I. Earth-Atmosphere System Energy Relationships

Here we'll examine what happens to the flow of radiant energy from the sun as it enters and travels through the Earth's atmosphere to the surface of the Earth

Heat Transfer :

  1. conduction: the transfer of heat energy by molecular activity - molecule to molecule contact
  2. convection: the transfer of heat energy by the movement of a mass or substance from one place to another
  3. radiation: can be transfered through a vacuum

Forms of Atmospheric Radiant Energy:

Sun (shortwave): ultraviolet, visible, near IR;

Earth-Atmos (longwave): thermal IR

Basic Radiation Laws:

  1. all objects emit radiant energy
  2. hotter objects radiate more total energy per unit area than cooler objects
  3. the hotter the radiating body, the shorter the wavelength of maximum radiation
  4. objects that are good absorbers of radiation are good emitters as well
  1. reflection - occurs at the interface between two different media (e.g. air & cloud) when some of the radiation striking the interface is thrown back

albedo - the ratio of reflected to incident radiation (an object w/albedo of 1 (or 100%) is a perfect reflector) - light colored objects have high albedos

dark objects have low albedos

2) scattering - dispersal of radiation in all directions

3) absorption - radiation is converted to heat and emits that heat (radiation) according to #2 (above)

Direct Insolation - insolation that is transmitted directly through the atmosphere to the earth's surface

Diffuse Insolation - insolation that is scattered &/or reflected to the earth's surface

The (Atmospheric) Greenhouse Effect

important selective absorbers:

water vapor (H2O) **

carbon dioxide (CO2) **

nitrous oxide (N2O)

methane (CH4)

Ozone (O3)

these gases are poor absorbers of visible (shortwave) radiation, but good absorbers of infrared (longwave) radiation