Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence
- Autores
- Andrés, Nahuel; Clark Di Leoni, Patricio; Mininni, Pablo Daniel; Dmitruk, Pablo Ariel; Sahraoui, F.; Matthaeus, W. H.
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Fil: Andrés, Nahuel. Centre National de la Recherche Scientifique; Francia
Fil: Clark Di Leoni, Patricio. Universita Tor Vergata; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Mininni, Pablo Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Dmitruk, Pablo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Sahraoui, F.. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Matthaeus, W. H.. Universidad de Buenos Aires; Argentina - Materia
-
TURBULENCE
ALFVEN WAVES
MHD
COMPRESSIBLE FLOWS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/61099
Ver los metadatos del registro completo
| id |
CONICETDig_2a93e86adbb0d641140b5e793a9b7b76 |
|---|---|
| oai_identifier_str |
oai:ri.conicet.gov.ar:11336/61099 |
| network_acronym_str |
CONICETDig |
| repository_id_str |
3498 |
| network_name_str |
CONICET Digital (CONICET) |
| spelling |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulenceAndrés, NahuelClark Di Leoni, PatricioMininni, Pablo DanielDmitruk, Pablo ArielSahraoui, F.Matthaeus, W. H.TURBULENCEALFVEN WAVESMHDCOMPRESSIBLE FLOWShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using 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.Fil: Andrés, Nahuel. Centre National de la Recherche Scientifique; FranciaFil: Clark Di Leoni, Patricio. Universita Tor Vergata; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Mininni, Pablo Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Dmitruk, Pablo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Sahraoui, F.. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Matthaeus, W. H.. Universidad de Buenos Aires; ArgentinaAmerican Institute of Physics2017-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/61099Andrés, Nahuel; Clark Di Leoni, Patricio; Mininni, Pablo Daniel; Dmitruk, Pablo Ariel; Sahraoui, F.; et al.; Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence; American Institute of Physics; Physics Of Plasmas; 24; 10; 10-2017; 1-91070-664XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/pdf/1707.09190.pdfinfo:eu-repo/semantics/altIdentifier/doi/10.1063/1.4997990info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-12T09:50:16Zoai:ri.conicet.gov.ar:11336/61099instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-11-12 09:50:17.11CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| title |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| spellingShingle |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence Andrés, Nahuel TURBULENCE ALFVEN WAVES MHD COMPRESSIBLE FLOWS |
| title_short |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| title_full |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| title_fullStr |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| title_full_unstemmed |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| title_sort |
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence |
| dc.creator.none.fl_str_mv |
Andrés, Nahuel Clark Di Leoni, Patricio Mininni, Pablo Daniel Dmitruk, Pablo Ariel Sahraoui, F. Matthaeus, W. H. |
| author |
Andrés, Nahuel |
| author_facet |
Andrés, Nahuel Clark Di Leoni, Patricio Mininni, Pablo Daniel Dmitruk, Pablo Ariel Sahraoui, F. Matthaeus, W. H. |
| author_role |
author |
| author2 |
Clark Di Leoni, Patricio Mininni, Pablo Daniel Dmitruk, Pablo Ariel Sahraoui, F. Matthaeus, W. H. |
| author2_role |
author author author author author |
| dc.subject.none.fl_str_mv |
TURBULENCE ALFVEN WAVES MHD COMPRESSIBLE FLOWS |
| topic |
TURBULENCE ALFVEN WAVES MHD COMPRESSIBLE FLOWS |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
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. Fil: Andrés, Nahuel. Centre National de la Recherche Scientifique; Francia Fil: Clark Di Leoni, Patricio. Universita Tor Vergata; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Mininni, Pablo Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Dmitruk, Pablo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Sahraoui, F.. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Matthaeus, W. H.. Universidad de Buenos Aires; Argentina |
| description |
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. |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017-10 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/61099 Andrés, Nahuel; Clark Di Leoni, Patricio; Mininni, Pablo Daniel; Dmitruk, Pablo Ariel; Sahraoui, F.; et al.; Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence; American Institute of Physics; Physics Of Plasmas; 24; 10; 10-2017; 1-9 1070-664X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/61099 |
| identifier_str_mv |
Andrés, Nahuel; Clark Di Leoni, Patricio; Mininni, Pablo Daniel; Dmitruk, Pablo Ariel; Sahraoui, F.; et al.; Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence; American Institute of Physics; Physics Of Plasmas; 24; 10; 10-2017; 1-9 1070-664X CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/pdf/1707.09190.pdf info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4997990 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| eu_rights_str_mv |
openAccess |
| rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
American Institute of Physics |
| publisher.none.fl_str_mv |
American Institute of Physics |
| dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
| reponame_str |
CONICET Digital (CONICET) |
| collection |
CONICET Digital (CONICET) |
| instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
| repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
| repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
| _version_ |
1848598106439942144 |
| score |
13.24909 |