Dynamics of Upward Jets with Newtonian Cooling
- Authors: Goncharov V.P.1, Pavlov V.I.2
-
Affiliations:
- Obukhov Institute of Atmospheric Physics
- UFR des Mathématiques Pures et Appliquées
- Issue: Vol 126, No 2 (2018)
- Pages: 276-283
- Section: Statistical, Nonlinear, and Soft Matter Physics
- URL: https://journals.rcsi.science/1063-7761/article/view/192847
- DOI: https://doi.org/10.1134/S106377611801003X
- ID: 192847
Cite item
Abstract
The Rayleigh–Taylor instability which is responsible for the occurrence of narrow upward jets is studied in the scope of the nonhydrostatic model with horizontally nonuniform density and the Newtonian cooling. As analysis shows, the total hierarchy of instabilities in this model consists of three regimes—collapse, algebraic instability, and inertial motion. Realization of these stages, mutual transitions, and interference depend on a ratio between two characteristic time scales—collapse time and cooling time.
About the authors
V. P. Goncharov
Obukhov Institute of Atmospheric Physics
Author for correspondence.
Email: v.goncharov@rambler.ru
Russian Federation, Moscow, 109017
V. I. Pavlov
UFR des Mathématiques Pures et Appliquées
Email: v.goncharov@rambler.ru
France, Lille, F-59000
Supplementary files
