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Where am I? Sensors and Methods for Mobile Robot Positioning

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Chapter 2: Heading <strong>Sensors</strong> 37<br />

be precisely equal in length to an integral number of wavelengths at the resonant frequency. This<br />

means the wavelengths (<strong>and</strong> there<strong>for</strong>e the frequencies) of the two counter- propagating be<strong>am</strong>s must<br />

change, as only oscillations with wavelengths satisfying the resonance condition can be sustained<br />

in the cavity. The frequency difference between the two be<strong>am</strong>s is given by [Chow et al., 1985]:<br />

f 2fr6<br />

c<br />

2r6<br />

<br />

(2.3)<br />

where<br />

f = frequency difference<br />

r = radius of circular be<strong>am</strong> path<br />

6 = angular velocity of rotation<br />

= wavelength.<br />

In practice, a doughnut-shaped ring cavity would be hard to realize. For an arbitrary cavity<br />

geometry, the expression becomes [Chow et al., 1985]:<br />

f 4A6<br />

P<br />

(2.4)<br />

where<br />

f = frequency difference<br />

A = area enclosed by the closed-loop be<strong>am</strong> path<br />

6 = angular velocity of rotation<br />

P = perimeter of the be<strong>am</strong> path<br />

= wavelength.<br />

For single-axis gyros, the ring is generally <strong>for</strong>med by aligning three highly reflective mirrors to<br />

create a closed-loop triangular path as shown in Figure 2.6. (Some systems, such as Macek’s early<br />

prototype, employ four mirrors to create a square path.) The mirrors are usually mounted to a<br />

monolithic glass-cer<strong>am</strong>ic block with machined ports <strong>for</strong> the cavity bores <strong>and</strong> electrodes. Most<br />

modern three-axis units employ a square block cube with a total of six mirrors, each mounted to the<br />

center of a block face as shown in Figure 2.6. The most stable systems employ linearly polarized light<br />

<strong>and</strong> minimize circularly polarized components to avoid magnetic sensitivities [Martin, 1986].<br />

The approximate quantum noise limit <strong>for</strong> the ring-laser gyro is due to spontaneous emission in the<br />

gain medium [Ezekiel <strong>and</strong> Arditty, 1982]. Yet, the ring-laser gyro represents the “best-case” scenario<br />

of the five general gyro configurations outlined above. For this reason the active ring-laser gyro<br />

offers the highest sensitivity <strong>and</strong> is perhaps the most accurate implementation to date.<br />

The fund<strong>am</strong>ental disadvantage associated with the active ring laser is a problem called frequency<br />

lock-in, which occurs at low rotation rates when the counter-propagating be<strong>am</strong>s “lock” together in<br />

frequency [Chao et al., 1984]. This lock-in is attributed to the influence of a very small <strong>am</strong>ount of<br />

backscatter from the mirror surfaces, <strong>and</strong> results in a deadb<strong>and</strong> region (below a certain threshold of<br />

rotational velocity) <strong>for</strong> which there is no output signal. Above the lock-in threshold, output<br />

approaches the ideal linear response curve in a parabolic fashion.<br />

The most obvious approach to solving the lock-in problem is to improve the quality of the mirrors<br />

to reduce the resulting backscatter. Again, however, perfect mirrors do not exist, <strong>and</strong> some finite

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