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- The long pathlength through the atmosphere when the sun is low
give means lots of blue and green photons get scattered out of
the line of sight leaving only the red light.
One more interesting sidelight:
Because of the gradient in atmosphere's density, it acts like a prism
- Red light is less ``bent'' than green or blue light so the ``red''
Sun sets first, followed by the ``green'' Sun, then the ``blue''
Sun. When the Sun is low on the horizon, all the blue light gets
scattered out, so, the last thing you see is a ``green flash''.
- When you see the Sun hit the horizon, it is already a full solar
diameter below the horizon.
Michael Bolte
Tue Jan 6 14:48:33 PST 1998