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

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...

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Main Authors: Tomáš Formánek, Ondřej Santolík, Jan Souček, David Píša, Arnaud Zaslavsky, Matthieu Kretzschmar, Milan Maksimovic, Christopher J. Owen, Georgios Nicolaou
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/add687
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author Tomáš Formánek
Ondřej Santolík
Jan Souček
David Píša
Arnaud Zaslavsky
Matthieu Kretzschmar
Milan Maksimovic
Christopher J. Owen
Georgios Nicolaou
author_facet Tomáš Formánek
Ondřej Santolík
Jan Souček
David Píša
Arnaud Zaslavsky
Matthieu Kretzschmar
Milan Maksimovic
Christopher J. Owen
Georgios Nicolaou
author_sort Tomáš Formánek
collection DOAJ
description 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.
format Article
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institution Kabale University
issn 2041-8205
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publishDate 2025-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal Letters
spelling doaj-art-4b63ca9e51b7465db8f95d332d1cd1c92025-08-20T03:53:51ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019852L2910.3847/2041-8213/add687Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar OrbiterTomáš Formánek0https://orcid.org/0000-0003-4766-638XOndřej Santolík1https://orcid.org/0000-0002-4891-9273Jan Souček2https://orcid.org/0000-0003-0462-6804David Píša3https://orcid.org/0000-0002-1322-7576Arnaud Zaslavsky4https://orcid.org/0000-0001-8543-9431Matthieu Kretzschmar5https://orcid.org/0000-0001-5796-6138Milan Maksimovic6https://orcid.org/0000-0001-6172-5062Christopher J. Owen7https://orcid.org/0000-0002-5982-4667Georgios Nicolaou8https://orcid.org/0000-0003-3623-4928Czech Academy of Sciences, Institute of Atmospheric Physics , Department of Space Physics, Boční II 1401, Prague 4, Czechia ; tomas.formanek@obspm.fr; LIRA, Observatoire de Paris, Université PSL , CNRS, Sorbonne Université, Université Paris-Cité, Meudon, FranceCzech Academy of Sciences, Institute of Atmospheric Physics , Department of Space Physics, Boční II 1401, Prague 4, Czechia ; tomas.formanek@obspm.fr; Charles University , Faculty of Mathematics and Physics, V Holesovickach 2, 18000 Prague 8, CzechiaCzech Academy of Sciences, Institute of Atmospheric Physics , Department of Space Physics, Boční II 1401, Prague 4, Czechia ; tomas.formanek@obspm.frCzech Academy of Sciences, Institute of Atmospheric Physics , Department of Space Physics, Boční II 1401, Prague 4, Czechia ; tomas.formanek@obspm.frLIRA, Observatoire de Paris, Université PSL , CNRS, Sorbonne Université, Université Paris-Cité, Meudon, FranceLPC2E, OSUC, CNRS/University of Orléans/CNES , 3A avenue de la Recherche Scientifique, 45071 Orléans, FranceLIRA, Observatoire de Paris, Université PSL , CNRS, Sorbonne Université, Université Paris-Cité, Meudon, FranceMullard Space Science Laboratory, University College London , Holmbury St Mary, Dorking, Surrey RH5 6NT, UKMullard Space Science Laboratory, University College London , Holmbury St Mary, Dorking, Surrey RH5 6NT, UKObservations 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.https://doi.org/10.3847/2041-8213/add687Solar radio emissionSolar windSpace plasmasPlasma physics
spellingShingle Tomáš Formánek
Ondřej Santolík
Jan Souček
David Píša
Arnaud Zaslavsky
Matthieu Kretzschmar
Milan Maksimovic
Christopher J. Owen
Georgios Nicolaou
Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
The Astrophysical Journal Letters
Solar radio emission
Solar wind
Space plasmas
Plasma physics
title Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
title_full Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
title_fullStr Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
title_full_unstemmed Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
title_short Polarization Analysis of Type III Langmuir/Z-mode Waves with Coherent Magnetic Component Observations by Solar Orbiter
title_sort polarization analysis of type iii langmuir z mode waves with coherent magnetic component observations by solar orbiter
topic Solar radio emission
Solar wind
Space plasmas
Plasma physics
url https://doi.org/10.3847/2041-8213/add687
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