An alternative to the plasma emission model: Particle-In-Cell, self-consistent electromagnetic wave emission simulations of solar type III radio bursts
D. Tsiklauri (Queen Mary University of London)

TL;DR
This study uses 1.5D Particle-In-Cell simulations to model electromagnetic wave emission in solar type III radio bursts, offering an alternative to classical plasma emission models by demonstrating wave generation from oblique electron beams.
Contribution
It presents the first fully kinetic simulation of type III radio bursts using a non-gyrotropic electron beam, providing new insights into wave generation mechanisms.
Findings
Oblique electron beams generate EM waves consistent with type III bursts.
Wave frequency drops as the beam moves into lower density regions.
Electrostatic standing waves are excited at plasma frequency.
Abstract
1.5D PIC, relativistic, fully electromagnetic (EM) simulations are used to model EM wave emission generation in the context of solar type III radio bursts. The model studies generation of EM waves by a super-thermal, hot beam of electrons injected into a plasma thread that contains uniform longitudinal magnetic field and a parabolic density gradient. In effect, a single magnetic line connecting Sun to earth is considered, for which several cases are studied. (i) We find that the physical system without a beam is stable and only low amplitude level EM drift waves (noise) are excited. (ii) The beam injection direction is controlled by setting either longitudinal or oblique electron initial drift speed, i.e. by setting the beam pitch angle. In the case of zero pitch angle, the beam excites only electrostatic, standing waves, oscillating at plasma frequency, in the beam injection spatial…
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