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Infrared energy is just one part of the electromagnetic spectrum that
encompasses radiation from gamma rays, x-rays, ultra violet, a thin
region of visible light, infrared, terahertz waves, microwaves, and
radio waves. These are all related and differentiated in the length of
their wave (wavelength). All objects emit a certain amount of black body
radiation as a function of their temperatures. Generally speaking, the
higher an object's temperature is, the more infrared radiation as
black-body radiation it emits. A special camera can detect this
radiation in a way similar to an ordinary camera does visible light. It
works even in total darkness because ambient light level does not
matter. This makes it useful for rescue operations in smoke-filled
buildings and underground.
Images from infrared cameras tend to have a single color channel
because the cameras generally use a sensor that does not distinguish
different wavelengths of infrared radiation. Color cameras require a
more complex construction to differentiate wavelength and color has less
meaning outside of the normal visible spectrum because the differing
wavelengths do not map uniformly into the system of color vision used by
humans. Sometimes these monochromatic images are displayed in
pseudo-color, where changes in color are used rather than changes in
intensity to display changes in the signal. This is useful because
although humans have much greater dynamic range in intensity detection
than color overall, the ability to see fine intensity differences in
bright areas is fairly limited. This technique is called density
slicing.
For use in temperature measurement the brightest (warmest) parts of
the image are customarily colored white, intermediate temperatures reds
and yellows, and the dimmest (coolest) parts blue. A scale should be
shown next to a false color image to relate colors to temperatures.
Their resolution is considerably lower than of optical cameras, mostly
only 160x120 or 320x240 pixels. Thermographic cameras are much more
expensive than their visible-spectrum counterparts, and higher-end
models are often deemed as dual-use and export-restricted.
In uncooled detectors the temperature differences at the sensor
pixels are minute; a 1 °C difference at the scene induces just a 0.03 °C
difference at the sensor. The pixel response time is also fairly slow,
at the range of tens of milliseconds.
Thermal imaging photography finds many other uses. For example,
firefighters use it to see through smoke, find persons, and localize
hotspots of fires. With thermal imaging, power line maintenance
technicians locate overheating joints and parts, a telltale sign of
their failure, to eliminate potential hazards. Where thermal insulation
becomes faulty, building construction technicians can see heat leaks to
improve the efficiencies of cooling or heating air-conditioning. Thermal
imaging cameras are also installed in some luxury cars to aid the
driver, the first being the 2000 Cadillac DeVille. Some physiological
activities, particularly responses, in human beings and other
warm-blooded animals can also be monitored with thermographic imaging.
Cooled infrared cameras can also be found at most major astronomy
research telescopes. Thermographic image of a ringtailed lemur
Thermographic image of a snake around an arm Thermographic image of
several lizards [edit] Types
Thermographic cameras can be broadly divided into two types: those
with cooled infrared image detectors and those with uncooled detectors.
[edit] Cooled infrared detectors
Cooled detectors are typically contained in a vacuum-sealed case or
Dewar and cryogenically cooled. The cooling is necessary for the
operation of the semiconductor materials used. Typical operating
temperatures range from 4 K to just below room temperature, depending on
the detector technology. Most modern cooled detectors operate in the 60
K to 100 K range, depending on type and performance level. Without
cooling, these sensors (which detect and convert light in much the same
way as common digital cameras, but are made of different materials)
would be 'blinded' or flooded by their own radiation. The drawbacks of
cooled infrared cameras are that they are expensive both to produce and
to run. Cooling is power-hungry and time-consuming. The camera may need
several minutes to cool down before it can begin working. The most
commonly used cooling systems are rotary Stirling engine cryocoolers.
Although the cooling apparatus is comparatively bulky and expensive,
cooled infrared cameras provide superior image quality compared to
uncooled ones. Additionally, the greater sensitivity of cooled cameras
also allow the use of higher F-number lenses, making high performance
long focal length lenses both smaller and cheaper for cooled detectors.
An alternative to Stirling engine coolers is to use gases bottled at
high pressure, nitrogen being a common choice. The pressurised gas is
expanded via a micro-sized orifice and passed over a miniature heat
exchanger resulting in regenerative cooling via the Joule–Thomson
effect. For such systems the supply of pressurized gas is a logistical
concern for field use.
Materials used for cooled infrared detection include photodetectors
based on a wide range of narrow gap semiconductors including:
* indium antimonide (3-5 μm) * indium arsenide * mercury cadmium
telluride (MCT) (1-2 μm, 3-5 μm, 8-12 μm) * lead sulfide * lead selenide
Infrared photodetectors can be created with structures of high band
gap semiconductors such as in Quantum well infrared photodetectors.
A number of superconducting and non-superconducting cooled bolometer
technologies exist.
In principle, superconducting tunneling junction devices could be
used as infrared sensors because of their very narrow gap. Small arrays
have been demonstrated. Their wide range use is difficult because their
high sensitivity requires careful shielding from the background
radiation.
Superconducting detectors offer extreme sensitivity, with some able
to register individual photons. For example ESA's Superconducting camera
(SCAM). However, they are not in regualr use outside of scientific
research. [edit] Uncooled infrared detectors Thermal imaging camera &
screen, photographed in an airport terminal in Greece. Thermal imaging
can detect elevated body temperature, one of the signs of the virus H1N1
(Swine influenza).
Uncooled thermal cameras use a sensor operating at ambient
temperature, or a sensor stabilized at a temperature close to ambient
using small temperature control elements. Modern uncooled detectors all
use sensors that work by the change of resistance, voltage or current
when heated by infrared radiation. These changes are then measured and
compared to the values at the operating temperature of the sensor.
Uncooled infrared sensors can be stabilized to an operating temperature
to reduce image noise, but they are not cooled to low temperatures and
do not require bulky, expensive cryogenic coolers. This makes infrared
cameras smaller and less costly. However, their resolution and image
quality tend to be lower than cooled detectors. This is due to
difference in their fabrication processes, limited by currently
available technology.
Uncooled detectors are mostly based on pyroelectric and ferroelectric
materials [1] or microbolometer technology. The material are used to
form pixels with highly temperature-dependent properties, which are
thermally insulated from the environment and read electronically.
Ferroelectric detectors operate close to phase transition temperature
of the sensor material; the pixel temperature is read as the highly
temperature-dependent polarization charge. The achieved NETD of
ferroelectric detectors with f/1 optics and 320x240 sensors is 70-80 mK.
A possible sensor assembly consists of barium strontium titanate
bump-bonded by polyimide thermally insulated connection.
Silicon microbolometers can reach NETD down to 20 mK. They consist of
a thin film vanadium pentoxide sensing element suspended on silicon
nitride bridge above the silicon-based scanning electronics. The
electric resistance of the sensing element is measured once per frame.
Current improvements of uncooled focal plane arrays (UFPA) are
focused primarily on higher sensitivity and pixel density.
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