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2021 |
Understanding how coronal structure propagates and evolves from the Sun and into the heliosphere has been thoroughly explored using sophisticated MHD models. From these, we have a reasonably good working understanding of the dynamical processes that shape the formation and evolution of stream interaction regions and rarefactions, including their locations, orientations, and structure. However, given the technical expertise required to produce, maintain, and run global MHD models, their use has been relatively restricted. In ... Published by: Frontiers in Physics Published on: may YEAR: 2021   DOI: 10.3389/fphy.2021.679497 Heliosphere (711); Solar wind streams; coronal mass ejection; Magnetohydrodynamics; space weather |
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