Wave–particle resonance condition test for ion-kinetic waves in the solar wind
Conditions for the Landau and cyclotron resonances are tested for 543 waves (identified as local peaks in the energy spectra) in the magnetic field fluctuations of the solar wind measured by the Cluster spacecraft on a tetrahedral scale of 100 km. The resonance parameters are evaluated using the...
| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2016-04-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/34/393/2016/angeo-34-393-2016.pdf |
| _version_ | 1818282196855685120 |
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| author | Y. Narita Y. Narita E. Marsch C. Perschke C. Perschke K.-H. Glassmeier K.-H. Glassmeier U. Motschmann U. Motschmann H. Comişel H. Comişel |
| author_facet | Y. Narita Y. Narita E. Marsch C. Perschke C. Perschke K.-H. Glassmeier K.-H. Glassmeier U. Motschmann U. Motschmann H. Comişel H. Comişel |
| author_sort | Y. Narita |
| collection | DOAJ |
| description | Conditions for the Landau and cyclotron resonances are tested for 543 waves
(identified as local peaks in the energy spectra) in the magnetic field
fluctuations of the solar wind measured by the Cluster spacecraft on a
tetrahedral scale of 100 km. The resonance parameters are evaluated using the
frequencies in the plasma rest frame, the parallel components of the
wavevectors, the ion cyclotron frequency, and the ion thermal speed. The
observed waves show a character of the sideband waves associated with the ion
Bernstein mode, and are in a weak agreement with the fundamental electron
cyclotron resonance in spite of the ion-kinetic scales. The electron
cyclotron resonance is likely taking place in solar wind turbulence near 1 AU
(astronomical unit). |
| first_indexed | 2024-12-13T00:17:11Z |
| format | Article |
| id | doaj.art-d8d9d2247a2f465b9c7ebf5f98459943 |
| institution | Directory Open Access Journal |
| issn | 0992-7689 1432-0576 |
| language | English |
| last_indexed | 2024-12-13T00:17:11Z |
| publishDate | 2016-04-01 |
| publisher | Copernicus Publications |
| record_format | Article |
| series | Annales Geophysicae |
| spelling | doaj.art-d8d9d2247a2f465b9c7ebf5f984599432022-12-22T00:05:45ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762016-04-013439339810.5194/angeo-34-393-2016Wave–particle resonance condition test for ion-kinetic waves in the solar windY. Narita0Y. Narita1E. Marsch2C. Perschke3C. Perschke4K.-H. Glassmeier5K.-H. Glassmeier6U. Motschmann7U. Motschmann8H. Comişel9H. Comişel10Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, AustriaInstitut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyInstitut für Experimentelle und Angewandte Physik, Christian-Albrechts Universität Kiel, Leibnizstr. 11, 24118 Kiel, GermanyInstitut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyInstitut für Theoretische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyInstitut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyMax-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, GermanyInstitut für Theoretische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyDeutsches Zentrum für Luft- und Raumfahrt, Institut für Planetenforschung, Rutherfordstr. 2, 12489 Berlin, GermanyInstitut für Theoretische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, GermanyInstitute for Space Sciences, Atomiştilor 409, P.O. Box MG-23, Bucharest-Măgurele, 077125, RomaniaConditions for the Landau and cyclotron resonances are tested for 543 waves (identified as local peaks in the energy spectra) in the magnetic field fluctuations of the solar wind measured by the Cluster spacecraft on a tetrahedral scale of 100 km. The resonance parameters are evaluated using the frequencies in the plasma rest frame, the parallel components of the wavevectors, the ion cyclotron frequency, and the ion thermal speed. The observed waves show a character of the sideband waves associated with the ion Bernstein mode, and are in a weak agreement with the fundamental electron cyclotron resonance in spite of the ion-kinetic scales. The electron cyclotron resonance is likely taking place in solar wind turbulence near 1 AU (astronomical unit).https://www.ann-geophys.net/34/393/2016/angeo-34-393-2016.pdf |
| spellingShingle | Y. Narita Y. Narita E. Marsch C. Perschke C. Perschke K.-H. Glassmeier K.-H. Glassmeier U. Motschmann U. Motschmann H. Comişel H. Comişel Wave–particle resonance condition test for ion-kinetic waves in the solar wind Annales Geophysicae |
| title | Wave–particle resonance condition test for ion-kinetic waves in the solar wind |
| title_full | Wave–particle resonance condition test for ion-kinetic waves in the solar wind |
| title_fullStr | Wave–particle resonance condition test for ion-kinetic waves in the solar wind |
| title_full_unstemmed | Wave–particle resonance condition test for ion-kinetic waves in the solar wind |
| title_short | Wave–particle resonance condition test for ion-kinetic waves in the solar wind |
| title_sort | wave particle resonance condition test for ion kinetic waves in the solar wind |
| url | https://www.ann-geophys.net/34/393/2016/angeo-34-393-2016.pdf |
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