Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter

Abstract Observations from the Solar Orbiter spacecraft provide unique insights into the interaction between electron beams and the plasma background in the source regions of type III radio emissions. We analyze this interaction by examining the high-frequency electric and magnetic components of in situ wave measurements, focusing on their polarization properties. Using electron data from onboard instruments, we model the electron velocity distribution function and numerically solve the dispersion relation. We compare the predicted polarization of the electric and magnetic components with the observations. Our findings are consistent with propagation in the Langmuir/Z-mode at an oblique wavevector. We explain the magnetic component and transverse polarization by the presence of small density fluctuations, without the need for mode conversion.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-05-22
DOI
https://doi.org/10.3847/2041-8213/add687
Citations
2
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
2.31

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article

Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter

Ondřej Santolík, Arnaud Zaslavsky, Christopher John Owen, M. Maksimović et al.
2 citations
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Solar and Space Plasma Dynamics
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article

Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter

Ondřej Santolík, Arnaud Zaslavsky, Christopher John Owen, M. Maksimović, J. Souček, David Píša, Georgios Nicolaou, Tomáš Formánek, M. Kretzschmar
article en
2 citations

Abstract

Abstract Observations from the Solar Orbiter spacecraft provide unique insights into the interaction between electron beams and the plasma background in the source regions of type III radio emissions. We analyze this interaction by examining the high-frequency electric and magnetic components of in situ wave measurements, focusing on their polarization properties. Using electron data from onboard instruments, we model the electron velocity distribution function and numerically solve the dispersion relation. We compare the predicted polarization of the electric and magnetic components with the observations. Our findings are consistent with propagation in the Langmuir/Z-mode at an oblique wavevector. We explain the magnetic component and transverse polarization by the presence of small density fluctuations, without the need for mode conversion.

The Astrophysical Journal LettersVol. 985(2)
Université d'Orléans (FR), Centre National de la Recherche Scientifique (FR), Université Paris Cité (FR), Charles University (CZ), Observatoire de Paris (FR), Sorbonne Université (FR), Sorbonne Paris Cité (FR), Czech Academy of Sciences, Institute of Atmospheric Physics (CZ), University College London (GB)
National Aeronautics and Space Administration, UK Space Agency, Agence Nationale de la Recherche, Grantová Agentura České Republiky, Centre National d’Etudes Spatiales, Science and Technology Facilities Council
Openalex Percentile: Top 12%
Solar and Space Plasma Dynamics
2.31
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