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
Winds
Lesson 12
Hurricanes
Lesson 13
Global Circulation
Lesson 14
Synoptic Scale
Lesson 15
Local Circulation
Lesson 16
Satellite Oceanography
Lesson 17
Precipitation

Geometry

The directional aspects of radiative transfer are most naturally expressed in spherical coordinates, illustrated in Figure 1. Location is specified by radius r from the origin, zenith angle q, and azimuthal angle j, with differential increments dr, rdq, and . The amount of radiation depends on direction, which in three dimensions is specified with solid angle W, measured in steradians (str). The differential element dW is the product of the polar and azimuthal angle differentials. There are 4p steradians in a sphere:

Polar angle is often replaced with its cosine , so that . Polar angle is measured relative to a beam directed upwards, so q=? and µ=-1 for a beam pointing straight down and µ>0 for radiation traveling upwards.
 
 

    polar angles and solid angle
  1. Geometry in polar coordinates. Radius r is measured from the origin, zenith angle q from the vertical, and azimuthal angle j from the south.



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