Deutsche Physikalische Gesellschaft The Institute of Physics Deutsche Physikalische Gesellschaft | Institute of Physics Quick Search:Help  
New Journal of Physics
Athens/Institutional login
IOP login: Password:   
Create account | Alerts | Contact us
IOP Journals Home | IOP Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help |
< Previous article | Next article * | This volume ^^ | This month ^ | Content finder *

Laboratory and modeling studies of cloud–clear air interfacial mixing: anisotropy of small-scale turbulence due to evaporative cooling

Szymon P Malinowski et al 2008 New J. Phys. 10 075020 (15pp)   doi: 10.1088/1367-2630/10/7/075020  Help

   PDF (3.67 MB) | HTML | References | Articles citing this article

Szymon P Malinowski1,5, Miroslaw Andrejczuk2, Wojciech W Grabowski3, Piotr Korczyk4, Tomasz A Kowalewski4 and Piotr K Smolarkiewicz3
1 Institute of Geophysics, University of Warsaw, Pasteura 7, 02-093 Warsaw, Poland
2 Los Alamos National Laboratory, Los Alamos, NM, USA
3 National Center for Atmospheric Research, Boulder, CO, USA
4 Institute of Fundamental Technological Research, Polish Academy of Sciences, Warsaw, Poland
5 Author to whom any correspondence should be addressed.
E-mail: malina@fuw.edu.pl

Part of Focus on Cloud Physics

Abstract. Small-scale mixing between cloudy air and unsaturated clear air is investigated in numerical simulations and in a laboratory cloud chamber. Despite substantial differences in physical conditions and some differences in resolved scales of motion, results of both studies indicate that small-scale turbulence generated through cloud–clear air interfacial mixing is highly anisotropic. For velocity fluctuations, numerical simulations and cloud chamber observations demonstrate that the vertical velocity variance is up to a factor of two larger than the horizontal velocity variance. The Taylor microscales calculated separately for the horizontal and vertical directions also indicate anisotropy of turbulent eddies. This anisotropy is attributed to production of turbulent kinetic energy (TKE) by buoyancy forces due to evaporative cooling of cloud droplets at the cloud–clear air interface. Numerical simulations quantify the effects of buoyancy oscillations relative to the values expected from adiabatic and isobaric mixing, standardly assumed in cloud physics. The buoyancy oscillations result from microscale transport of liquid water due to the gravitational sedimentation of cloud droplets. In the particular modeling setup considered here, these oscillations contribute to about a fifth of the total TKE production.

Received 6 February 2008
Published 31 July 2008

Bookmark and Share Post to CiteUlike | Post to Connotea | Post to Bibsonomy

 

Find related articles





Article options

Authors & Referees

 
< Previous article | Next article * | This volume ^^ | This month ^
Content finder
  Full Search
  Help


  
Setup information is available for Adobe Acrobat.
EndNote, ProCite ® and Reference Manager ® are registered trademarks of ISI Researchsoft.
Copyright © 1998-2009 Deutsche Physikalische Gesellschaft & Institute of Physics
 
Bioinspiration and Biomimetics reasearch banner