Small-scale inhomogeneity effects on coherent solar radio emission
Xiaowei Zhou, Patricio Munoz, Jan Benacek, Lijie Zhang, Dejin Wu, Ling, Chen, Zongjun Ning, Joerg Buechner

TL;DR
This study uses 2.5D PIC simulations to explore how plasma inhomogeneities in the solar corona affect the properties of coherent radio emissions, revealing impacts on wave spectra and potential diagnostic applications.
Contribution
It introduces the first detailed simulation analysis of inhomogeneity effects on solar radio burst emission mechanisms, focusing on magnetic field, density, and temperature variations.
Findings
Inhomogeneities influence the frequency bandwidth of emitted waves.
Density and temperature variations affect the spectral location of emissions.
The results aid in diagnosing plasma conditions at emission sites.
Abstract
Coherent radio emission mechanism of solar radio bursts is one of the most complicated and controversial topics in solar physics. To clarify the mechanism(s) of different types of solar radio bursts, (radio) wave excitation by energetic electrons in homogeneous plasmas has been widely studied via particle-in-cell (PIC) code numerical simulations. The solar corona is, however, inhomogeneous over almost all spatial scales. Inhomogeneities of the plasma could influence the emission properties of solar radio bursts. In this paper, we, hence, investigate effects of inhomogeneity (in the magnetic field, plasma density and temperature) of plasmas in the solar corona on radio wave emission by ring-beam distributed energetic electrons utilizing 2.5-dimensional PIC simulations. Both the beam and electron cyclotron maser (ECM) instabilities could be triggered with the presence of the energetic…
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Taxonomy
TopicsPhotovoltaic System Optimization Techniques · Radio Astronomy Observations and Technology · Solar and Space Plasma Dynamics
