Artículo
Spatial correlation of solar-wind turbulence from two-point measurements
Matthaeus, W. H.; Dasso, Sergio Ricardo
; Weygand, J. M.; Milano, L. J.; Smith, C. W.; Kivelson, M. G.
Fecha de publicación:
02/12/2005
Editorial:
American Physical Society
Revista:
Physical Review Letters
ISSN:
0031-9007
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.
Palabras clave:
Solar Wind
,
Mhd
,
Turbulence
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Colecciones
Articulos(IAFE)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Citación
Matthaeus, W. H.; Dasso, Sergio Ricardo; Weygand, J. M.; Milano, L. J.; Smith, C. W.; et al.; Spatial correlation of solar-wind turbulence from two-point measurements; American Physical Society; Physical Review Letters; 95; 23; 2-12-2005; 1-4; 231101
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