Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations

The method called “PVI” (Partial Variance of Increments) has been increasingly used in analysis of spacecraft and numerical simulation data since its inception in 2008. The purpose of the method is to study the kinematics and formation of coherent structures in space plasmas, a topic that has gained...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2018
Materias:
Coherent structures
Intermittency
Solar wind
Turbulence
Numerical models
Coherent structure
Identification method
Key feature
Review papers
Space plasmas
Theoretical research
Numerical methods
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v214_n1_p_Greco
http://hdl.handle.net/20.500.12110/paper_00386308_v214_n1_p_Greco
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00386308_v214_n1_p_Greco
record_format dspace
spelling paper:paper_00386308_v214_n1_p_Greco2023-06-08T15:03:05Z Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations Coherent structures Intermittency Solar wind Turbulence Numerical models Solar wind Turbulence Coherent structure Identification method Intermittency Key feature Review papers Space plasmas Theoretical research Numerical methods The method called “PVI” (Partial Variance of Increments) has been increasingly used in analysis of spacecraft and numerical simulation data since its inception in 2008. The purpose of the method is to study the kinematics and formation of coherent structures in space plasmas, a topic that has gained considerable attention, leading the development of identification methods, observations, and associated theoretical research based on numerical simulations. This review paper will summarize key features of the method and provide a synopsis of the main results obtained by various groups using the method. This will enable new users or those considering methods of this type to find details and background collected in one place. © 2017, Springer Science+Business Media B.V., part of Springer Nature. 2018 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v214_n1_p_Greco http://hdl.handle.net/20.500.12110/paper_00386308_v214_n1_p_Greco
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Coherent structures
Intermittency
Solar wind
Turbulence
Numerical models
Solar wind
Turbulence
Coherent structure
Identification method
Intermittency
Key feature
Review papers
Space plasmas
Theoretical research
Numerical methods
spellingShingle Coherent structures
Intermittency
Solar wind
Turbulence
Numerical models
Solar wind
Turbulence
Coherent structure
Identification method
Intermittency
Key feature
Review papers
Space plasmas
Theoretical research
Numerical methods
Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
topic_facet Coherent structures
Intermittency
Solar wind
Turbulence
Numerical models
Solar wind
Turbulence
Coherent structure
Identification method
Intermittency
Key feature
Review papers
Space plasmas
Theoretical research
Numerical methods
description The method called “PVI” (Partial Variance of Increments) has been increasingly used in analysis of spacecraft and numerical simulation data since its inception in 2008. The purpose of the method is to study the kinematics and formation of coherent structures in space plasmas, a topic that has gained considerable attention, leading the development of identification methods, observations, and associated theoretical research based on numerical simulations. This review paper will summarize key features of the method and provide a synopsis of the main results obtained by various groups using the method. This will enable new users or those considering methods of this type to find details and background collected in one place. © 2017, Springer Science+Business Media B.V., part of Springer Nature.
title Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
title_short Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
title_full Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
title_fullStr Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
title_full_unstemmed Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
title_sort partial variance of increments method in solar wind observations and plasma simulations
publishDate 2018
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v214_n1_p_Greco
http://hdl.handle.net/20.500.12110/paper_00386308_v214_n1_p_Greco
_version_ 1768541977971785728

Ejemplares similares