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Detection of Zwan-Wolf effect in the ionosphere of Mars
Journal article   Open access   Peer reviewed

Detection of Zwan-Wolf effect in the ionosphere of Mars

Christopher M. Fowler, Kathleen G. Hanley, James McFadden, David Mitchell, Jasper Halekas, Laila Andersson, Duncan Bark, Yingjuan Ma, Christopher Chaston, Beatriz Sanchez-Cano, …
Nature communications, Vol.17(1), 4224
05/18/2026
DOI: 10.1038/s41467-026-72251-9
PMCID: PMC13184130
PMID: 42151130
url
https://doi.org/10.1038/s41467-026-72251-9View
Published (Version of record) Open Access

Abstract

At planets that possess strong dipole magnetic fields, the Zwan-Wolf effect acts to squeeze plasma along magnetic flux tubes, aiding in the deflection of the solar wind flow about the planet. While the effect has been most studied at Earth, candidate observations have also been made at the outer planets. Here we present observations of the Zwan-Wolf effect occurring at Mars, an unmagnetized planet that lacks a dipole magnetic field. Our analysis of observations made by NASA’s Mars Atmosphere and Volatile EvolutioN spacecraft suggest that while the Zwan-Wolf effect is likely continuously active within the Martian ionosphere, it operates below detection thresholds of typical plasma analyzers most of the time. However, an interplanetary coronal mass ejection impact at Mars in December 2023 greatly enhanced the Zwan-Wolf effect within the ionosphere, allowing it to be observed, and highlighting the importance of space weather events for these unmagnetized planetary systems. At planets that possess strong dipole magnetic fields, charged particles can be squeezed along magnetic fields helping to deflect the solar wind flow about the planet. Here, the authors show this effect occurring in the ionosphere of Mars, a planet without a strong dipole magnetic field.
639/33/445/823 639/33/445/845 639/33/525/869 Article Humanities and Social Sciences multidisciplinary Science Science (multidisciplinary)

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