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long range flirlong range flir cameralong range plz flir cameraLong range thermal cameralong range thermal cameraspan tilt thermalpan tilt thermal imaging flir camerasptz flir cameraptz long range thermal flirptz thermalptz thermal camerasPTZ thermal imager
Long Range EO/IR thermal imaging flir cameras, gimbals optics and system for airborne, ground and marine applications
By spicorp@me.com September 20, 2020 September 27th, 2020 No Comments
EO/IR (Electro Optical / Infrared) systems and long range thermal cameras cover a wide range of distinct technologies based on the targets and mission to be accomplished.
Target phenomenology often dominates the choice of spectral band. For example, missile launch detection depends on the very hot missile exhaust, which produces significant radiation in the ultraviolet (UV) spectral region. The band choice is also influenced by the vagaries of atmospheric transmission and scattering
EO/IR missions divide roughly into dealing with point targets and extended fully imaged targets. For point targets, the challenge is to extract the target from a complex and cluttered background. For fully imaged targets (images of tanks, for example), the contrast between target and background is a critical parameter. The ability to detect dim targets, either point or extended, is a measure of the system's sensitivity. The resolution of a sensor is a measure of its ability to determine fine detail. Measures of resolution depend on the precise task. Use of eye-chart-like calibration targets is common in DoD applications. EO/IR sensors may be divided into scanning sensors, which use a limited number of detectors to scan across the scene, and staring sensors, which use large numbers of detectors in rectangular arrays.
Non-Imaging EO/IR Systems
Non-imaging point target EO/IR systems focus on the task of detecting targets at long range. For these applications, details of the target are irrelevant; for example, for IR sensors, only the total energy emitted matters, not the precise temperature and size of the target separately. The available energy can vary over many orders of magnitude, from the engine of a small UAV to an intercontinental ballistic missile (ICBM) launch.
Comparison of the available energy at the sensor to the noise level of the sensor provides the central metric of sensor performance, the noise equivalent irradiance or NEI. The problem of extracting the target from background clutter is addressed in two basic ways: through the choice of sensor band and algorithms. For missile launch detection, for example, one may use the "solar blind" UV band. The transmission in this band is very poor, and the general background is reduced to a level of near zero. However, the very bright missile signature is strong enough to still provide a useable signal. Algorithms for separating a point target from a structured background are a continuing source of improvement in performance, but their complexity may make their evaluation challenging.
THERMAL IMAGING FLIR PTZ CAMERA SELECTION:
M5 LONG RANGE PTZ THERMAL IMAGING FLIR CAMERA
M9 LONG RANGE PTZ MULTI SENSOR THERMAL IMAGING FLIR CAMERA
M11 LONG RANGE PTZ TJERMAL IMAGING FLIR SECURITY CAMERA
M2D LONG RANGE DRONE GYRO STABILIZED DRONE THERMAL IMAGING FLIR OTZ CAMERA GIMBAL FOR UAS UGV UAV AND SUAS
M1D VEHICLE MOBILE MARINE ROOF OR STATIONARY MOUNTED LONG RANGE PTZ THERMAL IMAGING FLIR TURRET CAMERA SYSTEM
The effectiveness of imaging systems can be degraded by many factors, including limited contrast and luminance, the presence of noise, and blurring due to fundamental physical effects. As a mathematical description of image blur, the MTF can be broken down into each component of the sensing, such as optics, detector, atmosphere, and display. This provides insight into the sources and magnitude of image degradation.
There are many ways to evaluate and describe the quality of an image, the use of which is determined by details of the application. Two examples have a broad application and a long history.
The Army Night Vision and Electronic Sensors Directorate (NVESD) maintains models for predicting image quality based on the targeting task performance (TTP) metric.1 This provides a rule-of-thumb for the number of bar pairs required on target to have a 50-percent probability of detecting, recognizing, or identifying the target.
The strategic intelligence community uses the National Imagery Interpretability Rating Scale (NIIRS) to evaluate the quality of still imagery. NIIRS is a qualitative scale, running from 0 to 9. Tables are published associating rating levels with tasks for EO, IR, synthetic aperture radar (SAR), civil imagery, multispectral imagery, and video. NIIRS can be estimated by the General Image Quality Equation (GIQE), an empirical model that has been designed to predict NIIRS from sensor system characteristics.
Each of these approaches represents a balance between two of the fundamental limits to any EO sensor: the resolution (how small) and the sensitivity (how dim) – that is, how small an object or feature can be usefully seen and how low can the signal be before it is overwhelmed by the noise. Figure ES-1 shows a comparison of a noise- limited case and a resolution-limited case.
1 The TTP metric is the successor of the Johnson criteria. See page 30 for additional discussion.
In modern digital sensors, these classical factors have been joined by a third, the sampling or pixelation of the sensor, as shown in Figure ES-2.
ES-2. Sampling Limited Image
The design of a sensor is a tradeoff between these three factors, placed in the context of characteristics of the target and environment. While in a balanced design, each of the factors needs to be evaluated. For any given sensor and state of the technology employed, it may be the case that the sensor is signal-to-noise limited; in this case, the S/N ratio is the single-most important parameter and rules-of-thumb may be developed to focus on S/N for the target and environment. In other cases, the sensor is resolution limited, and the characterization of the optics (the MTF) is the most important; an ideal sensor is said to be diffraction-limited, able to respond to spatial frequencies up to the diffraction limit, λ/D, where λ is the wavelength at which the sensor operates and D is the diameter of the optics. For these cases, rules-of-thumb may be developed that focus on the optical system. For sensors that are limited by the pixelation, the "Nyquist limit" is determined by the separation between detectors, S; the highest spatial frequency that can be correctly measured by the sensor is 1/2S. In these cases the Nyquist frequency may be an appropriate rule-of-thumb.
These trades can be followed in the history of personal cameras from the film era to the most modern Nikon or Canon. In the film era, the user could trade between sensitivity and resolution by changing the film used: so-called fast film (TRI-X) was sensitive but had a coarse grain size, limiting the resolution. It was useful for pictures in dim light or when high shutter speeds to photograph moving subjects were needed. In brighter light or for slowly moving objects the photographer might choose a slow film (PAN-X) that had a fine grain size but was not very sensitive. On top of this choice, the photographer could choose lenses with different f-numbers (to change sensitivity), different focal lengths (to change resolution), and different prices (to improve MTF).
In the last 2 decades, digital cameras have replaced film cameras in many applications. The earliest digital cameras were limited both by sensitivity (detectors were noisy) and by sampling. In consumer terms, the sampling resolution was specified by the
number of pixels; early cameras were 1 megapixel, about 1,000 by 1,000 detectors replacing the film. The need for relatively large detectors (10-20 μm) was driven by lack of detector sensitivity; the resulting reduction in resolution compared to the better films that had film grains of 2-3 μm was a consequence of this, rather than a technological limit to producing smaller detectors. As detector technology evolved, the noise in each detector was reduced (improving S/N and allowing dimmer light or faster motion) and the number of pixels was increased. Today, personal cameras can have 36 megapixels or more and begin to rival the finest grain films for resolution with detectors of 4 μm or smaller. The best personal cameras began as sensitivity and sampling limited; but as those barriers were overcome, they have returned to being resolution limited as determined by the quality of the optics. As these changes have taken place, the simple rules-of-thumb that characterize the camera have also changed.
The same three elements are present in all EO systems, but there is no unique balance point between them. This is determined by the state of technology but also the mission the sensor is trying to accomplish. Personal cameras emphasize images of people at close to moderate ranges; the signal is determined by reflected light, the noise by the technology of the detectors. Missile launch detection systems are looking for extremely bright points of light in a cluttered background. Infrared systems depend on the self-emission of the target (hot engines on aircraft and tanks) and are often limited by the environment (the transmission of the signal through the air). No matter what the sensor is, the evaluation of the sensor system involves characterizing it with the three metrics of noise, resolution, and sampling.
EO/IR sensor systems are often paired with a tracker. Examples of point target trackers include systems to track missile launches and infrared search and track systems, both discussed above. Many different algorithms are used to implement point trackers. Although different, they all involve the same basic steps: track initiation, data association, track smoothing, and track maintenance. Conversely, image-based trackers are used to track mobile objects on the ground [e.g., intelligence, surveillance, and reconnaissance (ISR) missions] or for aim point selection. Usually with image-based trackers, the target is initially located by a human operator viewing a display. After the target is acquired, a feedback control loop (track loop) continuously adjusts the gimbal to keep the target in the center of the sensor's field of view. Common image-based tracker algorithms include edge detection, centroid tracking, area correlation tracking, moving target indicators (MTI), multi-mode trackers, and feature-based algorithms.
Latest Trends in EO/IR System Development
Driven by missions such as Persistent Surveillance, an important recent trend in EO/IR sensors is the development of large-area, high-resolution cameras. For sensors operating in the visible band, this is simpler than for those operating in the mid-
wavelength infrared (MWIR) or long-wavelength infrared (LWIR) bands. In the visible band, silicon can be used for both sensing material and for readout electronics. This eliminates issues such as potential thermal mismatch between the two. For EO systems, it is also possible to group individual cameras together and then combine separate images into one. The current state of the art in MWIR focal plane arrays (FPAs) is roughly 4,000 by 4,000 detectors; for LWIR FPAs, it is closer to 2,000 by 2,000. The ARGUS sensor being developed by DARPA has 1.8 gigapixels. To reduce the amount of thermally generated noise in LWIR FPAs, these cameras operate at low temperatures. The required cryogenic equipment has important Size, Weight, and Power (SWaP) implications at the system level and can affect system reliability. To address this need, considerable effort has gone into development of uncooled sensors. Another recent development is the use of so-called III-V superlattices that use alternating layers such as aluminum gallium arsenide and gallium arsenide (AlGaAs/GaAs) and that allow one to change the device's spectral response by changing individual layer thicknesses. The short-wavelength infrared (SWIR) band extends from 1.0 μm to 3.0 μm. This radiation, often referred to as "airglow" or "nightglow," is non-thermal radiation emitted by the Earth's atmosphere. Military applications of SWIR include low-light/night-vision imaging, detection of laser designators, covert laser illumination, laser-gated imaging, threat-warning detection, ISR, and covert tagging. Hyperspectral imaging allows one to simultaneously gather both spatial and spectroscopic information for more accurate segmentation and classification of an image.
Aliasing is an almost inescapable feature of staring focal plane array sensors. Aliasing refers to the artifacts associated with sampling systems. They can range from Moiré patterns2 to ambiguously interpreted images of objects with complicated patterns of light and dark. The presence of aliasing in a system gives rise to a general rule based on the Nyquist frequency, which identifies the resolution of a system with the size of a sample (or pixel) on the target. This underrates the importance of other determiners of resolution such as the MTF. Performance may be better or worse than that suggested by Nyquist, depending on the task. The combination of MTF and aliasing can lead to some unintuitive tradeoffs. For example, poorer MTF may actually improve performance in some tasks if aliasing is a significant problem. For imaging systems with aliasing, the display of the sensor information becomes important, especially if the image is zoomed so that one display pixel is used to represent a single sensor sample value. An improper reconstruction of the sensor data can degrade performance. For all aliased systems, an understanding of the reconstruction algorithm is an important aspect of any system including a human operator.
2 Moiré patterns are interference patterns that are often the result of digital imaging artifacts. See page 59 for additional discussion.
Issues in Bayer Color Cameras
The use of Bayer pattern color cameras in imaging systems to reduce cost and data rate requirements may introduce additional dependence on algorithmic choices. In contrast to full color cameras, a Bayer camera does not have a color detector for all 3 colors (red, green, blue) at each location (a 12 "megapixel" Bayer sensor has 6 million green, 3 million red, and 3 million blue detectors). An algorithm is used to interpolate the missing values to produce a complete three-color image. This color aliasing is more severe than the aliasing intrinsic to any staring focal plane. Fortunately, in the natural world, color information is usually relatively immune to aliasing effects. However, a large number of different algorithms of varying complexity may be employed by a sensor manufacturer. Depending on the tasks to be performed and the details of the image, the algorithm may induce new artifacts that complicate system evaluation. Ideally, the user could be given some control over the interpolation algorithm to match it to the task.
A Tutorial on Electro-Optical/Infrared (EO/IR) Theory and Systems
Point targets
EO/IR Missions
– IRST (infrared search and track) and visible analogs. Detection and tracking of aircraft at long range against sky backgrounds.
Ship-based and fighter-based IRST systems have been developed in the past.
Applications to homeland security and anti-UAV.
– Missile launch warning. Detection of missile launch events andtracking against ground backgrounds.
• Satellite and aircraft based
Extended targets
– ISR systems• Satellite, manned aircraft, unmanned aircraft
• Any and all bands
• Usually oriented close to vertically or side-to-side
– Target acquisition and surveillance
• Night vision goggles
• Vehicle or aircraft mounted FLIRs (Forward Looking Infrared)• Usually oriented approximately horizontally with variable look-up or look- down angles
The most basic division in EO/IR sensors is between point and extended targets. A point target is one that is small enough, compared to the resolution capabilities of the sensor, to appear as a single point. The defining characteristic of an extended target is the presence of internal detail. Rather than detecting a point, the sensor presents an image of the target. The distinction between point and imaging targets is not the same as between non-imaging and imaging sensors. One can imagine a point target mission that scans the sky looking for a bright spot without ever forming an image (the original Sidewinder air-to-air missile seeker would be such as system); however, some imaging sensors form an image of the sky and then look for bright spots within the image.
Infrared search and track (IRST) systems represent a class of systems for which the targets remain point targets. The term primarily refers to IR sensors dedicated to detecting aircraft at long range. Aircraft are typically hotter than the sky or cloud background against which they are seen and appear as a bright point. Although originally conceived as an air-to-air aircraft finder or a ship-to-air missile finder (to detect anti-ship cruise missiles), the same approach has applications for homeland security and anti- unmanned aerial vehicle (UAV) search. Another class of systems is missile-launch detection systems. In this case, the launch is signaled with a very hot flash that can be
detected. In this case, the background is likely to be the ground rather than the sky for IRST systems; this affects the algorithms used to extract the target and even the band (wavelength) of the EO/IR sensor.
The extended target applications include intelligence, surveillance, and reconnaissance (ISR) systems providing long-term imaging of the ground, usually from a vertical perspective (e.g., surveillance satellites, UAV), and target acquisition systems in tactical systems [night vision goggles, tank forward-looking infrared (FLIR) systems], typically a more nearly horizontal view.
For all EO/IR systems
– Optical properties (resolution) – Sensitivity/noise
– Digital artifacts
– Detector properties
– Processing
The importance of some parameters varies with mission
– Target characteristics
– Platform characteristics
– For automated systems (IRST), algorithms for detecting targets (high probability of detection with limited false alarms)
– For observer-in-the-loop systems, displays For example, ISR systems
– Very high resolution (small instantaneous field of view, IFOV) to achieve good ground resolution from high altitudes
– Field of view
A 100-megapixel array with 1-foot ground sample distance covers only a 2 mile x 2 mile patch of ground
Older film cameras have 140 degree fields of view with a 72 mile wide x 2 mile image!
The definition of each of the terms mentioned above will be developed over the course of this paper.
It may be surprising to see film discussed in the 21st century; however, in some ways, film remains unsurpassed.
Developed in the early 1960s, the U-2's Optical Bar Camera (OBC) gave the spy plane an edge that has yet to be matched by its prospective successor: the Global Hawk unmanned aircraft. The film camera, which is mounted in a bay behind the aircraft's cockpit, captures high-resolution panoramic images covering an area 140 degrees across.
The OBC gets its name from its slit assembly, which forms the camera's bar. Unlike a conventional camera, in which an aperture opens and closes to allow light to expose the film (or, in the case of a digital camera, a charge coupled device chip), the slit exposes a roll of film mounted on a 3-foot-diameter rotating spindle. The entire lens assembly, with a 30-inch lens, rotates around the longitudinal axis of the aircraft to provide a field of view that extends 70 degrees to either side of the aircraft's flight path.
The OBC carries a roll of film measuring some two miles in length and weighs around 100 pounds. Each frame is 63 inches long by 5 inches wide.
A. Basics
The EO/IR Sensing Process
EO/IR systems are often plagued by the difficulty of providing precise predications of performance: in EO/IR, the answer is "It depends."
The majority of EO/IR systems (laser systems are the conspicuous exception, but searchlights are still used as well, and night vision goggles can be used with artificial illumination) are passive; that is, they are dependent on the illumination of the target by sunlight or moonlight (even sky shine) or the target's own emission of light. This is in contrast to radar systems that provide their own illumination. In addition, the EO/IR photons travel through a hostile medium, the atmosphere, which can refract, absorb, or scatter them. EO/IR is, in general, sensitive to the environment. Also, the target's characteristics can be quite important and variable, depending on the target temperature and even the paint used on the target. This variability poses a problem to the designer, tester, and operator.
The designer has more control over the sensor's design parameters, datalinks used to transfer information, and displays on which, for imaging sensors, the scenes are presented to the human operator.
UV (0.25 -0.38 m)
IR(0.75 to>14m)
Electro-optical/ Infrared Systems
EO/IR systems cover the range from UV through visible and IR. 0.38 -0.75 m
The wide range of EO/IR systems share some similarities:
– Lenses and mirrors rather than antennas
– Dependence on the environment
Although film systems remain in the inventory and are still preferred for some missions, new EO/IR systems will be digital.
The band chosen reflects the phenomenology of the target. Image Source:
LWIR: emitted radiation
D. G. Dawes and D. Turner, "Some Like It Hot," Photonics Spectra, December 2008.
SWIR: reflected radiation
The category of EO/IR sensors extends from the ultraviolet at a wavelength of 0.25 micrometers (μm) (which can be useful for very hot missile launch detection applications) through the visible region to the infrared region (wavelengths up to 14 μm or even greater). The design wavelength band is determined by the expected targets and mission.
Reflected and Emitted Light
• The energy coming from the target and background is a mixture of reflected and emitted light.
– Reflected light is the predominate element for visible sensors but also contributes in near-IR, short wave-IR, and mid-wave-IR.• Depends on natural or artificial illumination (for example, night vision goggles rely on ambient light in the near-IR).
– With artificial illumination, essentially any wavelength may lead to significant reflection.
– Emitted light is a natural feature of all objects: the amount of light radiated and at what wavelengths it is concentrated depends on the temperature and emissivity of the object.
– Reflectance and emissivity vary with wavelength.
• Snow is highly reflective in the visible but highly emissive in the IR.
– Incident radiation is either reflected, transmitted, or absorbed.
For opaque objects, the radiation is either reflected or absorbed.
In equilibrium energy that is absorbed is also emitted (but perhaps at adifferent wavelength).
As noted in the chart, the choice of wavelength is connected to the balance of emitted versus reflected light. One obvious difference is that human operators are accustomed to how objects appear in reflected visible light. The short wave IR, which almost entirely depends on reflected light, produces images that are very like visible images; mid-wave IR, less so; and for long-wave IR, the images seem unnatural in some aspects.
Planck's Law
Planck's law determines the energy radiated as a function of the wavelength, temperature, and emissivity (ε). The peak wavelength varies with temperature: higher temperature => shorter wavelengths.
– For objects near room temperature (300 K), the radiation peaks in the LWIR (long wave Infrared: 8-12 μm). For most natural objects ε is close to 1.
– In MWIR (mid-wave infrared: 3-5 μm) and most natural scene objects there is a mixture of emitted and reflected light. Emitted component increases with higher temperature.
– In SWIR (short-wave infrared: 1-3 μm), there is a mixture of emitted and reflected radiation.
– NIR (near infrared: 0.7-1.0 μm) depends upon reflected light and artificial illumination.
– In the visible, the radiance is almost entirely reflected light for typical temperatures (but things can be red or white hot!).
– UV applications depend primarily on emitted energy of very hot objects.
Radiance is conventionally measured in either: – Watts/cm2/ster; or
– Photons/sec/cm2/ster Lwatts ≈Lphotons hcλsensor
Emitted radiance (L) of blackbody3 with temperature T and emissivity ε between λ1
and λ2 is given by: 𝐿photons = �
2𝜀(λ) 2𝑐 𝑒 1 λ 4 h𝑐/𝑘𝑇λ
− 1 𝑑λ
2h𝑐1 1 h𝑐
2 λ 𝑑λ ≈ 𝐿 h𝑐/𝑘𝑇λ
𝐿 = �λ 𝜀(λ)
watts 2 λ𝑒 −1 photonsλ
λ1 λ5
For most modern EO/IR sensors, the photon representation is the more appropriate because the detectors are essentially photon counters. However, very early IR systems and some modern uncooled systems are bolometers, measuring the energy of the signal rather than the number of photons. For these systems, the radiance in terms of watts is the more useful. The terminology can be quite confusing and care must be taken to keep the units straight.
3 A blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency of angle of incidence. A blackbody at constant temperature emits electromagnetic radiation called blackbody radiation. The radiation is emitted according to Plank's law, meaning that it has a spectrum that is determined by the temperature alone and not by the body's shape or composition.
(wiki)
Only the radiance within specific atmospheric transmission windows is usually useful: in some cases, systems exploit the edges of the atmospheric window.
The atmosphere absorbs energy, particularly in IR and UV.
– The details of the absorption depend on the water vapor, CO2,
– The deep valleys (for example between 4-4.5 μm, at 9.5 μm) define the broad bands but there is a lot of fine structure that can be important for some applications.
– These determine the transmission, t, of the signal through the atmosphere.
The atmosphere scatters energy, particularly in the visible (fog, haze).– Depends strongly on the distribution of aerosol.
– Energy from the target scattered out of, other energy scattered
The atmosphere also radiates (primarily in the LWIR): this is called "path radiance."
Each of these reduce the contrast between the target and the background.
Elaborate models have evolved to predict transmission, scattering, and path radiance, paced by the improvement in computational speeds.
The complicated structure of the atmospheric transmission curves reflects the fact that the atmosphere is a mixture of different molecules with each species having its own set of absorption and emission lines. Because it is a mixture, the curves will depend on, for example, the absolute humidity (the water content of the air). Pollutants such as ozone or discharges from factories can be relevant, as can aerosols suspended in the air, including water (ordinary haze and fog), sand, dirt, and smoke.
Although it is common to assume a simple exponential decay of transmission with range (so-called Beer's Law), it is never safe to do so without checking the more elaborate calculations involving individual absorption lines, rather than averages over bandwidth ranges. The dependence of EO/IR on transmission is the primary factor that makes the predicting and testing of EO/IR systems challenging.
Contrast and Clutter
Separating targets from the background depends on the contrast: is the target brighter/darker than the background?
– The contrast is reduced by the transmission loss and may be masked by scattered energy or path radiance.
– Transmission loss increases with the range and is frequently
limiting factor in sensor performance (overwhelming naïve resolution estimates).
– Atmospheric variation is a primary cause of variability in performance.
– EO/IR sensors that perform well in clear weather will be degraded bydust, smoke, clouds, fog, haze, and even high humidity.
Even with sufficient contrast, the target must be extracted from the background.
– Non-imaging or point target detection: locating the dot in the complicated image (there are 4 added dots in image).
– Imaging systems: the people in the foreground are easy to see, but are there people in the trees?
• These concepts will be revisited in more detail in later charts.
Contrast can be defined in different ways depending on the application. At its most basic, it is simply the difference in sensor output between the target and background Cdifferential = (T-B). In other applications, it may be normalized to be dimensionless and between 0 and 1, Crelative = (T-B)/(T+B). This relative contrast is particularly common in display applications, partly because it reflects some features of human vision. The eye adapts to the overall illumination of a scene so that the relevant parameterization is the relative contrast. One speaks of a target that is 10 percent brighter than the background, for example. One may also see Calternative = (T-B)/B.
Resolution and Sensitivity
Resolution and sensitivity are the basic elements of a sensor description.
Resolution has many definitions depending on what task is to be done, but they are usually related to being able to make distinctions about the target.
– Rayleigh resolution criterion: Separating two images of a star (point target) Unresolved Resolved
– Bar targets: what is the smallest group of bars that can be resolved? ResolvedUnresolved Resolved
Resolution depends on the image contrast, which may be limited by the sensor's sensitivity: the signal must be greater than the noise.
There are many different definitions of resolution, each of which is connected to a specific task. For example, mathematically, the Rayleigh criterion requires the signal from one point (star) to fall to zero. Two stars are resolved when one star is located at the first zero point of the other. The Sparrow criterion for stars only requires that there be a dip in the brightness of the combined image; so two stars may be resolved on the Sparrow criterion, but not on the Rayleigh criterion.
Although the use of a calibration target with bar groups of different sizes is relatively standard, the results of a test will depend on the number of bars in a bar group, the aspect ratio of the bars, and the instructions to the test subject explaining the criterion for declaring a bar group resolved.
Types of Digital Systems
EO/IR digital systems can be divided into scanning and staring systems.
Scanners use a linear array of detectors (1 to a few rows). The image is developed by scanning the linear array across the scene.– Thenumberofrowsofdetectorsmaybe>1toprovide: • Staggered phasing to reduce sampling artifacts (aliasing)
• Additional signal gathering
• Multiple wavelength bands
– 2ndgenerationFLIRsusedaverticalarrayofdetectors scanned horizontally using scan mirrors.
– Pushbroomlinescannersuselineararraysthatare scanned by the motion of the aircraft.
Starers use a rectangular array of detectors that capture an entire image at time.– Modernsystems(bothEOandIR)aremovingtostaring arrays.– Limitationsincluderelativelysmallfieldofview, complexity of multi-band systems, and aliasing.
Behind the detectors are the read-out circuits.
Historically, the difficulty in manufacturing large square or rectangular focal plane arrays has meant that many sensors used scanning designs. There is a general migration from scanning to staring sensors. However, in some cases, a line-scanner may still provide the best solution. For example, if one wants a number of different colors or bands, a line-scanner can simply add more rows of detectors for the additional colors. Although some technologies provide, for example, a two-color IR array, achieving four or more colors requires a complicated design with multiple staring arrays. For applications requiring a wide field of view, it may be easier to create a 10,000-element linear array for a line-scanner than a 1-million element detector staring array.
Basics Summary
EO/IR systems cover a wide range of distinct technologies based on the targets and the mission to be accomplished. The target phenomenology may dominate the choice of spectral band. For example, missile launch detection depends on the very hot missile exhaust, which produces the majority of radiation in the UV. The band choice is also influenced by the vagaries of the atmosphere (transmission and scattering).
EO/IR missions divide roughly into dealing with point targets and fully imaged targets. For point targets, the challenge is to extract the target from a complex clutter background. For fully imaged targets (images of tanks, for example), the contrast between the target and the background is a central parameter. The ability to detect dim targets, either point or imaged, is a measure of the system's sensitivity.
The resolution of a sensor is a measure of its ability to determine fine detail. Measures of resolution depend on the precise task. The use of eye-chart-like calibration targets is common in DoD applications.
The technology used in EO/IR sensors may be divided into scanning sensors, using a limited number of detectors that scan across the scene, and staring sensors, using large numbers of detectors in rectangular arrays.
B. Non-Imaging EO/IR Systems
Non-imaging systems refer to unresolved or point targets.
– The simplest example of a point target is a star: in the sensor, a star produces an image that is called the point target response, impulse response, or blur circle. It may cover more than one detector element.
– An unresolved target is any object that produces an image in the sensor comparable to that of a star: there is no internal detail.
– For a resolved target, some amount of internal detail can be recovered.
– The rule of thumb is that a target is resolved if the sensor can put multiple detector fields of view on the target; unresolved if the target is entirely contained within one instantaneous field of view (IFOV).
– IFOV = detector size (d) / focal length (fl)
For a point target, the only signature characteristic is the amount of energy emitted in a specified direction or radiant intensity measured in watts/ster or spectrally (as a function of wavelength) watts/ster/μm– Radiant intensity ≈ Area target * radiance = AT * LT– LT is the power per unit solid angle per unit projected source area.– Radiant intensities for small aircraft (UAV) are the range of 0.05 watts/ster in MWIR and 0.25 watts/ster in LWIR.
– For ballistic missiles the signatures are much higher, megawatts/ster.
• Radiant intensity of the target is compared to that of the background:
radiant intensity contrast ≈ A *( L – L ) T T Background
Instead of using watts/ster,4 it is sometimes more convenient to describe the photon flux, photons/sec/ster. The common unit for IR systems is the watt, but, for visible systems, photons/sec is often employed.
The instantaneous field of view (IFOV) is a fundamental sensor parameter. At range R, a single IFOV covers a distance D = IFOV*R. As an example, detectors for visible digital cameras (Nikon, Canon) are about 10 μm in size. With a 100-mm lens the IFOV = (10*10-6)/(100*10-3) = 10-4. At a range of 1,000 meters, the IFOV covers 10 cm. If the target were 1 meter x 1 meter, we might say there were 10 x 10 = 100 IFOVs on target; this is usually replaced with the sloppier phrase, 100 pixels on target.
4 The steradian is a unit of solid angle. It is used to quantify two-dimensional angular spans in three- dimensional space, analogously to how the radian quantifies angles in a plane. (wiki)
Non-Imaging Applications
Air-to-air (Sidewinder) — First Sidewinders had a single detector behind a rotating reticle. Modern air-to-air missiles use focal plane arrays but, at long range, the target is a point target.
IRST (Infrared Search and Track)
– Air-to-Air — Permits passive operation of aircraft. Limited by cloud clutterbackground.
– Surface (Sea)-to-Air — Radar detection of sea-skimming cruise missiles may be adversely affected by environment effects. IR has different environmental problems and may provide a supplement to radar.
– Surface (Ground)-to-Air — For identification and tracking of small aircraft (UAV) EO/IR may offer advantages in resolution.
Missile launch detection
– Usually based on missile plume detection
– Tactical warning systems
– Strategic warning (DSP/SBIRS)The reticle was an engineering marvel. A reticle rotating disk has a pattern of transparent and opaque sectors. For a point target, the rotating pattern provided a blinking signal that could be distinguished from the background (clouds or sky), which did not vary as much. Further processing of the shape of the blink actually provided sufficient information to guide the missile to the target, directing it to maneuver up, down, left, or right.However, the problems of clutter rejection and dependence on atmospheric conditions are barriers to IRST use.
The irradiance of the target (measured in watts/cm2 or photons/sec/cm2) is defined by1 Irradiance = 4πR2
The sensor integrates this signal over a time, Tint. Signal = AopticsTint Irradiance
For any sensor to be evaluated, the first step in understanding the expected performance is to understand the signal produced by the target. The signal provided by a point target is particularly easy to understand. The example introduces several generally useful concepts. The radiant intensity contrast is a characteristic of the target at the source; using the photon (rather than watt) description, it represents the number of additional photons/sec/ster being radiated (or reflected) because the target is there.
In the Sensor
The signal is not necessarily captured by a single detector, even for a point target.
– If (most) of the received energy lies within a single detector, it cannot be located more precisely than 1⁄2 a detector width.
– If the energy is spread out over several detectors, the location can be made to a small fraction of the detector size if there is sufficient signal-to-noise ratio (SNR).
– The "ensquared energy" is the fraction falling on the primary detector (typical designs are for ensquared energy ≈ 1/3).
Finding point targets is easy if the target is bright and viewed against a dim background (stars against a dark sky): this is not usually the case.
– Non-imaging systems employ detection algorithms of varying complexity to extract possible point targets from the scene.
– All such algorithms have both a probability of detection (pd) and a false alarm rate (FAR).
– The performance of these algorithms depends on the SNR, the difficulties of the environment, and the detector performance characteristics.
The analysis of the signal given on the preceding chart implicitly assumed that all the photons from the target were easily counted. This would be the case if all the photons landed on a single detector. However, even if the point target image (or "blur circle") is small compared to the detector, the spot may land on the boundary between detectors so a fraction of the signal falls on one detector and another fraction on another. In the worst case, the signal would be reduced to 1⁄4 of the nominal value, divided among four detectors. The detection algorithms used in this limit may look at the detector output of several detectors to increase the detection range.
In the other limit, the size of the blur circle may be large compared to the detector. Surprisingly, this can be an advantage in some point target applications if the expected signal level is high enough. For a tiny blur circle, one can only say that the target is located somewhere in the field of view of that detector. If the blur circle covers several detectors, a model of how the signal should vary from detector to detector can allow an estimate of the location of the target to a fraction of an IFOV. This is also called "sub- pixel localization."
In most applications, the detection algorithms are as important in determining performance as the sensitivity of the detectors and IFOV. The point targets may be seen against a complicated clutter background; simply looking for a hot spot may produce an unacceptable number of false alarms.
The noise associated with a single detector is relatively straightforward.– Noise due to the average background
– "clutter noise" may be incorporated into the description – Other noise
– Intheabsenceofatarget,photonsstill
arrive on the detector. On average (using the photon flux form of the radiance).
Adetector AopticsTint Nave = 2
πfl
– Thisnumberwillvarystatisticallyevenforaconstantbackground,
providing a contribution to the noise of Nave1/2
– Ifthisistheprimarycontributiontothenoise,thesensoriscalled
background limited.
• Clutter noise — In many cases, the variation of the background can be incorporated into the noise. δN = Adetector AopticsTint δL
If this is dominant, the sensor is clutter πfl 2 clutter limited.
+δN2 +Other2 clutter
• Adding in any other noise, the total noise isNoise2 = N
In EO/IR sensors, estimating and characterizing noise and clutter is a vital element for understanding system performance. The use of a "clutter-noise" term is a common first order attempt to incorporate the clutter into performance estimates. However, since the scene is processed through a series of algorithms (which, in some applications may be quite complex), the effect of clutter has to be considered after the algorithms are run, not before. Estimates of performance require substantial testing or laboratory testing with scene simulators, the use of which must be examined carefully to ensure that the simulator presents the relevant features of the clutter. What sort of clutter is relevant depends on the algorithms!
To be more precise, the Lbackground should include not only the background radiation at the target but also the so-called "path radiance," radiation emitted between target and sensor by the atmosphere.
𝐿 = 𝐿 (𝐼𝑜 𝑜𝐼𝐼𝑆𝑒𝑜) + 𝑝𝐼𝑜h 𝐼𝐼𝑑𝐼𝐼𝑜𝑐𝑒 (𝑁𝑒𝑜𝑏𝑒𝑒𝑜 𝑜𝐼𝐼𝑆𝑒𝑜 𝐼𝑜𝑑 𝑜𝑒𝑜𝑜𝑜𝐼) 𝑡𝑜𝑡𝑎𝑙 𝑏𝑎𝑐𝑘𝑔𝑟𝑜𝑢𝑛𝑑
Noise Equivalent Irradiance (NEI)
For simplicity, assume all the signal is received on a single detector. Then the signal-to-noise ratio would be given bySNR = AopticsTint Irradiance Noise
The irradiance that would provide an SNR=1 is called the noise equivalent irradiance.
NEI photon = Noise NEI AopticsTint
= Noise hc
AopticsTint λsensor
• Note that the relationship between NEI and the system
parameters depends on whether the system is background or clutter limited.
• The actual signal and noise at the output of the algorithm used for target detection will differ from the signal and noise used here.
Noise equivalent irradiance (NEI) is an example of a number of similar figures of merit. For example, the irradiance of a target depends on the difference in the radiance of the target and background. For a system that utilizes the target's temperature and its emitted radiation, the radiance difference can be considered to be attributable to the difference in temperature between target and background. If the temperature difference is relatively small, the irradiance will be proportional to the temperature difference, ∆T.
Dealing with the Environment
Spectral band
– Forsomeapplications(detectingandtrackingaircraft),one chooses a spectral band with good transmission.
– Forsomeapplicationswithverybrighttargets(missilelaunch detection), the clutter problem is so severe that a band might be chosen with poor transmission to suppress background clutter.
Algorithms for extracting the target from the background may be spatial (essentially suppressing low spatial frequencies), temporal (subtracting two images to cancel non-moving clutter), or spatial-temporal combinations.– Simplealgorithmsmayhavelargefalsealarmrates.Forexample, cloud edges may produce false targets with simple spatial algorithms.
EO/IR systems are often dominated by environmental effects. Normally one chooses a band with good transmission, but, with good transmission, one can see all the clutter as well as the target. By choosing a band with poor transmission, very bright targets can still be seen but the clutter becomes invisible. If this trick isn't used, the targets must be separated from the background by means of detection algorithms. Any detection algorithm is associated with both a probability of detection (Pd) and a false alarm rate (FAR). Typically, internal parameters, or "thresholds" in the algorithm, permit the designer to trade off probability of detection and false alarm rate. The curve relating the two is termed the "ROC curve"; ROC is an acronym of ancient origin for "receiver operating characteristic." Testing and evaluating the detection algorithm is difficult because of the wide range of potential clutter backgrounds. Some systems may employ scene simulators that use models of background clutter to produce a wide range of scenes purported to span the circumstances of the real system in the real environment.
Point Target Summary
Non-imaging, point target EO/IR systems focus on the task of detecting targets at long ranges. For these applications, the details of the target are irrelevant; for example, for IR sensors, only the total energy emitted matters, not the precise temperature and size of the target separately. The energy available can vary over many orders of magnitude, from the engine of a small UAV to an intercontinental ballistic missile (ICBM) launch.
Comparison of the available energy at the sensor to the noise level of the sensor provides the central metric of sensor performance, the noise equivalent irradiance or NEI.
The problem of extracting the target from the background clutter is addressed in two basic ways: through the choice of sensor band and algorithms. For missile launch detection, for example, one may use the "solar blind" UV band. The transmission in this band is very poor and the general background is reduced to a level of near invisibility. However, the very bright missile signature is strong enough to still provide a useable signal. Algorithms for separating the point target from the structured background are a continuing source of improvement in performance, but their complexity may make the evaluation challenging.
C. Imaging EO/IR Systems
Image Clarity Issues
Original Contrast Luminance
Noise Sampling or Aliasing Blur
The choice of optics and detector affect the magnification provided and image clarity. Image quality includes measures of:
Contrast – Degree of difference between lightest and darkest portions of image
Luminance – Brightness of image
Noise – Random signal from sources outside the image itself
Sampling – Digitization due to binning of signal into pixels
Blur – Smearing of image due to diffraction and/or imperfect focus (e.g., due to jitter).
Modulation Transfer Function (MTF)
The MTF is a mathematical description of image blur: the MTF is the Fourier transform of the image of a point source.
Many components of the optical system can be represented by individual MTFs representing the impulse response of each part.
Total system MTF is a product of the individual MTFs that describe each component of the sensingMTFsystem = MTFoptics * MTFdetector * MTFatmosphere * MTFdisplay* MTFother
If the MTF is known (or equivalently, the blur function) one can convolvethe original scene with the blur to determine the effect of the optics on the imageOriginal MTF Original Image 2 FiltBerlur** = 100%0% 8
Distance FromCenter of a Line
The ability to calculate or estimate the different Modulation Transfer Function (MTF) factors varies. For perfect or "diffraction limited" optics, the MTF has a well- known analytic expression. For realistic optics, the different aberrations that reduce the MTF can be modeled well; computer-based ray-tracing programs can predict relatively accurately the overall optical MTF. The detector and display can be modeled accurately as well. However, the atmospheric effects are represented by statistical models and are a source of uncertainty. For any specific system, the "other" effects (including, for example, focus error) will often be represented empirically.
C la rity
The Modulation Transfer Function (MTF) is the single-most important characteristic of an optical system.
The MTF is simply the frequency response of the system:
– The image of a target can be decomposed into sinusoids of different frequencies; knowing how the system responds to each
frequency separately characterizes the system.
– If the signal has a component of A sin(2pfx) and the response is 0.8 * A sin(2pfx), then the MTF(f)=0.8.
In general, the wider the MTF(f), the better the resolution
– The blur circle or impulse response is the Fourier transform of the MTF(f): wide MTF narrow blur circle.
– A rule of thumb is that the resolution limit of the system is at the frequency for which MTF(f) = 0.1.
– Blur circle is short-hand for the shape of the impulse response: there is typically a smooth oscillating form.
Every element of the total system can affect the MTF – Optics themselves
– Film grain or detector size
– Vibration– Atmospheric distortions
– Electronics including display – Human eye!
Optics and Detector MTF
The primary contributors to the MTF curve in modern systems are the optics MTF and the detector MTF.
The ideal, or diffraction limited, optics MTF establishes a maximum spatial frequency of
– D/λ (measuring in cycles/radian) or
– 1/λf# (measuring on the focal plane incycles/m)where D is the diameter of the optics and f# is the f-number, f#=focal length/ D.
– The diffraction-limited MTF is nearly a straight line, but lens aberrations will reduce the MTF.
The ideal (square) detector MTF = sinc(pfd)
– Sinc(x)=sin(x)/x
– d= detector size
– Zeros of detector MTF = n/d, n = 1, 2,…
System design will determine relativelocation of detector MTF zero and optics MTF zero.
– Optics are typically "better" λf# < d.
– This can lead to sampling artifacts or "aliasing."
Classical MTF measurements in the laboratory are made more complicated by aliasing effects. One approach to overcome aliasing is to displace the image of the calibration target to provide different sample phasing (see p.60). For examples of other efforts made to work around the sampling artifacts, see Research Technology Organization Technical Report 75(II), Experimental Assessment Parameters and Procedures for Characterization of Advanced Thermal Imagers.
• Standard staring focal planes always the potential for aliasing.
– Asystemisnotaliasedifthemaximumfrequencyisless than half the sampling frequency = fNyquist.
• By degrading the optics (increasing the size of the
High Optics MTF "Matched" Optics MTF
Nyquist Optics MTF
blur circle), contrast islostbutaliasingis 0.8 reduced. 0.6
0 0.10.20.30.40.50.60.70.80.9 1 1.11.21.31.41.51.61.71.81.9 2
Aliasing refers to the inability to correctly represent spatial frequencies higher than the Nyquist frequency of a digital system. This will be discussed in detail in Section F.
This chart provides an initial discussion of why modern staring systems are typically aliased. For a staring array of square detectors, the detector MTF is given by
𝑀𝑇𝑀𝑑𝑒𝑡(𝑜) = 𝑜𝐼𝑜𝑐(𝜋𝑜𝜋) =
𝑜𝐼𝑜(𝜋𝑜𝑑) 𝜋𝑜𝑑
The detector MTF therefore extends to all frequencies. The first zero of the detector MTF is at f = 1/d; subsequent zeros are at multiples of that frequency, f = m/Wd m= 1, 2, 3….
However, the Nyquist frequency for such an array is fNyquist = 1/2d. Even if the frequencies beyond the first zero of the MTF are ignored (because of their diminishing amplitudes), the system is under-sampled by a factor of 2.
This may be modified by the consideration of the optics MTF, represented here by straight lines (correct for a square not circular lens!). If the blur circle of the detector (first zero) fits inside the detector, the optics MTF extends to 2/d (and is zero for high frequencies). This would mean being four times under-sampled (maximum frequency 4 x Nyquist). Degrading the optics until the blur occupies four detectors leads to the "matched optics" condition for which the optics MTF zero coincides with the first detector zero. Only if the blur occupies 16 detectors does the optics MTF zero match the Nyquist limit.
As shown in the preceding examples and to be developed further, this elimination of all potential aliasing reduces the system MTF (contrast) significantly. Most design trades permit some aliasing in order to preserve useable image contrast.
Minimum Resolvable Temperature
• Minimum Resolvable Temperature (MRT) is a system performance measure developed in the 1970s to balance two system characteristics
– Sensitivity, measured, for example, by the noise equivalent temperature difference (NETD)
• This was defined as the difference of the temperature between a (large) object and the background required to have a signal that produced a signal-to-noise ratio (SNR) of unity: SNR = 1
– Resolution, either measured in terms of the system modulation transfer function (MTF) or the size of a detector instantaneous field of view (IFOV)
For example, resolution defined as the spatial frequency, f, at which the MTF(f) = 0.1
IFOV = detector size / focal length
• MRT is defined in the laboratory with a 4-bar target
– Bar in 7:1 ratio so whole target represents a square
– The size of the target and the laboratory optics defineda specific spatial frequency as seen by the device, f.
– The 4 bars are maintained at a specified temperature above the background and inner bars.
– The temperature of the bars is lowered until the technician can no longer discern all four bars.
– This temperature was the minimum resolvable temperature MRT(f).
In classical noise equivalent temperature difference (NETD), the signal was compared to a measure of the temporal noise of the system (as measured through a standard electronic filter). In modern staring focal plane arrays, other noise sources must be considered. For example, each detector in the array will generally have a different response; this is called detector non-uniformity. Although an effort is made to provide non-uniformity correction, any residual non-uniformity represents a static spatial pattern noise. In addition, individual detectors may be uncorrectable, noisy, or dead.
The NVESD has introduced a three dimensional (3D) noise model to describe noise components in the temporal and two spatial dimensions.
MTF/MRT and Sampling Artifacts
The sampling artifacts of modern staring focal plane arrays make the definitions of the MTF (and hence, MRT) somewhat problematic for modern systems.
The first image shows a "well-sampled" image.
– Depending on the human observer, the smallest pattern that is resolved (counting 4 bars) is one of the two circled bar groups.
– This sensor will have an MTF (and MRT) that can be measured by classical approaches
The second image is "aliased".
– The bar groups are distorted and only the largest groupis resolved
– Modified techniques are required to measure (rather than model) the MTF and MRT.
Mission performance will be between the Nyquist and un-aliased limits. See discussion in section on aliasing and notes page below.
One approach taken by NVESD5 and others to represent the effect of aliasing on the MTF is to represent the MTF of the sampled system by squeezing (scaling) the MTF of the corresponding unsampled system.
The factor R = 1 – k SR, where SR is a metric representing the spurious response. The value of the constant k may vary with task (detection, recognition, identification) and different forms of the SR metric have been used. H(f) is the Fourier transform of the reconstruction function used. See Section G on aliasing.
Another approach is to treat aliasing as a noise term.6
An extension of the MRT task, the Minimum Temperature Difference Perceived (MTDP) has been introduced in Germany. This provides an extension beyond Nyquist.
5 Driggers, Vollmerhausen, and O'Kane, SPIE, Vol. 3701, pp. 61-73, 1999.
6 Vollmerhausen, Driggers and Wilson, JOSA-A, Vol 25, pp. 2055-2065, 2008.
From a user perspective and a testing perspective, controls over the digital image may affect performance significantly.
– In some missions, there may be insufficient time to explore alternative processing approaches.
– The effects of alternative processing are not completely modeled so performance may be better or worse than expected from standard models.
Basic controls include gain and level, but many options could be made available to the user/tester.
"Photoshop" operations
– Sharpening
– Histogram manipulation
– Zooming interpolation (reconstruction)
– Color balance
Hidden algorithms
– Producing full color images from Bayer cameras
– Combining images from multiple lens
– Combining images from multiple frames
• Red items will be discussed more completely in the appendixes.
Sharpened & equalized
Performance metrics can be affected even by simple gain and level adjustments.
Contrast = (Signal – Background)/Background = (S-B)/B
is unaffected by a change of scale (gain) but is changed dramatically with a level shift:
Contrast = ((S-L) – (B-L))/(B-L)= (S-B)/(B-L). Signal-to-noise (SNR) = (S-B)/Noise
is unaffected by gain or level as long as values are not truncated or saturated. In some applications, gain and level may not be under user control.
Key Concepts for Image Quality Modeling
Spatial frequency of image contentlow frequency high frequency
Contrast – shades of grey/color
high low reducing contrast
Eye Contrast Threshold Function (CTF) – Ability of eye to discern contrast
Modulation Transfer Function (MTF) – Degradation to image contrast caused by aspects of collection processCTGTMTF (observed target contrast)Spatial frequency
Considering bar targets, as in the discussion of minimum resolvable temperature (MRT), increasing spatial frequency (i.e., reducing the width of the bars) generally has a negative effect on the human eye's ability to resolve targets, as does reducing contrast (the difference in brightness between light and dark bars). A convenient way to capture the interaction between spatial frequency and contrast is to plot the eye contrast threshold function (CTF) in a graph of contrast versus spatial frequency. Such a plot shows that as the bars become narrower, greater contrast is required to distinguish black bars from white bars.7
The shape of the modulation transfer function in the contrast versus spatial frequency plot shows that, as spatial frequency increases, the ability of a system to transfer or portray contrast differences diminishes. The better the system (including optics, detector, atmosphere, and display) is, the shallower is the drop off of the curve with increasing spatial frequency.
7 Interestingly, at very low spatial frequencies, more contrast is required to distinguish bars, just as at higher spatial frequencies.
Evolution of Tactical Models for Predicting Image Quality
• Johnson Criteria: Started with experiments conducted by John Johnson, an Army Night Vision Laboratory [later renamed Army Night Vision and Electronic Sensors Directorate (NVESD)] scientist, in the 1950s
• In the 1950s, sensors were analog (film, TV). Johnson Criteria had to be translated into the digital sensor world.
• Targeting Task Performance (TTP): Today NVESD maintains community-standard models that predict the image quality and associated probabilities of detection, recognition, and identification for various vehicles and dismounts with differing backgrounds in the visible and infrared regions of the electromagnetic spectrum.
Visible – Solid State Camera and Image Processing (SSCamIP) Performance Model
IR – Night Vision Thermal and Image Processing (NVThermIP) Performance Model
In 1957 and 1958, John Johnson at the Army Night Vision Laboratory developed a series of experiments to analyze the ability of observers to perform visual tasks, such as detection, recognition, and identification. He came up with general rules for the number of bar pairs required on target to have a 50-percent probability of performing each of these tasks. Over time, this approach has evolved to account for the increasing sophistication of today's EO/IR sensors. The Army Night Vision and Electronic Sensors Directorate (NVESD) maintains models for predicting image quality based on the targeting task performance (TTP) metric, the successor to the Johnson criteria. Very recently, the visible and IR models, known as Solid State Camera and Image Processing (SSCamIP) and Night Vision Thermal and Image Processing (NVThermIP), respectively, have been combined into one software package, known as the Night Vision Integrated Performance Model (NV-IPM).
Johnson Criteria
• How many pixels are required to give a 50% probability of an observer discriminating an object to a specified level?
• Experiments with observers yielded the following
− Detect (determine if an object is present)
− Recognize (see what type of object it is; e.g., person, car, truck)
− Identify (determine if object is a threat)
1.5 pixels 6 pixels 12 pixels
• These are the number of pixels that must subtend the critical dimension of the object, determined by statistical analysis of the observations
− Critical dimension of human
− Critical dimension of vehicle
• Hence for a human, the requirements are
− Detect
− Recognize
− Identify
0.75 m 2.3 m
2 pixels/meter 8 pixels/meter 16 pixels/meter
• For a man who is 1.8 m x 0.5 m, this corresponds to requirements of
3.6 pixels tall by 1 pixel wide 14.4 pixels tall by 4 pixels wide 28.8 pixels tall by 8 pixels wide
As an example, the Johnson criteria can be applied to determine the number of pixels in an image required to detect, recognize, and identify a human subject. The calculations shown here are illustrated by the images on the chart below.
Images Illustrating Johnson Criteria
Detect: Something is Recognize: A person Identify: The person present. is present. is holding an object
that may pose a threat.
Eye Contrast Threshold Function (CTF)
One of the most common and useful ways of characterizing human vision
– One-dimensional sine waves are displayed to observer.
– For a given luminance level and signal spatial frequency, CTF is the minimum perceivable contrast vs. visual acuity (resolution).
– Derived from two-alternative forced choice experiment: observer must choose between sine wave and blank field.
– Repeat procedure for different average luminance levels.
*fL: luminance is expressed in units of foot-Lamberts
The eye contrast threshold function has been measured by repeated experimentation on a large group of observers. The experiment entails showing two fields to the observers. One field contains alternating black and white bars, and the second is constant gray of the same total luminance. The observers are asked to identify which of the images contains the alternating bars. This experiment is repeated as the contrast of the bar pattern is changed, while keeping the total luminance constant. The contrast at which 75 percent of the observers correctly identify the bar pattern is considered the threshold for that level of luminance. (The threshold is set at 75 percent because in a two- alternative forced choice experiment such as the one described here, the right answer will be selected 50 percent of the time simply by chance.) By conducting this experiment at varying spatial frequencies (i.e., bar spacings), one of the curves shown above can be measured. Differing levels of luminance give rise to the series of curves shown above.
How Good is the Human Eye?
Contrast 100%
Coarse 50% 1%
For each row, the viewer is asked which option contains alternating black and white lines and which option is a uniform grey bar.
This series of six rows demonstrates that it becomes more difficult to distinguish features as the contrast is decreased and as the features become finer.
An example of the experiment described in the previous chart is displayed here.
Approach to Measuring Sensor Effectiveness
• Night Vision Lab model (SSCAM, NVTHERM) estimates of target detection/recognition/ ID probability based on the TTP (targeting task performance) metric, which has supplanted Johnson criteria
− TTP = difference between target-background contrast and the eye's capability to distinguish contrast
Summed over all spatial frequencies
CTGT is a function of range
− Experimental data are "curve fit" based on the TTP value
target contrast
Modulation transfer function
(propagation, sensor, observation)
eye contrast threshold
quantifies threshold capabilities and limitationsofhumanvision
Detection probability (similar formula for recognition, ID)
CTGTMTF (observed target contrast)
TTP ("usable" contrast)
The TTP metric used by NVESD captures the difference between the target- background contrast and the eye's ability to distinguish that contrast. The square root functional form ensures that excessive amounts of "usable" contrast are not given too much weight in the metric. The probability of detection, recognition, or identification is related to the TTP, target size, target-sensor range, and V50 through the target transfer probability function, which is a logistics curve with an exponent determined by curve fitting. The task difficulty parameter, V50, is analogous to the Johnson N50 value that represents the number of resolvable cycles on the average target for a 50-percent probability of detection/recognition/identification. For each target type in a set of target options, V50 is determined by a series of calibration experiments involving human perception of the original image and images degraded by a known amount.
• CTGT-0 is the zero range contrast value for a target on a background.
– In visible, this is a measure of the difference in reflectivities between target and background.
– e.g., contrast for individual wearing white against concrete background is less than contrast for individual wearing black against same background.
– In IR, this is a measure of the difference in target and background temperatures.
The apparent target contrast at a distance is related to CTGT-0 via the extinctioncoefficient β from Beer's Law.
– CTGT = CTGT-0 e-βx where β is in km-1 and x is the range from target to sensor in km.
– Does not account for imaging through non-homogeneous media, such as the atmosphere.
Apparent target contrast is degraded by scattering of light into the path between target and sensor.
– This depends on the amount of aerosols and other particulates present, as well as any other potential sources of scatter, and it is particularly sensitive to the relative positions of the sun, target, and sensor.
– Army uses sky-to-ground ratio concept to account for this.
The zero range target contrast is a measure of the inherent contrast between the target and the background, independent of the distance between the target and sensor. In the visible, the contrast at each wavelength is integrated over the visible portion of the electromagnetic spectrum to determine the zero range target contrast. In the infrared, the contrast is due to the difference in thermal emission between target and background. The zero-range contrast is then attenuated by atmospheric effects, which can be treated as homogeneous or modeled in a complex computer program, such as MODTRAN (MODerate resolution atmospheric TRANsmission). The apparent target contrast is also degraded by scattering of light into the path between target and sensor.
Sky-to-Ground Ratio (SGR) • SGR is related to transmittance τ via τ = 1
1+SGR(eβx −1)
• SGR is a measure of the scattering of light into the path between
target and sensor.
In clear conditions with low relative humidity where direct sunlight is not close to the target-sensor path, a value of 1.4 may be used for SGR.
SGR approaches 10 or greater when direct sunlight is near the target- sensor path.
Extinction coefficients as a function of wavelength are tabulated for urban, rural, and maritime models.
Combined with representative SGRs, this allows for calculation of transmittance in a range of environmental situations.
The Army has introduced the concept of sky-to-ground ratio (SGR) to account for the scattering of light into the path between target and sensor. Values of SGR typically range from 1.4 in clear conditions with low relatively humidity to well over 10 when the path radiance is high, due to multiple scattering events, as would be encountered when the sun is shining directly on the target-sensor path or in a forest under overcast conditions.
National Imagery Interpretability Rating Scale (NIIRS)
Standard used by the strategic intelligence community to judge the quality of an image (versus the Johnson criteria/TTP approach used by the tactical intelligence community).
NIIRS of particular image is based on judgment of imagery analysts, guided by updated published scale of representative examples.
− e.g., NIIRS = 5 means can identify radar as vehicle-mounted or trailer-mounted • NIIRS can be estimated from General Image Quality Equation, derived from
curve fitting.
NIIRS 4 (≈ 6' GSD) NIIRS 6 (≈ 2' GSD) NIIRS 8 (≈ 6" GSD)
The strategic intelligence community uses the National Imagery Interpretability Rating Scale (NIIRS) to evaluate the quality of still imagery. NIIRS is a qualitative scale, running from 0 to 9, with guidance for imagery analysts provided in the form of a table of example operations that could be performed at various NIIRS values. The table for visible NIIRS values is provided on the following chart. There are also tables for IR NIIRS, synthetic aperture radar (SAR) NIIRS, civil imagery NIIRS, multi-spectral NIIRS, and video NIIRS.
NIIRS can be estimated with the General Image Quality Equation (GIQE), an empirical model that has been designed to predict NIIRS from sensor system characteristics. In the visible, the GIQE takes the form
NIIRS = 10.251 – a log GSD + b log RER – 0.656 H – 0.344 (G/SNR)
where GSD is the ground sample distance RER is the relative edge response H is the overshoot,
G is the gain,
SNR is the signal-to-noise ratio,
a = 3.16
b = 2.817 for RER < 0.9 and a = 3.32, b = 1.559 for RER ≥ 0.9.
The only change to the GIQE in the IR is that the constant term is 10.751, rather than 10.251. The GSD, RER, and overshoot will be defined and discussed in subsequent charts.
Definition of NIIRS Levels (Visible)
Ground sample distance (GSD) is the dominant term in the GIQE and ultimately provides an upper limit to the image quality, since all information in the area defined by the horizontal and vertical GSDs is incorporated into a single pixel. The GSD is defined by
where PP is the pixel pitch x is the slant range
FL is the focal length
GSD = ((PP * x)/FL)/cos θ
θ is the look angle, measured between nadir and the sight line.
For non-square pixels, the vertical and horizontal GSDs differ and are specified separately.
The blurring of the original image as adjacent pixels are averaged together is evident in comparing the image in the upper left quadrant to that in the upper right quadrant and finally to that in the lower left of the figure.
Relative Edge Response
The relative edge response is a measure of blur and is defined to be equal to the difference in the normalized edge response 0.5 pixels to either side of an edge. In a perfect image where a completely black area is adjacent to a completely white area, the pixel on one side of the edge has a luminance of one whereas the pixel on the other side has a luminance of zero. In reality, blurring of the black and white portions occurs in the vicinity of the edge. Edge analysis is conducted on real images to ascertain values of relative edge response (RER) for actual sensors.
Overshoot: the introduction of artifacts, such as halos, through excessive use of a digital process to make images appear better by making edges sharper
Sharpened Image
| Over-sharpened
Overshoot is due to excessive use of a digital process to sharpen imagery at edges (MTF compensation). It is defined to be the value of the peak normalized edge response in the region 1-3 pixels from the edge, unless the edge is monotonically increasing in that range, in which case, it is defined as the edge response at 1.25 pixels from the edge. This term partially offsets the improvement in NIIRS that a really sharp edge response provides.
Imaging EO/IR Systems Summary
The effectiveness of imaging systems can be degraded by many factors, including limited contrast and luminance, the presence of noise, and blurring due to fundamental physical effects.
MTF is a mathematical description of image blur and can be broken into each component of the sensing, such as optics, detector, atmosphere, and display, providing insight into the sources and magnitude of image degradation.
The Army NVESD maintains models for predicting image quality based on the TTP metric, the successor to the Johnson criteria, rules of thumb for the number of bar pairs required on target to have a 50-percent probability of detecting, recognizing, or identifying the target.
The strategic intelligence community uses NIIRS to evaluate the quality of still imagery.
– NIIRS is a qualitative scale, running from 0 to 9.
– Tables are published associating rating levels with tasks for EO, IR, SAR, civil imagery, multi-spectral, and video.
– NIIRS can be estimated by the GIQE, an empirical model that has been designed to predict NIIRS from sensor system characteristics.
D. Tracking
Tracking Point Targets (1)
Point trackers are used, e.g., to track missile launches or in infrared search and track systems.
Although different algorithms are used to implement a tracker, they all go through the same basic steps:
– Track Initiation
– Detection-to-Track Association (or Data Association)
– Track Smoothing
– Track Maintenance.
Track initiation is the process of creating a new track from an unassociated detection.
– Initially all detections are used to create new tracks, but once the tracker is running, only those that could not be used to update an existing track are used to start new ones.
– A new track is considered tentative until hits from subsequent updates have been successfully associated with it.
– Once several updates have been received, the track is confirmed.
• During the last N updates, at least M detections must have been associated with
the tentative track (M=3 and N=5 are typical values).
– The driving consideration at this stage is to balance the probability of detection and the false alarm rate.
Trackers are designed to follow the position of a target by responding to its emitted or reflected radiation. Most EO/IR tracking systems contain the following components:
A sensor that collects radiation from the target and generates a corresponding electrical signal
Tracker electronics that process the sensor output and produce a tracking error signal
An optical pointing system (e.g., a gimbal) that allows the sensor to follow target motion
A servo and stabilization system to control the gimbal position.Examples of point target trackers include systems to track missile launches and infrared search and track systems. Many different algorithms are used to implement a point target tracker. Although different, they all involve the same basic steps:
Track Initiation
Data Association
Track Smoothing
Track Maintenance.Track initiation involves creating a new track given a new unassociated detection. Initially all detections are used to create new tracks, but once the tracker is running, only those hits that could not be associated with an existing track are used to start new tracks. A new track is considered tentative until hits from subsequent updates have been
successfully associated with it. Tentative tracks are typically not shown to the operator to prevent potential false tracks from appearing on the screen. This, of course, causes some delay in first reporting a track. Once several updates have been received, the track is confirmed. The most common criterion for promoting a tentative track to a confirmed track is the so-called "M-of-N rule," which states that during the last N updates, at least M plots must have been associated with the tentative track (M=3 and N=5 are typical values). The driving consideration at this stage is to balance the probability of detection and the false alarm rate.
In the data association step, the tracker must determine which hits should be used to update which tracks.
– A given hit may be used to update one track, or a hit can be used to tentatively update several tracks.
– The latter approach recognizes the uncertainty surrounding to which track the detection belongs.
– This produces multiple versions of each track which are eventually "pruned."
Data association can be done in a number of ways:
– By defining an "acceptance gate" around the current track location and then selecting either the closest hit in the gate to the predicted position, or the strongest hit in the gate.
– Statistical approaches that choose the most probable location of a hit can also be used.
In the track-smoothing step, the latest track prediction is combined withthe associated hit to provide a new estimate of the target location.
– Algorithms of differing complexity and computational load can be used, including alpha- beta trackers, Kalman filters, and multiple hypothesis tracking.
Track maintenance involves deciding whether to terminate a track.
Common approaches include:
– If the target was not seen for the past M consecutive update opportunities
– If the target was not seen for the past M out of N most recent update opportunities
– If the target's track uncertainty has grown beyond a certain threshold.
In the data association step, the tracker must determine which hits should be used to update which tracks. This is a trivial exercise in the case where only a single target is being tracked. For those cases in which multiple targets are being tracked, a given hit may be used to update one track, or it can be used to tentatively update several tracks, recognizing that uncertainty exists in knowing to which track the detection actually belongs. This produces multiple versions of each track that are eventually "pruned." Either way, the first step in the process is to update all the existing tracks by predicting their new position based on the most recent state estimates (e.g., position, heading, speed, acceleration, etc.) and the assumed target motion model (e.g., constant velocity, constant acceleration, etc.). Having updated the estimates, it is possible to try to associate the new detections to the existing tracks. Data association can be done by defining an acceptance gate around the current track location and then selecting either the closest hit in the gate to the predicted position, or the strongest hit in the gate. Alternatively, statistical approaches that choose the most probable location of a hit can also be used.
Once a hit has been associated with a track, the next step involves combining the track prediction and the associated detection to generate a new estimate of the target's location, as well as to provide a revised estimate of the errors in this prediction. A variety of algorithms can be used for this process, including:
Alpha-beta tracker
Kalman Filter
Multiple hypothesis tracker (MHT)
Interacting multiple model (IMM).
The track maintenance step involves deciding whether to terminate a track. If a track was not associated with a hit during the data association phase, there is a chance that the target may no longer exist. Alternatively, however, the sensor may simply have failed to see the target at that update, but will find it again on the next one. Common approaches to deciding on whether to terminate a track include:
If the target was not seen for the past M consecutive update opportunities (typically M=3 or so)
If the target was not seen for the past M out of N most recent update opportunities
If the target's track uncertainty has grown beyond a given threshold.
Tracking Extended Targets (1)
Image-based trackers are used, e.g., to track mobile objects (cars) on the ground (ISR) or for aim point selection.
The target is initially located either by a human operator viewing a display or by some form of automatic target recognition system.
After the target is acquired, the tracking system locks on to it and maintains LOS autonomously.
A feedback control loop (the track loop) continuously adjusts the gimbal to keep the target in the center of the sensor's field of view.
– Target location estimation analyzes the sensor's imagery to determine the position of the target in sensor coordinates.
– The target location estimate is usually computed on a small sub-image (the gate) to reduce the effects of clutter and noise and to reduce the processing requirements.
– Having estimated the target's location, the processor generates the gimbal commands to correct the sensor's LOS.
– The sensor generates a new video stream and the process repeats.
Image-based trackers are used to track mobile objects on the ground (e.g., in ISR missions) or for aim point selection. Like point target trackers, image-based tracking systems include a sensor, tracker electronics, and an optical pointing assembly. With image-based trackers, a human operator initially locates the target by viewing a display. After the target is acquired, a feedback control loop (the track loop) continuously adjusts the gimbal to keep the target in the center of the sensor's field of view.
A generic tracking system is illustrated in this chart. Imagery from the sensor is passed to the track processor. The target location estimation process analyzes the imagery to determine the position of the target in sensor coordinates. This is done on a small sub-image (the gate) to reduce the effects of clutter and noise and to reduce the processing requirements. Having estimated the target's location, the processor generates the gimbal commands to correct the sensor's line of sight (LOS). The sensor then generates a new video stream and the process repeats.
No universal tracking system exists that can meet performance requirements specified for all applications.
Common Tracker types (target location estimation) include:
– Edge Detection Trackers: Identifies points in the image where the brightness changes abruptly thereby defining edges of the target
– Centroid Trackers: Determines target aim point by computing the geometric centroid of the target
– Area Correlation Trackers: Compare patterns via an autocorrelation function to develop an error signal
– Moving Target Indicators (MTI): Subtracts the present video frame from the preceding one to isolate moving targets
– Multi-mode Trackers: Combine point, area, and MTI schemes together as necessary
– Feature Based Trackers: the most current trend in advanced tracker development.
General Lock-on Requirements include
– Signal-to-Noise Ratio
– Signal-to-Clutter Ratio
– Contrast
– Pixels on Target
Determine fundamental performance limits
Set by designer to achieve more stable tracking in clutter
• Kalman filtering can provide optimum position estimate in noisy environments.
– Often used in trackers required to follow maneuvering airborne targets from high performance aircraft platforms.
The heart of the tracker is in the feedback control loop or the track loop. Common image-based tracker algorithms include: edge detection, centroid tracking, area correlation tracking, moving target indicators (MTIs), multi-mode trackers, and feature- based algorithms.
Examples of point target trackers include systems to track missile launches and infrared search and track systems.
Many different algorithms are used to implement point trackers. Although different, they all involve the same basic steps: track initiation, data association, track smoothing and track maintenance.
Image-based trackers are used to track mobile objects on the ground (ISR missions) or for aim point selection.
Usually with image-based trackers, a human operator initially locates the target by viewing a display.
After the target is acquired, a feedback control loop (the track loop) continuously adjusts the gimbal to keep the target in the center of the sensor's field of view.
Common image-based tracker algorithms include: edge detection, centroid tracking, area correlation tracking, MTIs, multi-mode trackers, and feature- based algorithms.
E. Latest Trends in Sensors
Large Area and High Resolution
– Number of pixels vs. Pixel Size
– Argus/Gorgon Stare/Angel Fire
Uncooled IRFPAs
• Advanced Processing
– Super-Resolution (microscanning)
• On-Chip Processing
– Non-uniformity Correction (NUC)
– Analog to Digital Conversion (ADC)
• Adaptive multi/hyperspectral imaging Independently tune spectral response of
– Microbolometers
• Extended Wavelength Response
(VLWIR) – • III-V Based FPAs
each pixel
Array of electronically programmable microspectrometers
– QWIPs, T2SLSs, QDIPs
Driven by missions such as Persistent Surveillance, an important recent trend in EO/IR sensors is the development of large-area, high-resolution cameras. For sensors operating in the visible band, this is simpler than for those operating in the mid- wavelength infrared (MWIR) or long-wavelength infrared (LWIR) bands. In the visible band, silicon can be used for both the sensing material and for readout electronics. This eliminates issues such as the potential thermal mismatch between the two. For EO systems it is also possible to group individual cameras together and then combine the separate images into one. The current state of the art in MWIR focal plane arrays (FPAs) is roughly 4,000 by 4,000 detectors; for LWIR FPAs, it is closer to 2,000 by 2,000. The ARGUS sensor being developed by DARPA has over 2 gigapixels.
To reduce the amount of thermally generated noise in LWIR FPAs, these cameras operate at low temperatures. The required cryogenic equipment has important Size, Weight, and Power (SWaP) implications at the system level and can affect system reliability. For some applications, a small lightweight camera that does not consume much power is required. To address this need, considerable effort has gone into the development of uncooled sensors. A recent NVESD program to develop uncooled microbolometers with detectors as small as 17 μm and array formats as large as 1024 x 768 is addressing the tradeoff between device sensitivity and temporal response. The goals of the program are a sensitivity of 35 mK and a time constant of 10 ms.
The detector material of choice for LWIR applications is mercury cadmium telluride (HgCdTe). The spectral band of these devices is determined by adjusting the
composition of the material, which can be difficult for longer cut-off wavelengths. An alternative approach involves the use of so-called superlattices of III-V semiconductors. This device structure consists of alternating layers of, e.g., gallium arsenide (GaAs) and aluminum gallium arsenide (AlGaAs). For these compounds, the spectral cut-off wavelength is changed by altering the layer thickness, which can be done very precisely.
In the past, sensor performance was limited by detector quality, due to detector material and fabrication. The improvement in these areas has reached the point where future gains in system performance will be achieved through advanced processing techniques. One such technique is known as super-resolution. The objective of super- resolution is to increase the spatial resolution of the sensor without physically altering the optics or focal plane. The technique involves the use of successive frames from a spatially under-sampled imager to process and construct a higher-resolution image. A number of fielded systems incorporate this concept to improve range performance. An example is the Lockheed Martin's Hawkeye system. This system is gimbaled and includes an indium antimonide (InSb) MWIR FLIR. The super-resolution algorithms result in range performance improvements of the order of 20 percent to 40 percent, depending on which optical field of view (FOV) the system is using. The Northrop Grumman LITENING AT pod also utilizes similar algorithms in an application for tactical jet aircraft targeting pods.
Army Third Generation FLIR
Benefits of Gen 3 FLIR
– Better day signatures (MWIR band)
– Better transmission (always have the best band)
– Better countermeasure rejection (against single bandlasers)
– Longer range identification (NFOV MWIR Channel)
– Faster Search (WFOV LWIR has shorter integration time)
– Less Motion Smearing (LWIR has shorter integration time) – Wider Dynamic Range (LWIR channel has more sensitivity) – Opportunity for Multi-color fusion
Disadvantages of Gen 3 FLIRs
– Increased Cost and Complexity
• Two-color FPAs
• Dual cold shield design • Dual channel optics
• More signal processing
An example of a proposed system that incorporates many of the developments described on the preceding chart is the Army's third-generation FLIR. The FPA is a large format (1280 x 720) staring array with a detector pitch of 20 μm. In addition, the device architecture, which is shown above, allows operation in both the MWIR and the LWIR spectral bands. The system has a dual F/# optical system (F/2.5 and F/6.0). The key advantage of two-color imaging infrared focal plane arrays (IRFPAs) is the ability to more easily detect and identify obscured targets in cluttered backgrounds. Other advantages are listed above. These come at the expense of increased cost and complexity.
SWIR Imagers (1)
The infrared spectrum
• Radiance of the night sky
– The origins and expected intensities of
hydroxyl (OH) are shown by the vertical lines
• MilitaryApplicationsofSWIRImaging – Low Light / Night Vision Imaging
– Detection of Laser Designators
– Covert Laser Illumination
– Laser Gated Imaging
– Threat Warning Detection – ISR
– Covert Tagging
• Size,WeightandPower
As discussed on page 7, the infrared portion of the electromagnetic spectrum is generally subdivided into numerous bands, including the near-infrared (NIR), the short- wavelength infrared (SWIR), the mid-wavelength infrared (MWIR), the long-wavelength infrared (LWIR), and the very long-wavelength infrared (VLWIR). The SWIR band extends from 1.0 μm to 3.0 μm and is defined by the carbon dioxide (CO2) and water (H2O) absorption lines at both the short- and long-wavelength ends of the band.
Radiation in the SWIR band is often referred to as "airglow" or "nightglow" and is non-thermal radiation emitted by the Earth's atmosphere. Its spectral radiance is of the order of 1 μW/(cm2∗Sr∗μm) with a spectral distribution characteristic of molecular emission. The primary source of this emission was identified by A.B. Meinel in 1950 as rotation-vibration bands of the hydroxyl (OH) molecule.
Military applications of SWIR imaging include low-light/night-vision imaging, detection of laser designators, covert laser illumination, laser-gated imaging, threat- warning detection, ISR, and covert tagging.
visible systems, scattering due to fog and dust can affect both visible and IR radiation.
Which band performs better in a given situation depends on the details of the aerosol present.
SWIR sensors rely primarily on reflected radiation similar to visible cameras. SWIR cameras produce finer resolution than imagers operating in the LWIR. This can lead to improved target ID. SWIR imagers can be combined with illuminators for imaging inside buildings and caves.
Most glass is opaque for λ > 3.5 μm.
Glass windows are transparent in the SWIR band but not in the LWIR.
Some transparency in the MWIR but poor optical transmission degrades the image. This is significant operationally but also has significant system implications.
• SWIR •
The frequency range where light scattering is most prominent depends upon the size of the particles/aerosols doing the scattering. Haze refers to obscuration of the lower atmosphere due to particles/aerosols in the 0.01 – 0.1 μm size range. For fog and dust, the particles/aerosols are larger; typically, 0.5 – 100 μm for fog and 1 – 100 μm for dust.
The ability of a SWIR camera to image through haze is illustrated in the top two figures, which show both a visible and a SWIR image of a hotel in haze at a range of roughly 2.4 km. The image was taken in late afternoon before dusk about 150 feet above the ground. As can be seen, the hotel is barely discernible in the visible, but is relatively clear in the SWIR band. The reason for this difference is that, in hazy conditions, the scattering efficiency for visible light is much higher than it is in the SWIR band; consequently, the longer wavelengths of the SWIR band transmit more readily.
Sensors operating in the SWIR spectral region detect differences in ambient light reflected from the target and background, similar to a camera operating in the visible. Thus a SWIR image looks much more like a visible image than does one produced by a thermal imager. This is illustrated in the middle pair of figures above. These figures also show the increased resolution possible with a SWIR camera compared to that with a long-wavelength infrared imager. This increased resolution, in turn, leads to improved target identification.
Optical glasses are transparent to light with wavelengths from around 0.2 to 3.5 μm. The optical transmission then goes to zero and stays at zero through the LWIR and very long wavelength infrared (VLWIR) spectral regions. This poor transmission is a result of strong absorption due to the presence of water and hydroxyl ions. Thus glass windows are not transparent in the LWIR but are in the SWIR spectral band. With some MWIR
cameras, it is possible to see through glass, but the poor optical transmission significantly degrades the image. The difference between the LWIR and SWIR spectral bands in terms of their ability to image through glass is illustrated in the bottom pair of figures. This is important not only from an operational point-of-view where it is often necessary to image into and out of windows, windshields, etc., but it also has significant system implications. The fact that standard glass optics and lenses can be used in the SWIR band is an important advantage in terms of cost and complexity compared to both MWIR and LWIR, which require optical systems that use more exotic materials such as germanium (Ge) and sapphire (Al2O3).
Multi-Spectral and Hyper-Spectral Sensors (1)
Multi-spectralandhyper-spectralsensors offer more than red, green, and blue.– Multi-spectral typically means up to 8-12 bands,– Hyper-spectral > 50 bands,
Formulti-spectralsystems,thebandsarechosen with very specific applications in mind.– Chlorophyll, algae, sediment– Oil spills, fire detection
Forhyper-spectralsystems,custombandchoices may be offered.
Multi-spectralandhyper-spectralsensorstypically scan across the direction offlight.
If the number of bands is small, 5-8,pushbroom scanners can be used.Dalsa 5-band chip (up to 12,000+ detectors wide)
Multi-spectral sensors produce images with a few discrete and somewhat broad spectral bands, e.g., Vis, NIR, MWIR, and/or LWIR. Hyper-spectral sensors, on the other hand, collect image data simultaneously in dozens or hundreds of narrow, adjacent spectral bands. These measurements make it possible to derive a continuous spectrum for each image cell. So a sensor with only 20 bands could also be hyper-spectral if it covered the range from 500 to 700 nm with 20 bands each 10 nm wide. A sensor with 20 discrete bands covering different parts of the Vis, NIR, SWIR, MWIR, and LWIR spectra would be considered multi-spectral.
Hyper-spectral sensors collect information as a set of images, one for each spectral band. These spectral images are then combined and form a 3D hyper-spectral data cube for processing and analysis – in other words, the spatial data are in the XY plane; the spectral data, the Z-axis. These systems typically have only moderate spatial resolution in each of up to 200 spectral sub-bands, with each spectral sub-band having a width of about 10 nm.
Hyper-spectral images are produced by instruments called imaging spectrometers. The most common approach to creating a hyper-spectral data cube takes advantage of 2D FPAs. The camera first maps an image strip onto a row of pixels on the FPA. Each pixel in this row is simultaneously spread into a Z column of spectral data and then that (spectral) frame is read. Then the imager scans to the next row. This is repeated until a 2D spatial image (in the X-Y plane) is built up. Thus, for example, a 320 x 240 array could capture 320 spatial pixels with 240 spectral sub-bands associated with each pixel. The point of obtaining an image cube is to allow one to compare the spectral intensity plot obtained from each pixel with a stored library of spectral reflectivity data.
VIMS is located on the Cassini Orbiter to provide 2D hyperspectral high resolution images to study Saturn's rings.
VIMS makes use of a reflective telescope and pushbroom imaging with a pointable primary mirror.
The spectral range is from 325 to 1025 nm, with spectral resolution of 1.46 nm.
The objective is to allow one to compare the spectral intensity plot obtained from each pixel with a stored library of spectral reflectivity data.
Challenges remain:
– Atmospheric transmission correction• Altitude Dependency
• Supporting Meteorological Instrumentation • Measurement Latency
– Database development
• Material Spectra Libraries
• Weathering Effects on Materials
• Possible CMs (design camouflage materialsthat match the background)
Military systems are largely focused on the SWIR spectral band for two reasons. First, most materials have high reflectivities in this region, and their reflectivity spectra differ strongly due to material-dependant molecular-absorption bands. Second, the strong solar illumination available during the day provides the very high signal levels needed to achieve an adequate SNR given the lack of light when working in very narrow spectral bands.
Numerous hyper-spectral data collection systems have been developed – most designed for airborne usage, but some are satellite mounted. Much of the development work in this area is in the field of remote sensing. A typical system might have 200 spectral bands each with 10-nm spectral resolution. In addition, the system might may have 1 mrad spatial resolution and provide a 50 to 70 degree sweep. For systems operating in the SWIR band, the FPA is typically InGaAs or HgCdTe while those operating in the MWIR band use HgCdTe or InSb FPAs.
The primary advantage to hyper-spectral imaging is that, because an entire spectrum is acquired at each point, the operator needs no prior knowledge of the sample, and post- processing allows all available information from the dataset to be mined. Hyper-spectral imaging can also take advantage of the spatial relationships among the different spectra in a neighborhood, allowing more elaborate spectral-spatial models for a more accurate segmentation and classification of the image.
The primary disadvantages are cost and complexity.
Latest Trends Summary
Missions such as persistent surveillance are driving the need for high resolution sensors with extremely large FOVs.
Uncooled microbolometers with detectors as small as 17 μm and array formats as large as 1024 x 768 will be important for applications with difficult SWaP constraints.
The use of so-called III-V superlattices, such as AlGaAs/GaAs, allow one to change the spectral response of the device by changing the layer thickness.
Because detector materials are operating close to theoretical limits, future gains in system performance will be achieved through advanced processing, such as super-resolution.
The SWIR band extends from 1.0 μm to 3.0 μm and is defined by the CO2 and H2O absorption lines at both the short- and the long-wavelength ends of the band.
Radiation in the SWIR band is often referred to as "airglow" or "nightglow" and is non-thermal radiation emitted by the Earth's atmosphere.
Military applications of SWIR imaging include low-light/night-vision imaging, detection of laser designators, covert laser illumination, laser-gated imaging, threat-warning detection, ISR, and covert tagging.
Hyper-spectral imaging allows one to simultaneously gather both spatial and spectroscopic information for more accurate segmentation and classification of an image.
F. Sampling, Aliasing, and Reconstruction
Most modern sensors are "sampled" producing an array of numbers that represent an image (like the CD representation of music).
This is in contrast to older technologies, such as film or image intensifiers (both still used), which represent the image continuously (like a vinyl LP or audio tape).
GSD, the distance on the ground between samples, is often used as shorthand for the resolution and hence performance of a digital system. Although the resolution is usually not far from the GSD, this over-simplifies the problem. For example, if the system is unaliased (which is possible for sufficiently high sampling or sufficiently poor optics), the resolution will be poorer than the GSD. How much poorer will be determined by the optics and detector MTF. If the system is aliased, the resolution will be determined by how the aliasing affects task performance; it may be greater or lesser than indicated by the GSD.
It is commonplace to assert that spatial frequencies below the Nyquist limit will be accurately reproduced; although true for non-aliased systems, this depends on the task for aliased systems. In general, one may expect the probability of task performance will degrade as the Nyquist frequency is approached.
Similarly, the task may be able to be performed above the Nyquist frequency, but, in many cases, the performance continues to degrade as the frequency increases above Nyquist. Often, task performance is statistical: for some phases of the sampling, the task is performable; for others, not.
Finally, it is insufficient to compare the "characteristic dimensions" of the object of interest with the GSD. Real objects represent a range of spatial frequencies ranging above and below characteristic dimensions. A complete analysis must take this into account or be made in the spatial, not frequency, domain.
How Does Aliasing Look?
TheMoirépattern.Thestronghighspatial frequency information represented by the brick pattern produces a low-frequency oscillating pattern and distortions of the high-frequency pattern (brick shape).
Interruptionsoflinearfeatures:thetele- phone lines are intermittently revealed.
A close examination of the image will also show apparent distortions of the apparent shapes of the bricks, which also varies depending on the position of the brick on the wall, which determines the phasing of the samples.
If the task is to determine the size and shape of the bricks or to confirm that each brick is the same size, then the task is severely affected by aliasing. If the task is to determine whether the wall is brick or cinder block, the task is not affected by aliasing at all.
As noted several times in the preceding charts, aliasing is the result of sampling. The figure shows a blue-and-orange striped "target." If only the samples shown as red circles in the upper figure were included in the sampled data set, the image would be interpreted as being entirely blue; if only the samples shown as yellow circles were taken, the target would be entirely orange. The red and yellow samples differ only in their phase with respect to the pattern of the target.
For the phases in the top image, if one had both red samples and yellow samples, one would have correctly deduced that the target had blue and orange panels. This corresponds, in a quick-and-dirty version of the Nyquist sampling theorem, to having (at least) one sample per characteristic feature.
One needs, in general, to have more than one sample per characteristic feature. This is illustrated by the lower figure, which has the same number of samples (red and yellow) as the upper figure but for which the samples are shifted – they have a different phase. In this case, each sample overlaps an equal amount of blue and orange; the structure is again lost and the color distorted.
Sampling and Reconstruction
All digital systems are sampled systems.
– For a given continuous signal g(x), there is a set of sample locations {xm} and sample values gm = g(xm).
– The sample locations are typically (but not always) chosen to have a uniform spacing between samples.xm = x0+ m*S where S = sample separation and x0 the initial phase
– The sampled signal could be represented as a series of delta functions or we can "reconstruct" the signal with smoother functions.gdelta(x)=∑gmSδ(x−xm) greconstruction(x)=∑gmh (x xm) − mm
In the Fourier (frequency) domain, if the Fourier transform of the original signal g(x) is G(f) then (letting x0 = 0 for convenience)
– Where H(f) is the Fourier transform of the smooth reconstruction function.
– The sampled signal consists of the original plus an infinite series of sideband copies of the original.
– The reconstruction controls how one deals with the sidebands and is an important part of the evaluation of any sampled system.
Digital systems are a subset of sampled systems. However, the digitization (quantization) is separable from sampling itself. Similarly, other techniques, such as fast Fourier transforms (FFT), although extremely useful for real-time processing, are irrelevant for the primary issues addressed in this series of presentations.
Digital signal processing emphasizes the direct manipulation of the digitized samples, transforming, for example, a N x N array of samples representing an image into another N x N array of modified samples. The emphasis here, in contrast, is on the continuous perspective.
The samples are taken from a continuous function; the goal is to extract the most information possible from those samples (without introducing artifacts) about the continuous image. In addition, having, at least conceptually, reconstructed the original image, the image can be manipulated in a variety of ways using the wider range tools available for a continuous image. These manipulations include, but are not limited to, smoothly interpolating the image so that it can be added to other images or corrected for various image distortions.
These manipulations may actually be done (indeed, must be done in practice) by digitally manipulating another array of data that is larger than the original array (MN x MN). However, the manipulations can be represented theoretically by smooth transformations, and the re-digitization needed to perform the calculations is a logically separate part.
Unaliased and Aliased Systems
In the most desirable case, the original signal is separated from the copies. This is the unaliased case. The original information is present and, in principle, recoverable.
– This requires that the original signal, G(f), is band-limited with a maximum frequency, fmax : and that the sample rate is sufficiently high.
– The sampling rate must be twice the maximum frequency to keep the copies fromoverlapping. f < f /2= f
– The Nyquist frequency is defined as 1⁄2 the sampling rate. max s Nyquist
When these conditions do not apply, the copies will overlap: the region of overlap is the aliased part of the frequency domain. fmax > fNyquist
– Moiré patterns and other sampling anomalies are now inevitable.
No signal with finite support (so no real image in a camera) is literally band-limited. However, within the approximation that there is an effective maximum frequency, fmax, a particular input frequency, finput, is unaffected by the aliased sidebands if fmax < fs /2. If fmax < fs, some region of frequencies is unaliased. This is important for some applications. For example, in point target detection (such as missile launches), the source image on the focal plane is determined by the optical blur of the system so that, if the system is not too aliased (meaning that the blur circle is not too small), the blur will cover more than one detector. It is therefore possible to estimate (if the background clutter and noise are not too high) the target's location by a suitable average of the different sample values.
The delta-function reconstruction gives equal weight to f+ and f-
Non-trivial reconstructions address the ambiguity by trying to assign relative weights to the higher (f > fNyquist ) and lower frequencies(f < fNyquist ).
– Most reconstructions favor the lower frequencies.
– In some cases, the higher frequencies might be the real ones!
There is no absolute theoretical approach to take: it will depend on the task.
It is commonly stated that frequencies higher than Nyquist "cannot" be represented and that frequencies below Nyquist can be reliably represented. Both statements are over simplifications. Even in the unaliased case, a correct statement of the sampling theorem is that, if the original signal lies entirely in one interval [M fNyquist, (M+1) fNyquist ], then it can be perfectly reconstructed.
If the signal was known to consist entirely of frequencies above Nyquist, then the frequencies below Nyquist should be eliminated.
The problem is that frequencies above and below Nyquist produce the same samples for cosines and samples differing only by an overall phase for sine terms.
Aliasing in Imaging Systems
The challenge in understanding aliasing in imaging systems is the conflict between two extremes (using the staring focal plane design case).
– The useful MTF might extend to the first zero of the detector MTF = 1/d.
– The Nyquist limit = 1/2d.
A factor of 2 difference exists in these two naive estimates ofperformance, which could correspond to a 2X difference in range.
The performance usually lies between these two limits: the "correct" performance estimate depends on the task to be performed (or the test to be executed).
Digital Image of a Calibration Target
Digital images can be hard to interpret at the limits of resolution.
Naively, we might think the resolution task corresponds to one pixel on a white bar, the next pixel on the black space, and so on.– But a bar group of a calibration target has a wide frequency range.– 3 rectangular bars do not make a sine wave.
The left most image of a bar group corresponds to the naive resolution case: detector width, W = sample spacing, S = bar size
Remaining images are quite bizarre– These represent cases where W = S > Bar– Equivalently, the notional bar group frequency (1/(2 Bar)) > 1⁄2 S– We are "past Nyquist," in the aliasing region
The model will distinguish between the detector width, W, and the sample spacing S. For the standard staring sensor, S=W. The image depends on the relationship between S and W and the width of a bar in the bar group, B.
The naive Nyquist theorem would suggest that the target should be resolvable if the sample distance is less than the bar width: S < B. However, this leaves open the question of how good task performance will be "beyond Nyquist" when S > B.
The question is complicated by the fact that a bar target is not a pure sine wave with wavelength 2B; it is a combination of many frequencies both above and below Nyquist. A simple frequency-based threshold will not address the question.
As indicated in the figure, the 4th horizontal bar group could be interpreted as a resolved 2-bar bar group. The task definition determines whether or not this bar group should be considered to be resolved.
For simple tasks, one can construct a model of task performance.
Consider defining resolution for bar targets.
– The result will depend on whether 2-bar, 3-bar, 4-bar, etc., targets are used.
– The system output is examined to see if it produces the anticipated up-down-up pattern of a 2-bar target or up-down-up-down-up of 3 bars.
– The task can be varied by asking whether or not the pattern has to becompletely clearly seen: should we define task completion as seeing 3-bars and 2 spaces for a 3-bar target, or seeing at least one clear space?
This may seem artificial, but it represents a range of possible tasks and can be computed explicitly.
The following charts show the probability of task performance as a function of how much higher than the Nyquist limit one tries to go.
– Depends on the MTF of the system (detector MTF and optics MTF).
– For some sample phases, the task can be performed; for others, it cannot.
In general, performance above Nyquist is stochastic: for any task and frequency above Nyquist, there is some probability of performing the task.
– With multiple opportunities (as in video) or with redundant information (the truck grill), the Nyquist limitation can be overcome.
Allowing an N-bar target to be called resolved when fewer than N bars can be counted may seem unusual. However, it is the basis of the MTDP figure of merit used in the German TRM3 model in the infrared case (proposed as a replacement for the MRT). It is based on the perception of the standard four-bar test pattern but accepts that fewer than four bars are resolvable beyond the Nyquist frequency.
Basic tasks of resolved 2-bar, 3-bar, and 4-bar targets (seeing all bars and spaces).
For all tasks, the probability of task performance is 100% at and below Nyquist, but declines as the frequency increases.
– The left chart shows results with "perfect" optics (using the detector MTF only).
– The right chart adds "matched optics" MTF (with optics MTF zero located atfirst detector zero).
For matched optics and the 2-bar task, the average expected performance will be 1.25 x the Nyquist limit.Detector MTF only Detector MTF and "matched optics"
If the more exotic task definitions are used, the performance extends even further.
For matched optics, and the "see one space in a four-bar target" task, performance extends to 1.5 x Nyquist.
50 percent of the possible sample phasing will permit accomplishment of the task.
If more than one image is available, giving more opportunities to succeed, even higher performance at higher spatial frequencies is possible.
This is the source of "super-resolution" (better to say "super-sampling") techniques but also applies to video.
• The reconstruction of an image (how it is displayed when there are more display pixels than image samples) has an effect on its interpretability.
– For unaliased images, there is a unique best way to reconstruct an image.
Since the sidebands don't overlap, can filter sidebands completely.
Corresponds to using a sinc function (sinc(x)=sin(x)/x)) tointerpolate between samples.
– For aliased images, there is always some image ambiguity.• Reconstruction typically becomes an issue when images are examined at the highest resolution – when the image is zoomed
Given a sampled system to be viewed by an observer or manipulated by an algorithm, the image must be reconstructed from the samples. The samples are only a list of numbers, not an image. Reconstruction can be done poorly and must be considered carefully to optimize the performance of the sensor. How reconstruction algorithms are designed depends on the sampling, detector, and optics.
There is some evidence9 that the loss of performance due to sampling artifacts depends primarily on aliased sidebands at frequencies greater than Nyquist.
𝑀𝑇𝑀 (𝑜) = 𝑀𝑇𝑀 (𝑜⁄𝑅);𝑅 = 1−𝑘𝑆𝑅 𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚 𝑢𝑛𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚 𝑜𝑢𝑡−𝑜𝑓−𝑏𝑎𝑛𝑑
𝑆𝑅 = ∫𝑓𝑠⁄2 | ∑𝑛≠0 𝑀𝑇𝑀𝑢𝑛𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚(𝑜 − 𝑜𝑜𝑠)𝐻(𝑜) |𝑑𝑜 −𝑓 ⁄2
𝑖𝑛−𝑏𝑎𝑛𝑑 𝑠 ∫∞ |𝑀𝑇𝑀𝑢𝑛𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚(𝑜 − 𝑜𝑜𝑠)𝐻(𝑜)|𝑑𝑜
−∞
𝑆𝑅 = ∫∞ | ∑𝑛≠0 𝑀𝑇𝑀𝑢𝑛𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚(𝑜 − 𝑜𝑜𝑠)𝐻(𝑜) |𝑑𝑜 −∞
𝑡𝑜𝑡𝑎𝑙 ∫∞ |𝑀𝑇𝑀𝑢𝑛𝑠𝑎𝑚𝑝𝑙𝑒𝑑−𝑠𝑦𝑠𝑡𝑒𝑚(𝑜 − 𝑜𝑜𝑠)𝐻(𝑜)|𝑑𝑜
𝑆𝑅−∞ = 𝑆𝑅 − 𝑆𝑅 𝑜𝑢𝑡−𝑜𝑓−𝑏𝑎𝑛𝑑 𝑡𝑜𝑡𝑎𝑙 𝑖𝑛−𝑏𝑎𝑛𝑑
9 Ph.D. dissertation of Steven K. Moyer, Georgia Institute of Technology, as well as NVESD and Driggers, Vollmerhausen, and O"Kane, J. Opt. Soc. Am. A,Vol. 16, No. 5,May 1999.
where H(f) is the Fourier transform of the reconstruction function. Using a reconstruction close to the sinc interpolation would significantly reduce the effects since the in-band spurious response would be zero. An IDA study10 suggested that the least squares approach might provide an additional margin of performance (since the reconstruction is superior to the sinc reconstruction), but a complete human observers study has not been performed.
10 Wiener Interpolation Function for Aliased Imagery, IDA Document NS-D-4122, October 2010.
• In many practical cases, dealing with zooming is a matter of training.
– Don't over-zoom: If "jaggies" appear, one has zoomed too far.
– Jaggies represent unphysical information from the aliased signal sidebands.
• Why does the size matter?
– One's eyes cannot see the jaggies unless one zooms: eyes act as
reconstruction filters.
• A proper reconstruction can reduce the need for training and improve performance: performance on calibration targets can be improved 20%
Reconstruction appears most often in the context of zooming in on an image. Zooming implies that more than one display pixel is used for each sample, and therefore a reconstruction approach must be made, no matter whether the choice is apparent to the user. It is important to recall that the appearance of the image can depend on the size of the displayed image. The small image, for which the pixel boundaries are difficult to perceive, is more interpretable than the larger version of the same image. In the large version, pixilation (or jaggies) is very distracting if viewed directly especially for the 45- degree patterns shown. (The square pixel reconstruction is not compatible with the rotated image).
Experienced observers can be trained not to "over zoom." A general rule is to stop zooming just as jaggies become visible. However, the existence of jaggies at any zoom level is an artifact of the reconstruction approach. In the terminology of in-band versus out-of-band aliasing, jaggies, which are seen when over-zooming, are part of the out-of- band spurious response.
System Trades: MTF versus Sampling
• Reducing the overall MTF reduces contrast but also reduces the risk of aliasing artifacts.
For a high sampling rate, the high MTF image is clearly the superior image.
High MTF/High Sampling Rate Low MTF/High Sampling Rate
High MTF/Low Sampling Rate
Low MTF/Low Sampling Rate
System trades: Reconstruction vs. MTF
• These sensor trades depend on how the digital information is displayed.
This section addresses the question of how digital samples should be represented in a final image. This is directly relevant for humans observing the image, but this can also matter if multiple images are to be combined. The images on the top row are low sample rate images with high and low MTF. In this case, the sample values are displayed (reconstructed) with more than one display pixel (pixel is a word for a "picture element" and properly should be used only in the context of the display of an image) for each sample. Each sample is represented by a small square of pixels, each having the same pixel value. This results in the appearance of "pixilation." The severe aliasing of the upper left image may lead to the lower MTF upper right image being preferred.
The second row uses the same sampled data and again represents each sample with more than one pixel. However, in this case, the pixel values are not the same for each pixel in the small square: they vary according to a reconstruction algorithm. The distracting pixelation effects are removed and the images may be more interpretable.
It is important to stress that the lower row is not "blurred" compared to the upper row. The appearance of sharp edges (particularly in the upper right), which may suggest higher sharpness, is an illusion. The sharp edges are an artifact of the "pixel replication" algorithm used to display the image and are not a real part of the image.
As the images show, choosing a reconstruction algorithm can be an important factor in image interpretability.
Reconstruction 2 Reconstruction 1
A complete MTF characterization and not merely Nyquist arguments are needed to evaluate the anticipated performance.
Performance at frequencies below Nyquist are less likely to be disrupted by sampling effects, but can be (Moiré patterns are low-frequency artifacts produced by strong high-frequency content of the scene).
Performance above Nyquist will define the ultimate limiting performance (maximum range at which any specified task can be performed).
Performance may range from 1.25 to 1.5 x the Nyquist limit.
– Multiple images (giving multiple looks) will extend performance. further
– Even single images with multiple effective sample phases maypermit task performance.
– Improvements may extend to 2 * Nyquist.
Performance above Nyquist will depend crucially on the task.
– Toy tasks such as reading calibration targets are susceptible to analysis.
– The relationship of these tasks to military tasks is uncertain.
– Testing should endeavor to have a mix of analyzable tasks (for system characterization) and operational tasks.
– Operational tasks at "higher" levels such as target identification (rather than simply detection) are hard to define in fully analytical terms.
Sampling, Aliasing, and Reconstruction Summary
Aliasing is an almost inescapable feature of staring focal plane array sensors and refers to the artifacts associated with sampling systems. They can range from Moiré patterns to ambiguously interpreted images of objects with complicated patterns of light and dark.
The presence of aliasing in a system gives rise to a commonly used rule of thumb based on the Nyquist frequency, identifying the resolution of a system with the size of a sample (or pixel) on the target. This underrates the importance of other determiners of resolution such as the modulation transfer function or MTF. Performance may be poorer than that suggested by Nyquist or better than Nyquist, depending on the task. The combination of MTF and aliasing can lead to some unintuitive tradeoffs: poorer MTF may actually improve performance in some tasks if aliasing is a significant problem.
For imaging systems with aliasing, the display of the sensor information becomes important, especially if the image is zoomed so that one display pixel is used to represent a single sensor sample value. An improper reconstruction of the sensor data can reduce performance. For all aliased systems, an understanding of the reconstruction algorithm is an important aspect of any system including a human operator.
G. Color Aliasing in Bayer Cameras
Seeing Color in Black and White
Color aliasing is a common property of commercial Bayer reconnaissance cameras (but not amateur cameras like Nikon, Canon, Olympus, and Sony)
The purpose of this section is to discuss additional issues that arise from the use of Bayer pattern cameras. In addition to the aliasing usually associated with digital sensors, Bayer pattern cameras may have color aliasing.
Just as the aliasing of a monochromic camera may be addressed by different reconstruction functions, the effects of the color aliasing depend on the deBayering (or demosaicing) algorithm used to generate the interpolated red, green, and blue values.
In the image shown, the combination of sensor MTF and demosaicing algorithm have produced severe color aliasing. The white bars on the black background of the calibration target appear to have colors, a blue-green and orange. At the triangular fiducial marks, the bars of the target are blurred together to form blue-green or orange blurs.
Color Systems
Full color systems have multiple lenses (Intergraph DMC , Vexel UltraCam) or beam splitters (Leica ADS-80) with separate arrays for each color.
Bayer systems use arrays of mixed red, green, and blue detectors ("pixels").
– Cheaper
– Exploits consumer electronics for arrays
– Large fields of view using multiple Bayer arrays
– Lower storage and bandwidth requirements.
Bayer systems have color aliasing in addition to ordinary aliasing: the space between red samples is 2 x detector size.
– For a "4 megapixel" array, only 1 million red, 1 million blue, and 2 million green.
– An algorithm is required to produce 4 million R,G, B values.
– The algorithm will affect system performance, including resolution.
Full color systems have separate focal planes for each color (red, green, blue and, in some cases, near infrared). Since the focal planes are separate, they require separate optical paths.
In some cases, this is performed by completely separate lens systems as illustrated in the upper photograph. On the left, the UltraCam by Vexel uses separate optics for red, green, blue, and infrared, supplemented by four additional panchromatic lenses for higher resolution. On the right is the DMC II by Intergraph, which uses one panchromatic camera and the four additional red, green, blue, and near infrared.
For line-scanners, such as the Leica ADS-40, a single primary optical system can include a beam splitter separating the light into different bands directed to different rows of detectors.
Bayer pattern cameras can be less complex and expensive than full-color cameras. By providing color information in a single focal plane (at the cost of increasing the sample distance for each color), significant savings can be made.
For both types of color cameras, additional complexity may be introduced to provide a wider field of view. The lower photograph shows a multi-lens system [manufactured by the Russian firm NPO KSI (Scientific Production Union – KSI)] that uses several Bayer pattern focal planes with each lens, interleaving them to form a final image.
Bayer Patterns
Providing a full set of R, G, and B values at each site is called "deBayering" or "demosaicing."
There are many different approaches to deBayering
– Linear interpolations:
Band-by-band (missing G pixels depend only on G pixels)
Cross-band (missing G pixels depend on G and R/B pixels)
– Hue based – Assuming G pixels provide brightness and then useR/B pixels to determine hue (colorizing)
– Gradient estimators – Avoiding averaging across an edge
– Other approaches use non-linear techniques (median filters)
Approaches can be simple, using only the nearest neighbors or complex with a larger number of measured values involved
DeBayering is the process of generating by some algorithm estimates of the sample values that would have been produced by a full-color array. For example, for each red sample value, three additional sample values must be produced.
An enormous range of algorithms exist for deBayering. However, in contrast to the Wiener filter, there is no established theoretical basis for choosing one algorithm over another. The filters can be linear: averaging sample values from the measured detectors to interpolate new values. This can be done for each color separately, but it has been found useful by some authors to mix colors, using the intensity of green samples as indicators of brightness and using those values to influence nearby red interpolated values. An example will be shown in a subsequent chart.
Another algorithm uses the more numerous green values to estimate the panchromatic brightness of the scene, and then using the red and blue values to estimate the color. This may work on scenes that are not too dramatically colored.
The source of the blue-green and orange errors on the black-and-white calibration target can be understood in the simple nearest-neighbor linear deBayering algorithm. Imagine that the detector locations fell on the white stripes as shown at the left, with only blue and green detectors on the white stripes and red detectors always on the black background.
Consider a red site between two of the white stripes. There is no red value at that site, so in the simple algorithm, the red value in the final result will be zero. However, both blue and green values will be assigned since there are blue and green neighbors.
Similarly, along the white stripe, no red values will be assigned, but both blue and green values will be assigned at each point.
The result will be a blue-green color assigned along the white bars and along the black spaces between the bars. The bars will disappear into a blue-green smear.
Interpolation Errors • Original and two Bayered then deBayered images
Original (full-color camera) Bayered: DeBayered with Bayered: DeBayered with simple linear interpolation Microsoft interpolation
Just as some image interpreters prefer the jaggies of pixel-replication zooming (primarily because of familiarity but also because allows recognition of over-zooming), some interpreters prefer the image with color aliasing to the apparently superior image produced by the Microsoft algorithm.
As in the case of zooming, there is no way to avoid some algorithm for deBayering, and there is no reason not to use more sophisticated algorithms.
Exotic Bayer Artifacts • Colors can go beyond blue-green and orange.
– Notice that the horizontal bars on the left are apparently vertical (and orange)
The Bayer artifacts may extend over long distances depending on how large a region is used for the interpolation.
– In the lower image, the top row of bars has a small separation between groups of bars; the demosaicing algorithm connects across different bar groups producing the dramatic colors.
– By separating the bar groups, the Bayer anomalies are removed.
The Bayer artifacts will depend on the algorithm and the objects imaged!
The presence of color artifacts depends upon both the demosaicing algorithm and the scene.11 In general, algorithms with less color aliasing are more expensive computationally.
Color Aliasing in Bayer Cameras Summary
• The use of Bayer pattern color camera in imaging systems in order to reduce cost and data rate requirements may introduce additional dependence on algorithmic choices. In contrast to full-color cameras, a Bayer camera does not have a color detector for all three colors (red, green, blue) at each location (a 12 "megapixel" Bayer sensor has 6 million green, 3 million red, and 3 million blue detectors). An algorithm is used to interpolate the missing values to produce a complete three-color image.
This color aliasing is more severe than the aliasing intrinsic to any staring focal plane. Fortunately, in the natural world, the color information is usually relatively immune to aliasing effects. However, a large number of different algorithms of varying complexity may be employed by a sensor manufacturer. Depending on the tasks to be performed and the details of the image, the algorithm may induce new artifacts that complicate the evaluation of the system.
Ideally, the user could be given some control over the interpolation algorithm to match it to the task.
11 Patrick C. Hytla, Demosaicing Algorithm Performance for the Open Skies Treaty (White Paper), Sensor Systems Division, University of Dayton Research Institute, Dayton, OH, May 25, 2011.
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Appendix A Acronyms and Terms
3D three dimensional
ADC Analog to Digital Conversion Al2O3 sapphire
AlGaAs aluminum gallium arsenide
CO2 carbon dioxide
CTF Contrast Threshold Function
DSP Defense Support Program EO electro-optical
FAR false alarm rate
FFT fast Fourier transform
FLIRS forward-looking infrared systems FOV field of view
FPA focal plane array
GaAs gallium arsenide
Ge germanium
GIQE General Image Quality Equation GSD ground sample distance
H2O water
HgCdTe mercury cadmium telluride
ICBM intercontinental ballistic missile IFOV instantaneous field of view IMM interacting multiple model InGaAs indium gallium arsenide
InSb indium antimonide
IR infrared
IRFPA infrared focal plane array
IRST infrared search and track
ISR intelligence, surveillance, and reconnaissance
L emitted radiance
LOS line of sight
LWIR long-wavelength infrared
MHT multiple hypothesis tracker
MODTRAN MODerate resolution atmospheric TRANsmission MRT minimum resolvable temperature
MTDP minimum temperature difference perceived
MTF Modulation Transfer Function
MTI moving target indicator
MWIR mid-wavelength infrared
NEI noise equivalent irradiance
NETD noise equivalent temperature difference
NIIRS National Imagery Interpretability Rating Scale NIR near-infrared
NUC Non-uniformity Correction
NVESD Night Vision and Electronic Sensors Directorate NV-IPM Night Vision Integrated Performance Model
NVThermIP Night Vision Thermal and Image Processing
OBC Optical Bar Camera OH hydroxyl
Pd probability of detection RER relative edge response
SAR synthetic aperture radar
SBIRS Space-Based Infrared System
SGR sky-to-ground ratio
SNR signal-to-noise ratio
SSCamIP Solid State Camera and Image Processing SWaP Size, Weight, and Power
SWIR short-wavelength infrared
TTP Targeting Task Performance
UAV unmanned aerial vehicle
UDRI University of Dayton Research Institute UV ultraviolet
VLWIR very long-wavelength infrared μm micrometer
Bayer pattern color camera
deBayerization (demosaicing)
Detector Detector size
Detector pitch Full color camera Luminance
Minimum Resolvable Temperature (MRT)
Modulation Transfer Function (MTF):
Nyquist frequency
Radiance Reconstruction
Sample Sampling rate
A consequence of modern digital sampling. Introduces distortions into the image.
Focal plane includes a mixture of detectors for red, green, and blue.
Interpolating missing red, green, and blue values for a Bayer camera.
Photo-sensitive device for measuring incident radiation. Detectors are typically square with size ranging from 4 (visible) to 25 m (IR)
The spacing between detectors. The detector size is ≤ the detector pitch.
Separate focal planes for red, green, and blue detectors. Contrast with Bayer camera.
A measure of emitted or reflected light per area, expressed in units of foot-Lamberts or candela per square meter.
An IR performance measure giving the temperature difference required to resolve features at different spatial frequency.
The frequency response of an optical system including the optics, lenses, vibration, etc.
1⁄2 the sampling rate of a digital system. If the highest spatial frequency in a scene is less than the Nyquist frequency, the system is unaliased.
Properly, a displayed "picture element." Loosely, a detector or sample.
The energy radiated or reflected by an object.
The process of taking digital data and displaying it or interpolating it.
The result of digitizing the output of a detector. The spacing between digital samples. May be expressed in angular terms or spatial terms.
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