Q. What kinds of radiation pass through the atmosphere, and what kinds are absorbed?
A. Visible radiation ranges from about 0.35 to about 0.75 micrometers in wavelength. Very little visible radiation is absorbed by gases in the atmosphere. About 30-31 percent of incoming solar radiation is reflected and about 19 percent more is absorbed, mostly by clouds and particulate matter rather than by carbon dioxide and water vapor and oxygen. Those gases absorb a small amount of visible light, but not much. This is in contrast to the infrared (wavelengths greater than about 0.75 micrometer) radiation emitted by the earth's surface. This radiation has wavelengths mostly between about 2 and 20 micrometers and over 90% of it is absorbed by water vapor, carbon dioxide, methane, ozone, nitrous oxide, fluorocarbons, and other radiatively active ("greenhouse") gases on the way up.
Radiatively active gases are active in specific wavelengths of radiation. For example, if we could see in the infrared spectrum between 5 and 8 micrometers, we could not see the earth's surface (even on a clear day) from an aircraft at 10 km altitude. This is because water vapor is "opaque" in those wavelengths, and there is water vapor in the atmosphere even when there are no clouds. On the other hand, on a clear day, you can see snow-capped mountains pretty clearly at distances of over 100 km, because water vapor is transparent in the visible wavelengths. Admittedly, at large distances (e.g., about 100 km), things usually get pretty hazy because of light scattering by particulate matter and other aerosols in the atmosphere, which increase with line-of-sight distance. However, this reduction in visibility is not due to absorption by atmospheric gases. Because "seeing" in the infrared is not a part of most people's everyday experience (unless they work for the border patrol or as a bombardier), it is a little difficult to come up with "everyday" examples of what things would be like, for comparison with "everyday" visibility.
Probably the best example from "everyday" experience in the visible range, at least for those of us who fly a lot, is to notice that the moon is not any brighter when you're flying above 80% of the atmosphere than it is at the ground on a clear night. (Checking this by looking at the sun is NOT recommended, you can injure your retina pretty badly that way). If you live near the mountains, you can vary your elevation without having to fly. Also, a temperature map of the United States reveals that surface temperature is more related to latitude and distances from the coast than to elevation; the amount of solar radiation available to warm the earth's surface is about the same at high elevations as it is near sea level. In fact, at a given latitude it's often colder at higher elevations (one would expect it to be warmer if higher elevations get more solar radiation), but this is due to factors other than solar radiation.
Solar radiation" and "visible light" are not exactly the same thing. Solar radiation contains some wavelengths less than 0.35 micrometers, and some longer than 0.75 micrometers. Fortunately for us and other living things, most of the ultraviolet radiation (wavelengths shorter than visible) from the sun is picked off in the high atmosphere. This highly energetic radiation can strip electrons from atoms, causing the ionosphere and its associated phenomena such as aurora and the variations in your radio's ability to pick up distant broadcasting stations. Ozone in the middle and high stratosphere also picks off a lot of ultraviolet radiation, thereby preventing it from reaching the surface and causing skin cancers. The atmosphere's ability to absorb radiation drops off sharply between about 0.3 micrometers (near-visible ultraviolet) and 0.4 micrometers (visible blue-violet). Thus, we are protected from the harmful ultraviolet radiation, but still can see clearly for large distances. This differentiation is not always made in meteorology textbooks, so students sometimes come away thinking that the small percentage of "solar radiation" absorbed by the atmosphere is a part of the visible spectrum; instead, a lot of it is in the ultraviolet. [TJB]