25.10.2012 Views

City of Light: The Story of Fiber Optics

City of Light: The Story of Fiber Optics

City of Light: The Story of Fiber Optics

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

A VISION OF THE FUTURE 89<br />

<strong>of</strong> the light that entered a one-mile length would emerge from the other end.<br />

(In metric terms, loss was 1.6 decibels per kilometer, and 70 percent would<br />

emerge from a one-kilometer length.) That was about 10 times better than<br />

the theoretical loss <strong>of</strong> Wheeler-style light pipes under the same conditions. 42<br />

Eaglesfield estimated his optical pipeline could carry light around very gradual<br />

bends, with a radius <strong>of</strong> about half a mile (0.8 kilometer).<br />

To test the idea, STL assembled 35 four-foot (1.2-meter) segments, coated<br />

inside with epoxy resin to provide a smooth base for the silver film. After<br />

considerable trouble joining the pipes, STL technicians stretched them along<br />

eight concrete posts sunk deep into the ground to give a sound footing. <strong>The</strong><br />

assembly was within 1/16 inch (1.6 millimeters) <strong>of</strong> being perfectly straight,<br />

but the results were disappointing. Eaglesfield had predicted 97 percent <strong>of</strong> the<br />

light should emerge after a 276-foot (84-meter) round trip, but the measured<br />

amount was under 9 percent, corresponding to a loss <strong>of</strong> more than 200<br />

decibels a mile. 43 That meant that only 10 �20 <strong>of</strong> the input light would have<br />

emerged from a mile-long pipe. Eaglesfield complained that the measurements<br />

didn’t do his idea justice, and a few years later Czech engineers did somewhat<br />

better. 44 However, Reeves held out little hope and went looking for other<br />

ideas.<br />

One came from Ramsay, who suggested arranging a series <strong>of</strong> lenses along<br />

the inside <strong>of</strong> a pipe such that each one focused an image <strong>of</strong> the previous lens<br />

onto the next lens (figure 7-3). Such a ‘‘confocal lens waveguide’’ could relay<br />

light along the pipe such that none was lost by hitting the sides. 45<br />

<strong>The</strong> little team also began looking at optical analogs <strong>of</strong> a less common<br />

kind <strong>of</strong> microwave waveguide made out <strong>of</strong> a nonconductive material like glass<br />

or plastic. <strong>The</strong> edges <strong>of</strong> such ‘‘dielectric’’ materials also can guide electromagnetic<br />

waves. <strong>The</strong> materials absorb microwaves, so thick rods that guide<br />

microwaves inside themselves do not work well. However, in the late 1940s,<br />

engineers at RCA Laboratories in Princeton found they could do much better<br />

with plastic rods thinner than about a quarter <strong>of</strong> the microwave wavelength.<br />

46 In that case, most <strong>of</strong> the microwaves travel along the outside <strong>of</strong> the<br />

waveguide, not inside where the material can absorb it. That means that thin<br />

plastic waveguides have very low loss, but only if they are perfectly straight;<br />

like many other waveguides, they radiate energy at bends. This was a serious<br />

practical problem at microwave frequencies, but it didn’t keep STL engineers<br />

from considering making dielectric waveguides <strong>of</strong> transparent materials for<br />

optical communications.<br />

Figure 7-3: A confocal waveguide guided light from lens to lens without hitting<br />

the walls <strong>of</strong> the pipe.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!