You don't know what you're talking about. The reason the light is "redder in the fall is because the earth is moving away from the sun. This stretches or lengthens the light waves and creates a red shift. As we get closer to the sun in the spring and early summer, this wave becomes compressed and creates a "blue shift". That is why a bluer spectrum is better for vegging and a redder spectrum is better for budding.
But... In Autumn, we are moving towards the sun. It's the angle (of inclination? I've been up like three days straight and worked my eight plus a few OT today, lol) that changes (causing Winter to be... Winter. Which is why when we have Winter, the opposite point on the planet has Summer, and why the equator has tropical weather most of the time). Err... I didn't state that well, but we're closest to the sun in deepest Winter.
If the planet is moving towards/away from the sun, it's going to be the whole planet - not just half of it - so that red-/blue-shift would be the same planetwide.
I was also under the impression that this phenomenon was best measured (without instrumentation, I mean, such as that perceivable by the eye as far as visible light - for example - is concerned; obviously that's how radar guns work) in velocities approaching the relativistic. A 1% redshift corresponds to 1% of the speed of light (
relatively speaking, lol). Also in LARGE distances. Often extra-galactic, and when the terms of "local" and "nearby" observations are mentioned, they generally mean "within the Milky Way Galaxy."
Oh yeah, there's something that I'm missing (the answer), but I'm wiped.