Bridging the Gap Between the Earth's Ionosphere and Plasmasphere

Abstract Cold plasma distribution in the ionosphere‐plasmasphere system governs wave‐particle interactions, plasma energization and loss, and radio wave propagation. A longstanding observational gap at altitudes 800–8,000 km has largely prevented studying the coupled dynamics of the two regions. Here, we show that observations by JAXA's Arase mission can bridge this gap. Electron densities inferred from the upper hybrid resonance frequencies measured by Arase are highly consistent with radio occultation profiles from the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC) mission, with a median difference of 5%. Using the combined COSMIC‐Arase data set, we provide a convenient way to reconcile the two regions in empirical models based on the analytical Chapman function inversion for scale height. Our results enable studying fundamental questions about the ionosphere‐plasmasphere coupling, their transition, and life cycle of cold plasma in near‐Earth space.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-12-07
DOI
https://doi.org/10.1029/2025gl119267
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Bridging the Gap Between the Earth's Ionosphere and Plasmasphere

Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

Bridging the Gap Between the Earth's Ionosphere and Plasmasphere

article en

Abstract

Abstract Cold plasma distribution in the ionosphere‐plasmasphere system governs wave‐particle interactions, plasma energization and loss, and radio wave propagation. A longstanding observational gap at altitudes 800–8,000 km has largely prevented studying the coupled dynamics of the two regions. Here, we show that observations by JAXA's Arase mission can bridge this gap. Electron densities inferred from the upper hybrid resonance frequencies measured by Arase are highly consistent with radio occultation profiles from the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC) mission, with a median difference of 5%. Using the combined COSMIC‐Arase data set, we provide a convenient way to reconcile the two regions in empirical models based on the analytical Chapman function inversion for scale height. Our results enable studying fundamental questions about the ionosphere‐plasmasphere coupling, their transition, and life cycle of cold plasma in near‐Earth space.

Geophysical Research LettersVol. 52(23)
Kanazawa University (JP), NSF National Center for Atmospheric Research (US), NSF NCAR High Altitude Observatory (US), Southwest Research Institute (US), Planetary Science Institute (US), Goddard Space Flight Center (US), Sendai University (JP), Geological Survey of Finland (FI), University of California, Los Angeles (US), University of Potsdam (DE), Tohoku University (JP), University Corporation for Atmospheric Research (US), Istituto Nazionale di Geofisica e Vulcanologia (IT), Finnish Geospatial Research Institute (FI), GFZ Helmholtz Centre for Geosciences (DE), Nagoya University (JP), University of Maryland, College Park (US), University of Vaasa (FI), Ludwig-Maximilians-Universität München (DE)
National Science Foundation, National Aeronautics and Space Administration, Deutsche Forschungsgemeinschaft, Nuclear Safety and Security Commission
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Openalex Percentile: Top 38%
Ionosphere and magnetosphere dynamics
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