Technique for measuring and correcting the Taylor microscale

Autores
Chuychai, P.; Weygand, J. M.; Matthaeus, W. H.; Dasso, Sergio Ricardo; Smith, C. W.; Kivelson, M. G.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We discuss and develop methods to estimate and refine measurements of the Taylor microscale from discrete data sets. To study how well a method works, we construct a time series of discrete data with a known power spectrum and Taylor scale, but with various truncations of the resolution that eliminate higher frequencies in a controlled fashion. We compute the second-order structure function and correlation function, assuming that the unresolved dissipation range spectrum has various values of spectral index. A series of Taylor scale estimates are obtained from parabolic fits to subsets of the correlation function data, and these are extrapolated to the limit of zero separation. The error in this procedure, for finite time resolution sampling, depends on the spectral index in the dissipation range. When the spectral form is known, we can compute a correction factor that improves the estimate of the Taylor microscale value determined from the extrapolation method and band-limited data. Application of this technique to spacecraft observations of solar wind fluctuations is illustrated.
Fil: Chuychai, P.. Mae Fah Luang University; Estados Unidos. Ministry of Education; Tailandia
Fil: Weygand, J. M.. University of California; Estados Unidos
Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos
Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomia y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomia y Física del Espacio; Argentina
Fil: Smith, C. W.. University of New Hampshire; Estados Unidos
Fil: Kivelson, M. G.. University of California; Estados Unidos
Materia
Turbulence
magnetohydrodynamics
Taylor microscale
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/16500

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spelling Technique for measuring and correcting the Taylor microscaleChuychai, P.Weygand, J. M.Matthaeus, W. H.Dasso, Sergio RicardoSmith, C. W.Kivelson, M. G.TurbulencemagnetohydrodynamicsTaylor microscalehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We discuss and develop methods to estimate and refine measurements of the Taylor microscale from discrete data sets. To study how well a method works, we construct a time series of discrete data with a known power spectrum and Taylor scale, but with various truncations of the resolution that eliminate higher frequencies in a controlled fashion. We compute the second-order structure function and correlation function, assuming that the unresolved dissipation range spectrum has various values of spectral index. A series of Taylor scale estimates are obtained from parabolic fits to subsets of the correlation function data, and these are extrapolated to the limit of zero separation. The error in this procedure, for finite time resolution sampling, depends on the spectral index in the dissipation range. When the spectral form is known, we can compute a correction factor that improves the estimate of the Taylor microscale value determined from the extrapolation method and band-limited data. Application of this technique to spacecraft observations of solar wind fluctuations is illustrated.Fil: Chuychai, P.. Mae Fah Luang University; Estados Unidos. Ministry of Education; TailandiaFil: Weygand, J. M.. University of California; Estados UnidosFil: Matthaeus, W. H.. University of Delaware; Estados UnidosFil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomia y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomia y Física del Espacio; ArgentinaFil: Smith, C. W.. University of New Hampshire; Estados UnidosFil: Kivelson, M. G.. University of California; Estados UnidosAmerican Geophysical Union2014-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16500Chuychai, P.; Weygand, J. M.; Matthaeus, W. H.; Dasso, Sergio Ricardo; Smith, C. W.; et al.; Technique for measuring and correcting the Taylor microscale; American Geophysical Union; Journal Of Geophysical Research; 119; 6; 6-2014; 4256-42650148-0227enginfo:eu-repo/semantics/altIdentifier/doi/10.1002/2013JA019641info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/2013JA019641/abstractinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:56:13Zoai:ri.conicet.gov.ar:11336/16500instacron: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 09:56:13.783CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Technique for measuring and correcting the Taylor microscale
title Technique for measuring and correcting the Taylor microscale
spellingShingle Technique for measuring and correcting the Taylor microscale
Chuychai, P.
Turbulence
magnetohydrodynamics
Taylor microscale
title_short Technique for measuring and correcting the Taylor microscale
title_full Technique for measuring and correcting the Taylor microscale
title_fullStr Technique for measuring and correcting the Taylor microscale
title_full_unstemmed Technique for measuring and correcting the Taylor microscale
title_sort Technique for measuring and correcting the Taylor microscale
dc.creator.none.fl_str_mv Chuychai, P.
Weygand, J. M.
Matthaeus, W. H.
Dasso, Sergio Ricardo
Smith, C. W.
Kivelson, M. G.
author Chuychai, P.
author_facet Chuychai, P.
Weygand, J. M.
Matthaeus, W. H.
Dasso, Sergio Ricardo
Smith, C. W.
Kivelson, M. G.
author_role author
author2 Weygand, J. M.
Matthaeus, W. H.
Dasso, Sergio Ricardo
Smith, C. W.
Kivelson, M. G.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Turbulence
magnetohydrodynamics
Taylor microscale
topic Turbulence
magnetohydrodynamics
Taylor microscale
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 discuss and develop methods to estimate and refine measurements of the Taylor microscale from discrete data sets. To study how well a method works, we construct a time series of discrete data with a known power spectrum and Taylor scale, but with various truncations of the resolution that eliminate higher frequencies in a controlled fashion. We compute the second-order structure function and correlation function, assuming that the unresolved dissipation range spectrum has various values of spectral index. A series of Taylor scale estimates are obtained from parabolic fits to subsets of the correlation function data, and these are extrapolated to the limit of zero separation. The error in this procedure, for finite time resolution sampling, depends on the spectral index in the dissipation range. When the spectral form is known, we can compute a correction factor that improves the estimate of the Taylor microscale value determined from the extrapolation method and band-limited data. Application of this technique to spacecraft observations of solar wind fluctuations is illustrated.
Fil: Chuychai, P.. Mae Fah Luang University; Estados Unidos. Ministry of Education; Tailandia
Fil: Weygand, J. M.. University of California; Estados Unidos
Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos
Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomia y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomia y Física del Espacio; Argentina
Fil: Smith, C. W.. University of New Hampshire; Estados Unidos
Fil: Kivelson, M. G.. University of California; Estados Unidos
description We discuss and develop methods to estimate and refine measurements of the Taylor microscale from discrete data sets. To study how well a method works, we construct a time series of discrete data with a known power spectrum and Taylor scale, but with various truncations of the resolution that eliminate higher frequencies in a controlled fashion. We compute the second-order structure function and correlation function, assuming that the unresolved dissipation range spectrum has various values of spectral index. A series of Taylor scale estimates are obtained from parabolic fits to subsets of the correlation function data, and these are extrapolated to the limit of zero separation. The error in this procedure, for finite time resolution sampling, depends on the spectral index in the dissipation range. When the spectral form is known, we can compute a correction factor that improves the estimate of the Taylor microscale value determined from the extrapolation method and band-limited data. Application of this technique to spacecraft observations of solar wind fluctuations is illustrated.
publishDate 2014
dc.date.none.fl_str_mv 2014-06
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/11336/16500
Chuychai, P.; Weygand, J. M.; Matthaeus, W. H.; Dasso, Sergio Ricardo; Smith, C. W.; et al.; Technique for measuring and correcting the Taylor microscale; American Geophysical Union; Journal Of Geophysical Research; 119; 6; 6-2014; 4256-4265
0148-0227
url http://hdl.handle.net/11336/16500
identifier_str_mv Chuychai, P.; Weygand, J. M.; Matthaeus, W. H.; Dasso, Sergio Ricardo; Smith, C. W.; et al.; Technique for measuring and correcting the Taylor microscale; American Geophysical Union; Journal Of Geophysical Research; 119; 6; 6-2014; 4256-4265
0148-0227
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1002/2013JA019641
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/2013JA019641/abstract
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 American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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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score 13.070432