Implementing accelerated particle beams in a 3D simulation of the quiet Sun
L. Frogner, B. V. Gudiksen

TL;DR
This paper presents a novel parallel implementation of electron beam energy transport in a 3D solar atmosphere simulation, demonstrating efficient trajectory tracing and scalability challenges due to workload imbalance.
Contribution
It introduces a new numerical method for simulating energetic particle beams in 3D MHD models with parallel processing capabilities.
Findings
Efficient adaptive beam trajectory tracing with minimal communication overhead.
Parallel scalability is sublinear due to workload imbalance.
Validated implementation with analytical magnetic field lines.
Abstract
Context. The magnetic field in the solar atmosphere continually reconnects and accelerates charged particles to high energies. Simulations of the atmosphere in three dimensions that include the effects of accelerated particles can aid our understanding of the interplay between energetic particle beams and the environment where they emerge and propagate. We presented the first attempt at such a simulation in a previous paper, emphasising the physical model of particle beams. However, the numerical implementation of this model is not straightforward due to the diverse conditions in the atmosphere and the way we must distribute computation between multiple CPU cores. Aims. Here, we describe and verify our numerical implementation of energy transport by electron beams in a 3D magnetohydrodynamics code parallelised by domain decomposition. Methods. We trace beam trajectories using a…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Meteorological Phenomena and Simulations
