On Modeling ICME Cross-Sections as Static MHD Columns
Solar coronal mass ejections are well-known to expand as they propagate through the heliosphere. Despite this, their cross-sections are usually modeled as static plasma columns within the magnetohydrodynamics (MHD) framework. We test the validity of this approach using in-situ plasma data from 151 m...
Main Authors: | Bhattacharjee, D. (Author), Bothmer, V. (Author), Nieves-Chinchilla, T. (Author), Subramanian, P. (Author), Vourlidas, A. (Author) |
---|---|
Format: | Article |
Language: | English |
Published: |
Springer Science and Business Media B.V.
2022
|
Subjects: | |
Online Access: | View Fulltext in Publisher |
Similar Items
-
Microwave radio emissions as a proxy for coronal mass ejection speed in arrival predictions of interplanetary coronal mass ejections at 1 AU
by: Matamoros Carolina Salas, et al.
Published: (2017-01-01) -
Three-dimensional MHD simulation of the 2008 December 12 coronal mass ejection: from the Sun to Interplanetary space
by: Zhang Man, et al.
Published: (2019-01-01) -
Editorial: Magnetic Flux Ropes: From the Sun to the Earth and Beyond
by: Rui Liu, et al.
Published: (2020-11-01) -
Radial Speed Evolution of Interplanetary Coronal Mass Ejections During Solar Cycle 23
by: Fujiki, K., et al.
Published: (2013) -
Analysis of Deformation and Erosion during CME Evolution
by: Skralan Hosteaux, et al.
Published: (2021-07-01)