A Linear Stability Study of the Gradient Zone of a Solar Pond

Author:

Rebaï L. Kaffel1,Mojtabi A. K.2,Safi M. J.3,Mohamad A. A.4

Affiliation:

1. Unité de Recherche en Mécanique et Energétique, Ecole Nationale d’Ingénieurs de Tunis, 2000 Tunis, Tunisia and IMFT, UMR 5502 CNRS, Université Paul Sabatier, 118 route de Narbonne, 31062 Toulouse, France

2. IMFT, UMR 5502 CNRS, Université Paul Sabatier, 118 route de Narbonne, 31062 Toulouse, France

3. Unité de Recherche en Mécanique et Energétique, Ecole Nationale d’Ingénieurs de Tunis, 2000 Tunis, Tunisia

4. Department of Mechanical and Manufacturing Engineering, The University of Calgary, Calgary, AB, T2N 1N4, Canada

Abstract

The linear stability of a plane layer with horizontal temperature and concentration stratification corresponding to gradient zone of a solar pond is investigated. The problem is described by Navier-Stokes equations with Boussinesq-Oberbeck approximation. Two source terms are introduced in the energy equations: the absorption of solar energy characterized by the extinction radiative coefficient μe and by the parameter f defined as the ratio of extracted heat flux to absorbed heat flux in the lower convective zone. The influence of the parameters μe and f on the onset of thermosolutal convection in the case of confined and infinite layers is analyzed. It is found that convection starts in an oscillatory state, independently of the RaS value. Different convection solutions were found for marginal stability and steady state.

Publisher

ASME International

Subject

Energy Engineering and Power Technology,Renewable Energy, Sustainability and the Environment

Reference17 articles.

1. The Physics of the Solar Pond;Weinberger;Sol. Energy

2. Solar Ponds;Tabor;Sol. Energy

3. Solar Ponds for Space Heating;Rabl;Sol. Energy

4. Salinity—Gradient Solar Ponds

5. Physical Model of Gradient Zone Erosion in Thermohaline Systems;Hull;Int. J. Heat Mass Transfer

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