Polarization of Langmuir waves observed by RPW-TDS instrument on Solar Orbiter during Type III radio bursts - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2022

Polarization of Langmuir waves observed by RPW-TDS instrument on Solar Orbiter during Type III radio bursts

Résumé

We investigate the polarization of Langmuir waves observed by the Time Domain Sampler (TDS) module of the Radio and Plasma Waves instrument on Solar Orbiter during several extensive Type III burst events. During its two-year-long cruise phase, Solar orbiter often crossed the source region of the Type III radio emission and observed the Langmuir waves generated by solar energetic electrons. The waves are known to exhibit complex modulation and often non-trivial elliptical polarization which sometimes rapidly changes on the timescales of tens of milliseconds. We show that the observed waveforms are typically composed of multiple sub-packets with a relatively short coherence length. We investigate the correlation between the polarization of the waves, simultaneously observed energetic electrons beams and other plasma properties.
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Dates et versions

insu-04089914 , version 1 (05-05-2023)

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Jan Soucek, Sampath Bandara, David Pisa, Ondrej Santolik, Milan Maksimovic, et al.. Polarization of Langmuir waves observed by RPW-TDS instrument on Solar Orbiter during Type III radio bursts. EGU22, 2022, à renseigner, Unknown Region. ⟨10.5194/egusphere-egu22-3859⟩. ⟨insu-04089914⟩
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