Science through Machine Learning: Quantification of Poststorm Thermospheric Cooling
Richard J. Licata, Piyush M. Mehta, Daniel R. Weimer, Douglas P. Drob,, W. Kent Tobiska, Jean Yoshii

TL;DR
This study employs machine learning models to analyze thermospheric density data, revealing post-storm cooling effects that traditional models fail to capture, with significant density reductions observed after geomagnetic storms.
Contribution
The paper demonstrates that machine learning models can identify post-storm cooling in thermospheric data, providing insights beyond traditional empirical models.
Findings
ML models reveal post-storm cooling not captured by traditional models
Density reductions of up to 40% occur 1-3 days after storms
ML models outperform traditional models in post-storm analysis
Abstract
Machine learning (ML) is often viewed as a black-box regression technique that is unable to provide considerable scientific insight. ML models are universal function approximators and - if used correctly - can provide scientific information related to the ground-truth dataset used for fitting. A benefit to ML over parametric models is that there are no predefined basis functions limiting the phenomena that can be modeled. In this work, we develop ML models on three datasets: the Space Environment Technologies (SET) High Accuracy Satellite Drag Model (HASDM) density database, a spatiotemporally matched dataset of outputs from the Jacchia-Bowman 2008 Empirical Thermospheric Density Model (JB2008), and an accelerometer-derived density dataset from CHAllenging Minisatellite Payload (CHAMP). These ML models are compared to the Naval Research Laboratory Mass Spectrometer and Incoherent…
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