MHD Modeling of the Background Solar Wind in the Inner Heliosphere From 0.1 to 5.5 AU: Comparison With In Situ Observations

MHD Modeling of the Background Solar Wind in the Inner Heliosphere From 0.1 to 5.5 AU: Comparison With In Situ Observations

Abstract The accurate prediction of solar wind conditions in the interplanetary space is crucial in the context of both scientific research and technical applications. In this study, we simulate the solar wind throughout the heliosphere from 0.1 to 5.5 astronomical units (AU) with our improved helio...

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Bibliographic Details
Main Authors: Y. X. Wang, X. C. Guo, C. Wang, V. Florinski, F. Shen, H. Li, M. Blanc
Format: Article
Language:English
Published: Wiley 2020-06-01
Series:Space Weather
Subjects:
magnetohydrodynamics (MHD)
solar wind
Sun
heliosphere
Juno
Jupiter
Online Access:https://doi.org/10.1029/2019SW002262
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https://doi.org/10.1029/2019SW002262

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