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...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00386308_v214_n1_p_Greco |
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todo:paper_00386308_v214_n1_p_Greco2023-10-03T14:49:11Z Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations Greco, A. Matthaeus, W.H. Perri, S. Osman, K.T. Servidio, S. Wan, M. Dmitruk, P. 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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 Greco, A. Matthaeus, W.H. Perri, S. Osman, K.T. Servidio, S. Wan, M. Dmitruk, P. 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. |
| format |
JOUR |
| author |
Greco, A. Matthaeus, W.H. Perri, S. Osman, K.T. Servidio, S. Wan, M. Dmitruk, P. |
| author_facet |
Greco, A. Matthaeus, W.H. Perri, S. Osman, K.T. Servidio, S. Wan, M. Dmitruk, P. |
| author_sort |
Greco, A. |
| 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 |
| url |
http://hdl.handle.net/20.500.12110/paper_00386308_v214_n1_p_Greco |
| work_keys_str_mv |
AT grecoa partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT matthaeuswh partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT perris partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT osmankt partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT servidios partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT wanm partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations AT dmitrukp partialvarianceofincrementsmethodinsolarwindobservationsandplasmasimulations |
| _version_ |
1807317695167725568 |