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Accelerated particle beams in a 3D simulation of the quiet Sun. Effects of advanced beam propagation modelling
L. Frogner, B. V. Gudiksen
Charged particles are constantly accelerated to non-thermal energies by the reconnecting magnetic field in the solar atmosphere. Our understanding of the interactions between the p…
Implementing accelerated particle beams in a 3D simulation of the quiet Sun
L. Frogner, B. V. Gudiksen
Context. The magnetic field in the solar atmosphere continually reconnects and accelerates charged particles to high energies. Simulations of the atmosphere in three dimensions tha…
Accelerated particle beams in a 3D simulation of the quiet Sun
L. Frogner, B. V. Gudiksen, H. Bakke
Observational and theoretical evidence suggest that beams of accelerated particles are produced in flaring events of all sizes in the solar atmosphere, from X-class flares to nanof…
Non-thermal electrons from solar nanoflares
Helle Bakke, Lars Frogner, Boris Vilhelm Gudiksen
Context. We introduce a model for including accelerated particles in pure magnetohydrodynamics (MHD) simulations of the solar atmosphere. Aims. We show that the method is viable an…