Harmonic Radio Emission in Randomly Inhomogeneous Plasma

نویسندگان

چکیده

Abstract In the present paper, we describe a theoretical model of generation harmonic emissions type III solar radio bursts. The goal our study is to fully take into account most efficient physical processes involved in electromagnetic emission via nonlinear coupling Langmuir waves randomly inhomogeneous plasma wind ( ). We revisit conventional mechanism coalescence primarily generated and back-scattered quasihomogeneous plasma. Additionally, propose investigate another that generates only strongly plasma: incident reflected inside localized regions with enhanced density (clumps), close vicinity reflection point. Both mechanisms imply presence strong fluctuations use results probabilistic beam–plasma interaction evaluate efficiency energy transfer from emission. infer are significantly more intense than found previous studies. wave conversion expected be higher at large heliospheric distances for operating small heliocentric one evaluation intensity may also applied II radiation pattern both cases quadrupolar, show clumps efficiently contribute visibility

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2021

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/abd2bd