Electron cyclotron maser emission mode coupling to the z-mode on a longitudinal density gradient in the context of solar type III bursts
Roman Pechhacker, David Tsiklauri

TL;DR
This study uses particle-in-cell simulations to explore how electron cyclotron maser emission couples to the z-mode on a density gradient, providing insights into solar type III bursts and related phenomena.
Contribution
It demonstrates that the electron cyclotron maser can couple to the z-mode on a density gradient, enabling wave propagation at plasma frequencies in a plasma with a beam of hot electrons.
Findings
Emission is generated by the perpendicular component of the beam.
Wave pulsations occur at twice the relativistic cyclotron frequency.
Wave coupling allows propagation at plasma frequencies.
Abstract
A beam of super-thermal, hot electrons was injected into maxwellian plasma with a density gradient along a magnetic field line. 1.5D particle-in-cell simulations were carried out which established that the EM emission is produced by the perpendicular component of the beam injection momentum. The beam has a positive slope in the distribution function in perpendicular momentum phase space, which is the characteristic feature of a cyclotron maser. The cyclotron maser in the overdense plasma generates emission at the electron cyclotron frequency. The frequencies of generated waves were too low to propagate away from the injection region, hence the wavelet transform shows a pulsating wave generation and decay process. The intensity pulsation frequency is twice the relativistic cyclotron frequency. Eventually, a stable wave packet formed and could mode couple on the density gradient to reach…
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