Application of a Modified Spheromak Model to Simulations of Coronal Mass Ejection in the Inner Heliosphere

Application of a Modified Spheromak Model to Simulations of Coronal Mass Ejection in the Inner Heliosphere

Abstract The magnetic fields of interplanetary coronal mass ejections (ICMEs), which originate close to the Sun in the form of a flux rope, determine their geoeffectiveness. Therefore, robust flux rope‐based models of CMEs are required to perform magnetohydrodynamic (MHD) simulations aimed at space...

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Bibliographic Details
Main Authors: Talwinder Singh, Tae K. Kim, Nikolai V. Pogorelov, Charles N. Arge
Format: Article
Language:English
Published: Wiley 2020-05-01
Series:Space Weather
Subjects:
MHD
coronal mass ejections
solar wind
space weather
prediction
flux ropes
Online Access:https://doi.org/10.1029/2019SW002405
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https://doi.org/10.1029/2019SW002405

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