Falling particle receivers are being evaluated as an alternative to conventional fluid-based solar receivers to enable higher temperatures and higher efficiency power cycles with direct storage for concentrating solar power (CSP) applications. This paper presents studies of the particle mass flow rate, velocity, particle-curtain opacity and density, and other characteristics of free-falling ceramic particles as a function of different discharge slot apertures. The methods to characterize the particle flow are described, and results are compared to theoretical and numerical models for unheated conditions. Results showed that the particle velocities within the first 2 m of release closely match predictions of free-falling particles without drag due to the significant amount of air entrained within the particle curtain, which reduced drag. The measured particle-curtain thickness (∼2 cm) was greater than numerical simulations, likely due to additional convective air currents or particle–particle interactions neglected in the model. The measured and predicted particle volume fraction in the curtain decreased rapidly from a theoretical value of 60% at the release point to less than 10% within 0.5 m of drop distance. Measured particle-curtain opacities (0.5–1) using a new photographic method that can capture the entire particle curtain were shown to match well with discrete measurements from a conventional lux meter.
Characterization of Particle Flow in a Free-Falling Solar Particle Receiver / Ho, Clifford K.; Christian, Joshua M.; Romano, David; Yellowhair, Julius; Siegel, Nathan; Savoldi, Laura; Zanino, Roberto. - In: JOURNAL OF SOLAR ENERGY ENGINEERING. - ISSN 0199-6231. - STAMPA. - 139:2(2016), p. 021011.
|Titolo:||Characterization of Particle Flow in a Free-Falling Solar Particle Receiver|
|Data di pubblicazione:||2016|
|Digital Object Identifier (DOI):||http://dx.doi.org/10.1115/1.4035258|
|Appare nelle tipologie:||1.1 Articolo in rivista|