Geometrical comparison of inline and staggered stack wire mesh absorbers for solar volumetric receivers
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Abstract
Open volumetric receivers using air as the heat transfer fluid can operate at higher temperatures
and thermal efficiencies than the current state of the art in central receiver systems. Optimising
their design requires detailed understanding of two critical operational attributes: the heat
transfer coefficient (HTC) and the pressure drop. This work examines these attributes in two
dense wire mesh absorber arrangements, inline (IL) and staggered (ST), with single-mesh porosities
of 80 % and wire diameters of 0.7, 0.4 and 0.1 mm. A 2D porous model or homogeneous
equivalent model (HEM) with local thermal non-equilibrium (LTNE) is developed, using a flux
density of 600 kW/m2 and an air inlet velocity of 1 m/s. The model is experimentally validated
and subsequently used to evaluate the generalised correlations (GCs) obtained for the thermofluid-
dynamic attributes with those derived from the individual correlations (ICs). In addition,
the model assesses the impact of the different wire diameters and arrangements on thermal and
fluid flow performance. The findings reveal that the ST arrangement generally outperforms the IL
arrangement in thermal efficiency, except for the 0.1 mm wire diameter. Conversely, the IL
arrangement demonstrates superior hydrodynamic performance. Finally, the results are corroborated
with existing literature, which further validates the reliability of the numerical model and
its conclusions.
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