Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence
Using spatio-temporal spectra, we show direct evidence of excitation of magnetosonic and Alfvén waves in three-dimensional compressible magnetohydrodynamic turbulence at small Mach numbers. For the plasma pressure dominated regime, or the high β regime (with β the ratio between fluid and magnetic pr...
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Otros Autores: | , , , , |
Formato: | Capítulo de libro |
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American Institute of Physics Inc.
2017
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005 | 20240930105541.0 | ||
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024 | 7 | |2 scopus |a 2-s2.0-85031940434 | |
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040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
100 | 1 | |a Andrés, Nahuel | |
245 | 1 | 0 | |a Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
260 | |b American Institute of Physics Inc. |c 2017 | ||
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506 | |2 openaire |e Política editorial | ||
520 | 3 | |a Using spatio-temporal spectra, we show direct evidence of excitation of magnetosonic and Alfvén waves in three-dimensional compressible magnetohydrodynamic turbulence at small Mach numbers. For the plasma pressure dominated regime, or the high β regime (with β the ratio between fluid and magnetic pressure), and for the magnetic pressure dominated regime, or the low β regime, we study magnetic field fluctuations parallel and perpendicular to a guide magnetic field B0. In the low β case, we find excitation of compressible and incompressible fluctuations, with a transfer of energy towards Alfvénic modes and to a lesser extent towards magnetosonic modes. In particular, we find signatures of the presence of fast magnetosonic waves in a scenario compatible with that of weak turbulence. In the high β case, fast and slow magnetosonic waves are present, with no clear trace of Alfvén waves, and a significant part of the energy is carried by two-dimensional turbulent eddies. © 2017 Author(s). |l eng | |
536 | |a Detalles de la financiación: Labex | ||
536 | |a Detalles de la financiación: Agence Nationale de la Recherche, ANR, ANR-11-IDEX-0004–02 | ||
536 | |a Detalles de la financiación: Secretaría de Ciencia y Técnica, Universidad de Buenos Aires, UBACyT, 20020130100738BA | ||
536 | |a Detalles de la financiación: Seventh Framework Programme, FP7 | ||
536 | |a Detalles de la financiación: NNX17AB79G | ||
536 | |a Detalles de la financiación: European Research Council, ERC | ||
536 | |a Detalles de la financiación: NNX14AI63G | ||
536 | |a Detalles de la financiación: European Research Council, ERC, 339032 | ||
536 | |a Detalles de la financiación: 2011-1529, 2015-3530 | ||
536 | |a Detalles de la financiación: N.A. is supported through an École Polytechnique Postdoctoral Fellowship and by LABEX Plas@Par through a grant managed by the Agence Nationale de la Recherche (ANR), as a part of the program “Investissements d’Avenir” under the reference ANR-11-IDEX-0004–02. F.S. and N.A. acknowledge financial support from the Programme National Soleil-Terre (PNST). P.C., P.D.M., and P.D. acknowledge the support from the UBACYT Grant No. 20020130100738BA and the PICT Grant Nos. 2011-1529 and 2015-3530. W.H.M. is supported in part by the NASA Heliophysics Grand Challenge (NNX14AI63G), and the LWS (NNX14AI63G) and Heliophysics GI (NNX17AB79G) programs. P.C.D.L. acknowledges funding from the European Research Council under the European Community’s Seventh Framework Program, ERC Grant Agreement No. 339032. | ||
593 | |a LPP, CNRS, Ecole Polytechnique, UPMC Univ. Paris 06, Observatoire de Paris, Université Paris-Saclay, Sorbonne Universités, PSL Research University, Palaiseau, F-91128, France | ||
593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, Buenos Aires, 1428, Argentina | ||
593 | |a Instituto de Física de Buenos Aires, CONICET-UBA, Ciudad Universitaria, Buenos Aires, 1428, Argentina | ||
593 | |a Department of Physics and INFN, University of Rome Tor Vergata, Via della Ricerca Scientifica 1, Rome, 00133, Italy | ||
593 | |a Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States | ||
690 | 1 | 0 | |a ENERGY TRANSFER |
690 | 1 | 0 | |a INCOMPRESSIBLE FLOW |
690 | 1 | 0 | |a MAGNETIC FIELDS |
690 | 1 | 0 | |a MAGNETISM |
690 | 1 | 0 | |a MAGNETOHYDRODYNAMICS |
690 | 1 | 0 | |a TURBULENCE |
690 | 1 | 0 | |a GUIDE MAGNETIC FIELD |
690 | 1 | 0 | |a MAGNETIC FIELD FLUCTUATIONS |
690 | 1 | 0 | |a MAGNETIC PRESSURE |
690 | 1 | 0 | |a MAGNETOHYDRODYNAMIC TURBULENCE |
690 | 1 | 0 | |a MAGNETOHYDRODYNAMICS TURBULENCES |
690 | 1 | 0 | |a MAGNETOSONIC MODE |
690 | 1 | 0 | |a MAGNETOSONIC WAVES |
690 | 1 | 0 | |a PLASMA PRESSURES |
690 | 1 | 0 | |a MAGNETOPLASMA |
700 | 1 | |a Clark di Leoni, P. | |
700 | 1 | |a Mininni, P.D. | |
700 | 1 | |a Dmitruk, P. | |
700 | 1 | |a Sahraoui, F. | |
700 | 1 | |a Matthaeus, W.H. | |
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