Preliminary investigation into two-way fluid structure interaction of heliostat wind loads Josh Wolmarans

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Preliminary investigation into two-way fluid structure interaction of heliostat wind loads Josh Wolmarans Supervisor: Prof Ken Craig Clean Energy Research Group (CERG), Department of Mechanical and Aeronautical Engineering, UNIVERSITY OF PRETORIA STERG SolarPACES symposium, 13-14 July 2017 Stellenbosch 1

Outline Introduction ABL validation LH-2 validation Matty validation FSI validation 2-way FSI 2

Introduction Trends show shift to renewable energy sector, especially solar energy CSP technology has advantage of storing heat during times of no sun Central Receivers consist of an array of heliostats that reflect solar radiation to a central receiver Designs may differ significantly Cost-saving in heliostat design can be significant 3

Peterka-ABL validation Characterize the Atmospheric Boundary Layer (ABL) Homogeneous- inlet, approach, incident profiles Horizontally homogeneous High mesh near surface Roughness length < roughness height Log law profile, not a power law Equation used to match velocity profile (U(z)) using leastsquares approach, similar equation used for Turbulence Intensity (TI) Can optimize for velocity or turbulence, not both Peterka (1986) 4

LH-2 steady-state validation using RWDI data The LH-2 heliostat is used in the Brightsource Ivanpah project 173 500 heliostats in three power plants Steady-state CFD validation done using RWDI experimental data (Huss, S (2011)) Employed realizable k-ε (RKE) Reynolds Averaged Navier- Stokes (RANS) Better results than RWDI CFD for most elevation angles WT=wind tunnel CFD=current CFD 5

LH- 2 computational model Block-structured mesh of domain before adaption with roughly 4.7mil cells 6

LH-2 Transient simulation Unsteady RANS (URANS) in attempt to capture vortex shedding A regional mesh adaption in ANSYS Fluent Mesh of roughly 8 million cells k-ω SST model was used instead of the more accurate RKE Run at the CHPC using 192 cores, 30 hours Drag of heliostat and velocity in wake of heliostat 7

LH-2 Modal analysis A structural modal analysis was performed Possible resonance failure of the heliostat is investigated Matty (1979) predicted the vortex frequency could be roughly 1.4Hz to 2Hz for a velocity of 45m/s for a square-plate heliostat Vortex shedding may therefore excite the natural frequencies Case for 2-way fluid structure interaction Mode Freq [Hz] 1 1.8294 2 2.1829 ANSYS Mechanical model 3 2.6907 4 5.4507 5 6.0299 6 6.2795 7 7.4327 8 12.627 9 17.216 10 17.783 8

Matty Validation Matty (1979) is used as an additional transient validation case for the URANS simulations Reynolds number of around 150 000 k-ω SST used instead of RKE Cell count of 2.5mil adapted up to about 10 million cells Run on the CHPC with 192 cores Computational domain Simplified Heliostat in upright position 9

Matty Validation (cont.) Run for 10sec (25 domain flow-throughs) Transient behaviour found in drag and velocity point monitors The FFT shows a dominating frequency of 6.1Hz,within 17.3% of the 7.38Hz Matty experiments 2-way FSI may be plausible with URANS Scaled up in ANSYS Fluent to simulate the LH-2 Re of 2.5million: no transient behaviour observed Vortex shedding may not be attainable with URANS for this geometry and Re number 10

FSI Validation test case 2-way FSI validation using ANSYS WorkBench system coupling 2-D fixed sphere, slightly off centre, flexible beam attached to the rear as seen below (T Dunne and R Rannacher (2006)) FSI on 3-D geometry so 1-cell thick domain was used Beam displacement at point A as well as FFT available A Oscillation of beam obtained as 1.953Hz (exactly the same benchmark) Lift coefficient oscillation obtained as 4.4Hz (benchmark is given as 4.99Hz) Successful validation for laminar case 11

FSI Validation (cont.) Turbulent LES FSI validation was carried out by Breuer,M (2010) on the same case Fluid density 1000 times smaller the FFT finds a Strouhal number 0.175 which is the same as the rigid body case Implementation in ANSYS WB 12

LH-2 2-way FSI (in progress) 1-way FSI as well as static data transfers between CFD and Mechanical models have been conducted in the ANSYS environment 2-way FSI using URANS with ANSYS system coupling has been performed on various fluid mesh sizes ranging from 1 to 10 mil The ANSYS WorkBench setup is seen below for full 2- way FSI of the LH-2 heliostat 13

LH-2 2-way FSI (cont.) Preliminary results for the smaller mesh cases show no transient behaviour in the fluid flow and decaying transient behaviour from the structure due to the initial displacement. Smaller cases run on 8 cores for 5 days 10 million cell case run on 16 cores for 5 days for 18% completion only System coupling seems to be buggy and very computationally intensive (even for URANS) Not computationally realistic to use Scale-Resolving Simulation (SRS) CFD (e.g., DES, ELES) ANSYS WB graphical environment not currently available at the CHPC 14

Future work 2-D vortex shedding URANS simulations to establish shedding frequencies cheaply 2-D 2-way FSI simulations provided the CFD is successful High fidelity Scale Resolving Simulation of the LH-2 using SAS, DES or ELES. External data import 1-way FSI using the SRS CFD data Relatively cheap structural optimisation of the LH-2 using the same SRS data 15

Thank You 16