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

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Critical angular velocities- <strong>of</strong> a singledisk<br />

rotor with allowance for gyroscopic<br />

niornen t<br />

Let the disk in a shaft-disk system be attached to the shaft<br />

asymmetrically (Fig. 3.68); therefore, during precession gyroscopic<br />

moment will act on- the shaft in addition to centrifugal force. Let<br />

us ,make- the following assumpti6ns..<br />

1)' <strong>The</strong> shaft is weightless -but it<br />

has elas-tic properties (the<br />

mass <strong>of</strong> the shaft is negligible as compared with the mass <strong>of</strong> the disfk).<br />

To reduce calculation error the weight <strong>of</strong> the shaft can be reduced<br />

to the weight <strong>of</strong> the disk.<br />

2) <strong>The</strong> shaft supports are absolutely rigid.<br />

3) <strong>The</strong> forces <strong>of</strong> resistance to the motion <strong>of</strong> the disk <strong>and</strong> the<br />

shaft are negligible.<br />

During the precession <strong>of</strong> the disk its instantaneous position<br />

in space can be determined by coordinates x, y, <strong>and</strong> z <strong>and</strong> projections<br />

0 <strong>and</strong> 4 on the xOz <strong>and</strong> yOz planes <strong>of</strong> the angle between the tangent to<br />

the elastic line at the disk attachment point <strong>and</strong> the z-axis.<br />

To obtain equations <strong>of</strong> motion for the studied system we shall<br />

ise a Lagrange equation <strong>of</strong> the 2nd kind;<br />

- .(3.105)<br />

dUti Oq Oq<br />

where q are the generalized coordinates (in our case, x, y, w<strong>and</strong> o);<br />

q = dq/•t-i-tie- gen-~lized velocity;<br />

T is the kinetic energy <strong>of</strong> the precessing disk;<br />

n is the potential energy <strong>of</strong> the system.<br />

358

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