Loading…

Redefining Flux Ropes in Heliophysics

Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance on the fundamental understanding of heliospheric flux ropes and provides the motivation to significantly improve the sta...

Full description

Saved in:
Bibliographic Details
Published in:Frontiers in astronomy and space sciences 2023-03, Vol.10
Main Authors: Nieves-Chinchilla, Teresa, Pal, Sanchita, Salman, Tarik M, Guidoni, Silvina E, Narock, Ayris, Balmaceda, Laura A, Lynch, Benjamin J, Al-Haddad, Nada, Rodriguez-Garcia, Laura, Narock, Thomas W, Santos, Luiz F G dos, Regnault, Florian, Kay, Christina, Winslow, Reka M, Palmerio, Erika, Davies, Emma E, Scolini, Camilla, Weiss, Andreas J, Alzate, Nathalia, Juenon, Mariana, Pujadas, Roger
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance on the fundamental understanding of heliospheric flux ropes and provides the motivation to significantly improve the status quo of flux rope research through the novel and requisite approaches. It briefly discusses the current understanding of flux rope formation and evolution, and summarizes the strategies that have been undertaken to understand the dynamics of heliospheric structures. The challenges and recommendations put forward to address them are expected to broaden the in-depth knowledge of our nearest star, its dynamics, and its role in its region of influence, the heliosphere.
ISSN:2296-987X
2296-987X
DOI:10.3389/fspas.2023.1114838