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 language | English |
|---|---|
| Pages (from-to) | 609-623 |
| Number of pages | 15 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 536 |
| Issue number | 1 |
| Early online date | 3 Dec 2024 |
| DOIs | |
| Publication status | Published - 1 Jan 2025 |
Keywords
- Acceleration of particles
- Magnetic fields
- Sun: activity
- Sun: flares
- Sun: X-rays, gamma rays
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A detailed investigation of particle energisation mechanisms in models of collapsing magnetic traps (dataset)
Mowbray, K. (Creator), Neukirch, T. (Contributor) & Threlfall, J. (Contributor), University of St Andrews, 11 Dec 2024
DOI: 10.17630/dd7f39b7-d519-46bd-a6c2-f6dd2090a45f
Dataset