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) |
|---|---|
| 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