Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence
The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environment, which underlies various astrophysical phenomena. Its diffusive character depends on the distance along the field l...
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th-mahidol.871352023-06-20T11:54:45Z Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence Yannawa C. Mahidol University Earth and Planetary Sciences The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environment, which underlies various astrophysical phenomena. Its diffusive character depends on the distance along the field line, the initial separation, and the characteristics of the magnetic turbulence. This work considers the separation of two magnetic field lines in general transverse turbulence in terms of the magnetic power spectrum in three-dimensional wavenumber space. We apply non-perturbative methods using Corrsin's hypothesis and assume random ballistic decorrelation to calculate the ensemble average field line separation for general transverse magnetic turbulence. For 2D + slab power spectra, our analytical formulae and computer simulations give similar results, especially at low slab fraction. Our analytical expression also demonstrates several features of field line separation that are verified by computer simulations. 2023-06-20T04:54:45Z 2023-06-20T04:54:45Z 2023-07-01 Article Monthly Notices of the Royal Astronomical Society Vol.522 No.4 (2023) , 5098-5106 10.1093/mnras/stad1296 13652966 00358711 2-s2.0-85161586484 https://repository.li.mahidol.ac.th/handle/123456789/87135 SCOPUS |
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Earth and Planetary Sciences Yannawa C. Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
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The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environment, which underlies various astrophysical phenomena. Its diffusive character depends on the distance along the field line, the initial separation, and the characteristics of the magnetic turbulence. This work considers the separation of two magnetic field lines in general transverse turbulence in terms of the magnetic power spectrum in three-dimensional wavenumber space. We apply non-perturbative methods using Corrsin's hypothesis and assume random ballistic decorrelation to calculate the ensemble average field line separation for general transverse magnetic turbulence. For 2D + slab power spectra, our analytical formulae and computer simulations give similar results, especially at low slab fraction. Our analytical expression also demonstrates several features of field line separation that are verified by computer simulations. |
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Mahidol University |
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Mahidol University Yannawa C. |
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Yannawa C. |
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Yannawa C. |
title |
Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
title_short |
Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
title_full |
Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
title_fullStr |
Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
title_full_unstemmed |
Magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
title_sort |
magnetic field line separation by random ballistic decorrelation in transverse magnetic turbulence |
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2023 |
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https://repository.li.mahidol.ac.th/handle/123456789/87135 |
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