Abstract
Hydrodynamic turbulence in 3D is characterized by a non-linear transfer of energy from large to small scales. Here, we provide a geometrical view of energy transfer by relating it to the deformation of fluid volumes under Lagrangian dynamics. The energy flux is parametrized in terms of the coarse-grained velocity difference tensor together with the tensor describing the shape of the volume. Our construction provides an intepretation for the non-trivial time dependence of the energy of relative motion within a "cloud" of Lagrangian particles observed in the direct numerical simulation turbulence.
Original language | English (US) |
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Pages (from-to) | 379-385 |
Number of pages | 7 |
Journal | Europhysics Letters |
Volume | 56 |
Issue number | 3 |
DOIs | |
State | Published - Nov 11 2001 |
Externally published | Yes |
ASJC Scopus subject areas
- General Physics and Astronomy