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Design and Stress Analysis of Extraterrestrial ... - The Black Vault

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a) arB 0 if the disk does not bear a load on the external radius;<br />

b) are = ar .if blades are attached on the disk crown.<br />

Allowing for nonuniform disk heating<br />

(determining thermal stresses)<br />

In turbine operation heat flux is propagated from blades through<br />

the joints to the disk, <strong>and</strong> in the disk from the crown to the hub.<br />

Thus, disk temperature rises along the radius from the center to the<br />

crown. Due to this, thermal stresses appear in the disk, which<br />

can be <strong>of</strong> the same order <strong>of</strong> magnitude as the stresses from centrifugal<br />

forces, <strong>and</strong> they must be taken into account.<br />

<strong>The</strong>rmal stresses can be determined separately for nonrotating<br />

disks <strong>and</strong> then algebraically added with the stresses from centrifugal<br />

forces.<br />

In order to avoid high thermal stresses, the disk material must<br />

have the smallest possible coefficient <strong>of</strong> linear expansion (thermal<br />

strain will be less) <strong>and</strong> considerable heat conductivity (temperature<br />

gradient along the disk radius will be less).<br />

<strong>The</strong> disk material<br />

must have the appropriate mechanical properties with allowance for<br />

their reduction at high temperatures.<br />

In our analysis we shall assume that the temperature in the<br />

disk changes only along the radius (on a given radius we shall assume<br />

the temperature is constant throughout the -hickness).<br />

<strong>The</strong> modulus <strong>of</strong> elasticity E <strong>and</strong> the coefficient <strong>of</strong> linear<br />

expansion a will be considered constant within each <strong>of</strong> the sections<br />

in which the disk is divided during analysis.<br />

<strong>The</strong> equation <strong>of</strong> equilibrium for a nonrotating disk is obtained<br />

2<br />

from equation (3.55) if we assume C = pw = 0:<br />

S~316<br />

d (,rzh)<br />

dr "(3.69)<br />

31<br />

1*..-i

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