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The spectrum of light in the atmosphere and at the Earth's surface is shown below.
Insolation arrives at the edge of our atmosphere primarily as short wavelength radiation (179 kcal/cm2/yr).
The amount of insolation which reaches the Earth's surface depends on site latitude and season. Imagine a disk in front of the Earth that is just big enough to shield all solar radiation from the Earth. Each square meter of the disk surface will receive the same amount of insolation. Regions of the Earth's surface near the equator are almost parallel to the disk and will receive about the same amount of insolation/m2 if we remove the disk, but regions near the poles will receive much less insolation/m2 because the surface is at a large angle to the disk...
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