Empirical Parametric Model for Venus Plasma Boundaries Based on Venus Express Data

Venus’s induced magnetosphere is characterized by regions with different plasma and magnetic field properties, which are separated by plasma boundaries. These boundaries’ locations and shapes vary with upstream solar wind conditions, and these variations have been characterized by several previous s...

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Bibliographic Details
Main Authors: Umberto Rollero, Sebastián Rojas Mata, Tielong Zhang, Moa Persson, Sofia Bergman, Yoshifumi Futaana
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/add14d
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