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

Describing Electromagnetic Waves

Electromagnetic waves can be characterized in terms of their velocity c, the frequency of oscillation n, and the wavelength l. These quantities are related:

  1. .

  2. Wavelength is the distance between successive maxima of field strength and has dimensions of length, while frequency has dimensions of inverse time, so velocity is measured in distance per time. In a vacuum the speed of light c=m s-1. This value can change in other materials depending on the index of refraction m, which varies with frequency. In air  so c is nearly unchanged; in water at visible wavelengths , so within cloud drops the speed of light is diminished by about 25%. The inverse of wavelength is the wavenumber . In atmospheric applications wavelength is commonly measured in microns (1µm=10-6m), nanometers (1 nm=10-9 m), or Angstroms (1Å=10-10m), with frequency in megahertz (1MHz=106 s-1= 06 Hz) or gigahertz (1 GHz=109 Hz) and wavenumber expressed in inverse centimeters.

    Name
    Spectral Region
    X-rays l < 10nm
    Ultraviolet (UV) 10 < l < 400nm
    Visible 0.4 < l < 0.7µm
    Near-Infrared (Near-IR) 0.7 < l < 3.5µm
    Middle-IR 3.5< l < 30µm
    Far-IR 30 < l < 100µm
    Microwave 1mm<l<1m

    The plane in which the electric field oscillates determines the polarization of the radiation. In the atmosphere, though, this plane is rarely constant (i.e. radiation in the atmosphere is usually unpolarized) so we’ll ignore this aspect.




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