Topic
7. Detecting electromagnetic radiation
General principle: For radio signals, the size of the receiving
antenna is about the same as the size of the wavelength it is designed to
receive.
For electromagnetic waves used for communications (radio,
TV, cell phones, etc.) , it is common to use an antenna that is one-quarter of
the wavelength of the wave to be generated.
Unlike a transmitter, the size of the antenna is often driven by other
considerations – the physical size of a cell phone, for example.
In addition to tuning the receiver based on the
length of the antenna, there are usually additional frequency-selective
elements in a receiver.
Many modern receivers use digital tuning, in which
the frequency-selection is made using software.
The radio frequency portion of the spectrum extends
from very low frequencies on the order of kHz to frequencies of 20 GHz (or even
higher in some applications). The
corresponding wavelengths range from hundreds of meters for the low frequencies
to several centimeters for the highest frequencies so that it is feasible to
construct antennas that are comparable in size to the wavelength of the desired
signal.
The wavelengths of optical signals are too short to
design antennas based on these considerations. Optical detectors tend to be
based on the interaction between the electromagnetic radiation and atoms or
molecules, which often respond only to specific wavelengths or to a specific
range of wavelengths. The details of the detection mechanism depend on the
detailed properties of the material, and understanding these mechanisms
requires complex calculations using quantum mechanics.
Since a black body absorbs all of the energy that is
incident on it and uses the energy to raise its internal temperature, the
temperature of a black body can be used as a relatively crude indicator of the
size of a received signal. By definition (a black body absorbs everything
equally well), this sort of detector cannot provide any information on the
frequency of the incident radiation. A very sensitive detector based on this
principle is called a bolometer, which is basically a black body combined with
a very sensitive thermometer.
Another common detection method uses the
photoelectric effect, in which an incident light wave transfer enough energy to
an electron in the receiving material to cause the electron to escape from the
material. The energy with which the electron is ejected from the material is
related to the wavelength of the incident radiation. This electron can be
captured by a nearby electrode, and it can be detected in this way. Variations
on this idea are used in television cameras, to turn street lights on at dusk,
etc. As with other interactions between light and matter, a detailed
understanding of the photoelectric effect requires quantum mechanics.
In addition to discrimination based on the frequency
or wavelength of a signal, many receivers include complex pattern-matching
algorithms. These algorithms are gradually growing more complex as the spectrum
becomes more crowded and more applications share the same frequency allocation.
Pattern-matching algorithms are common in cell phones, pagers, and optical
processing. They are especially important in real-world optical applications,
such as distinguishing between red T-shirts and red traffic lights.
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