Numerical modelling of wind and dust patterns around a full-scale paraboloidal solar dish

dc.contributor.authorChristo, F.C.
dc.date.issued2012
dc.description.abstractThis study reports on numerical predictions of velocity and pressure fields, and dust particles trajectories in steady and unsteady flows around a full-scale paraboloidal solar dish. Calculations are performed for three wind speeds of 4.16, 9.72, and 15.2 m s-1, and dish pitch angles from 0 degrees to 180 degrees. The flow field structure, lift and drag coefficients are calculated for each flow configuration. Using the predicted mean flow velocity field, analytical expressions for the aerodynamic coefficients, as a function of the pitch angle, are developed. The unsteady-state flow is characterised by formation of stable vortices behind the dish for most flow configurations, except at 60 degrees and 150 degrees pitch angles. At these angles vortex-shedding occurred with a strong flow oscillation extending downstream the dish. The calculations of dust particles trajectories provide a qualitative assessment of the deposition rate, dish orientation, and surface locations where dust accumulation is most likely to occur. The study also presents an initial assessment of the effectiveness of various windbreaks installed upstream of the dish in reducing aerodynamics drag.
dc.identifier.citationRenewable Energy, 2012; 39(1):356-366
dc.identifier.doi10.1016/j.renene.2011.08.038
dc.identifier.issn0960-1481
dc.identifier.urihttps://hdl.handle.net/1959.8/123630
dc.language.isoen
dc.publisherPergamon
dc.rightsCopyright 2011 Elsevier
dc.source.urihttps://doi.org/10.1016/j.renene.2011.08.038
dc.subjectturbulent flow
dc.subjectdust deposition
dc.subjectparaboloidal solar dish
dc.subjectCFD
dc.subjectwindbreaks
dc.titleNumerical modelling of wind and dust patterns around a full-scale paraboloidal solar dish
dc.typeJournal article
pubs.publication-statusPublished
ror.mmsid9915909580001831

Files

Collections