Radar was developed in World War II to detect enemy aircraft. It has subsequently been refined to detect a large variety of objects, including ships, helicopters, satellites, and land vehicles. Radar systems typically work on the principle of bouncing microwave radiation off an object and analyzing the reflected signal (echo). The reflected signal can be used to develop information about the object, e.g., by measuring the round trip signal (echo) time the distance to the object can be determined, and by determining a Doppler shift of the echo a velocity of the object may be estimated. With sophisticated system design, object shape and size may be analyzed. Finally, a temporal analysis of sequential echoes may be used to detect a motion vector and characteristics of moving parts of the object.
Radar systems thus emit an electromagnetic wave or pulse, and analyze a reflection pattern to determine a characteristic of the object, distinguishing the object from clutter and background based on a return time of the echo. Radar is typically employed to determine an object profile, or shape, distance (range) and/or its velocity.
Electromagnetic detection techniques have developed to include radio frequency and microwave Radar, laser Radar (Lidar), FLIR (forward looking infrared), fluorescence techniques (especially to detect jet engine combustion emissions) and visual techniques.
Once Radar saw widespread use, military planners saw the military advantage that would accrue from having craft that are invisible to Radar. After decades of research and development, the United States began deployment of so called stealth aircraft in the 1980's. The next generation of helicopters, ships and missiles are also designed to be “stealthy”. Any craft can be designed to be stealthy, including land craft and satellites. The design principles of stealth aircraft are principally to (a) reduce radar reflections, especially retroreflections, of all kinds, and (b) to particularly hide or reduce characteristic signatures of aircraft, such as signals produced by engine turbine blades and wing surfaces.
The primary method for making an object stealthy is to reduce its radar cross section. While much of the performance of stealth aircraft is classified, it has been claimed a stealth fighter has the radar cross section of a normal plane the size of a bird, i.e., that it reflects no more microwave energy back to the detection device than a non-stealth plane the size of a bird.
There are several techniques, applied together, that are used to effect stealth. One is to design the craft so that flat surfaces are divided into small areas of various inclinations, disposed to avoid reflecting the signal directly back to the receiver. The craft is designed such that exposed surfaces present oblique angles or rounded surfaces that scatter or diffuse the signal away from the source of the radar beam. In addition, surfaces are coated with materials that absorb microwave radiation, and honeycomb sections are formed which trap microwaves, preventing reflections. See, U.S. Pat. Nos. 5,808,577, 5,697,394, 5,694,763, 5,536,910, 5,420,588, 5,276,477, 5,036,323, 4,606,848, 4,173,018, 4,117,485, 4,030,098, 4,019,699, expressly incorporated herein by reference.
The United States no longer has a monopoly on stealth craft. After the efficacy of stealth was proved during the Persian Gulf War, Germany, Russia, South Africa and other developed countries accelerated their development of stealth craft, and now not only have stealth craft for their own use, but are poised to sell stealth craft to developing countries, some of which are hostile to the United States.
Therefore, it is becoming increasing important for any military to be able to detect stealth craft.
The existing methods for detection of stealth aircraft include thermal signatures, exhaust signatures, acoustic signatures (see, U.S. Pat. No. 4,811,308, expressly incorporated herein by reference), radar employing non-traditional wavelengths (see, U.S. Pat. Nos. 5,850,285, and 5,657,022, expressly incorporated herein by reference), satellite imagery, and analysis of radio frequency emissions from the aircraft. However, none of these methods replaces traditional Radar monitoring.
U.S. Pat. No. 5,990,822 (Honigsbaum, Nov. 23, 1999), expressly incorporated herein by reference, describes a system for detecting stealthcraft based on silhouette methods, e.g., where the receiver aperture is aligned with an outgoing transmitted beam. Distance to an object is estimated by triangulation and sequence of beam returns.
The present invention therefore provides a method and apparatus for the detection of objects, e.g., all craft types, regardless of whether they are designed to have a low radar profile or not, and thus including both stealth craft as well as non-stealth craft. In particular, it is sought to detect airplanes, Intercontinental Ballistic Missiles (ICBM), helicopters, satellites, cruise missiles, pilotless drones, balloons, High Altitude Long Endurance (HALE) platforms (which are robotically piloted dirigibles or winged craft), ships, boats, submarines, tanks, trucks, armored personnel carriers, and cars.
The present invention operates by detecting, not the echo of an electromagnetic wave reflecting off an object, but rather an attenuation of an electromagnetic wave pattern due to obstruction of beam propagation by the object. Therefore, design principles of stealth craft which seek to absorb microwave radiation will increase contrast, making them “visible”.
While beam interruption sensors are well known and used in security systems and industrially, the present system includes a number of distinctions. The system according to the present invention does not seek to provide a narrow beam that is fully blocked by the object to be detected. Rather, at the typical region of intersection between the beam and the craft, the beam illuminates a much larger area than the cross section of the craft. The present invention, in fact, seeks a wide area of coverage, and therefore provides a region of detection significantly larger than a “line of sight”. It is noted that, in traditional systems, detection is limited to “line of sight”, possibly with predetermined reflections of the beam, and off axis sensitivity is extremely limited by design. Thus, according to the present invention, a large volume of space may be monitored by a detector node, similar to traditional Radar installations and in contrast to known shadow detectors.
Video detectors are also known. These detectors monitor pixels of an imaging sensor for illumination changes, which may be due to shadowing of a background. These systems, however, are limited to certain electromagnetic bands, for example mid- or near infrared to X-ray ranges. As such, these systems are only employed in limited range applications, since beam propagation may be limited by atmospheric conditions or noise, and typically are difficult to accurately detect over long distances through the atmosphere. In contrast, the present invention employs a long range detection system, for example having a detection range of at least several miles, and detection over a large volume, for example at least several cubic miles.
The principal of the Negative Radar can best be explained in terms of an analogy. Suppose an airplane was coated with a surface that absorbed all visible light, thus reflecting no light. If, during the night, you aimed a search light at the airplane, you would not see any reflected light, making the plane not visible, thus effectively invisible. However, if you observed the same airplane flying the next day against a blue sky, you could see the silhouette of the airplane.
Similarly, the present invention provides a method and apparatus for detecting an alteration in a background radiation pattern resulting from an object interfering with transmission thereof.
In order to be effective, the electromagnetic wave path between the region to be monitored and the receiver must have a set of convergent wave paths. Typically, this is effected by providing an intermediate scattering of the electromagnetic beam. While this intermediate scattering reduces beam power efficiency as compared to a substantial retroreflection, in typical applications thus reduction in sensitivity is compensated by an increase in output power, or the use of an existing high power irradiation source.
It is noted that one method for defeating the detection method and apparatus according to present invention is to emit a radiation pattern from the object corresponding to a presumed or measured background pattern, in order to avoid detection. In order for such a system to also defeat detection by normal Radar and radio frequency emission monitoring methods, a phased array antenna must accurately detect the incident illumination pattern and a phased array antenna on an opposing craft surface must retransmit the corresponding pattern, wherein the phased array antennas must encompass an area on each face of the craft (e.g., top, bottom, sides, front and rear) and must be themselves “stealth” designs. Such an anti-detection system is therefore another aspect of the present invention. See, U.S. Pat. No. 4,684,952, expressly incorporated herein by reference.
In one embodiment of the invention, specific artificial sources of radar emissions are deployed and/or employed to specifically define a pattern to be interrupted by the craft to be detected. It is noted that typical stealth designs make presumptions regarding the angle between the emitted Radar wave for detection and the receiver, i.e., that these are close or identical. Therefore, a particular design principle of stealth craft is to avoid any direct reflections or retroreflections of microwave energy. These presumptions fail where the angle is substantially different from zero, for example the limit case of obscurance of a microwave source. However, these methods also fail under other circumstances.
As used herein, the phrase Negative Radar refers to the effect wherein the silhouette of any craft, including a stealth craft, will block transmission of a Radar beam, resulting in detectability of the attenuation of the microwave radiation. The Negative Radar approach can be used with active or passive detection techniques.
In an active detection technique, electromagnetic energy, such as radio frequency, microwave, visible light, or infrared light (from a laser) is directed toward a target, and the interaction of the emitted energy with the target is used to detect the presence of the target, and to derive characteristics of the target, such as distance, bearing, speed, size, and profile. According to the present invention, the beam transmission characteristics are used for detection, rather than reflection characteristics.
In an active detection scheme according to the present invention for Negative Radar, an electromagnetic wave is bounced off a large reflector, such as the Earth, and the silhouette (or attenuation of the electromagnetic wave) produced by the craft, by blocking part of the wave or part of the reflection of the wave, is detected.
In a passive detection embodiment of the invention, no energy is intentionally directed toward the target. Instead, natural or preexisting (and relatively uncontrolled) sources of electromagnetic radiation are employed to look for the silhouette (or attenuation of the beam) of the craft. Typically, the passive detection techniques will employ background radiation from the sky (e.g., 3 degree K black body radiation), or the infrared energy emitted by the Earth (e.g., 300 degree K black body radiation). Another useful source of “passive” energy is man-made satellites, for example GPS satellites and the Iridium satellite constellation, which each have almost complete coverage of the globe and well defined radiation characteristics.
It is therefore an object of the invention to provide a method for the remote detection of an object within a large space, comprising detecting a normal pattern of illumination of the space with electromagnetic radiation, allowing the object to enter the space, and detecting an attenuation from the normal pattern resulting therefrom. In this case, the space is substantially larger than the object, and the aperture of the receiver is wide.
It is also an object of the invention to provide a method of operating a negative radar device for detecting objects, e.g., stealth craft or non-stealth craft, herein called “Stealth Craft”, comprising the steps of either detecting the absence of microwave radiation, or both transmitting microwave radiation and detecting the absence of microwave radiation, due to the stealth craft attenuating (blocking) the microwave radiation when it positioned between the source of microwave radiation (or a reflection from the source) and the microwave detector or receiver (or surface that reflects microwave to the detector or receiver).
It is a further object of the invention to provide a method and apparatus for detecting an object, comprising the steps of defining expected characteristics of a scattered invisible electromagnetic radiation pattern to be detected at a receiver, attenuating at least a portion of an invisible electromagnetic radiation field by a presence of an object within a path of invisible electromagnetic radiation, said invisible electromagnetic radiation propagating off axis with respect to the receiver toward a scattering medium, and detecting the attenuation to indicate a presence of the object. The electromagnetic radiation may be man made or natural, and therefore sources such as earth (terrestrial) background radiation in the infrared band and cosmic background radiation in the microwave bands may advantageously be employed. The present invention may also use incidental effects from man-made radiation transmitted for unrelated purposes, or cooperating transmitters and receivers. The transmitter and/or receiver may be highly directional (collimated), in order to provide precision in localization or higher signal to noise ratio. Antenna apertures may be mechanically scanned, or comprise synthetic aperture systems with logically defined apertures. Adaptive background analysis techniques may be performed to differentiate dynamic effects from static effects.
According to a preferred embodiment of the invention, a receiver is provided displaced (e.g., substantially spaced) from the source of the electromagnetic radiation, wherein the perturbation in the electromagnetic radiation is detected as a displaced shadow on a distant scattering medium, such as the earth, or overhead, such as clouds or atmospheric particulates. The present invention also provides a system and method wherein a transmitter generates the electromagnetic radiation, a receiver detects the electromagnetic radiation, the transmitter and receiver having known positions with respect to the Earth, with a distance to the object being determined based on the known location of the receiver and the transmitter and by the vector from the receiver to a shadow of the electromagnetic radiation formed by the object on the Earth. Likewise, at least two electromagnetic radiation waves may be generated by at least two transmitters and a receiver, each with a known position, wherein a distance to the object is determined based on the known location of the receiver and both transmitters and by the vector from the receiver to the shadow from the first transmitter in geometric relationship with the vector from the receiver to the shadow from the second transmitter.
The object may be identified based on a computed distance to the object, the detected attenuation of the electromagnetic radiation, and a predetermined characteristic of the object. A system is also provided wherein a wavelength of a radio wave transmission is varied about a range including the effective size of the object, wherein as the wave exceeds the effective size, the objects apparently disappears. By monitoring perturbation (e.g., attenuation) of the silhouette (i.e., transmitted wave propagation axis and receiver aperture aligned) or shadow (i.e., transmitted wave propagation axis and receiver aperture not aligned), the effective size of the object may be determined. Typical objects of interest have sized and effective sizes in the range of between about 1 to 100 meters, and therefore a transceiver system adapted to operate in the 1 to 100 meter band may be used for such detection.
The invention also provides a negative radar device for detecting an object, e.g., stealth craft or non-stealth craft, comprising either a microwave receiver and optionally a microwave transmitter, said detector detecting the absence or attenuation of microwave radiation due to attenuation of the microwave radiation when the object is within the aperture of the receiver, e.g., generally positioned between the transmitter or other source of microwave radiation (or a reflection from the transmitter or other source) and the microwave receiver (or surface that reflects microwave to the detector).
Microwave, as generally used herein, may also encompass any electromagnetic radiation capable of attenuation by the object, unless specifically limited by the context. The object may be, e.g., any type of craft, e.g., airplanes, Intercontinental Ballistic Missiles (ICBM), helicopters, satellites, cruise missiles, pilotless drones, balloons, High Altitude Long Endurance (HALE) platforms, marine ships, boats, submarines, tanks, trucks, armored personnel carriers, and cars.
The microwave radiation may be, for example, the omnipresent cosmic background radiation, the blackbody radiation from the Earth, microwave radiation reflected from the ground or sky. The system may provide a single microwave transceiver for emitting and receiving the microwaves, or the transmitter and receiver may be spatially separated.
In order to collimate the microwaves for detection of small areas within the detection space, tubes may be used to limit the field of view that is seen by each detector, thus increasing the percentage attenuation caused by a Stealth Craft in that pixel of the Sky.
The aperture of a transmitter or/or receiver may be limited, to provide one or more narrow bands of electromagnetic radiation or apertures for receipt of radiation, in the form of a “picket fence”. These bands may be static or swept. For example, the receiver may be omni-directional, while the transmitter sweeps the sky with bands of directional radiation. Alternately, the transmitter may be omni-directional, while the receiver may sweep the “sky” with bands of directional “beam” sensitivity, through the use of a moving mechanical antenna or a phased array radar system.
The distance to an object, e.g., a stealth craft, may be determined from the known location of both receiver and transmitter and by the vector from the receiver to the shadow of the stealth craft on the Earth in geometric relationship to the vector from the receiver to the silhouette of the stealth craft against the Earth.
According to another embodiment, there are at least two transmitters and at least one receiver, or there are at least two receivers. For example, two transmitters are provided, and the distance to the stealth craft is determined from the known location of the receiver and both transmitters, and by the vector from the receiver to the shadow from the first transmitter in geometric relationship with the vector from the receiver to the shadow from the second transmitter.
The transmitter need not be controlled or coupled to the detection system. For example, the transmitter may be a non-cooperating source of microwave radiation, such as a Direct Broadcast TV satellite, geopositioning (e.g., GPS or GLONASS) satellite, or a personal communication satellite. Therefore, the system need only provide a receiver and phased array antenna to detect and/or determine the distance to Stealth Craft.
In analyzing the received signal, an adaptive receiver design may be employed to cancel the normal illumination pattern. In this case, the background normally reflects or scatters the radiation. However, an obscuring object reduces the return signal. When compared with the adapted baseline signal, however, the silhouette and shadow of the stealth craft is seen as a positive indication of change in pattern.
The distance to the object, e.g., stealth craft, may be determined by comparing the apparent size of the stealth craft to a presumed actual size of the stealth craft, using geometrical techniques well known in the art.
These and other objects will be apparent from an understanding of the preferred embodiments.
These and further objects and advantages of the invention will be more apparent upon reference to the following specification, claims and appended drawings wherein:
The preferred embodiments will now be described by way of example, in which like reference numerals indicate like elements.
Active Detection
In standard active detection, a beam of electromagnetic energy, such as microwave, visible light, or infrared light (from a laser) is directed toward a target and the energy reflected from the target is used to detect the presence of the target, and to derive characteristics of the target, such as distance, bearing, speed, and size.
However, according to the present invention, negative radar, a microwave beam is bounced off a large reflector, such as the Earth, and the silhouette (or attenuation of the microwave) that the object produces against the beam or a reflection of the beam is detected. This method can also be used with non-stealth craft, since the Doppler shift of microwaves reflected from a non-stealth craft can be used to differentiate it from the microwave reflected from, e.g., the Earth, so that the microwaves reflected directly from the non-stealth craft can be ignored or separately analyzed.
The Doppler shift can also be used to detect and defeat a possible electronic countermeasure against negative radar. If a stealth craft emanated microwave radiation in an attempt appear transparent to the rays, e.g., not to produce a “silhouette” for the negative radar, the Doppler shift could be used to differentiate the microwave emanated from the stealth craft from the microwave reflected from, e.g., the Earth. Therefore, a successful countermeasure would not only have to emit radiation in the appropriate pattern, it would also have to be Doppler compensated. This would require, for example, a complex phased array transceiver system which measures electromagnetic radiation on any one surface and reemits it on an opposite surface, potentially requiring simultaneous transmission and reception in the same range or frequencies from all surfaces.
The following is an example of Negative Radar and active (as opposed to passive) detection. An aircraft, HALE craft, or satellite is provided at an altitude above that of the craft to be detected. A down-looking beam of electromagnetic energy is swept across the ground. The beam, in this case, could be infrared light (via a laser), microwave (with the beam steered either mechanically or electronically with a phased array antenna), or some other electromagnetic radiation, although microwave radiation is preferred. It is presumed that the ground below scatters the radiation, and therefore, the illuminated area will be substantially visible to the receiver.
For example, an aircraft is provided having a phased array Radar antenna, to allow for a full sweep of the entire zone of interest. As shown in
When a Stealth Craft 1025 crosses an individual beam, the strength of the beam reflected from the ground is attenuated, because the Stealth Craft blocks a portion of the beam coming from the craft to ground, as well as part of the reflection of the beam from ground back to the aircraft. Therefore, in this case, it is possible to visualize the Stealth Craft as a “dark” area against the “white” background of Microwave reflected from the ground. This analysis, of course, preferably automated, and may involve high levels of analysis, for example to reduce noise, check consistency with other sensor systems, and adaptively process the signal. Typically, a background or normal radiation pattern from the ground is determined, and the received radiation compared with the background to determine the characteristics of the reflected components.
As shown in
One way to find the distance to the Stealth Craft is a method of triangulation, as shown in
Since we know the absolute position of the two detecting craft, e.g., by the use of GPS, and we know the angle of the Stealth Craft relative to the two detecting craft, and we know the Z position of the Stealth Craft, we can form a triangle, and calculate, using basic geometry, the X, Y, Z position of the Stealth Craft, and thus the distance from each Radar to the Stealth Craft. The accuracy of the distance determination depends upon, for example, the width of the individual beams.
If only one Radar is used, the traditional way to determine the distance to a non-stealth Craft is to measure the time that it takes to receive the Microwave echo from the craft. Since the speed of Microwave in the air is known, about 300,000 KM/second, the distance to the craft may be determined. With a Stealth Craft, the echo from the craft is presumed unusable, so the distance to the Stealth Craft must be determined by other means.
One way to determine the distance is to compare the apparent size of the Stealth Craft to the actual size of the Stealth Craft, using geometrical techniques well known in the art and presumptions of the nature of the Stealth Craft. The apparent size is the size of the silhouette. The actual size can thus be determined by reading a computer reference file for the aircraft dimensions of the particular Stealth Craft suspected of detection. Ambiguities may be resolved by other data, such as maximum velocity, and radar signature characteristics. It is noted that traditional Radar is ineffective in detecting the presence of a Stealth Craft because of the large number of possible interfering signal sources and noise. On the other hand, where a specific position of a craft is suspected, numerous techniques may be employed to verify the existence of the craft.
Another way to find the actual size of the Stealth Craft is by increasing the wavelength of the Microwave until the silhouette disappears, i.e., until the size of the craft (cross-section) becomes a fraction of the wavelength, so that the Stealth Craft does not effectively attenuate the Microwave signal and thus becomes “invisible” to the Microwave.
The azimuth resolution, i.e., the minimum size of a feature you can detect, is dependent on the size of the antenna, the distance from the Radar to the object, and the wavelength, and is given by:
Resolution=(Wavelength×Range)/antenna length
Wavelength=(Resolution×Antenna length)/range
Thus, for a given antenna size, range and desired resolution, the wavelength needed to effect the needed resolution is defined, e.g.,
Wavelength=(1 m×20 m)/10,000 m
Wavelength=0.002 m
=2 mm
The aforementioned distance measurement techniques would also work for non-stealth craft, since the Doppler shift of microwaves reflected from the non-stealth craft could be used to differentiate it from microwave reflected from the ground, so that the microwaves reflected from the craft could be ignored. Thus, by providing a filter to detect microwaves shifted by an amount representing a minimum presumed velocity of an aircraft, background clutter may be effectively eliminated.
Active downlooking Radar will show clutter, i.e., reflection from the ground. The varying characteristics of the surface of the ground and items on the surface will result in a varying amount of reflected microwave signal from the ground.
This ground clutter can be eliminated by the use of cancellation, a technique well known in the art.
As shown in
However, the delay is selected such that as the Stealth Craft transverses the detection zone, the edge of the Stealth Craft will be shown as a “white” edge, i.e., all microwave energy reflected will be cancelled, except that at the edge of the craft. As shown in
Thus, the leading and trailing edges of the craft will be the only areas where the microwave will not be either blocked or cancelled. While this technique is subject to noise limitations, the precision may be improved by correlating leading and trailing edge detections, which should be spaced in time according to the size and speed of the craft. The transverse distance the Stealth Craft moves during each pulse determines the “width” of the leading edge of the Stealth Craft. At a speed of 1 KM/sec., the Craft would move 1/300 KM during a 1/300-second pulse interval, thus the leading edge would be about 3.3 meter.
When a Stealth Craft is detected, another option is to freeze the background cancellation, i.e., to cancel with the same (pre-stealth craft detection) background as long as the Stealth Craft is being detected, such as with a analog amplitude adjusted phase lock loop or digital background cancellation. This results in the craft (actually the silhouette of the craft) being entirely “white” (microwave source) as shown in the
In addition to detecting the silhouette of a Stealth Craft against a microwave source, another method of detecting a Stealth Craft is to detect the shadow the Stealth Craft makes on a reflecting surface, such as the Earth.
As in detecting a silhouette, the attenuation of the Microwave by the Stealth Craft is to be detected. Thus results in a “dark” area on a “white” (reflecting) surface.
As with detection of a silhouette, background cancellation may be used to cancel the background and make the shadow “white”, so that a “white” patch on a “dark” background is sought. In this case, a moving average cancellation technique may be employed, for example with a time constant of about 15 seconds. In this case, as a Stealth Craft enters the aperture, the change against the background will be apparent, yet changes in the background over a slower time-course will be compensated. Alternately, an adaptive cancellation system may be implemented, which may, for example, halt adaptation during the period of detection of an event, to provide maximum “contrast” of the event. Other, more complex filtering algorithms may also be employed. In any case, as a Stealth Craft is being detected, then the shadow of the stealth craft becomes “white” (microwave source) and the non-shadow background becomes “dark” (no microwave) as shown in
As discussed above, the negative Radar technique works for non-stealth craft, as well as for stealth craft. This is important because it may not be determined, a priori, if a craft being detected is a stealth craft or non-stealth craft, and thus a single detection system, compatible with both types of craft, may be desired.
An electronic picket fence can be established such that the craft transmitting the microwave is a satellite, high-flying aircraft, or High Altitude Long Endurance (HALE) craft and the receiver is on a second craft that is passively receiving the microwaves, without itself transmitting any microwave signal. The transmitter could be, for example, a phased array Radar sweeping a beam, creating a series of electronic picket fences.
As shown in
Thus, the detecting craft can itself be a Stealth Craft, and the system operational without transmitting any microwaves that could be used to detect it, or used by, e.g., a radar-seeking missile (such as HARM), to destroy it.
A satellite used to illuminate the object need not be a cooperating satellite. There are many commercial, government, and military satellites in orbit. For example, a direct broadcast TV satellite or a geopositioning (e.g., GPS or GLONASS) satellite could be used, without the cooperation of the satellite owner, as long as the microwave carrier wavelength and ground coverage are appropriate. Stability and predictability of the carrier may also be important. As of 1998, there were 220 communication satellites in orbit. Between 1998 and 2003, this is expected to grow to over 1000 satellites, with the orbiting of new fleets of satellites for satellite based cellular telephone service, which are often referred to as personal communication satellites. Some of these satellites will be in low-Earth orbit or mid-Earth orbit, and others will be in geosynchronous orbit.
If two detecting craft detect the Stealth Craft, the distance to the Stealth Craft could be determined by the previously mentioned method of triangulation.
If there is one detecting craft but two or more transmitting sources, as shown in
The transmitted beams 140m and 140n reflect off the ground, and by use of a phased array receiver, having narrow beam input sensitivity, i.e., directional receiving, with two simultaneous “beams” 140t and 140u, the shadow of the Stealth Craft for beam 140m and the shadow for beam 140n may be detected.
Since the location of transmitters 140a, and 140b, and shadows 140e and 140f, and receiver “beams” 140t and 140u and the receiver 140r are known for the time of receipt, simple geometric techniques, well known in the art, can be used to determine the distance 140d from receiver 140r to Stealth Craft 140s.
If there is only one transmitter and one receiver, and they are spatially separated, yet another method of triangulation can be used to determine the distance to the Stealth Craft. As shown in
If either standard triangulation or the triangulation methods shown in
It should be understood that the craft holding the receiver antenna in this case has access to receive a clean representation of the satellite transmission from above, thereby allowing homodyne-type detection and/or the use of phase locked loops.
In an active detection system, there is a transmitted beam and a detected reflected beam. As shown in
Passive Detection
In a passive detection system, no energy is intentionally directed to the target. Instead, the silhouette (or attenuation of the microwave) of the Stealth Craft against an existing energy background, such as the cosmic background radiation in the sky, or the infrared energy emitted by the Earth, is detected.
The cosmic background radiation is an omnipresent microwave source, and is the same in any direction up to 1 part in 100,000. The cosmic background radiation is equivalent to the radiation emitted by a black body at 2.7 degrees Kevin (−270 Centigrade).
The Earth can also be considered a black body, or a gray body, at the temperature of the Earth's surface. The radiation emitted by a gray body depends on its temperature, its emissisity (determined primarily by its roughness) and its reflectivity.
This background energy is much weaker than that used in typical Radar systems. While an x-band Radar has a typical power (brightness) of 4800 watts/meter squared/Hz/steradian, a typical Earth brightness might be 5.4×10−24, in the same microwave frequency range.
Therefore, specialized receivers called Radiometers are used to measure the brightness of background radiation from thermal sources. A bolometer (or superconducting bolometer) may also be used to detect Earth background radiation.
The background radiation is examined to look for either the silhouette of the Stealth Craft or the attenuation of the background that is caused by the Stealth Craft. The Stealth Craft itself can be considered a gray body, but since it is coated with Microwave absorbing material, it should not reflect much microwave nor should it emit much microwave energy. Thus, passive detection of a Stealth Craft against the cosmic background radiation may be more effective for Stealth Craft than non-Stealth Craft.
In addition to detecting Stealth craft, another advantage of passive Negative Radar over conventional Radar is that the detector can be a device that transmits or emanates no microwave radiation. This makes it much harder for the enemy to find and destroy, with e.g., the use of a microwave seeking missile.
If the weak cosmic background radiation is used, a very sensitive receiver, cooled to close to absolute zero (−273 degrees Centigrade) could be used, which is sensitive to this wavelength of radiation. The Cosmic Background Explorer satellite used differential microwave radiometers to look for anisotropy of 1 part in 100,000 in the cosmic microwave background radiation. The NASA Microwave Anisotropy Probe satellite, to be launched in 2000, will also be able to detect anisotropy of 1 part in 100,000. Therefore, systems that analyze spatial variations in this radiation are well known.
The apparatus according to the present invention will look, at any given time, at a small enough piece of the sky so that a Stealth Craft will cause an attenuation of at least 1/100,000 in the strength of the cosmic background radiation. This will be achieved by insuring that the area (pixel) of the sky being observed at any instance is no more than 100,000 times the size of the Stealth Craft to be detected.
For example, the F117a stealth fighter, with a length 60 feet and height of 12 feet, has a cross section of 720 square feet. Thus, (72,000,000 square feet of sky (720*100,000) (about three square miles) around the craft (at the distance of the craft) could be observed at any given instance, and the craft would obscure 1/100,000 of the cosmic background radiation. The detection system would therefore compare the strength of microwaves at the time of detection (time X) to a previous time (time X−1) for that pixel.
As shown in
There are various ways to insure that the area of the sky being observed is no more than 100,000 times the size of a Stealth Craft. For example, if thousands of receivers are used, each can observe a small pixel of the sky. Alternately, one receiver (radiometer) could be rapidly swept, sequentially sensitive to different small regions (pixels) of the sky.
A cosmic background radiation-based system must be directed away from Earth, and is typically limited to coverage of a radius of 50-100 miles, with a height window of 0.5-20 miles. With a 0.5 square mile pixel area at maximum range, (2×100×π×20/0.5) 24,000 pixels would be required. This may be provided, for example, as a rotationally moving scanner with a 64×64 array of detector elements, or as multiple stationary arrays each looking in a somewhat different direction.
As shown in
To allow for the use of a less sensitive receiver, a plurality of tubes can be pointed to one field of view. The microwave signal from all of the tubes could then be combined to form a stronger signal that could be detected by a less sensitive (and perhaps less costly) receiver.
Because of the weakness of cosmic background radiation, and attenuation of the microwaves by Earth's atmosphere, in particular the water vapor in the atmosphere, the use of cosmic background microwave will be most effective when the receiver (radiometer) is in a high flying aircraft, HALE craft, or satellite, and the craft being searched for is a high flying stealth aircraft, stealth HALE craft, or stealth satellite.
Another background radiation source that can be used is the Earth itself. As mentioned above, the Earth can also be considered a black body, or a gray body, at the temperature of the Earth's surface or about 300 degrees K. For example, an infrared receiver on a detecting craft can look at small areas (pixels) of the ground at sequential times, for detecting the attenuation of the infrared radiation produced by a Stealth Craft obscuring part of the radiation from the ground pixel. Since the wavelength corresponding to 300 degrees K is in the infrared range, the normal microwave stealth techniques do not obscure in this wavelength. The skin temperature of the stealth craft is not likely to closely correspond to the ground temperature of the earth below. Thus, the craft will produce a contrast.
Determination of Distance to Target
As shown in
The invention may be embodied in other specific forms without departing from the spirit or essential characteristics thereof. The present embodiments are, therefore, to be considered in all respects as illustrative and not restrictive, the scope of the invention being indicated by the appended claims rather than by the foregoing description, and all changes which come within the meaning and range of equivalency of the claims are, therefore, intended to be embraced therein.
The term “comprising”, as used herein, shall be interpreted as including, but not limited to inclusion of other elements not inconsistent with the structures and/or functions of the other elements recited.
The present application is a Continuation of U.S. patent application Ser. No. 13/471,648, filed May 15, 2012, now U.S. Pat. No. 8,890,744, issued Nov. 18, 2014, which is a Continuation of U.S. patent application Ser. No. 13/093,447, filed Apr. 25, 2011, now U.S. Pat. No. 8,179,299, issued May 15, 2012, which is a continuation of U.S. Ser. No. 09/545,407, filed Apr. 7, 2000, now U.S. Pat. No. 7,952,511, issued May 31, 2011, which is a non-provisional of U.S. Provisional Patent Application No. 60/128,233, filed Apr. 7, 1999, the entirety of which are expressly incorporated herein by reference.
Number | Name | Date | Kind |
---|---|---|---|
3665466 | Hibbard | May 1972 | A |
3715748 | Hicks | Feb 1973 | A |
3725914 | Davidson | Apr 1973 | A |
3881154 | Lewis | Apr 1975 | A |
4337376 | Gruenberg | Jun 1982 | A |
4530087 | Yamamoto | Jul 1985 | A |
4710944 | Nossen | Dec 1987 | A |
4736371 | Tejima et al. | Apr 1988 | A |
4750198 | Harper | Jun 1988 | A |
4797879 | Habbab et al. | Jan 1989 | A |
4937580 | Wills | Jun 1990 | A |
5075863 | Nagamune | Dec 1991 | A |
5134715 | Parl et al. | Jul 1992 | A |
5151919 | Dent | Sep 1992 | A |
5153595 | Harmuth | Oct 1992 | A |
5159343 | Harmuth | Oct 1992 | A |
5173704 | Buehler | Dec 1992 | A |
5203018 | Hirose | Apr 1993 | A |
5228025 | Le Floch et al. | Jul 1993 | A |
5239677 | Jasinski | Aug 1993 | A |
5241544 | Jasper et al. | Aug 1993 | A |
5260968 | Gardner et al. | Nov 1993 | A |
5289499 | Weerackody | Feb 1994 | A |
5295159 | Kerpez | Mar 1994 | A |
5315584 | Savary et al. | May 1994 | A |
5325095 | Vadnais | Jun 1994 | A |
5345599 | Paulraj et al. | Sep 1994 | A |
5404355 | Raith | Apr 1995 | A |
5422733 | Merchant et al. | Jun 1995 | A |
5442625 | Gitlin et al. | Aug 1995 | A |
5448602 | Ohmori et al. | Sep 1995 | A |
5469465 | Birchler et al. | Nov 1995 | A |
5471647 | Gerlach et al. | Nov 1995 | A |
5479444 | Malkamaki et al. | Dec 1995 | A |
5479447 | Chow et al. | Dec 1995 | A |
5481570 | Winters | Jan 1996 | A |
5491837 | Haartsen | Feb 1996 | A |
5493712 | Ramesh et al. | Feb 1996 | A |
5506861 | Bottomley | Apr 1996 | A |
5509003 | Snijders et al. | Apr 1996 | A |
5510779 | Maltby et al. | Apr 1996 | A |
5515378 | Roy, III et al. | May 1996 | A |
5528581 | De Bot | Jun 1996 | A |
5534868 | Gjessing | Jul 1996 | A |
5537435 | Carney et al. | Jul 1996 | A |
5548819 | Robb | Aug 1996 | A |
5566209 | Forssen et al. | Oct 1996 | A |
5579304 | Sugimoto et al. | Nov 1996 | A |
5592490 | Barratt et al. | Jan 1997 | A |
5606729 | D'Amico et al. | Feb 1997 | A |
5634199 | Gerlach et al. | May 1997 | A |
5638369 | Ayerst et al. | Jun 1997 | A |
5642353 | Roy, III et al. | Jun 1997 | A |
5649287 | Forssen et al. | Jul 1997 | A |
5677909 | Heide | Oct 1997 | A |
5691727 | Cyzs | Nov 1997 | A |
5694129 | Fujinawa | Dec 1997 | A |
5729542 | Dupont | Mar 1998 | A |
5752173 | Tsujimoto | May 1998 | A |
5787122 | Suzuki | Jul 1998 | A |
5790550 | Peeters et al. | Aug 1998 | A |
5796775 | Aoyama | Aug 1998 | A |
5809019 | Ichihara et al. | Sep 1998 | A |
5818813 | Saito et al. | Oct 1998 | A |
5822374 | Levin | Oct 1998 | A |
5831977 | Dent | Nov 1998 | A |
5832044 | Sousa et al. | Nov 1998 | A |
5832387 | Bae et al. | Nov 1998 | A |
5859875 | Kato et al. | Jan 1999 | A |
5867478 | Baum et al. | Feb 1999 | A |
5867539 | Koslov | Feb 1999 | A |
5883887 | Take et al. | Mar 1999 | A |
5886988 | Yun et al. | Mar 1999 | A |
5889826 | Takahashi | Mar 1999 | A |
5905721 | Liu et al. | May 1999 | A |
5920285 | Benjamin | Jul 1999 | A |
5959965 | Ohkubo et al. | Sep 1999 | A |
5960039 | Martin et al. | Sep 1999 | A |
5966094 | Ward et al. | Oct 1999 | A |
5973638 | Robbins et al. | Oct 1999 | A |
5982327 | Vook et al. | Nov 1999 | A |
6005876 | Cimini, Jr. et al. | Dec 1999 | A |
6011963 | Ogoro | Jan 2000 | A |
6049548 | Bruno et al. | Apr 2000 | A |
6058105 | Hochwald et al. | May 2000 | A |
6067290 | Paulraj et al. | May 2000 | A |
6072779 | Tzannes et al. | Jun 2000 | A |
6084915 | Williams | Jul 2000 | A |
6097771 | Foschini | Aug 2000 | A |
6115354 | Weck | Sep 2000 | A |
6115427 | Calderbank et al. | Sep 2000 | A |
6122247 | Levin et al. | Sep 2000 | A |
6131016 | Greenstein et al. | Oct 2000 | A |
6141388 | Servais et al. | Oct 2000 | A |
6141542 | Kotzin et al. | Oct 2000 | A |
6141567 | Youssefmir et al. | Oct 2000 | A |
6144711 | Raleigh et al. | Nov 2000 | A |
6154661 | Goldburg | Nov 2000 | A |
6163296 | Lier et al. | Dec 2000 | A |
6167031 | Olofsson et al. | Dec 2000 | A |
6175588 | Visotsky et al. | Jan 2001 | B1 |
6178196 | Naguib et al. | Jan 2001 | B1 |
6192256 | Whinnett | Feb 2001 | B1 |
6205410 | Cai | Mar 2001 | B1 |
6219341 | Varanasi | Apr 2001 | B1 |
6222888 | Kao et al. | Apr 2001 | B1 |
6232918 | Wax et al. | May 2001 | B1 |
6266528 | Farzaneh | Jul 2001 | B1 |
6275543 | Petrus et al. | Aug 2001 | B1 |
6278726 | Mesecher et al. | Aug 2001 | B1 |
6292917 | Sinha et al. | Sep 2001 | B1 |
6298035 | Heiskala | Oct 2001 | B1 |
6298092 | Heath, Jr. et al. | Oct 2001 | B1 |
6308080 | Burt et al. | Oct 2001 | B1 |
6314113 | Guemas | Nov 2001 | B1 |
6314147 | Liang et al. | Nov 2001 | B1 |
6314289 | Eberlein et al. | Nov 2001 | B1 |
6317612 | Farsakh | Nov 2001 | B1 |
6320113 | Griffin et al. | Nov 2001 | B1 |
6330277 | Gelblum et al. | Dec 2001 | B1 |
6330293 | Klank et al. | Dec 2001 | B1 |
6330462 | Chen | Dec 2001 | B1 |
6333953 | Bottomley et al. | Dec 2001 | B1 |
6339399 | Andersson et al. | Jan 2002 | B1 |
6345036 | Sudo et al. | Feb 2002 | B1 |
6346910 | Ito | Feb 2002 | B1 |
6347234 | Scherzer | Feb 2002 | B1 |
6348036 | Looney et al. | Feb 2002 | B1 |
6351499 | Paulraj et al. | Feb 2002 | B1 |
6362781 | Thomas et al. | Mar 2002 | B1 |
6363267 | Lindskog et al. | Mar 2002 | B1 |
6369758 | Zhang | Apr 2002 | B1 |
6377631 | Raleigh | Apr 2002 | B1 |
6377632 | Paulraj et al. | Apr 2002 | B1 |
6377636 | Paulraj et al. | Apr 2002 | B1 |
6377812 | Rashid-Farrokhi et al. | Apr 2002 | B1 |
6377819 | Gesbert et al. | Apr 2002 | B1 |
6380910 | Moustakas et al. | Apr 2002 | B1 |
6385264 | Terasawa et al. | May 2002 | B1 |
6396885 | Ding et al. | May 2002 | B1 |
6400699 | Airy et al. | Jun 2002 | B1 |
6426971 | Wu et al. | Jul 2002 | B1 |
6442214 | Boleskei et al. | Aug 2002 | B1 |
6445342 | Thomas et al. | Sep 2002 | B1 |
6452981 | Raleigh et al. | Sep 2002 | B1 |
6463290 | Stilp et al. | Oct 2002 | B1 |
6473393 | Ariyavisitakul et al. | Oct 2002 | B1 |
6473467 | Wallace et al. | Oct 2002 | B1 |
6477207 | Lindholm | Nov 2002 | B1 |
6477210 | Chuang et al. | Nov 2002 | B2 |
6478422 | Hansen | Nov 2002 | B1 |
6492942 | Kezys | Dec 2002 | B1 |
6493399 | Xia et al. | Dec 2002 | B1 |
6504506 | Thomas et al. | Jan 2003 | B1 |
6542556 | Kuchi et al. | Apr 2003 | B1 |
6556173 | Moustakas et al. | Apr 2003 | B1 |
6567387 | Dulin et al. | May 2003 | B1 |
6584147 | Schaumont et al. | Jun 2003 | B1 |
6587526 | Li et al. | Jul 2003 | B1 |
6603806 | Martone | Aug 2003 | B2 |
6608859 | De et al. | Aug 2003 | B2 |
6614861 | Terry et al. | Sep 2003 | B1 |
6618454 | Agrawal et al. | Sep 2003 | B1 |
6625203 | De et al. | Sep 2003 | B2 |
6636568 | Kadous | Oct 2003 | B2 |
6647015 | Malkemes et al. | Nov 2003 | B2 |
6647078 | Thomas et al. | Nov 2003 | B1 |
6650653 | Horng et al. | Nov 2003 | B1 |
6654429 | Li | Nov 2003 | B1 |
6661856 | Calderbank et al. | Dec 2003 | B1 |
6662024 | Walton et al. | Dec 2003 | B2 |
6678253 | Heath, Jr. et al. | Jan 2004 | B1 |
6683916 | Sartoni et al. | Jan 2004 | B1 |
6686879 | Shattil | Feb 2004 | B2 |
6687492 | Sugar et al. | Feb 2004 | B1 |
6690680 | Marchok et al. | Feb 2004 | B1 |
6701129 | Hashem et al. | Mar 2004 | B1 |
6711412 | Tellado et al. | Mar 2004 | B1 |
6721367 | Miya et al. | Apr 2004 | B1 |
6721569 | Hashem et al. | Apr 2004 | B1 |
6741635 | Lo et al. | May 2004 | B2 |
6751187 | Walton et al. | Jun 2004 | B2 |
6751261 | Olsson et al. | Jun 2004 | B1 |
6757265 | Sebastian et al. | Jun 2004 | B1 |
6757321 | Pan et al. | Jun 2004 | B2 |
6757322 | Schilling | Jun 2004 | B2 |
6757337 | Zhuang et al. | Jun 2004 | B2 |
6760388 | Ketchum et al. | Jul 2004 | B2 |
6760882 | Gesbert et al. | Jul 2004 | B1 |
6771706 | Ling et al. | Aug 2004 | B2 |
6775329 | Alamouti et al. | Aug 2004 | B2 |
6782257 | Moustakas et al. | Aug 2004 | B1 |
6785341 | Walton et al. | Aug 2004 | B2 |
6785520 | Sugar et al. | Aug 2004 | B2 |
6795392 | Li et al. | Sep 2004 | B1 |
6801580 | Kadous | Oct 2004 | B2 |
6807240 | Alamouti et al. | Oct 2004 | B2 |
6816470 | Kim et al. | Nov 2004 | B2 |
6826240 | Thomas et al. | Nov 2004 | B1 |
6834043 | Vook et al. | Dec 2004 | B1 |
6834079 | Strait et al. | Dec 2004 | B1 |
6839335 | Sudo | Jan 2005 | B1 |
6842487 | Larsson | Jan 2005 | B1 |
6850481 | Wu et al. | Feb 2005 | B2 |
6850498 | Heath et al. | Feb 2005 | B2 |
6850741 | Lei et al. | Feb 2005 | B2 |
6853688 | Alamouti et al. | Feb 2005 | B2 |
6859503 | Pautler et al. | Feb 2005 | B2 |
6862271 | Medvedev et al. | Mar 2005 | B2 |
6862272 | Dulin et al. | Mar 2005 | B2 |
6865237 | Boariu et al. | Mar 2005 | B1 |
6868109 | Kohno et al. | Mar 2005 | B2 |
6870515 | Kitchener et al. | Mar 2005 | B2 |
6873651 | Tesfai et al. | Mar 2005 | B2 |
6888809 | Foschini et al. | May 2005 | B1 |
6888899 | Raleigh et al. | May 2005 | B2 |
6891897 | Bevan et al. | May 2005 | B1 |
6898418 | Rauschmayer | May 2005 | B2 |
6912195 | Vook et al. | Jun 2005 | B2 |
6917820 | Gore et al. | Jul 2005 | B2 |
6917821 | Kadous et al. | Jul 2005 | B2 |
6922445 | Sampath et al. | Jul 2005 | B1 |
6925258 | Lo | Aug 2005 | B2 |
6927728 | Vook et al. | Aug 2005 | B2 |
6928062 | Krishnan et al. | Aug 2005 | B2 |
6934320 | Tujkovic et al. | Aug 2005 | B2 |
6937592 | Heath, Jr. et al. | Aug 2005 | B1 |
6937665 | Vandenameele | Aug 2005 | B1 |
6937843 | Foschini et al. | Aug 2005 | B2 |
6947507 | Kelkar et al. | Sep 2005 | B2 |
6954655 | Rudrapatna et al. | Oct 2005 | B2 |
6956907 | Ketchum | Oct 2005 | B2 |
6963619 | Gesbert et al. | Nov 2005 | B1 |
6965762 | Sugar et al. | Nov 2005 | B2 |
6975666 | Affes et al. | Dec 2005 | B2 |
6980600 | Ratnarajah | Dec 2005 | B1 |
6987819 | Thomas et al. | Jan 2006 | B2 |
6993293 | Bevan et al. | Jan 2006 | B1 |
6993299 | Sugar et al. | Jan 2006 | B2 |
6996195 | Kadous | Feb 2006 | B2 |
6996197 | Thomas et al. | Feb 2006 | B2 |
6999724 | Chizhik et al. | Feb 2006 | B2 |
7002900 | Walton et al. | Feb 2006 | B2 |
7006041 | Fujii et al. | Feb 2006 | B2 |
7006579 | Kuchi et al. | Feb 2006 | B2 |
7006804 | Clark et al. | Feb 2006 | B1 |
7006810 | Winters et al. | Feb 2006 | B1 |
7006848 | Ling et al. | Feb 2006 | B2 |
7010053 | El-Gamal et al. | Mar 2006 | B2 |
7010054 | El-Gamal et al. | Mar 2006 | B2 |
7012978 | Talwar | Mar 2006 | B2 |
7020072 | Li et al. | Mar 2006 | B1 |
7020110 | Walton et al. | Mar 2006 | B2 |
7020446 | Mehta et al. | Mar 2006 | B2 |
7027523 | Jalali et al. | Apr 2006 | B2 |
7027533 | Abe et al. | Apr 2006 | B2 |
7031371 | Lakkis | Apr 2006 | B1 |
7031419 | Piirainen | Apr 2006 | B2 |
7031669 | Vaidyanathan et al. | Apr 2006 | B2 |
7031753 | Hashem et al. | Apr 2006 | B2 |
7035201 | Fu et al. | Apr 2006 | B2 |
7035672 | Nakaya et al. | Apr 2006 | B2 |
7039370 | Laroia et al. | May 2006 | B2 |
7042857 | Krishnan et al. | May 2006 | B2 |
7042858 | Ma et al. | May 2006 | B1 |
7042956 | El-Gamal et al. | May 2006 | B2 |
7046651 | Terry | May 2006 | B2 |
7047016 | Walton et al. | May 2006 | B2 |
7050510 | Foschini et al. | May 2006 | B2 |
7054378 | Walton et al. | May 2006 | B2 |
7058146 | Paulraj et al. | Jun 2006 | B2 |
7058367 | Luo et al. | Jun 2006 | B1 |
7061854 | Tarokh et al. | Jun 2006 | B2 |
7065144 | Walton et al. | Jun 2006 | B2 |
7068628 | Li et al. | Jun 2006 | B2 |
7068705 | Schilling | Jun 2006 | B2 |
7072413 | Walton et al. | Jul 2006 | B2 |
7072693 | Farlow et al. | Jul 2006 | B2 |
7076263 | Medvedev et al. | Jul 2006 | B2 |
7079870 | Vaidyanathan | Jul 2006 | B2 |
7082159 | Larsson | Jul 2006 | B2 |
7088782 | Mody et al. | Aug 2006 | B2 |
7092436 | Ma et al. | Aug 2006 | B2 |
7092450 | Al-Dhahir | Aug 2006 | B1 |
7095709 | Walton et al. | Aug 2006 | B2 |
7095790 | Krishnan et al. | Aug 2006 | B2 |
7095812 | Chan et al. | Aug 2006 | B2 |
7099413 | Chuang et al. | Aug 2006 | B2 |
7099678 | Vaidyanathan | Aug 2006 | B2 |
7099698 | Tarokh et al. | Aug 2006 | B2 |
7103325 | Jia et al. | Sep 2006 | B1 |
7106802 | Heiskala et al. | Sep 2006 | B1 |
7106816 | Filipovic | Sep 2006 | B2 |
7110350 | Li et al. | Sep 2006 | B2 |
7110464 | El-Gamal et al. | Sep 2006 | B2 |
7113808 | Hwang et al. | Sep 2006 | B2 |
7116722 | Foschini et al. | Oct 2006 | B2 |
7116725 | Ketchum et al. | Oct 2006 | B2 |
7120199 | Thielecke et al. | Oct 2006 | B2 |
7120201 | Huang et al. | Oct 2006 | B2 |
7120395 | Tong et al. | Oct 2006 | B2 |
7123669 | Ye et al. | Oct 2006 | B2 |
7126996 | Classon et al. | Oct 2006 | B2 |
7130353 | Brunel | Oct 2006 | B2 |
7130355 | Al-Dhahir et al. | Oct 2006 | B1 |
7133459 | Onggosanusi et al. | Nov 2006 | B2 |
7133461 | Thomas et al. | Nov 2006 | B2 |
7133646 | Miao | Nov 2006 | B1 |
7136410 | Choi et al. | Nov 2006 | B2 |
7136437 | Benesty et al. | Nov 2006 | B2 |
7139321 | Giannakis et al. | Nov 2006 | B2 |
7139328 | Thomas et al. | Nov 2006 | B2 |
7139527 | Tamaki et al. | Nov 2006 | B2 |
7139964 | Shen et al. | Nov 2006 | B2 |
7142864 | Laroia et al. | Nov 2006 | B2 |
7145971 | Raleigh et al. | Dec 2006 | B2 |
7148845 | Rooyen et al. | Dec 2006 | B2 |
7149254 | Sampath | Dec 2006 | B2 |
7154960 | Liu et al. | Dec 2006 | B2 |
7155171 | Ebert et al. | Dec 2006 | B2 |
7167684 | Kadous et al. | Jan 2007 | B2 |
7173973 | Borran et al. | Feb 2007 | B2 |
7177365 | El-Gamal et al. | Feb 2007 | B2 |
7184713 | Kadous et al. | Feb 2007 | B2 |
7190734 | Giannakis et al. | Mar 2007 | B2 |
7194042 | Walton et al. | Mar 2007 | B2 |
7194237 | Sugar et al. | Mar 2007 | B2 |
7197282 | Dent et al. | Mar 2007 | B2 |
7203249 | Raleigh et al. | Apr 2007 | B2 |
7203490 | Karabinis et al. | Apr 2007 | B2 |
7209522 | Shirali | Apr 2007 | B1 |
7212579 | Claussen et al. | May 2007 | B2 |
7215704 | Fujii et al. | May 2007 | B2 |
7218683 | Ko et al. | May 2007 | B2 |
7230991 | Sang et al. | Jun 2007 | B2 |
7233634 | Hassell Sweatman et al. | Jun 2007 | B1 |
7236536 | Hochwald et al. | Jun 2007 | B2 |
7236539 | Deng et al. | Jun 2007 | B2 |
7236750 | Vaidyanathan et al. | Jun 2007 | B2 |
7242720 | Sugiyama et al. | Jul 2007 | B2 |
7242727 | Liu et al. | Jul 2007 | B2 |
7245679 | Aoki et al. | Jul 2007 | B2 |
7245881 | Sugar et al. | Jul 2007 | B2 |
7248638 | Banister | Jul 2007 | B1 |
7248647 | Claussen et al. | Jul 2007 | B2 |
7248841 | Agee et al. | Jul 2007 | B2 |
7251460 | Khatri | Jul 2007 | B2 |
7251469 | Sudo | Jul 2007 | B2 |
7257170 | Love et al. | Aug 2007 | B2 |
7257424 | Hamalainen et al. | Aug 2007 | B2 |
7260153 | Nissani | Aug 2007 | B2 |
7269127 | Mody et al. | Sep 2007 | B2 |
7269224 | Stuber et al. | Sep 2007 | B2 |
7280604 | Giannakis et al. | Oct 2007 | B2 |
7283798 | Winters et al. | Oct 2007 | B1 |
7286961 | Kildal | Oct 2007 | B2 |
7289068 | Fujio et al. | Oct 2007 | B2 |
7292644 | Whang et al. | Nov 2007 | B2 |
7296045 | Sehitoglu | Nov 2007 | B2 |
7302009 | Walton et al. | Nov 2007 | B2 |
7305054 | Talwar | Dec 2007 | B2 |
7308287 | Vaidyanathan | Dec 2007 | B2 |
7313194 | Bar-Ness et al. | Dec 2007 | B2 |
7315570 | El-Gamal et al. | Jan 2008 | B2 |
7317750 | Shattil | Jan 2008 | B2 |
7317770 | Wang | Jan 2008 | B2 |
7317771 | Brunel | Jan 2008 | B2 |
7319714 | Sakata et al. | Jan 2008 | B2 |
7321564 | Ikram et al. | Jan 2008 | B2 |
7324193 | Lally et al. | Jan 2008 | B2 |
7324583 | Hooli et al. | Jan 2008 | B2 |
7324792 | Sim et al. | Jan 2008 | B2 |
7324794 | Chari et al. | Jan 2008 | B2 |
7327795 | Oprea | Feb 2008 | B2 |
7327798 | Won | Feb 2008 | B2 |
7327800 | Oprea et al. | Feb 2008 | B2 |
7327811 | Molnar | Feb 2008 | B2 |
7327812 | Auer | Feb 2008 | B2 |
7327983 | Mehta et al. | Feb 2008 | B2 |
7328033 | Rappaport et al. | Feb 2008 | B2 |
7330513 | Tsai et al. | Feb 2008 | B2 |
7330697 | Bolt et al. | Feb 2008 | B1 |
7330698 | Bolt et al. | Feb 2008 | B1 |
7333455 | Bolt et al. | Feb 2008 | B1 |
7333540 | Yee | Feb 2008 | B2 |
7333549 | Lee et al. | Feb 2008 | B2 |
7333551 | Hwang et al. | Feb 2008 | B2 |
7333560 | Jalali et al. | Feb 2008 | B2 |
7336719 | Gore et al. | Feb 2008 | B2 |
7336727 | Mukkavilli et al. | Feb 2008 | B2 |
7339980 | Grant et al. | Mar 2008 | B2 |
7340018 | Tynderfeldt | Mar 2008 | B2 |
7340671 | Jones et al. | Mar 2008 | B2 |
7342875 | Hammons, Jr. et al. | Mar 2008 | B2 |
7342970 | Liu | Mar 2008 | B2 |
7346040 | Weinstein | Mar 2008 | B2 |
7346104 | Yu et al. | Mar 2008 | B2 |
7346114 | Iancu et al. | Mar 2008 | B2 |
7356089 | Jia et al. | Apr 2008 | B2 |
7359311 | Paranjpe et al. | Apr 2008 | B1 |
7359313 | Chan et al. | Apr 2008 | B2 |
7366222 | Song et al. | Apr 2008 | B2 |
7366248 | Wang et al. | Apr 2008 | B2 |
7366520 | Haustein et al. | Apr 2008 | B2 |
7372830 | Jung et al. | May 2008 | B2 |
7376173 | Yedidia et al. | May 2008 | B2 |
7382840 | Molisch et al. | Jun 2008 | B2 |
7391815 | Lakkis | Jun 2008 | B2 |
Number | Date | Country |
---|---|---|
9809381 | Mar 1998 | WO |
Entry |
---|
Foschini, Luigi. “Is Science going through a critical stage?.” arXiv preprint physics/9807009 (1998). |
Foschini, Luigi. Undecidability in quantum mechanics. No. quant-ph/9804040. 1998. |
Jöngren, George, and Björn Ottersten. “Combining Transmit Antenna Weights with Orthogonal Space-Time Block Coding.” Proceedings Nordiskt radioseminarium 1999. 1999. |
Kaleka, Jaspreet Singh. Weighted multilevel space-time trellis codes for rayleigh fading channels. Diss. Thapar University, 1956. |
Thielecke, Jörn, and Udo Wachsmann. “Capacity Assessment of MIMO Transmission Techniques.” (2002). |
Driessen, Peter F. “Future Mobile Telecommunications Systems.” (1997). |
Z Zhang, SW Cheung, Ti Yuk, “Exact evaluation of block-error rate using correct . . . ” Trans. Inform. Theory, 1998—hub.hku.hk. |
Ning Zhang, Ada Poon, David Tse and Robert Brodersen, “Trade-offs of Performance and Single Chip Implementation of Indoor Wireless Multi-Access Receivers” 0-7803-5668-3/99 1999 IEEE. |
Giuseppe Caire, et al., “Optimum Power Control Over Fading Channels”, IEEE Transactions on Information Theory, vol. 45, No. 5, Jul. 1999, 1468-1489. |
Sergey Loyka, “The Influence of Electromagnetic Environment on Operation of Active Array Antennas: Analysis and Simulation Techniques”, IEEE Antennas and Propagation magazine, 41(6) (Dec. 1999) 23-39. |
Wu, YC; Serpedin, E, “Non-data-aided ML symbol timing estimation in MIMO correlated fading channels”, The 62nd IEEE VTS Vehicular Technology Conference Proceedings, Dallas, Texas, USA, Sep. 25-28, 2005, v. 4, p. 2091-2095. |
Aradhana Narula, Mitchell D. Trott, and Gregory W. Wornell, “Performance Limits of Coded Diversity Methods for Transmitter Antenna Arrays”, IEEE Transactions on Information Theory, vol. 45, No. 7, Nov. 1999, 2418-2433. |
Francois Horlin Eduardo Lopez-Estraviz Liesbet Van der Perre, “Space-Time Block Coding for Uplink Single-Carrier CDMA with Joint Detection in the Frequency Domain”, IEEE Trans. Wireless Comm., Jun. 2007, 2096-2105. |
Frederik Petre, Geert Leus, Marc Moonen, “Multi-Carrier Block-Spread CDMA for Broadband Cellular Downlink”, Eurasip Journal on Applied Signal Processing (Submitted) Feb. 28, 2003. |
F. Petre, Geert Leus, Luc Deneire, M.G.E. Engels, M. Moonen, et al.. Space-time block coding for single-carrier block transmission DS-CDMA downlink. IEEE Journal on Selected Areas in Communications, Institute of Electrical and Electronics Engineers (IEEE), 2003, 21 (3), pp. 350-361. <10.1109/JSAC.2003.809630>. <hal-00187763>. |
Nadine Chapalain, David Mottier, Damien Castelain, “An OFCDM Uplink Transmission System with Channel Estimation Based on Spread Pilots”—ISTMCS04 (2004). |
Georgios B. Giannakis, Paul A. Anghel, Zhengdao Wang, “Wideband Generalized Multi-Carrier CDMA Over Frequency-Selective Wireless Channels”, ICASSP00 (2000). |
Georgios B. Giannakis, Anastasios Stamoulis, Zhengdao Wang, Paul A. Anghel, “Load-Adaptive MUI/ISI-Resilient Generalized Multi-Carrier CDMA with Linear and DF Receivers”, May 17, 2000. |
Sergey L. Loyka, Juan R. Mosig, “Nonlinear Modeling and Simulation of Active Array Antennas”, 5th COST 260 MC & WG Meeting, Wroclaw, Poland, Jun. 30-Jul. 2, 1999. |
Bjovn Ottersten, A. Lee Swindlehurst, “Antenna Arrays for Wireless Networks”, IEEE Signal Processing Magazine Mar. 1999. |
Li et al.: Spatial—Temporal Equalization for IS-136 TDMA Systems, IEEE Transactions on Vehicular Technology, vol. 48, No. 4, Jul. 1999. |
Richard Todd Causey, “Blind Multiuser Detection Based on Second-Order Statistics”, PhD Thesis, Georgia Institute of Technology, Jul. 30, 1999. |
Gregory J. Pottie, Wireless Multiple Access Adaptive Communications Techniques, CRC Press—1999—500 pages. |
Foschini, Gerard J. “Layered space-time architecture for wireless communication in a fading environment when using multi-element antennas.” Bell labs technical journal 1.2 (1996): 41-59. |
Sylla, Lamine, Paul Fortier, and Huu Tuê Huynh. “Performance of COFDM using turbo codes.” Proc. of IEEE Canadian Conference on Electrical and Computer Engineering, Edmonton, Alta, Canada. 1999. |
Vikalo, Haris, and Babak Hassibi. “Maximum-likelihood sequence detection of multiple antenna systems over dispersive channels via sphere decoding.” EURASIP Journal on Advances in Signal Processing 2002.5 (1900): 525-531. |
Fricke, Justus Ch, et al. “Impact of the Gaussian approximation on the performance of the probabilistic data association MIMO decoder.” EURASIP Journal on Wireless Communications and Networking 2005.5 (1900): 796-800. |
Caire, Giuseppe, Giorgio Taricco, and Ezio Biglieri. “Optimum power control over fading channels.” Information Theory, IEEE Transactions on 45.5 (1999): 1468-1489. |
Chen, Jiunn-Tsair, Constantinos Papadias, and Gerard J. Foschini. “Space-time dynamic signature assignment for the reverse link of DS-CDMA systems.” Communications, IEEE Transactions on 52.1 (2004): 120-129. |
Liu, Zhiqiang, Yan Xin, and Georgios B. Giannakis. “Space-time-frequency coded OFDM over frequency-selective fading channels.” Signal Processing, IEEE Transactions on 50.10 (2002): 2465-2476. |
Ma, Xiaoli, and Georgios B. Giannakis. “Space-time coding for doubly selective channels.” Circuits and Systems, 2002. ISCAS 2002. IEEE International Symposium on. vol. 3. IEEE, 2002. |
Liu, Zhiqiang, Xiaoli Ma, and Georgios B. Giannakis. “Space-time coding and Kalman filtering for time-selective fading channels.” Communications, IEEE Transactions on 50.2 (2002): 183-186. |
Petré, Frederik, et al. “Space-time block coding for single-carrier block transmission DS-CDMA downlink.” Selected Areas in Communications, IEEE Journal on 21.3 (2003): 350-361. |
Narula, Aradhana, Mitchell D. Trott, and Gregory W. Wornell. “Performance limits of coded diversity methods for transmitter antenna arrays.” Information Theory, IEEE Transactions on 45.7 (1999): 2418-2433. |
Horlin, Francois, Eduardo Lopez-Estraviz, and Liesbet Van der Perre. “Space-time block coding for uplink single-carrier CDMA with joint detection in the frequency domain.” Wireless Communications, IEEE Transactions on 6.6 (2007): 2096-2105. |
Zheng, Haitao, Angel Lozano, and Mohamed Haleem. “Multiple ARQ processes for MIMO systems.” Personal, Indoor and Mobile Radio Communications, 2002. The 13th IEEE International Symposium on. vol. 3. IEEE, 2002. |
Knessl, Charles. “A diffusion model for two parallel queues with processor sharing: transient behavior and asymptotics.” International Journal of Stochastic Analysis 12.4 (1999): 311-338. |
OFDM and MIMO-OFDM System. Penerbit Universiti Teknologi Malaysia, 2008. |
Biglieri, Ezio, John Proakis, and Shlomo Shamai. “Fading channels: Information-theoretic and communications aspects.” Information Theory, IEEE Transactions on 44.6 (1998): 2619-2692. |
Peppas, Kostas, et al. “Performance evaluation at the system level of reconfigurable space-time coding techniques for HSDPA.” EURASIP Journal on Advances in Signal Processing 2005.11 (1900): 1656-1667. |
Tarokh, Vahid, Nambi Seshadri, and A. Robert Calderbank. “Space-time codes for high data rate wireless communication: Performance criterion and code construction.” Information Theory, IEEE Transactions on 44.2 (1998): 744-765. |
Wolniansky, Peter W., et al. “V-BLAST: An architecture for realizing very high data rates over the rich-scattering wireless channel.” Signals, Systems, and Electronics, 1998. ISSSE 98. 1998 URSI International Symposium on. IEEE, 1998. |
Tarokh, Vahid, Hamid Jafarkhani, and A. Robert Calderbank. “Space-time block coding for wireless communications: performance results.” Selected Areas in Communications, IEEE Journal on 17.3 (1999): 451-460. |
Golden, G. D., et al. “Detection algorithm and initial laboratory results using V-BLAST space-time communication architecture.” Electronics letters 35.1 (1999): 14-16. |
Foschini, Gerard J., et al. “Simplified processing for high spectral efficiency wireless communication employing multi-element arrays.” Selected Areas in Communications, IEEE Journal on 17.11 (1999): 1841-1852. |
Negi, Rohit, Ardavan Maleki Tehrani, and John Cioffi. “Adaptive antennas for space-time coding over block-time invariant multipath fading channels.” Vehicular Technology Conference, 1999 IEEE 49th. vol. 1. IEEE, 1999. |
Diggavi, Suhas N. “Analysis of multicarrier transmission in time-varying channels.” Communications, 1997. ICC'97 Montreal, Towards the Knowledge Millennium. 1997 IEEE International Conference on. vol. 3. IEEE, 1997. |
Tehrani, Ardavan Maleki, et al. “An implementation of discrete multi-tone over slowly time-varying multiple-input/multiple-output channels.” Global Telecommunications Conference, 1998. GLOBECOM 1998. The Bridge to Global Integration. IEEE. vol. 5. IEEE, 1998. |
A. R. Calderbank, “The Art of Signaling: Fifty Years of Coding Theory”, IEEE Transactions on Information Theory, vol. 44, No. 6, Oct. 1998. |
Tehrani, Ardavan Maleki, Rohit Negi, and John Cioffi. “Space-time coding over a code division multiple access system.” Wireless Communications and Networking Conference, 1999. WCNC. 1999 IEEE. IEEE, 1999. |
Jongren, George, and Björn Ottersten. “Combining transmit antenna weights and orthogonal space-time block codes by utilizing side information.” Signals, Systems, and Computers, 1999. Conference Record of the Thirty-Third Asilomar Conference on. vol. 2. IEEE, 1999. |
Knopp, Raymond, and Giuseppe Caire. “Power control schemes for TDD systems with multiple transmit and receive antennas.” Global Telecommunications Conference, 1999. GLOBECOM'99. vol. 5. IEEE, 1999. |
Wong, Kai-Kit, K. Ben Letaief, and Ross David Murch. “Investigating the performance of smart antenna systems at the mobile and base stations in the down and uplinks.” Vehicular Technology Conference, 1998. VTC 98. 48th IEEE. vol. 2. IEEE, 1998. |
Caire, Giuseppe, P. D. Torino, and E. Biglieri. “Capacity of multi-antenna block-fading channels.” Communication Theory Mini-Conference, 1999. IEEE, 1999. |
Khaled, Nadia, et al. “Spatial-mode selection for the joint transmit and receive MMSE design.” EURASIP Journal on Advances in Signal Processing 2004.9 (1900): 1199-1211. |
Dasgupta, Soura, Chris Schwarz, and Brian DO Anderson. “Optimum subband coding of cyclostationary signals.” Acoustics, Speech, and Signal Processing, 1999. Proceedings., 1999 IEEE International Conference on. vol. 3. IEEE, 1999. |
Blum, Rick S. “Maximum MIMO system mutual information with antenna selection and interference.” EURASIP Journal on Advances in Signal Processing 2004.5 (1900): 676-684. |
Hottinen, Ari, Risto Wichman, and Dinesh Rajan. “Soft weighted STTD for W-CDMA.” Allerton Conference on Communication, Control and Computing. 1999. |
Diggavi, Suhas N. Communication in the presence of uncertain interference and channel fading. Diss. stanford university, 1998. |
Shiu, Da-Shan, et al. “Fading correlation and its effect on the capacity of multielement antenna systems.” Communications, IEEE Transactions on 48.3 (2000): 502-513. |
Hughes, Brian L. “Differential space-time modulation.” Information Theory, IEEE Transactions on 46.7 (2000): 2567-2578. |
Raleigh, G. C., and John M. Cioffi. “Spatio-temporal coding for wireless communication.” Communications, IEEE Transactions on 46.3 (1998): 357-366. |
Johansson, Sven, et al. “Evaluation of a Multiple—versus a Single—Reference MIMO ANC Algorithm on Dornier 328 Test Data Set.” ISMA 23, 1998 International Conference on Noise and Vibration Engineering. Katholieke Universiteit Leuven, Division of Production Engineering, Machine Design & Automation, 1998. |
Tarokh, Vahid, Hamid Jafarkhani, and A. Robert Calderbank. “Space-time block codes from orthogonal designs.” Information Theory, IEEE Transactions on 45.5 (1999): 1456-1467. |
Marzetta, Thomas L. “BLAST training: Estimating channel characteristics for high capacity space-time wireless.” Proceedings of the Annual Allerton Conference on Communication Control and Computing. vol. 37. The University; 1998, 1999. |
Chit Lo, Todd K. Mason, Optimal Detection and Signaling in fast Fading Channels, Utah State University, Mar. 16, 2002. |
Driessen, Peter F., and Gerard J. Foschini. “On the capacity formula for multiple input-multiple output wireless channels: A geometric interpretation.” IEEE Transactions on Communications 47.2 (1999): 173-176. |
Shiu, Da-Shan, and Joseph M. Kahn. “Layered space-time codes for wireless communications using multiple transmit antennas.” Communications, 1999. ICC'99. 1999 IEEE International Conference on. vol. 1. IEEE, 1999. |
Naguib, Ayman F., et al. “A space-time coding modem for high-data-rate wireless communications.” Selected Areas in Communications, IEEE Journal on 16.8 (1998): 1459-1478. |
Shiu, Da-shan, and Joseph M. Kahn. “Scalable layered space-time codes for wireless communications: performance analysis and design criteria.” Wireless Communications and Networking Conference, 1999. WCNC. 1999 IEEE. IEEE, 1999. |
Liu, Youjian, and Michael P. Fitz. “Space-time turbo codes.” Proceedings of the Annual Allerton Conference on Communication Control and Computing. vol. 37. The University; 1999. |
Negi, Rohit, Ardavan Maleki Tehrani, and John Cioffi. “Adaptive antennas for space-time coding over block-time invariant multipath fading channels.” Vehicular Technology Conference, 1999 IEEE 49th. vol. 1, IEEE, 1999. |
Tehrani, Ardavan Maleki, Rohit Negi, and John Cioffi. “Space-time coding and transmission optimization for wireless channels.” Signals, Systems Computers, 1998. Conference Record of the Thirty-Second Asilomar Conference on. vol. 2. IEEE, 1998. |
Hochwald, Bertrand M., and Thomas L. Marzetta. “Space-time modulation for unknown fading.” AeroSense'99. International Society for and and Photonics, 1999. |
Safar, Zoltan, and K. J. Liu. “Systematic design of space-time trellis codes for diversity and coding advantages.” EURASIP Journal on Advances in Signal Processing 2002.3 (1900): 221-235. |
Grant, Alex. “Rayleigh fading multi-antenna channels.” EURASIP Journal on Advances in Signal Processing 2002.3 (1900): 316-329. |
Chen, Jiunn-Tsair, Constantinos B. Papadias, and Gerard J. Foschini. “Dynamic signature assignment for reverse-link CDMA systems.” Communications, 1999. ICC'99. 1999 IEEE International Conference on. vol. 2. IEEE, 1999. |
Sampath, H., and A. Paulraj. “Space-time processing TDMA wireless testbed.” Acoustics, Speech, and Signal Processing, 1999. Proceedings., 1999 IEEE International Conference on. vol. 4. IEEE, 1999. |
Marzetta, Thomas L., and Bertrand M. Hochwald. “Capacity of a mobile multiple-antenna communication link in Rayleigh flat fading.” Information Theory, IEEE Transactions on 45.1 (1999): 139-157. |
Tehrani, Ardavan Maleki, et al. “An implementation of discrete multi-tone over slowly time-varying multiple-input/ multiple-output channels.” Global Telecommunications Conference, 1998. GLOBECOM 1998. The Bridge to Global Integration. IEEE. vol. 5. IEEE, 1998. |
Ponnekanti, Seshaiah. “An overview of smart antenna technology for heterogeneous networks.” IEEE Communication Surveys 2.4 (1999): 14-23. |
Foschini, Luigi. “On the logic of quantum physics and the concept of the time.” arXiv preprint quant-ph/9804040 (1998). |
Narula, Aradhana, et al. “Efficient use of side information in multiple-antenna data transmission over fading channels.” Selected Areas in Communications, IEEE Journal on 16.8 (1998): 1423-1436. |
Abou-Faycal, Ibrahim, and Bertrand M. Hochwald. “Coding requirements for multiple-antenna channels with unknown Rayleigh fading.” Bell Labs., Lucent Technol., Murray Hill, NJ, Tech. Rep 10 (1999). |
Winters, Jack H. “Smart antennas for wireless systems.” Personal Communications, IEEE 5.1 (1998): 23-27. |
Number | Date | Country | |
---|---|---|---|
60128233 | Apr 1999 | US |
Number | Date | Country | |
---|---|---|---|
Parent | 13471648 | May 2012 | US |
Child | 14541698 | US | |
Parent | 13093447 | Apr 2011 | US |
Child | 13471648 | US | |
Parent | 09545407 | Apr 2000 | US |
Child | 13093447 | US |