|
 |
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:
-
.
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.
Next
Back
Return to Lesson 2
Return to Satellite Meteorology Main Page
|