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Appendix A — GPS Primer<br />

Knowing your distance from Point C further refines the positional information (see Figure A-4).<br />

A<br />

B<br />

You are here<br />

FIGURE A-4: Knowing your distance from three points provides a lot of information.<br />

This is an example of two-dimensional trilateration (2-D trilateration). What GPS does is take<br />

this into three dimensions (3-D trilateration or triangulation).<br />

In principle, three-dimensional trilateration doesn’t differ much from two-dimensional trilateration,<br />

but it is trickier to grasp. What you need to do is imagine the radii of the circles from the<br />

preceding examples going off in all directions, so instead of a getting a series of circles, you get<br />

a series of spheres.<br />

If you know you are fifteen miles from Point A (or satellite A in the sky), you could be anywhere<br />

on the surface of a huge, imaginary sphere with a fifteen-mile radius. If you also know you are<br />

eighteen miles from satellite B, you can overlap the first sphere with second, larger sphere. These<br />

spheres all intersect in a perfect circle. Finally, if you know the distance to satellite C, you get a<br />

third sphere, which will intersect with the other circles at two points, as shown in Figure A-5.<br />

The Earth itself acts as another sphere. It is assumed that you are on the Earth, so you can<br />

eliminate the other point in outer space, as shown in Figure A-6.<br />

C<br />

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