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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Autor principal: Andrés, Nahuel
Otros Autores: Clark di Leoni, P., Mininni, P.D, Dmitruk, P., Sahraoui, F., Matthaeus, W.H
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: American Institute of Physics Inc. 2017
Acceso en línea:Registro en Scopus
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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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