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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/16500
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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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |