Density and magnetic field signatures of interplanetary 1/f noise
- Autores
- Matthaeus, W.H.; Breech, B.; Dmitruk, Pablo Ariel; Bemporad, A.; Poletto, German Ariel; Velli, M.; Romoli, M.
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We investigate the occurrence of 1/f noise in the interplanetary density and the magnetic field at varying heliocentric latitudes. The characteristic spectral amplitudes can be found in Ulysses density and magnetic data in the expected frequency ranges at all available latitudes, ranging from the ecliptic plane to more than 80°. Average spectra indicate a latitudinal variation, with a 1/f density signal becoming more pronounced in higher latitude bands. Azimuthal spectral analysis of solar magnetogram data using the SOHO Michelson Doppler Interferometer also shows 1/f noise in the photospheric magnetic field, most clearly at high latitude. Accordingly, we discuss possibilities that the 1/f signal arises at varying altitudes, possibly surviving coronal dynamics. This raises questions that may be addressed in future studies using spectroscopic, white light, and radio scintillation data. © 2007. The American Astronomical Society. All rights reserved.
Fil: Matthaeus, W.H.. Bartol Research Institute; Reino Unido
Fil: Breech, B.. Bartol Research Institute; Reino Unido
Fil: Dmitruk, Pablo Ariel. Bartol Research Institute; Reino Unido. 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: Bemporad, A.. Osservatorio Astrofisico Di Arcetri; Italia
Fil: Poletto, German Ariel. Osservatorio Astrofisico Di Arcetri; Italia
Fil: Velli, M.. Università degli Studi di Firenze; Italia
Fil: Romoli, M.. Università degli Studi di Firenze; Italia - Materia
-
MHD
PLASMAS
SOLAR WIND
TURBULENCE
WAVES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/71633
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Density and magnetic field signatures of interplanetary 1/f noiseMatthaeus, W.H.Breech, B.Dmitruk, Pablo ArielBemporad, A.Poletto, German ArielVelli, M.Romoli, M.MHDPLASMASSOLAR WINDTURBULENCEWAVEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We investigate the occurrence of 1/f noise in the interplanetary density and the magnetic field at varying heliocentric latitudes. The characteristic spectral amplitudes can be found in Ulysses density and magnetic data in the expected frequency ranges at all available latitudes, ranging from the ecliptic plane to more than 80°. Average spectra indicate a latitudinal variation, with a 1/f density signal becoming more pronounced in higher latitude bands. Azimuthal spectral analysis of solar magnetogram data using the SOHO Michelson Doppler Interferometer also shows 1/f noise in the photospheric magnetic field, most clearly at high latitude. Accordingly, we discuss possibilities that the 1/f signal arises at varying altitudes, possibly surviving coronal dynamics. This raises questions that may be addressed in future studies using spectroscopic, white light, and radio scintillation data. © 2007. The American Astronomical Society. All rights reserved.Fil: Matthaeus, W.H.. Bartol Research Institute; Reino UnidoFil: Breech, B.. Bartol Research Institute; Reino UnidoFil: Dmitruk, Pablo Ariel. Bartol Research Institute; Reino Unido. 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: Bemporad, A.. Osservatorio Astrofisico Di Arcetri; ItaliaFil: Poletto, German Ariel. Osservatorio Astrofisico Di Arcetri; ItaliaFil: Velli, M.. Università degli Studi di Firenze; ItaliaFil: Romoli, M.. Università degli Studi di Firenze; ItaliaIOP Publishing2007-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/71633Matthaeus, W.H.; Breech, B.; Dmitruk, Pablo Ariel; Bemporad, A.; Poletto, German Ariel; et al.; Density and magnetic field signatures of interplanetary 1/f noise; IOP Publishing; Astrophysical Journal; 657; 2 II; 12-2007; 121-1240004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1086/513075info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:17:07Zoai:ri.conicet.gov.ar:11336/71633instacron: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:34982025-09-29 10:17:07.823CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Density and magnetic field signatures of interplanetary 1/f noise |
title |
Density and magnetic field signatures of interplanetary 1/f noise |
spellingShingle |
Density and magnetic field signatures of interplanetary 1/f noise Matthaeus, W.H. MHD PLASMAS SOLAR WIND TURBULENCE WAVES |
title_short |
Density and magnetic field signatures of interplanetary 1/f noise |
title_full |
Density and magnetic field signatures of interplanetary 1/f noise |
title_fullStr |
Density and magnetic field signatures of interplanetary 1/f noise |
title_full_unstemmed |
Density and magnetic field signatures of interplanetary 1/f noise |
title_sort |
Density and magnetic field signatures of interplanetary 1/f noise |
dc.creator.none.fl_str_mv |
Matthaeus, W.H. Breech, B. Dmitruk, Pablo Ariel Bemporad, A. Poletto, German Ariel Velli, M. Romoli, M. |
author |
Matthaeus, W.H. |
author_facet |
Matthaeus, W.H. Breech, B. Dmitruk, Pablo Ariel Bemporad, A. Poletto, German Ariel Velli, M. Romoli, M. |
author_role |
author |
author2 |
Breech, B. Dmitruk, Pablo Ariel Bemporad, A. Poletto, German Ariel Velli, M. Romoli, M. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
MHD PLASMAS SOLAR WIND TURBULENCE WAVES |
topic |
MHD PLASMAS SOLAR WIND TURBULENCE WAVES |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We investigate the occurrence of 1/f noise in the interplanetary density and the magnetic field at varying heliocentric latitudes. The characteristic spectral amplitudes can be found in Ulysses density and magnetic data in the expected frequency ranges at all available latitudes, ranging from the ecliptic plane to more than 80°. Average spectra indicate a latitudinal variation, with a 1/f density signal becoming more pronounced in higher latitude bands. Azimuthal spectral analysis of solar magnetogram data using the SOHO Michelson Doppler Interferometer also shows 1/f noise in the photospheric magnetic field, most clearly at high latitude. Accordingly, we discuss possibilities that the 1/f signal arises at varying altitudes, possibly surviving coronal dynamics. This raises questions that may be addressed in future studies using spectroscopic, white light, and radio scintillation data. © 2007. The American Astronomical Society. All rights reserved. Fil: Matthaeus, W.H.. Bartol Research Institute; Reino Unido Fil: Breech, B.. Bartol Research Institute; Reino Unido Fil: Dmitruk, Pablo Ariel. Bartol Research Institute; Reino Unido. 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: Bemporad, A.. Osservatorio Astrofisico Di Arcetri; Italia Fil: Poletto, German Ariel. Osservatorio Astrofisico Di Arcetri; Italia Fil: Velli, M.. Università degli Studi di Firenze; Italia Fil: Romoli, M.. Università degli Studi di Firenze; Italia |
description |
We investigate the occurrence of 1/f noise in the interplanetary density and the magnetic field at varying heliocentric latitudes. The characteristic spectral amplitudes can be found in Ulysses density and magnetic data in the expected frequency ranges at all available latitudes, ranging from the ecliptic plane to more than 80°. Average spectra indicate a latitudinal variation, with a 1/f density signal becoming more pronounced in higher latitude bands. Azimuthal spectral analysis of solar magnetogram data using the SOHO Michelson Doppler Interferometer also shows 1/f noise in the photospheric magnetic field, most clearly at high latitude. Accordingly, we discuss possibilities that the 1/f signal arises at varying altitudes, possibly surviving coronal dynamics. This raises questions that may be addressed in future studies using spectroscopic, white light, and radio scintillation data. © 2007. The American Astronomical Society. All rights reserved. |
publishDate |
2007 |
dc.date.none.fl_str_mv |
2007-12 |
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/11336/71633 Matthaeus, W.H.; Breech, B.; Dmitruk, Pablo Ariel; Bemporad, A.; Poletto, German Ariel; et al.; Density and magnetic field signatures of interplanetary 1/f noise; IOP Publishing; Astrophysical Journal; 657; 2 II; 12-2007; 121-124 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/71633 |
identifier_str_mv |
Matthaeus, W.H.; Breech, B.; Dmitruk, Pablo Ariel; Bemporad, A.; Poletto, German Ariel; et al.; Density and magnetic field signatures of interplanetary 1/f noise; IOP Publishing; Astrophysical Journal; 657; 2 II; 12-2007; 121-124 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1086/513075 |
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 |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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 |
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1844614121088090112 |
score |
13.070432 |