Comparative Analysis of Ion and Electron Contributions to Ionospheric Ionization at Auroral and Subauroral Latitudes

Abstract Electron and proton precipitation into the nightside ionosphere is a key process in magnetosphere–ionosphere coupling. Although auroral electron precipitation at –10 keV is traditionally considered the main driver of auroral emissions, recent studies show that keV electrons and protons can significantly contribute to ionospheric energy deposition, especially during storms. While energetic electron precipitation has been studied extensively, the role of energetic proton precipitation remains poorly quantified. Here, we use coordinated ELFIN and DMSP nightside observations during two substorm events, resolving electron and proton precipitation spectra from eV to ∼MeV. We show that keV proton precipitation, consistent with curvature scattering, can have an impact on E‐region ionization comparable to that of energetic electrons. These analyses are further supported by magnetospheric observations from the Arase and THEMIS spacecraft and ground‐based incoherent scatter radar measurements from PFISR.

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Publication Details

Journal
Geophysical Research Letters
Published
2026-08-18
DOI
https://doi.org/10.1029/2026gl123777
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
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article

Comparative Analysis of Ion and Electron Contributions to Ionospheric Ionization at Auroral and Subauroral Latitudes

Yoshiya Kasahara, Shoya Matsuda, Iku Shinohara, Kazuhiro Yamamoto et al.
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

Comparative Analysis of Ion and Electron Contributions to Ionospheric Ionization at Auroral and Subauroral Latitudes

Yoshiya Kasahara, Shoya Matsuda, Iku Shinohara, Kazuhiro Yamamoto, Jun Liang, S. R. Kamaletdinov, Xiao‐Jia Zhang, Y. Nishimura, Shoichiro Yokota, Yangyang Shen, M. Teramoto, Anton Artemyev, Kazushi Asamura, K. Keika, Atsushi Kumamoto, Tomoaki Hori, Ayako Matsuoka, V. Angelopoulos, Asti Bhatt, Satoshi Kasahara, Yoshizumi Miyoshi, Atsuki Shinbori, F. Tsuchiya
article en

Abstract

Abstract Electron and proton precipitation into the nightside ionosphere is a key process in magnetosphere–ionosphere coupling. Although auroral electron precipitation at –10 keV is traditionally considered the main driver of auroral emissions, recent studies show that keV electrons and protons can significantly contribute to ionospheric energy deposition, especially during storms. While energetic electron precipitation has been studied extensively, the role of energetic proton precipitation remains poorly quantified. Here, we use coordinated ELFIN and DMSP nightside observations during two substorm events, resolving electron and proton precipitation spectra from eV to ∼MeV. We show that keV proton precipitation, consistent with curvature scattering, can have an impact on E‐region ionization comparable to that of energetic electrons. These analyses are further supported by magnetospheric observations from the Arase and THEMIS spacecraft and ground‐based incoherent scatter radar measurements from PFISR.

Geophysical Research LettersVol. 53(16)
Kanazawa University (JP), SRI International (US), Planetary Science Institute (US), Osaka University of Economics (JP), University of Alberta (CA), University of California, Los Angeles (US), The University of Texas at Dallas (US), University of Calgary (CA), The University of Texas at Arlington (US), Tohoku University (JP), Kyushu Institute of Technology (JP), Kyoto University (JP), Japan Aerospace Exploration Agency (JP), Osaka City University (JP), Institute of Space and Astronautical Science (JP), Astronomy and Space (AU), Nagoya University (JP), The University of Tokyo (JP), The University of Osaka (JP)
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Ionosphere and magnetosphere dynamics
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