Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?
Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the joint observations performed by Parker Solar Probe and the Metis coronagraph on board Solar Orbiter, local measurem...
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2023-01-01
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Online Access: | https://doi.org/10.3847/1538-4357/acb693 |
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author | Daniele Telloni Gary P. Zank Laxman Adhikari Lingling Zhao Roberto Susino Ester Antonucci Silvano Fineschi Marco Stangalini Catia Grimani Luca Sorriso-Valvo Daniel Verscharen Raffaele Marino Silvio Giordano Raffaella D’Amicis Denise Perrone Francesco Carbone Alessandro Liberatore Roberto Bruno Gaetano Zimbardo Marco Romoli Vincenzo Andretta Vania Da Deppo Petr Heinzel John D. Moses Giampiero Naletto Gianalfredo Nicolini Daniele Spadaro Luca Teriaca Aleksandr Burtovoi Yara De Leo Giovanna Jerse Federico Landini Maurizio Pancrazzi Clementina Sasso Alessandra Slemer |
author_facet | Daniele Telloni Gary P. Zank Laxman Adhikari Lingling Zhao Roberto Susino Ester Antonucci Silvano Fineschi Marco Stangalini Catia Grimani Luca Sorriso-Valvo Daniel Verscharen Raffaele Marino Silvio Giordano Raffaella D’Amicis Denise Perrone Francesco Carbone Alessandro Liberatore Roberto Bruno Gaetano Zimbardo Marco Romoli Vincenzo Andretta Vania Da Deppo Petr Heinzel John D. Moses Giampiero Naletto Gianalfredo Nicolini Daniele Spadaro Luca Teriaca Aleksandr Burtovoi Yara De Leo Giovanna Jerse Federico Landini Maurizio Pancrazzi Clementina Sasso Alessandra Slemer |
author_sort | Daniele Telloni |
collection | DOAJ |
description | Evidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the joint observations performed by Parker Solar Probe and the Metis coronagraph on board Solar Orbiter, local measurements of the solar wind can be linked with the large-scale structures of the solar corona. The results suggest that the dynamics of the current sheet layers generates turbulence, which in turn creates a sufficiently strong temperature anisotropy to make the solar-wind plasma unstable to anisotropy-driven instabilities such as the Alfvén ion cyclotron, mirror-mode, and firehose instabilities. The study of the polarization state of high-frequency magnetic fluctuations reveals that ICWs are indeed present along the current sheet, thus linking the magnetic topology of the remotely imaged coronal source regions with the wave bursts observed in situ. The present results may allow improvement of state-of-the-art models based on the ion cyclotron mechanism, providing new insights into the processes involved in coronal heating. |
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institution | Directory Open Access Journal |
issn | 1538-4357 |
language | English |
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spelling | doaj.art-a0e6bdc5e34e43b8964493e77cd5287d2023-09-03T14:08:31ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-01944222710.3847/1538-4357/acb693Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?Daniele Telloni0https://orcid.org/0000-0002-6710-8142Gary P. Zank1https://orcid.org/0000-0002-4642-6192Laxman Adhikari2https://orcid.org/0000-0003-1549-5256Lingling Zhao3https://orcid.org/0000-0002-4299-0490Roberto Susino4https://orcid.org/0000-0002-1017-7163Ester Antonucci5https://orcid.org/0000-0003-4155-6542Silvano Fineschi6https://orcid.org/0000-0002-2789-816XMarco Stangalini7https://orcid.org/0000-0002-5365-7546Catia Grimani8https://orcid.org/0000-0002-5467-6386Luca Sorriso-Valvo9https://orcid.org/0000-0002-5981-7758Daniel Verscharen10https://orcid.org/0000-0002-0497-1096Raffaele Marino11https://orcid.org/0000-0002-6433-7767Silvio Giordano12https://orcid.org/0000-0002-3468-8566Raffaella D’Amicis13https://orcid.org/0000-0003-2647-117XDenise Perrone14https://orcid.org/0000-0003-1059-4853Francesco Carbone15https://orcid.org/0000-0002-3559-5273Alessandro Liberatore16https://orcid.org/0000-0002-0016-7594Roberto Bruno17https://orcid.org/0000-0002-2152-0115Gaetano Zimbardo18https://orcid.org/0000-0002-9207-2647Marco Romoli19https://orcid.org/0000-0001-9921-1198Vincenzo Andretta20https://orcid.org/0000-0003-1962-9741Vania Da Deppo21https://orcid.org/0000-0001-6273-8738Petr Heinzel22https://orcid.org/0000-0002-5778-2600John D. Moses23https://orcid.org/0000-0001-9670-2063Giampiero Naletto24https://orcid.org/0000-0003-2007-3138Gianalfredo Nicolini25https://orcid.org/0000-0002-9459-3841Daniele Spadaro26https://orcid.org/0000-0003-3517-8688Luca Teriaca27https://orcid.org/0000-0001-7298-2320Aleksandr Burtovoi28https://orcid.org/0000-0002-8734-808XYara De Leo29https://orcid.org/0000-0003-2426-2112Giovanna Jerse30https://orcid.org/0000-0002-0764-7929Federico Landini31https://orcid.org/0000-0001-8244-9749Maurizio Pancrazzi32https://orcid.org/0000-0002-3789-2482Clementina Sasso33https://orcid.org/0000-0002-5163-5837Alessandra Slemer34https://orcid.org/0000-0001-7762-280XNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itCenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville , Huntsville, AL 35805, USA; Department of Space Science, University of Alabama in Huntsville , Huntsville, AL 35805, USACenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville , Huntsville, AL 35805, USACenter for Space Plasma and Aeronomic Research, University of Alabama in Huntsville , Huntsville, AL 35805, USANational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itItalian Space Agency , Via del Politecnico snc, I-00133 Roma, ItalyUniversity of Urbino Carlo Bo , Department of Pure and Applied Sciences, Via Santa Chiara 27, I-61029 Urbino, Italy; National Institute for Nuclear Physics , Section in Florence, Via Bruno Rossi 1, I-50019 Sesto Fiorentino, ItalyNational Research Council, Institute for the Science and Technology of Plasmas , Via Amendola 122/D, I-70126 Bari, Italy; Swedish Institute of Space Physics , Ångström Laboratory, Lägerhyddsvägen 1, SE-751 21 Uppsala, SwedenMullard Space Science Laboratory, University College London , Holmbury St. Mary, RH5 6NT Dorking, UKUniversité de Lyon, Centre National de la Recherche Scientifique, École Centrale de Lyon, Institut National des Sciences Appliquées de Lyon , Université Claude Bernard Lyon 1, Laboratoire de Mécanique des Fluides et d’Acoustique, F-69134 Écully, FranceNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics, Institute for Space Astrophysics and Planetology , Via del Fosso del Cavaliere 100, I-00133 Roma, ItalyItalian Space Agency , Via del Politecnico snc, I-00133 Roma, ItalyNational Research Council, Institute of Atmospheric Pollution Research , c/o University of Calabria, I-87036 Rende, ItalyJet Propulsion Laboratory, California Institute of Technology , Pasadena, CA 91109, USANational Institute for Astrophysics, Institute for Space Astrophysics and Planetology , Via del Fosso del Cavaliere 100, I-00133 Roma, ItalyUniversity of Calabria , Department of Physics, Ponte Pietro Bucci Cubo 31C, I-87036 Rende, ItalyUniversity of Florence , Department of Physics and Astronomy, Via Giovanni Sansone 1, I-50019 Sesto Fiorentino, ItalyNational Institute for Astrophysics , Astronomical Observatory of Capodimonte, Salita Moiariello 16, I-80131 Napoli, ItalyNational Research Council, Institute for Photonics and Nanotechnologies , Via Trasea 7, I-35131 Padova, ItalyCzech Academy of Sciences, Astronomical Institute , Fričova 298, CZ-25165 Ondřejov, Czechia; University of Wrocław ,Centre of Scientific Excellence Solar and Stellar Activity, ul. Kopernika 11, PLâ51â622 Wrocław, PolandNational Aeronautics and Space Administration , Headquarters, Washington, DC 20546, USAUniversity of Padua , Department of Physics and Astronomy, Via Francesco Marzolo 8, I-35131 Padova, ItalyNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics , Astrophysical Observatory of Catania, Via Santa Sofia 78, I-95123 Catania, ItalyMax Planck Institute for Solar System Research , Justus-von-Liebig-Weg 3, D-37077 Göttingen, GermanyNational Institute for Astrophysics , Astrophysical Observatory of Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, ItalyMax Planck Institute for Solar System Research , Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany; University of Catania , Department of Physics and Astronomy, Via Santa Sofia 64, I-95123 Catania, ItalyNational Institute for Astrophysics , Astronomical Observatory of Trieste, Località Basovizza 302, I-34149 Trieste, ItalyNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics , Astrophysical Observatory of Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy ; daniele.telloni@inaf.itNational Institute for Astrophysics , Astronomical Observatory of Capodimonte, Salita Moiariello 16, I-80131 Napoli, ItalyNational Research Council, Institute for Photonics and Nanotechnologies , Via Trasea 7, I-35131 Padova, ItalyEvidence for the presence of ion cyclotron waves (ICWs), driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the joint observations performed by Parker Solar Probe and the Metis coronagraph on board Solar Orbiter, local measurements of the solar wind can be linked with the large-scale structures of the solar corona. The results suggest that the dynamics of the current sheet layers generates turbulence, which in turn creates a sufficiently strong temperature anisotropy to make the solar-wind plasma unstable to anisotropy-driven instabilities such as the Alfvén ion cyclotron, mirror-mode, and firehose instabilities. The study of the polarization state of high-frequency magnetic fluctuations reveals that ICWs are indeed present along the current sheet, thus linking the magnetic topology of the remotely imaged coronal source regions with the wave bursts observed in situ. The present results may allow improvement of state-of-the-art models based on the ion cyclotron mechanism, providing new insights into the processes involved in coronal heating.https://doi.org/10.3847/1538-4357/acb693MagnetohydrodynamicsInterplanetary turbulenceAlfven wavesSolar coronaSolar coronal heatingCoronagraphic imaging |
spellingShingle | Daniele Telloni Gary P. Zank Laxman Adhikari Lingling Zhao Roberto Susino Ester Antonucci Silvano Fineschi Marco Stangalini Catia Grimani Luca Sorriso-Valvo Daniel Verscharen Raffaele Marino Silvio Giordano Raffaella D’Amicis Denise Perrone Francesco Carbone Alessandro Liberatore Roberto Bruno Gaetano Zimbardo Marco Romoli Vincenzo Andretta Vania Da Deppo Petr Heinzel John D. Moses Giampiero Naletto Gianalfredo Nicolini Daniele Spadaro Luca Teriaca Aleksandr Burtovoi Yara De Leo Giovanna Jerse Federico Landini Maurizio Pancrazzi Clementina Sasso Alessandra Slemer Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? The Astrophysical Journal Magnetohydrodynamics Interplanetary turbulence Alfven waves Solar corona Solar coronal heating Coronagraphic imaging |
title | Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? |
title_full | Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? |
title_fullStr | Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? |
title_full_unstemmed | Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? |
title_short | Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves? |
title_sort | does turbulence along the coronal current sheet drive ion cyclotron waves |
topic | Magnetohydrodynamics Interplanetary turbulence Alfven waves Solar corona Solar coronal heating Coronagraphic imaging |
url | https://doi.org/10.3847/1538-4357/acb693 |
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