A detailed investigation of particle energisation mechanisms in models of collapsing magnetic traps

Kate Mowbray*, Thomas Neukirch, James Threlfall

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

In this paper, we provide a detailed investigation of the energization processes in two-dimensional, two and a half-dimensional, and three-dimensional collapsing magnetic trap models. Using kinematic magnetohydrodynamic models of collapsing magnetic traps, we examine the importance of Fermi acceleration in comparison with betatron acceleration in these models. We extend previous work by investigating particle orbits in two-dimensional models without and with a guide field component and from full three-dimensional models. We compare the outcomes for the different models and how they depend on the chosen initial conditions. While in the literature betatron acceleration has been emphasized as the major mechanism for particle energization in collapsing magnetic traps, we find that Fermi acceleration can play a significant role as well for particle orbits with suitable initial conditions.
Original languageEnglish
Article numberstae2668
Pages (from-to)609-623
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume536
Issue number1
Early online date9 Dec 2024
DOIs
Publication statusPublished - 1 Jan 2025

Keywords

  • Acceleration of particles
  • Magnetic fields
  • Sun: activity
  • Sun: flares
  • Sun: X-rays
  • Gamma rays

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