Frontiers in Astronomy and Space Sciences (Mar 2023)

Redefining flux ropes in heliophysics

  • Teresa Nieves-Chinchilla,
  • Sanchita Pal,
  • Sanchita Pal,
  • Tarik M. Salman,
  • Tarik M. Salman,
  • Fernando Carcaboso,
  • Fernando Carcaboso,
  • Silvina E. Guidoni,
  • Silvina E. Guidoni,
  • Hebe Cremades,
  • Ayris Narock,
  • Ayris Narock,
  • Laura A. Balmaceda,
  • Laura A. Balmaceda,
  • Benjamin J. Lynch,
  • Nada Al-Haddad,
  • Laura Rodríguez-García,
  • Thomas W. Narock,
  • Luiz F. G. Dos Santos,
  • Florian Regnault,
  • Christina Kay,
  • Christina Kay,
  • Réka M. Winslow,
  • Erika Palmerio,
  • Emma E. Davies,
  • Camilla Scolini,
  • Andreas J. Weiss,
  • Nathalia Alzate,
  • Nathalia Alzate,
  • Mariana Jeunon,
  • Mariana Jeunon,
  • Roger Pujadas,
  • Roger Pujadas

DOI
https://doi.org/10.3389/fspas.2023.1114838
Journal volume & issue
Vol. 10

Abstract

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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 our understanding of the fundamental physics of heliospheric flux ropes and provides the motivation to significantly improve the status quo of flux rope research through 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.

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