ORIGINAL RESEARCH article

Front. Astron. Space Sci.

Sec. Space Physics

Volume 12 - 2025 | doi: 10.3389/fspas.2025.1630911

This article is part of the Research TopicPredicting Near-Earth Space Environment: New Perspective and Capabilities in the AI AgeView all 3 articles

Predicting Cutoff L-shells of Solar Protons Using the GPPSn Particle Dataset

Provisionally accepted
Yue  ChenYue Chen1*Steven  MorleySteven Morley1Matthew  R CarverMatthew R Carver2Andrew  S HooverAndrew S Hoover1Cordell  J DelzerCordell J Delzer1Katherine  E GattikerKatherine E Gattiker1Elizabeth  C AudenElizabeth C Auden1
  • 1Los Alamos National Laboratory (DOE), Los Alamos, United States
  • 2Carver Scientific, Santa Fe, United States

The final, formatted version of the article will be published soon.

Solar energetic protons (SEPs) arriving at the Earth trigger severe radiation storms in the near-Earth space, directly impacting space missions operating at various altitudes. Therefore, monitoring SEP events and predicting the penetration depths of solar protons are critical for aerospace sectors. Building on previous efforts, here we demonstrate the feasibility of using proton measurements from the Global Prompt Proton Sensor network (GPPSn), enabled by Los Alamos National Laboratory developed combined X-ray dosimeters aboard GPS satellites, to characterize and predict the penetration of solar protons into the geomagnetic field. The inclined medium-Earth-orbits (MEOs) of the global GPS constellation offer a unique advantage of allowing simultaneous measurements of penetrating solar protons inside both open-and closed-field line regions. Therefore, the L-profiles of ~10s-100 MeV solar protons and their associated cutoff L-shells can be determined from the GPPSn dataset, using predefined threshold proton flux values rather than traditional flux ratios. After examining a list of SEP event intervals across solar cycles 23, 24 and 25-including the 2024 Mother's Day superstorm, we showcase how the latest GPPSn proton dataset (release v1.10), reprocessed and calibrated, can not only be used to monitor solar proton distributions inside the dynamic geomagnetic field for individual events, but also to derive a new empirical model linking cutoff L-shells with several key space weather parameters. This newly developed SEPCL-MEO model demonstrates high predictive performance; for example, predictions for >30 MeV solar protons yield a correlation coefficient of 0.85 and performance efficiency of 0.67 when validated against GPPSn observations. Results from this pilot study underscores the scientific and operational value of the GPPSn dataset, and this dataset-when paired with machine-learning techniques-can play a critical role in observing and predicting the effects of future incoming SEP events, including extreme ones.

Keywords: solar energetic protons, Predicting Cutoff L-shells, GPPSn Dataset, GPS CXD Particle Instrument, SEPCL-MEO Model

Received: 18 May 2025; Accepted: 15 Jul 2025.

Copyright: © 2025 Chen, Morley, Carver, Hoover, Delzer, Gattiker and Auden. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Yue Chen, Los Alamos National Laboratory (DOE), Los Alamos, United States

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