数据优先级。具体来说,该方法利用主成分分析和单类支持向量机生成数据的替代表示,并为每个点提供数据的科学用途潜力指示。该技术的性能和通用性通过应用于观测间隔得到证明,包括来自 CASSIOPE e-POP/Swarm-Echo 和 MMS 任务的磁场数据和等离子体矩。
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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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