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Theoretical and Numerical Investigation of Flow Stability in Porous Materials Applied as Volumetric Solar Receivers

Becker, Manfred and Fend, Thomas and Hoffschmidt, Bernhard and Pitz-Paal, Robert and Reutter, Oliver and Stamatov, Veselin and Steven, Martin and Trimis, Dimosthenis (2006) Theoretical and Numerical Investigation of Flow Stability in Porous Materials Applied as Volumetric Solar Receivers. Solar Energy (80), pp. 1241-1248.

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Abstract

Hot spots have been experimentally observed in porous materials in several applications as volumetric solar receivers. In this application, cold ambient air flows through a solid, which is heated by concentrated solar radiation. After that the hot porous material transfers the heat to the cold air flow. The heated air then transfers its heat to an air-water heat exchanger. The evaporated water drives a conventional steam turbine process. To obtain high efficiencies, a high absorptivity in the visible and near infrared range has to be combined with a high porosity of the volumetric solar receiver to create large surfaces for convective heat transfer from the solid absorber to the fluid. For the durability of the receiver materials it is of key importance to avoid the occurrence of hot spots. Following studies showed that these hot spots have been caused by flow instabilities, which generally may occur, if cold air flows through a heated porous material. This phenomenon is due to the temperature dependent viscosity properties of air. In a theoretical analysis it could be shown that heat conductivity as well as permeability properties of the porous materials have significant influence on the probability of the occurrence of flow instabilities. A numerical study has been performed to investigate the occurrence of instable flow in heated ceramic foam materials. In the simulations a constant heat flow of radiation, that is absorbed in a defined volume, and constant permeability coefficients are assumed. Boundary conditions similar to those of the 10MW Solucar Solar project have been chosen. In a three dimensional, heterogeneous two phase heat transfer model it was possible to simulate local overheating of the porous structure. The parameters heat conductivity, turbulent permeability coefficient and radial dispersion coefficient have been varied systematically. Consequently, for a heat flux density of 1 MW/m2 a parameter chart could be generated, showing the possible occurrence of “instable” or “stable” thermal and fluid mechanical behaviour. These numerical results are beneficial for the design of optimized materials for volumetric receivers. In order to be able to make use of these results, a precise knowledge of the mentioned quantities heat conductivity, turbulent permeability coefficient and radial dispersion coefficient is necessary. Experimental methods to determine these quantities are described or reviewed.

Item URL in elib:https://elib.dlr.de/46288/
Document Type:Article
Title:Theoretical and Numerical Investigation of Flow Stability in Porous Materials Applied as Volumetric Solar Receivers
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Becker, ManfredUNSPECIFIEDUNSPECIFIED
Fend, ThomasUNSPECIFIEDUNSPECIFIED
Hoffschmidt, BernhardSolar Institut JülichUNSPECIFIED
Pitz-Paal, RobertUNSPECIFIEDUNSPECIFIED
Reutter, OliverUNSPECIFIEDUNSPECIFIED
Stamatov, VeselinUniversität Erlangen-NürnbergUNSPECIFIED
Steven, MartinUniversität Erlangen-NürnbergUNSPECIFIED
Trimis, DimosthenisUniversität Erlangen-NürnbergUNSPECIFIED
Date:2006
Journal or Publication Title:Solar Energy
Open Access:Yes
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Page Range:pp. 1241-1248
Status:Published
Keywords:Instable Flow Solar Air Receiver
HGF - Research field:Energy
HGF - Program:Renewable Energies
HGF - Program Themes:E SF - Solar research (old)
DLR - Research area:Energy
DLR - Program:E SF - Solar research
DLR - Research theme (Project):E - Applikationsentwicklung (old)
Location: Köln-Porz
Institutes and Institutions:Institute of Engineering Thermodynamics > Solar Research
Deposited By: Fend, Dr.-Ing. Thomas
Deposited On:04 Jan 2007
Last Modified:31 Jul 2019 19:18

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