1. CONTENT AND BASIC PROPERTIES OF THE ATMOSPHERE


1.1 Composition

The composition of the atmosphere is important in any understanding of the role which the atmosphere plays in remote sensing and in interactions with electromagnetic radiation. The atmosphere is largely a mixture of gases, some with fairly constant concentrations, others that are variable in space and time. In addition there are suspended particles (e.g. aerosol, smoke, ash etc.) and hydrometeors (e.g. cloud droplets, raindrops, snow, ice crystals, etc). About 99% of the mass lies below an altitude of 30km. Table 1 below shows the composition of the atmosphere below 100km.


Table 1: Main constituents of the earth's atmosphere

* a concentration near the earth's surface


Nitrogen, oxygen and argon account for about 99.99% of the permanent gases. Of the variable constituents, carbon dioxide can be somewhat variable in concentration on a localised basis at low levels. Water vapour content may vary from about 0 to 4%, and ozone concentrations also vary markedly. In addition to these variable constituents there are also aerosols and hydrometeors which can vary widely in space and time.

Atmospheric gases critically affect the earth's global energy balance through absorption and re-emission and through the role they play in global geophysical cycles. Solar radiation reaching the earth's surface is determined by atmospheric gases. For example harmful UV radiation is blocked by the ozone layer. Also, "windows" in which atmospheric effects are minimal allow ground-based measurements of celestial objects, and satellite-based measurements of the earth's surface or clouds for remote sensing applications.

Table 2 gives the main atmospheric gases which absorb radiation along with their absorbing regions, at ultraviolet (UV), visible, infrared (IR) and microwave wavelengths. The main spectral regions ("windows") for which atmospheric absorption is small, are listed at the bottom of the table.


Table 2: From Smith (1985), p391



Atmospheric absorption features are shown in Figure1 for ground level and at an altitude of 11 km. Regions of minimal absorption (windows) are the troughs in the curves.



Figure 1: (a) Atmospheric absorption at ground level for diffuse terrestrial radiation and for solar radiation, with a zenith angle of 50 degrees. (b) Same as in a but for the layer of atmosphere above 11km. After Wallace and Hobbs (1977), p332.


Figure 2 shows solar radiation at the top of the atmosphere and the actual radiation at sea level which has been reduced due to absorption by atmospheric gases. The dashed curve is a blackbody at 5900K for comparison with the solar curve outside the earth's atmosphere.



Figure 2: Solar irradiance at the top and bottom of the earth's atmosphere, for the sun at the zenith. Shaded areas indicate absorption by atmospheric gases. After Valley (1965).

Dr D C Griersmith