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contributor authorZhou, Xinping
contributor authorXu, Yangyang
date accessioned2019-02-28T11:07:35Z
date available2019-02-28T11:07:35Z
date copyright1/31/2018 12:00:00 AM
date issued2018
identifier issn0199-6231
identifier othersol_140_02_024502.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4252959
description abstractThis technical brief develops a theoretical model of all the pressure losses in the solar chimney power plant (SCPP, also called solar updraft power plant) and analyzes the pressure losses for different chimney internal stiffening appurtenance (SA) structures, different roof heights, and different collector support parameters. Results show that the exit dynamic pressure drop (EDPD) accounts for the majority of the total pressure loss (TPL), while other losses constitute only small proportions of the TPL, and the collector inlet loss is negligible. Pressure losses are strongly related to the mass flow rate, while reasonable mass flow rates excluding too low flow rates have little influence on the pressure loss ratios (PLRs, defined as the ratios of the pressure losses to the TPL) and the total effective pressure loss coefficient (TEPLC). Designing of the SA structure in view of reducing the drag, for example, using the ring stiffeners without wire spoked instead of the spoked bracing wheels (SBWs), reducing the width of the chimney internal rims of SAs, or reducing the number of SAs results in large reduction of the SA PLR and the TPL. Lower roof leading to higher velocity inside the collector, larger supports, or shorter intersupport distance leads to the increase in the support PLR. This technical brief lays a solid foundation for optimization of SCPPs in future.
publisherThe American Society of Mechanical Engineers (ASME)
titlePressure Losses in Solar Chimney Power Plant
typeJournal Paper
journal volume140
journal issue2
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.4038962
journal fristpage24502
journal lastpage024502-7
treeJournal of Solar Energy Engineering:;2018:;volume( 140 ):;issue: 002
contenttypeFulltext


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