arXiv:2608.23458cs.LGastro-ph.IM2026-08

用影响函数实现光谱数据溯源,助力太空任务中的模型可信度评估

Traceable Spectral Inference via Influence Functions: Efficient Data Attribution and Error Proxies for the Ariel Mission

论文配图:Traceable Spectral Inference via Influence Functions: Efficient Data Attribution and Error Proxies for the Ariel Mission
图 1 · 摘自论文原文
  • 基于预测而非损失重构影响函数,无需标签即可部署
  • 利用极限学习机闭式解高效计算微小预测影响
  • 通过传播训练残差生成保守误差代理,适合科学级模型监控

在缺乏地面真值的科学太空任务中,可解释性至关重要。本文针对欧空局的Ariel任务,研究通过影响函数进行训练数据溯源,并提出三项关键贡献:首先,将影响重新定义为对预测的影响而非损失,实现无标签部署;其次,利用极限学习机的闭式岭解,高效计算微小预测影响;第三,通过传播训练残差至影响敏感度,推导出基于影响的保守误差代理。在模拟光谱上的评估表明,该代理与谱线尺度和形状误差高度相关。此外,影响函数可识别最具影响力的样本并近似最有害样本。这些结果表明,该方法可作为科学机器学习的运行框架。

原文摘要 · Abstract (English)

Interpretability is critical for machine learning models deployed in scientific space missions such as ESA's Ariel, where ground truth is unavailable during operations and physical plausibility must be assessed. While most explainable AI methods focus on feature attribution, this work investigates training data attribution through influence functions and introduces three key contributions for operational spectroscopy pipelines. First, influence is reformulated in terms of prediction rather than loss, enabling label-free deployment. Second, by leveraging the closed-form ridge solution of an Extreme Learning Machine, infinitesimal prediction influence is efficiently computed. Third, an influence-based conservative error proxy is derived by propagating training residuals through the influence sensitivities. Evaluated against simulated spectra, the proposed proxy correlates strongly with scale and shape-based spectral errors. Furthermore, influence functions enable the identification of the most influential samples and the approximation of the most harmful ones. Together, these results suggest that this approach can serve as an operational framework for scientific machine learning.

可解释性影响函数光谱分析航天任务

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