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2.1.2: Selective Absorption by the Atmosphere

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    21650
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    The gasses that comprise our atmosphere are selective absorbers of radiation because each gas absorbs only particular wavelengths of light. Selective absorption by particular gasses and the atmosphere as a whole is shown in Figure \(\PageIndex{1}\). The graph shows very little absorption for the atmosphere as a whole in the shortwave end of the spectrum, especially in the visible light band (the band of maximum emission for the Sun), from 0.4 to 0.75 micrometers. The atmosphere absorbs far better in the longwave end of the electromagnetic spectrum which is the region of maximum emission (10\(\mu m\)) for the Earth. The human eyes (and animal eyes) have evolved over millions of years to see exactly that light that is most abundantly available, i.e. shortwave light that is not absorbed by the atmosphere.

    selective absorbers
    Figure \(\PageIndex{1}\): Absorption of the entire atmosphere and of selected gasses in the atmosphere.

    The IR (infra-red) windows are found at about 8 - 14 \(\mu m\). It is through this portion of the electromagnetic spectrum that infrared radiation is transferred through the atmosphere and into space. These windows can be "closed" by clouds which absorb infrared radiation. That is why the earth's surface and the air above it are warmer on mornings after cloudy nights than on mornings after clear nights: the clouds absorb and re-emit some of the outgoing IR (infra-red) radiation.

    To understand why the atmosphere behaves as a selective absorber, see "Digging Deeper: Selective Absorption by the Atmosphere" or continue reading.


    2.1.2: Selective Absorption by the Atmosphere is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by LibreTexts.