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Miniature Dungey-like cycle at Mars
Journal article   Open access   Peer reviewed

Miniature Dungey-like cycle at Mars

Shaosui Xu, James P McFadden, David L Mitchell, Janet G Luhmann, Jasper S Halekas, Kathleen G Hanley, Christian X Mazelle, Jared R Espley and Shannon M Curry
Nature communications, Vol.17(1), 6129
07/23/2026
DOI: 10.1038/s41467-026-75019-3
PMID: 42493503
url
https://doi.org/10.1038/s41467-026-75019-3View
Published (Version of record) Open Access

Abstract

With its non-uniform distribution of crustal magnetic fields, Mars exhibits complex and highly variable auroral patterns related to both planetary rotation and solar wind conditions. Using in situ electron, ion, and magnetic field data from the Mars Atmospheric and Volatile EvolutioN (MAVEN) mission, we show that auroral processes associated with these small-scale crustal magnetic fields can be understood in terms of a miniature cycle of magnetic flux and plasma circulations that resemble a miniature version of what occurs at the Earth. However, at Earth, this Dungey cycle, named after its discoverer, operates in the presence of a global intrinsic dipole field with a strength approximately 100 times stronger and spatial scales roughly 20 times larger. From a universal perspective, the current finding adds an entry to the zoo of auroral concepts that enriches our understanding of the diversity of (exo)planetary plasma and our understanding of how planets interact with their space environments.

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