Kinetic‐Scale Turbulence in the Venusian Magnetosheath

Kinetic‐Scale Turbulence in the Venusian Magnetosheath

Abstract While not specifically designed as a planetary mission, NASA's Parker Solar Probe (PSP) mission uses a series of Venus gravity assists (VGAs) in order to reduce its perihelion distance. These orbital maneuvers provide the opportunity for direct measurements of the Venus plasma environm...

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Bibliographic Details
Main Authors: T. A. Bowen, S. D. Bale, R. Bandyopadhyay, J. W. Bonnell, A. Case, A. Chasapis, C. H. K. Chen, S. Curry, T. Dudok de Wit, K. Goetz, K. Goodrich, J. Gruesbeck, J. Halekas, P. R. Harvey, G. G. Howes, J. C. Kasper, K. Korreck, D. Larson, R. Livi, R. J. MacDowall, D. M. Malaspina, A. Mallet, M. D. McManus, B. Page, M. Pulupa, N. Raouafi, M. L. Stevens, P. Whittlesey
Format: Article
Language:English
Published: Wiley 2021-01-01
Series:Geophysical Research Letters
Subjects:
Instability
kinetic
plasma
PSP
turbulence
Venus
Online Access:https://doi.org/10.1029/2020GL090783
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