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: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Springer Science and Business Media B.V.
2022
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |