dor_id: 4132231

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590.#.#.d: Los artículos enviados a la revista "Geofísica Internacional", se juzgan por medio de un proceso de revisión por pares

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650.#.4.x: Físico Matemáticas y Ciencias de la Tierra

336.#.#.b: article

336.#.#.3: Artículo de Investigación

336.#.#.a: Artículo

351.#.#.6: http://revistagi.geofisica.unam.mx/index.php/RGI

351.#.#.b: Geofísica Internacional

351.#.#.a: Artículos

harvesting_group: RevistasUNAM

270.1.#.p: Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

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270.#.#.d: MX

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883.#.#.1: https://www.publicaciones.unam.mx/

883.#.#.q: Dirección General de Publicaciones y Fomento Editorial

850.#.#.a: Universidad Nacional Autónoma de México

856.4.0.u: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/501/517

100.1.#.a: Ojeda González, Arian; Mendes Junior, Odim; Oliveira Domingues, Margarete; Everton Menconi, Varlei

524.#.#.a: Ojeda González, Arian, et al. (2014). Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations. Geofísica Internacional; Vol. 53 Núm. 2: Abril 1, 2014; 101-115. Recuperado de https://repositorio.unam.mx/contenidos/4132231

245.1.0.a: Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Geofísica, UNAM

264.#.0.c: 2014

264.#.1.c: 2014-04-01

653.#.#.a: electrodinámica espacial; nubes magnéticas; análisis de series temporales; transformada wavelet discreta; clima espacial; space electrodynamics; magnetic clouds; time series analysis; discrete wavelet transform; space weather

506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC-SA 4.0 Internacional, https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es, para un uso diferente consultar al responsable jurídico del repositorio por medio del correo electrónico revistagi@igeofisica.unam.mx

884.#.#.k: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/501

001.#.#.#: 063.oai:revistagi.geofisica.unam.mx:article/501

041.#.7.h: spa

520.3.#.a: We have studied a set of 41 magnetic clouds (MCs) measured by the ACE spacecraft, using the discrete orthogonal wavelet transform (Daubechies wavelet of order two) in three regions: Pre-MC (plasma sheath), MC and Post-MC. We have used data from the IMF GSM-components with time resolution of 16 s. The mathematical property chosen was the statistical mean of the wavelet coefficients (⟨Dd1⟩). The Daubechies wavelet coefficients have been used because they represent the local regularity present in the signal being studied. The results reproduced the wellknown fact that the dynamics of the sheath region is more than that of the MC region. This technique could be useful to help a specialist to find events boundaries when working with IMF datasets, i.e., a best form to visualize the data. The wavelet coefficients have the dvantage of helping to find some shocks that are not easy to see in the IMF data by simple visual inspection. We can learn that fluctuations are not low in all MCs, in some cases waves can penetrate from the sheath to the MC. This methodology has not yet been tested to identify some specific fluctuation patterns at IMF for any other geoeffective interplanetary events, such as Co-rotating Interaction Regions (CIRs), Heliospheric Current Sheet (HCS) or ICMEs without MC signatures. In our opinion, as is the first time that this technique is applied to the IMF data with this purpose, the presentation of this approach for the Space Physics Community is one of the contributions of this work.doi: https://doi.org/10.1016/S0016-7169(14)71494-1

773.1.#.t: Geofísica Internacional; Vol. 53 Núm. 2: Abril 1, 2014; 101-115

773.1.#.o: http://revistagi.geofisica.unam.mx/index.php/RGI

022.#.#.a: ISSN-L: 2954-436X; ISSN impreso: 0016-7169

310.#.#.a: Trimestral

300.#.#.a: Páginas: 101-115

264.#.1.b: Instituto de Geofísica, UNAM

doi: https://doi.org/10.1016/S0016-7169(14)71494-1

handle: 00a8cf7ef4ea35d4

harvesting_date: 2023-06-20 16:00:00.0

856.#.0.q: application/pdf

file_creation_date: 2014-04-07 16:08:46.0

file_modification_date: 2022-07-07 18:14:55.0

file_creator: Arian Ojeda González

file_name: 951d44a6317ea4bbfcb0ab7be2058d0aca65f41ecae877b856739fcf0b8065d1.pdf

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245.1.0.b: Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations

last_modified: 2023-06-20 16:00:00

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Artículo

Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations

Ojeda González, Arian; Mendes Junior, Odim; Oliveira Domingues, Margarete; Everton Menconi, Varlei

Instituto de Geofísica, UNAM, publicado en Geofísica Internacional, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Entidad o dependencia
Instituto de Geofísica, UNAM
Revista
Repositorio
Contacto
Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

Cita

Ojeda González, Arian, et al. (2014). Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations. Geofísica Internacional; Vol. 53 Núm. 2: Abril 1, 2014; 101-115. Recuperado de https://repositorio.unam.mx/contenidos/4132231

Descripción del recurso

Autor(es)
Ojeda González, Arian; Mendes Junior, Odim; Oliveira Domingues, Margarete; Everton Menconi, Varlei
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations
Fecha
2014-04-01
Resumen
We have studied a set of 41 magnetic clouds (MCs) measured by the ACE spacecraft, using the discrete orthogonal wavelet transform (Daubechies wavelet of order two) in three regions: Pre-MC (plasma sheath), MC and Post-MC. We have used data from the IMF GSM-components with time resolution of 16 s. The mathematical property chosen was the statistical mean of the wavelet coefficients (⟨Dd1⟩). The Daubechies wavelet coefficients have been used because they represent the local regularity present in the signal being studied. The results reproduced the wellknown fact that the dynamics of the sheath region is more than that of the MC region. This technique could be useful to help a specialist to find events boundaries when working with IMF datasets, i.e., a best form to visualize the data. The wavelet coefficients have the dvantage of helping to find some shocks that are not easy to see in the IMF data by simple visual inspection. We can learn that fluctuations are not low in all MCs, in some cases waves can penetrate from the sheath to the MC. This methodology has not yet been tested to identify some specific fluctuation patterns at IMF for any other geoeffective interplanetary events, such as Co-rotating Interaction Regions (CIRs), Heliospheric Current Sheet (HCS) or ICMEs without MC signatures. In our opinion, as is the first time that this technique is applied to the IMF data with this purpose, the presentation of this approach for the Space Physics Community is one of the contributions of this work.doi: https://doi.org/10.1016/S0016-7169(14)71494-1
Tema
electrodinámica espacial; nubes magnéticas; análisis de series temporales; transformada wavelet discreta; clima espacial; space electrodynamics; magnetic clouds; time series analysis; discrete wavelet transform; space weather
Idioma
spa
ISSN
ISSN-L: 2954-436X; ISSN impreso: 0016-7169

Enlaces