Solar Orbiter in Venus' Ionosphere: Observations From the 4th Flyby

Abstract Solar Orbiter entered the topside ionosphere of Venus for the first time when performing its 4th flyby of the planet, reaching an altitude of 378 km on 18 Feb 2025. High‐cadence electron density measurements showed previously unresolved fine‐structuring within plasma regions and boundaries, particularly at the ionopause. During the rapid flyby, a rare snapshot of the entire induced magnetosphere was captured during calm solar wind conditions around solar maximum. A well‐structured and a relatively steady plasma environment was observed. Assuming an electron temperature of 0.5 eV, pressure balance was found across the ionopause, while at the same time quasi‐periodic density and magnetic field variations suggest boundary oscillations. Near closest approach, non‐force free magnetic flux ropes were observed. Small‐scale perturbations in both magnetic field strength and density across them indicate them being dynamically evolving, rather than in a stationary state.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2026-04-30
DOI
https://doi.org/10.1029/2025ja034813
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
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article

Solar Orbiter in Venus' Ionosphere: Observations From the 4th Flyby

Konstantin Kim, David Píša, M. Kretzschmar, Marina I. F. Galand et al.
Journal of Geophysical Research Space Physics
Planetary Science and Exploration
article

Solar Orbiter in Venus' Ionosphere: Observations From the 4th Flyby

Konstantin Kim, David Píša, M. Kretzschmar, Marina I. F. Galand, Jordi Boldu, Thomas Chust, David J. Andrews, Antonio Vecchio, Chris J. Owen, Moa Persson, Yuri V. Khotyaintsev, Jan Souček, Anders I. Eriksson, Niklas J. T. Edberg, Lina Z. Hadid, Lorenzo Matteini, Stuart D. Bale, Milan Maksimovic, Timothy S. Horbury
article en

Abstract

Abstract Solar Orbiter entered the topside ionosphere of Venus for the first time when performing its 4th flyby of the planet, reaching an altitude of 378 km on 18 Feb 2025. High‐cadence electron density measurements showed previously unresolved fine‐structuring within plasma regions and boundaries, particularly at the ionopause. During the rapid flyby, a rare snapshot of the entire induced magnetosphere was captured during calm solar wind conditions around solar maximum. A well‐structured and a relatively steady plasma environment was observed. Assuming an electron temperature of 0.5 eV, pressure balance was found across the ionopause, while at the same time quasi‐periodic density and magnetic field variations suggest boundary oscillations. Near closest approach, non‐force free magnetic flux ropes were observed. Small‐scale perturbations in both magnetic field strength and density across them indicate them being dynamically evolving, rather than in a stationary state.

Journal of Geophysical Research Space PhysicsVol. 131(5)
Uppsala University (SE), Université d'Orléans (FR), Centre National de la Recherche Scientifique (FR), Swedish Institute of Space Physics (SE), École Polytechnique (FR), Radboud University Nijmegen (NL), Université Paris Sciences et Lettres (FR), Sorbonne Université (FR), Czech Academy of Sciences, Institute of Atmospheric Physics (CZ), Laboratoire de Physique des Plasmas (FR), University College London (GB), Imperial College London (GB), University of California, Berkeley (US)
Openalex Percentile: Top 9%
Planetary Science and Exploration
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