Page 92 - Wind Energy Handbook
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66                         AERODYNAMICS OF HORIZONTAL-AXIS WIND TURBINES


          and by the time it reaches the edge viscosity has sapped much of the kinetic energy.
          As the boundary layer flows around the disc edge it accelerates causing a large
          drop in static pressure (Bernoulli). To flow around the disc edge would require very
          high velocity and there is insufficient static pressure to provide the necessary
          kinetic energy. The flow, therefore, separates from the disc and continues in the
          general stream-wise direction. In the region directly behind the disc there is slow
          moving, almost stagnant, air at the low static pressure of the flow separating at the
          disc edge. At the front of the disc, at the very centre, the flow is brought to rest and
          so there is a large increase in static pressure as the kinetic energy is converted to
          pressure energy. Elsewhere on the front surface the flow moves radially with a
          velocity, outside the boundary layer, which increases towards the disc edge. The
          static pressure is generally higher on the front of the disc than on the rear and so
          the disc experiences a pressure drag force.
            A similar process happens with a spinning rotor at high tip speed ratios. The air
          which does not pass through the rotor disc moves radially outwards and separates
          at the disc edge causing a low static pressure to develop behind the disc; the drop
          in static pressure caused by the separation increases as the tip speed ratio rises and
          the axial flow factor increases. The air which does pass through the rotor emerges
          into a low pressure region and is moving slowly. There is insufficient kinetic energy
          to provide the rise in static pressure necessary to achieve the ambient atmospheric
          pressure that must exist in the far wake. The air can only achieve atmospheric
          pressure by gaining energy from the mixing process in the turbulent wake. The
          shear layer in the flow between the free-stream air and the wake air is what
          becomes of the boundary layer that develops on the front of the disc. The shear
          layer is unstable and breaks up into the turbulence that causes the mixing and re-
          energization of the wake air.


          3.6.2 Modification of rotor thrust caused by flow separation

          The low static pressure downstream of the rotor disc caused by the separation of
          the free-stream flow at the edge of the disc and the high static pressure at the
          stagnation point on the upstream side causes a large thrust on the disc, much larger
          than that predicted by the momentum theory. Some experimental results reported
          by Glauert (1926) for a whole rotor can be seen in Figure 3.16 where the simple
          expression for the thrust force coefficient, as derived from the momentum theory
          (C T ¼ 4a(1   a)), is given for comparison.
            The thrust (or drag) coefficient for a simple, flat circular plate is given by Hoerner
          (1965) as 1.17 but, as demonstrated in Figure 3.16, the thrust on the rotating disc is
          higher. It might have been expected that when a ¼ 1 the rotor would have the same
          thrust coefficient as the circular plate. The principal difference between the circular
          plate and the rotor is that the latter is rotating and, as Hoerner also describes, this
          causes energy to be dissipated in a thicker, rotating boundary layer on the upstream
          surface of the rotor disc giving rise to an even lower pressure on the downstream
          side.
            It would follow from the above arguments that for high values of the axial
          induction factor most of the pressure drop across the disc is not associated with
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