Proposal of a fluid flow layout to improve the heat transfer in the active absorber surface of solar central cavity receivers

The main objective of concentrated solar power is to increase the thermal energy of a fluid, for the fluid to be used, for example, in a power cycle to generate electricity. Such applications present the requirement of appropriately designing the receiver active absorber surface, as the incident radiation flux can be very high. Besides that, the solar image in the receiver is not uniform, so conventional boilers designs are not well suited for these purposes. That point is particularly critical in solar central receivers systems (CRS), where concentrated solar flux is usually above 500 kW/m2, causing thermal and mechanical stress in the absorber panels.This paper analyzes a new thermofluidynamic design of a solar central receiver, which optimizes the heat transfer in the absorber surface. This conceptual receiver presents the following characteristics: the fluid flow pattern is designed according to the radiation flux map symmetry, so more uniform fluid temperatures at the receiver outlet are achieved; the heat transfer irreversibilities are reduced by circulating the fluid from the lower temperature region to the higher temperature region of the absorber surface; the width of each pass is adjusted to the solar flux gradient, to get lower temperature differences between the side tubes of the same pass; and the cooling requirement is ensured by means of adjusting the fluid flow velocity per tube, taking into account the pressure drop.This conceptual scheme has been applied to the particular case of a molten salt single cavity receiver, although the configuration proposed is suitable for other receiver designs and working fluids.

▸ The solar receiver design proposed optimizes heat transfer in the absorber surface. ▸ The fluid flow pattern is designed according to the solar flux map symmetry at noon. ▸ The fluid circulates from the lower to the higher temperature regions. ▸ The width of each pass is adjusted to the solar flux gradient. ▸ The refrigeration is ensured by means of adjusting the fluid flow velocity per tube.