| When a beam of light impings at some angle on the smooth
flat surface of an optically dense medium, the wave "sees" a
vast array of very closely spaced atoms that will somehow scatter it. (At
the wavelengths of light -- d=500nm -- the Earch's atmosphere at STP has
about 106 molecules in such a d3-cube). As the
wavefront descends, it excites one scatterer after another, each of which
reradiates a stream of photons that can be thought of as a hemispherical
wavelet in the incident medium. Because the wavelength is so much greater
than the separation between the molecules, the wavelets advance together
and add constructively in only one directions, and there is one
well-defined reflected beam. The wavelets bend as they cross the
boundary, because of the speed change. For similar reason, they form one
well-defined refracted beam.

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