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Wake Modelling using an actuator disk model in openFOAM - DiVA PDF

152 Pages·2013·11.67 MB·English
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Wake Modelling using an actuator disk model in openFOAM Anne Mette I Nodeland Master of Energy and Environmental Engineering Submission date: June 2013 Supervisor: Lars Sætran, EPT Norwegian University of Science and Technology Department of Energy and Process Engineering Preface This thesis concludes my (cid:28)ve year Master of Technology education in En- ergy and Environmental Engineering at NTNU in Trondheim. The thesis was performed during spring 2013 and after 20 weeks and 300,000 processor hours, you (cid:28)nally hold the (cid:28)nished product in your hands. The thesis was created in collaboration with the wind department at IFE, Institute for Energy technology. I want to thank my main supervisor at IFE, Roy Stenbro, who did his best to answer all the questions I had, and to provide me with council on my ideas and problems. I am also grateful to Luca Oggiano from IFE who helped me organize the cooperation. In addition, I would like to thank Tor Anders Nyg(cid:229)rd who came with helpful knowledge within CFD. I want to extend my gratitude to Siri Kvalvig from the University of Sta- vanger and Eirik Manger at Acona Flow Technology who provided me with the model turbine set-up in OpenFOAM and took their time to answer my questions and helped me understand the actuator line model. Tommy Fredriksen also worked with the actuator line code during his mas- ter thesis, and I would like to thank him for the many hours of discussions we had about the code and our results. I would also like to thank my supervisor at NTNU Lars S(cid:230)tran, for his assistance with my thesis and for providing me with many processing hours at the NTNU supercomputer. Last but not least, I would like to thank my friend Anders who used his computer knowledge to help me improve the e(cid:30)ciency of my data process- ing,andmyfamilyandfriendssupportingmethrough(cid:28)veyearsofstudying. Anne Mette Nodeland, Trondheim 10.06.13 Abstract Two "Blind tests" have been performed at NTNU. Researchers were asked to send in results from a simulation of a model turbine in a wind tunnel to compare the di(cid:27)erent results with the measured values. There was a large spread in the simulation results, showing that additional testing and devel- opment needs to be made in order to increase the accuracy of the modelling methods. This thesis uses the "Blind test 1" as the set-up for the numerical simu- lations, and the actuator line code created by NREL to model the wind turbine. The actuator line method divides each blade into actuator line elements and distributes the forces from the line elements onto the grid. A parameter study has been performed using the actuator line code, and guidelines have been created describing how to use the code to achieve the best possible results. This thesis has pointed out a few current problems with the actuator line implementation, including a di(cid:30)culty with achieving a grid independent solution. The actuator line code mostly overestimated both thrust and power compared to the experimental values, and the best resultswherefoundfromthegridproducingtheminimumthrustandpower values. The numerical results have been compared to the "Blind test 1" and "Blind test 2" experimental values, including thrust, power and velocity de(cid:28)cit and turbulent kinetic energy in the wake behind the turbines. The hub and towerhasbeenincludedinthenumericalsimulation,provingtohavealarge e(cid:27)ect on the turbulent kinetic energy. The conclusion is that by following the introduced guidelines, the method is able to predict the experimental results from both of the "Blind tests" in a good manner. i Sammendrag To blindtester har blitt utfłrt ved NTNU. Forskere ble bedt om (cid:229) sende inn resultater fra en simulering av en modellvindmłlle i en vindtunnel, for (cid:229) sammenlignedeforskjelligeresultatenemedm(cid:229)lteverdier. Deinnsendtere- sultatenehaddestorspredning,noesomindikereratmertestingogutvikling m(cid:229) bli utfłrt for (cid:229) łke nłyaktigheten p(cid:229) simuleringsmetodene. Denne studien tar utgangspunkt i "Blind test 1" for (cid:229) lage det numeriske oppsettet, og "actuator line"-koden laget av NREL har blitt brukt til (cid:229) simulere vindturbinen. "Actuator line"-koden deler hvert blad inn i en rekke "actuator line"-elementer, for s(cid:229) (cid:229) distribuere kreftene fra elementene til cellene i det numeriske nettverket rundt. Det har blitt gjennomfłrt en parameterstudie ved (cid:229) bruke "actuator line" koden,ogretningslinjerforhvordankodenkanbrukesfor(cid:229)oppn(cid:229)bestmulig resultat har blitt laget. Denne studien har oppdaget et par problemer med denn(cid:229)v(cid:230)rendeimplementasjonenav"actuatorline"-koden,inkludertatdet er vanskelig (cid:229) oppn(cid:229) en lłsning som er uavhengig av det numeriske nettver- ket. "Actuator line"-koden overestimerer for det meste b(cid:229)de skyvekraft og e(cid:27)ekt sammenlignet med de eksperimentelle verdiene, og de beste resul- tatene ble funnet ved (cid:229) velge det numeriske nettverket som gav minimum skyvekraft og e(cid:27)ekt. De numeriske resultatene har blitt sammenlignet med de eksperimentelle verdiene fra "Blind test 1" og "Blind test 2", inkludert skyvekraft, e(cid:27)ekt og hastighet og turbulent kinetisk energi i vaken bak turbinene. Nav og t(cid:229)rn harblittinkludertidennumeriskesimuleringen, noesomvisteseg(cid:229)hastor e(cid:27)ekt p(cid:229) turbulent kinetisk energi. Konklusjonen er at ved (cid:229) fłlge de introduserte retningslinjene, klarer koden (cid:229) predikere de eksperimentelle resultatene p(cid:229) en god m(cid:229)te. ii List of symbols Roman letters A area [m2] a coe(cid:30)cient in the (cid:28)nite volume discretized equations [-] B constant in the law of the wall [-] b number of blade elements [-] c chord length [m] C drag force coe(cid:30)cient [-] D C , C , C constants in the k−(cid:15) model [-] µ 1(cid:15) 2(cid:15) C power coe(cid:30)cient [-] P C thrust coe(cid:30)cient [-] T D di(cid:27)usion conduction [kg/s] d distance [m] e unit vector [-] F convection mass (cid:29)ux [kg/s] F,f force vector [kgm/s2] g gravity vector [m/s2] i, j tensor indices [-] k turbulent kinetic energy [m2/s2] L characteristic length [m] m mass [kg] n outer normal vector [-] p,P pressure [N/s2] P power [W] r radius [m] S source term [-] Φ S non-uniform part of the source term [-] r S uniform part of the source term [-] u u,u,U,v,w velocity [m/s] uˆ,vˆ pseudo velocities in the SIMPLER algorithm [m/s] T thrust [N] iii T1 upstream turbine [-] T2 downstream turbine [-] t time [s] u friction velocity [m/s] τ V volume [m3] x,y,z Cartesian coordinates [m] Greek letters α angle of attack [-] α under-relaxation factor for the pressure [-] p ∆x,∆y,∆z grid spacings [m] δ Kronecker delta [-] ij ∂Ω boundary [m2] (cid:15) rate of viscous dissipation of k [m2/s3] (cid:15) Gaussian width parameter [m] η regulation kernel [-] (cid:15) Γ di(cid:27)usion coe(cid:30)cient [kg/sm] κ von Karmann’s constant [-] λ local pitch angle [-] µ viscosity [kg/sm] µ turbulent viscosity [kg/sm] t ν kinematic viscosity [m2/s] ρ density [kg/m3] σ Prandtl number [-] τ wall shear stress [kg/ms2] w Φ conserved variable [-] ϕ angle between relative velocity and rotor plane [-] Ω control volume [m3] ω angular rotor velocity [rad/s] Superscript iv

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program is low, and beginners are confronted with a steep learning curve. 2 The CFD tool ANSYS CFX was used, with RANS equations .. A short tutorial and.
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