Lesson 1
Meteorological Satellite Orbits
Lesson 2
Review of Radiative Transfer
Lesson 3
Visible Image Interpretation
Lesson 4
Infrared Image Interpretation
Lesson 5
Multispectral Image Interpretation
Lesson 6
Fires & Aerosols
Lesson 7
Winds
Lesson 8
Sounders
Lesson 9
Fog and Stratus
Lesson 10
Thunderstorm
Lesson 11
Energy Budget
Lesson 12
Hurricanes
Lesson 13
Global Circulation
Lesson 14
Synoptic Scale
Lesson 15
Local Circulation
Lesson 16
Satellite Oceanography
Lesson 17
Precipitation

Lesson 2: Practice

A useful form of the equation for the transfer of infrared radiation is

Il is the observed radiance at wavelength l , Tsfc is the surface temperature, Tlis the transmittance and Bl(T) is the Planck function containing information on the atmospheric temperature. The term

is referred to as the weighting function. The intensity measured by a satellite radiometer due to the emission from a layer in the atmosphere at location z, is determined from the layer black body emission Bl(T)weighted by the factor W(z). The weighting function is of fundamental importance to vertical sounding the atmosphere from satellite observations. The weighting distribution depends on the strength and distribution of the absorbing gas.

Use this applet to explore the relationship between line-strength and gas concentration on the weighting function.

Radiation multiple choice



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