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| "Night Vision” as
referenced here is that technology that provides us with the miracle of vision
in total darkness and the improvement of vision in low light environments. This
technology is an amalgam of several different methods each having its own
advantages and disadvantages. The most common methods as described below are
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and
. The most common applications include night driving or flying, night security and
surveillance, wildlife observation, sleep lab monitoring and search and rescue.
A wide range of are available to suit the various requirements
that may exist for these applications
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Low-Light
Imaging
Today, the most popular and well known method of performing night vision is
based on the use of image intensifiers. are commonly used in and
. More recently, on-chip gain multiplication CCD cameras have become
popularized for performing low-light security, surveillance and astronomical
observation.
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| Image intensifiers |
| How they work: This method of night vision amplifies
the available light to achieve better vision. An objective lens focuses
available light (photons) on the photocathode of an image intensifier. The
light energy causes electrons to be released from the cathode which are
accelerated by an electric field to increase their speed (energy level). These
electrons enter holes in a microchannel plate and bounce off the internal
specially-coated walls which generate more electrons as the electrons bounce
through. This creates a denser “cloud” of electrons representing an intensified
version of the original image. |
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The final stage of the image intensifier involves electrons hitting a phosphor
screen. The energy of the electrons makes the phosphor glow. The visual light
shows the desired view to the user or to an attached photographic camera or
video device. A green phosphor is used in these applications because the human
eye can differentiate more shades of green than any other color, allowing for
greater differentiation of objects in the picture. |
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| All image intensifiers operate in the above fashion. Technological
differences over the past 40 years have resulted in substantial improvement to
the performance of these devices. The different paradigms of technology have
been commonly identified by distinct
. Intensified camera systems usually incorporate an image intensifier to create a
brighter image of the low-light scene which is then viewed by a traditional
camera. |
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Excellent low-light level sensitivity
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Enhanced visible imaging yields the best possible recognition and
identification performance.
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High resolution
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Low power and cost
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Ability to identify people
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Because they are based on amplification methods, some light is required. This
method is not useful when there is essentially no light.
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Inferior daytime performance when compared to daylight-only methods
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Possibility of blooming and damage when observing bright sources under
low-light conditions.
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| Image intensifier based products: |
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| On-chip Gain
Multiplication Cameras |
| How they work: In order to overcome some of the disadvantages of image
intensifiers, CCD image detector manufacturers have substantially improved the
sensitivity of certain CCD detectors by incorporating an on-chip multiplication
gain technology to multiply photon-generated charge above the detector’s noise
levels. The multiplication gain takes place after photons have been detected in
the device’s active area but before one of the detector’s primary noise sources
(e.g. readout noise). In a new multiplication register, electrons are
accelerated from pixel-to-pixel by applying high CCD clock voltages. As a
result, secondary electrons are generated via an impact-ionization process.
Gain can be controlled by varying the clock voltages. |
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| Because the signal boost occurs before the charge reaches the
on-chip readout amplifier and gets added to the primary noise source, the
signal-to-noise ratio for this device is significantly improved over standard
CCD cameras and yields low-light imaging performance far superior than
traditional CCD cameras. However, since the CCD temperature also affects the
on-chip gain multiplication (lower temperatures yield higher gain) and because
other noise sources exist that occur before the multiplication (i.e. dark
noise), it is prudent in these systems to temperature stabilize these detectors
at temperatures about of below room temperature. |
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| Another method for improving a CCD camera’s sensitivity is to
perform averaging to reduce noise either temporally (where sequential video
frames are averaged) or spatially (where neighboring pixels are “binned” or
added together). |
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High sensitivity in low-light.
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Reduced likelihood of damage to the imaging detector due to viewing bright
sources.
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High speed imaging capability.
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Good daytime imaging performance.
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High power dissipation due to the necessity to have a temperature stabilizer.
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Blooming when viewing bright sources in dark scenes.
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| On-chip Gain Multiplication
Camera-based products: |
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Thermal Imaging
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Different from low-light imaging methods of night vision (which require some
ambient light in order to produce an image), thermal imaging night vision
methods do not require any ambient light at all. They operate on the principal
that all objects emit infrared energy as a function of their temperature. In
general, the hotter an object is, the more radiation it emits. A thermal imager
is a product that collects the infrared radiation from objects in the scene and
creates an electronic image. Since they do not rely on reflected ambient light,
thermal imagers are entirely ambient light-level independent. In addition, they
also are able to penetrate obscurants such as smoke, fog and haze. There are
two types of thermal imaging detectors: cooled and uncooled.
require cryogenic cooling to very cold temperatures (below 200K).
are normally either temperature stabilized (at room temperatures) or entirely
unstabilized.
Thermal images are normally black and white in nature, where black objects are
cold and white objects are hot. Some thermal cameras show images in color. This
false color is an excellent way of better distinguishing between objects at
different temperatures.
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Cooled-detector Infrared Cameras
How they work: Cooled infrared detectors are typically housed in a vacuum-sealed
case and cryogenically cooled. The detector designs are similar to other more
common imaging detectors and use semiconductor materials. However, it is the
effect of absorbed infrared energy that causes changes to detector carrier
concentrations which in turn affect the detector’s electrical properties.
Cooling the detectors (typically to temperatures below 110 K, a value much
lower than the temperature of objects being detected) greatly increases their
sensitivity. Without cooling, the detectors would be flooded by their own
self-radiation.
Materials used for infrared detection include a wide range of narrow gap
semiconductor devices, where mercury cadmium telluride (HgCdTe) and indium
antimonide (InSb) are the most common.
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The highest possible thermal sensitivity.
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Able to detect people and vehicles at great distances.
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Not affected by bright light sources.
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Able to perform high speed infrared imaging.
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Able to perform multi-spectral infrared imaging.
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Expensive to purchase and to operate.
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Limited cooler operating lifetime.
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May require several minutes to cool down upon initiation.
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Bulky.
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Cooled-detector Infrared Cameras |
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Uncooled-detector Cameras
How they work: Unlike the cryogenically cooled detectors described above,
uncooled infrared detectors operate at or near room temperature rather than
being cooled to extremely low temperatures by bulky and expensive cryogenic
coolers. When infrared radiation from night-time scenes are focused onto
uncooled detectors, the heat absorbed causes changes to the electrical properties
of the detector material. These changes are then compared to baseline values
and a thermal image is created. Despite lower image quality than cooled detectors,
uncooled detector technology makes infrared cameras smaller and less costly and
opens many viable commercial applications.
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Uncooled detectors are mostly based on materials that change their electrical
properties due to pyroelectric (capacitive) effects or microbolometer (resistive) effects.
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Relatively inexpensive compared to other thermal imaging technologies.
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High contrast in most night-time scenarios.
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Easily detects people and vehicles.
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Not affected by bright light sources.
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Higher reliability than cooled detector thermal imagers.
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Less sensitive than cooled detector thermal imagers.
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Cannot be used for multispectral or high-speed infrared applications.
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| Uncooled-detector Thermal Imaging products: |
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Near Infrared Illumination
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A popular and sometimes inexpensive method for performing night vision is by
near infrared illumination. In this method, a device that is sensitive to
invisible near infrared radiation is used in conjunction with an infrared
illuminator. The popularized this method. Because of the IR sensitivity
of the camcorder’s CCD detector and since Sony installed an infrared light
source in the camcorder, infrared illumination was available to augment
otherwise low-light video scenes and produce reasonable image quality in
low-light situations.
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The method of near-infrared illumination has been used in a variety of night
vision applications including perimeter protection where, by integrating with
video motion detection and intelligent scene analysis devices, a reliable
low-light video security system can be developed.
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IR illumination
How they work: Several different near infrared illumination devices are
available today, including:
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Filtered incandescent lamps: A standard high power lamp that is covered by an
infrared filter designed to pass the lamp’s near infrared radiation and block
the visible light component. These devices typically need good heat transfer
properties since the intense visible light is internally absorbed and
dissipated as heat.
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LED type illuminators: These illuminators utilize an array of standard infrared
emitting LEDs.
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Laser type: The most efficient infrared illuminator, these devices are based on
an infrared laser diode that emits near infrared energy.
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| Near infrared illuminators are typically available in
a range of wavelengths (e.g. 730nm, 830nm, 920nm). Providing supplemental
infrared illumination of an appropriate wavelength not only eliminates the
variability of available ambient light, but also allows the observer to
illuminate only specific areas of interest while eliminating shadows and
enhancing image contrast. The supplemental near infrared lighting not only
improves the quality of image intensifier devices (which have both a visible
and a near-infrared response), but also permits the use of solid state cameras,
which also have the ability to convert near infrared images to visible.
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Lowest cost compared to other night vision technologies.
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Eliminate shadows and reveal identifying lettering, numbers and objects. Can
also be used to perform facial identification.
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Able to perform high-speed video capture (such as reading license plates of
moving vehicles).
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IR illuminators can see through night-time fog, mist, rain and snowfall as well
as windows.
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Eliminates the variability of ambient light.
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Users of infrared illuminators can be detected by others that have
near-infrared viewing devices.
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| IR Illumination products: |
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Glossary of Night Vision Terms
Atmospheric transmission
Absorption of the infrared energy by the atmosphere. High transmission ranges
are known as “atmospheric windows” through which infrared imaging over very
long distances can be performed.
Electromagnetic spectrum
The electromagnetic spectrum divides up the regions of electromagnetic
radiation into different ranges having unique characteristics. This radiation
is divided up rather arbitrarily into a number of regions based on wavelength:
Gamma < 10 nanometers, Ultraviolet radiation, Visible light 0.4 to 0.7
micrometers, Infrared Radiation, Microwaves, Radio waves. The following is a
sub-categorization for the infrared range relevant for night vision:
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Short wave
infrared range (SWIR):
Also known as the Near infrared range, that portion of the infrared spectrum
from 750nm to 2500nm.
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Mid wave
infrared range (MWIR):
That portion of the infrared spectrum from about 3 microns to 5 microns.
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Long wave
infrared range (LWIR): That portion of the infrared spectrum from about 8 microns to 12 microns.
Generations of image
intensifiers
The different paradigms of image intensifier technology have been identified by
“generations” of technology (also known as “Gen”). Generation 0 technology
first developed in the 1950s depended on near infrared illumination to produce
reasonable night vision images. After the light was converted to electrons,
these electrons were accelerated so they hit a phosphor screen with greater
energy, creating a visible image. Unfortunately, the accelerated electrons were
somewhat distorted and vision with this method was impaired. Generation 1 image
intensifiers were then developed that used a photocathode material that was
better than Gen 0 in converting light to electrons. These units were able to
operate at lower light levels than the Gen 0 and, became known as "starlight
scopes" since near infrared illumination was not required. When three tubes
were cascaded together, the sensitivity was sufficient for most night vision
applications, but distortion existed. Generation 2 image intensifiers marked
the development of a microchannel plate which multiplies the number of
electrons by the thousands. A single unit of a Generation 2 image intensifier
produced the same sensitivity as a 3-tube cascaded Generation 1 device but in a
much small package and without distortion. Generation 3 is the most
sophisticated night vision technology available today. The image intensifier’s
photocathode is coated with sensitive gallium arsenide, which allows for a more
efficient conversion of light to electrical energy at extremely low levels of
light. Generation 3 provides the clearest, sharpest night vision image
available.
Image intensifier tube
An electro-optical device which converts photons to electrons, amplifies them,
then converts them back to photons so the user can see at light levels that are
normally too low.
Infrared
The range of electromagnetic radiation having a wavelength longer than that of
visible light and shorter than that of microwave radiation. The name “infrared”
translates to "below red", where red is the color of visible light of longest
wavelength. Infrared radiation spans the wavelengths between approximately 750
nm (0.75 microns) and 1 mm (1000 microns). For a bit of history about infrared, .
Microbolometer
An infrared detector that absorbs the IR radiation and warms slightly; the
electrical resistance across the bolometer changes as a function of
temperature, which can be measured and made into a thermal image.See also
Pyroelectric
An infrared detector that absorbs the IR radiation and warms slightly; the
electrical capacitance across the detector changes as a function of
temperature, which can be measured and made into a thermal image.See also
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