Particle emissions from a high-temperature falling particle receiver with an open aperture were modeled using computational and analytical methods and compared to U.S. particle-emissions standards to assess potential pollution and health hazards. The modeling was performed subsequent to previous on-sun testing and air sampling that did not collect significant particle concentrations at discrete locations near the tower, but the impacts of wind on collection efficiency, especial for small particles less than 10 microns, were uncertain. The emissions of both large (∼350 microns) and small (<10 microns) particles were modeled for a large-scale (100 MWe) particle receiver system using expected emission rates based on previous testing and meteorological conditions for Albuquerque, New Mexico. Results showed that the expected emission rates yielded particle concentrations that were significantly less than either the pollution or inhalation metrics of 12 µg/m3 (averaged annually) and 15 mg/m3, respectively. Particle emission rates would have to increase by a factor of ∼400 (∼0.1 kg/s) to begin approaching the most stringent standards.
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11 December 2020
SOLARPACES 2019: International Conference on Concentrating Solar Power and Chemical Energy Systems
1–4 October 2019
Daegu, South Korea
Research Article|
December 11 2020
Investigating environmental impacts of particle emissions from a high-temperature falling particle receiver
Clifford K. Ho;
Clifford K. Ho
a)
1
Concentrating Solar Technologies, Sandia National Laboratories
, P.O. Box 5800, MS-1127, Albuquerque, NM 87185-1127, USA
a)Corresponding author: [email protected]
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Christian A. Pattyn
Christian A. Pattyn
2
Environmental Systems, Sandia National Laboratories
, P.O. Box 5800, Albuquerque, NM 87185, USA
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a)Corresponding author: [email protected]
AIP Conf. Proc. 2303, 030019 (2020)
Citation
Clifford K. Ho, Christian A. Pattyn; Investigating environmental impacts of particle emissions from a high-temperature falling particle receiver. AIP Conf. Proc. 11 December 2020; 2303 (1): 030019. https://doi.org/10.1063/5.0029219
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