Bridging the Gap Between the Earth's Ionosphere and Plasmasphere

dc.contributor.authorSmirnov, Artem
dc.contributor.authorShprits, Yuri
dc.contributor.authorLuhr, Hermann
dc.contributor.authorKronberg, Elena A.
dc.contributor.authorGoldstein, Jerry
dc.contributor.authorMiyoshi, Yoshizumi
dc.contributor.authorProl, Fabricio
dc.contributor.authorPignalberi, Alessio
dc.contributor.authorBuzulukova, Natalia
dc.contributor.authorPedatella, Nicholas
dc.contributor.authorHaas, Bernhard
dc.contributor.authorWang, Dedong
dc.contributor.authorKasahara, Yoshiya
dc.contributor.authorTsuchiya, Fuminori
dc.contributor.authorMatsuda, Shoya
dc.contributor.authorShinbori, Atsuki
dc.contributor.authorMatsuoka, Ayako
dc.date.accessioned2026-01-21T07:52:00Z
dc.date.issued2025
dc.description.abstractCold 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.en
dc.description.notification© 2025. The Author(s). This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
dc.description.reviewstatusfi=vertaisarvioitu|en=peerReviewed|
dc.identifier.urihttps://osuva.uwasa.fi/handle/11111/19670
dc.identifier.urnURN:NBN:fi-fe202601215310
dc.language.isoen
dc.publisherJohn Wiley & Sons
dc.relation.doihttps://doi.org/10.1029/2025GL119267
dc.relation.funderSuomen Akatemiafi
dc.relation.funderAcademy of Finlanden
dc.relation.grantnumber362096
dc.relation.ispartofjournalGeophysical research letters
dc.relation.issn1944-8007
dc.relation.issn0094-8276
dc.relation.issue23
dc.relation.urlhttps://doi.org/10.1029/2025GL119267
dc.relation.urlhttps://urn.fi/URN:NBN:fi-fe202601215310
dc.relation.volume52
dc.rightshttps://creativecommons.org/licenses/by/4.0/
dc.source.identifierWOS:001633018300001
dc.source.identifier2-s2.0-105024061673
dc.source.identifier48f04ccf-37ea-4d52-985a-a038411004e6
dc.source.metadataSoleCRIS
dc.subjectionosphere
dc.subjectplasmasphere
dc.subjectUHR frequency
dc.subjectradio occultation
dc.subjectGNSS
dc.subjectplasma density
dc.subject.disciplinefi=Tietotekniikka tekn|en=Information Technology tech|
dc.titleBridging the Gap Between the Earth's Ionosphere and Plasmasphere
dc.type.okmfi=A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä (vertaisarvioitu)|en=A1 Journal article (peer-reviewed)|
dc.type.publicationarticle
dc.type.versionpublishedVersion

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