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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" (2018) Space Science Reviews. 214(1)
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Abstract:

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.

Registro:

Documento: Artículo
Título:Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations
Autor:Greco, A.; Matthaeus, W.H.; Perri, S.; Osman, K.T.; Servidio, S.; Wan, M.; Dmitruk, P.
Filiación:Dipartimento di Fisica, Università della Calabria, Via P. Bucci, Cubo 31 C, Rende (CS), 87036, Italy
Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States
Centre for Fusion, Space and Astrophysics, University of Warwick, Coventry, CV4 7AL, United Kingdom
Department of Mechanics and Aerospace Engineering, South University of Science and Technology of China, Shenzhen, Guangdong 518055, China
Departamento de Fìsica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires and IFIBA, CONICET, Ciudad Universitaria, Buenos Aires, 1428, Argentina
Palabras clave: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
Año:2018
Volumen:214
Número:1
DOI: http://dx.doi.org/10.1007/s11214-017-0435-8
Título revista:Space Science Reviews
Título revista abreviado:Space Sci Rev
ISSN:00386308
CODEN:SPSRA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v214_n1_p_Greco

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Citas:

---------- APA ----------
Greco, A., Matthaeus, W.H., Perri, S., Osman, K.T., Servidio, S., Wan, M. & Dmitruk, P. (2018) . Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations. Space Science Reviews, 214(1).
http://dx.doi.org/10.1007/s11214-017-0435-8
---------- CHICAGO ----------
Greco, A., Matthaeus, W.H., Perri, S., Osman, K.T., Servidio, S., Wan, M., et al. "Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations" . Space Science Reviews 214, no. 1 (2018).
http://dx.doi.org/10.1007/s11214-017-0435-8
---------- MLA ----------
Greco, A., Matthaeus, W.H., Perri, S., Osman, K.T., Servidio, S., Wan, M., et al. "Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations" . Space Science Reviews, vol. 214, no. 1, 2018.
http://dx.doi.org/10.1007/s11214-017-0435-8
---------- VANCOUVER ----------
Greco, A., Matthaeus, W.H., Perri, S., Osman, K.T., Servidio, S., Wan, M., et al. Partial Variance of Increments Method in Solar Wind Observations and Plasma Simulations. Space Sci Rev. 2018;214(1).
http://dx.doi.org/10.1007/s11214-017-0435-8