The effects of density inhomogeneities on the radio wave emission in electron beam plasmas
Xin Yao, Patricio A. Mu\~noz, J\"org B\"uchner, Xiaowei Zhou, and Siming Liu

TL;DR
This study uses kinetic plasma simulations to explore how density inhomogeneities affect radio wave emissions from electron beams in plasmas, revealing increased Langmuir wave harmonics due to inhomogeneities.
Contribution
It introduces a detailed kinetic simulation approach to analyze the impact of density inhomogeneities on radio emissions in electron beam plasmas, highlighting new mechanisms for harmonic generation.
Findings
Density inhomogeneities increase the number of Langmuir wave harmonics.
Additional Langmuir wave harmonics are produced via coalescence processes.
Density inhomogeneities influence frequency shifts in electron resonances.
Abstract
Type III radio bursts are radio emissions associated with solar flares. They are considered to be caused by electron beams traveling from the solar corona to the solar wind. Magnetic reconnection is a possible accelerator of electron beams in the course of solar flares since it causes unstable distribution functions, and density inhomogeneities (cavities). The properties of radio emission by electron beams in an inhomogeneous environment are still poorly understood. We capture the non-linear kinetic plasma processes of generation of beam-related radio emissions in inhomogeneous plasmas by utilizing fully-kinetic Particle-In-Cell (PIC) code numerical simulations. Our model takes into account initial electron velocity distribution functions (EVDFs) as they are supposed to be created by magnetic reconnection. We focus our analysis on low-density regions with strong magnetic fields. The…
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