Scaling laws and coherent structures in the solar wind (Articolo in rivista)

Type

• Articolo in rivista (Classe)
• Prodotto della ricerca (Classe)

Label

• Scaling laws and coherent structures in the solar wind (Articolo in rivista) (literal)

Anno

• 2007-01-01T00:00:00+01:00 (literal)

Alternative label

• Bruno, R; D'Amicis, R; Bavassano, B; Carbone, V; Sorriso-Valvo, L (2007)
  Scaling laws and coherent structures in the solar wind
  in Planetary and space science
  (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori

• Bruno, R; D'Amicis, R; Bavassano, B; Carbone, V; Sorriso-Valvo, L (literal)

Pagina inizio

• 2233 (literal)

Pagina fine

• 2238 (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume

• 55 (literal)

Rivista

• Planetary and space science (Rivista)

Note

• ISI Web of Science (WOS) (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni

• Ist Fis Spazio Interplanetario, INAF, I-00133 Rome, Italy; Univ Calabria, Dipartmento Fis, I-87036 Arcavacata Di Rende, Italy; Univ Calabria, LICRYL, INFM, CNR, I-87036 Arcavacata Di Rende, Italy; Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy (literal)

Titolo

• Scaling laws and coherent structures in the solar wind (literal)

Abstract

• The interplanetary medium is characterized by a very high Reynolds number and is pervaded by fluctuations providing information on a wide range of scales, from fractions of second up to the solar rotation period. In the past decade or so, turbulence in the solar wind has been used as a large wind tunnel to investigate scaling laws of turbulent fluctuations and multifractal models. Moreover, new interesting insights in the theory of turbulence have been derived from the point of view which considers a turbulent flow as a complex system, a sort of benchmark for the theory of dynamical systems. Important finding like the lack of a strict self-similarity of the fluctuations with the consequent nonapplicability of strict scale invariance, the strong anisotropy of velocity and magnetic field fluctuations, the clear lack of equipartition between magnetic and kinetic fluctuations all contributed to suggest the idea that interplanetary fluctuations could possibly be due to a mixture of propagating waves and static structures convected by the wind. In this paper we further discuss this point and bring new evidence about the fact that the presence of a background magnetic field introduces not only a symmetry breaking in interplanetary space but also organizes fluctuations about its large scale orientation. (c) 2007 Elsevier Ltd. All rights reserved. (literal)

Prodotto di

• Soft Matter e nanotecnologie per elettro-ottica e di interesse biomedico e applicazioni tecnologiche correlate (MD.P01.016.001) (Modulo)
• Istituto per i processi chimico-fisici (IPCF) (Istituto)
• Soft Matter e nanotecnologie per elettro-ottica e di interesse biomedico e applicazioni tecnologiche correlate (MD.P01.015.009) (Modulo)

Autore CNR

• LUCA SORRISO VALVO (Unità di personale interno)

Insieme di parole chiave

• Keywords of "Scaling laws and coherent structures in the solar wind" (Insieme di parole chiave)

Incoming links:

Prodotto

• Istituto per i processi chimico-fisici (IPCF) (Istituto)
• Soft Matter e nanotecnologie per elettro-ottica e di interesse biomedico e applicazioni tecnologiche correlate (MD.P01.015.009) (Modulo)
• Soft Matter e nanotecnologie per elettro-ottica e di interesse biomedico e applicazioni tecnologiche correlate (MD.P01.016.001) (Modulo)

Autore CNR di

• LUCA SORRISO VALVO (Unità di personale interno)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#rivistaDi

• Planetary and space science (Rivista)

Insieme di parole chiave di

• Keywords of "Scaling laws and coherent structures in the solar wind" (Insieme di parole chiave)