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Vincenzo Carbone

4 papers hereh-index 8368 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • nlin.CD4
same name
  • Vincenzo Carbone — 4 papers, h 11
  • Vincenzo Carbone — 3 papers, h 4
  • Vincenzo Carbone — 2 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedAnalysis of cancellation in two-dimensional magnetohydrodynamic turbulence

55 citations · 134 across the 4 of their papers we have counts for

collaborators

4 papers

nlin.CD2002★ 44 cited

To what extent can dynamical models describe statistical features of turbulent flows?

V. Carbone, R. Cavazzana, V. Antoni +9

Statistical features of "bursty" behaviour in charged and neutral fluid turbulence, are compared to statistics of intermittent events in a GOY shell model, and avalanches in differ…

nlin.CD2001★ 55 cited

Analysis of cancellation in two-dimensional magnetohydrodynamic turbulence

L. Sorriso-Valvo, V. Carbone, A. Noullez +3

A signed measure analysis of two-dimensional intermittent magnetohydrodynamic turbulence is presented. This kind of analysis is performed to characterize the scaling behavior of th…

nlin.CD2001★ 35 cited

Non-gaussian probability distribution functions in two dimensional Magnetohydrodynamic turbulence

L. Sorriso-Valvo, V. Carbone, P. Veltri +2

Intermittency in MHD turbulence has been analyzed using high resolution 2D numerical simulations. We show that the Probability Distribution Functions (PDFs) of the fluctuations of…

nlin.CD2001

Intermittency in plasma turbulence

V. Carbone, P. Giuliani, L. Sorriso-Valvo +4

Intermittency in fluid turbulence can be evidentiated through the analysis of Probability Distribution Functions (PDF) of velocity fluctuations, which display a strong non-gaussian…

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