Drift towards isotropization during the 3D hydrodynamic turbulence onset

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Agafontsev, D. S., Il'yn, A. S., Kopyev, A. V.
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866914304336330752
author Agafontsev, D. S.
Il'yn, A. S.
Kopyev, A. V.
author_facet Agafontsev, D. S.
Il'yn, A. S.
Kopyev, A. V.
contents The incompressible three-dimensional Euler equations develop very thin pancake-like regions of exponentially increasing vorticity. The characteristic thickness of such regions decreases exponentially with time, while the other two dimensions do not change considerably, making the flow near each pancake strongly anisotropic. The pancakes emerge in increasing number with time, which may enhance the anisotropy of the flow, especially if they orient similarly in space. In the present paper, we study numerically the anisotropy by analyzing the evolution of the so-called isotropy markers [Phys. Rev. Fluids 10, L022602 (2025)]. We show that these functions drift slowly towards unity, indicating the process of slow isotropization, which takes place without the viscous scales getting exited and despite the similar orientation of the emerging pancakes.
format Preprint
id arxiv_https___arxiv_org_abs_2512_04665
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Drift towards isotropization during the 3D hydrodynamic turbulence onset
Agafontsev, D. S.
Il'yn, A. S.
Kopyev, A. V.
Fluid Dynamics
The incompressible three-dimensional Euler equations develop very thin pancake-like regions of exponentially increasing vorticity. The characteristic thickness of such regions decreases exponentially with time, while the other two dimensions do not change considerably, making the flow near each pancake strongly anisotropic. The pancakes emerge in increasing number with time, which may enhance the anisotropy of the flow, especially if they orient similarly in space. In the present paper, we study numerically the anisotropy by analyzing the evolution of the so-called isotropy markers [Phys. Rev. Fluids 10, L022602 (2025)]. We show that these functions drift slowly towards unity, indicating the process of slow isotropization, which takes place without the viscous scales getting exited and despite the similar orientation of the emerging pancakes.
title Drift towards isotropization during the 3D hydrodynamic turbulence onset
topic Fluid Dynamics
url https://arxiv.org/abs/2512.04665