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Handbook of Turbomachinery Second Edition Revised - Ventech!

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Figure 22 Single-stage impulse turbine.<br />

is due to unrecoverable losses across the blade row, since the flow is<br />

nonreversible. Analytical methods exist for quantifying the difference<br />

between V2 and V1 and are mentioned in the turbine section <strong>of</strong> this chapter.<br />

With the flow conditions specified, we can set about discussion <strong>of</strong> the<br />

turbine axial force components. The resultant turbine axial force is made up<br />

<strong>of</strong> a summation <strong>of</strong> two main components. These are a pressure force on the<br />

turbine due to a static pressure difference across the rotor, and a momentum<br />

force due to a change in fluid axial momentum across the turbine. The<br />

turbine pressure force can be thought <strong>of</strong> (for convenience) as itself consisting<br />

<strong>of</strong> two components. These are a static pressure difference across the bladerow<br />

annulus, and the difference <strong>of</strong> the pressure forces acting across the top<br />

and bottom <strong>of</strong> the turbine disk. For a true impulse-type turbine stage, the<br />

blade-row annulus pressure force is obviously zero, since no static pressure<br />

difference exists across the blade row. The pressure forces acting on the top<br />

and bottom (rotor inlet and rotor outlet) sides <strong>of</strong> the turbine disk are not so<br />

straightforward. If we refer again to Fig. 22, we can see that both turbine<br />

disk faces are subjected to vortex-type flow <strong>of</strong> the turbine working fluid. In<br />

the case <strong>of</strong> the rotor inlet side, the disk (which is moving at a velocity U) is<br />

subjected to flow that moves radially inward, beginning at the disk periphery<br />

where flow is moving at a velocity V1 cos a relative to the disk. Due to<br />

interactions between the disk and the layers <strong>of</strong> fluid adjacent to it, the<br />

tangential component <strong>of</strong> the disk-relative fluid velocity is affected in a<br />

Copyright © 2003 Marcel Dekker, Inc.

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