Category: Antennas

  • AFIT, Locata Partner on GPS Technology Development

    AFIT, Locata Partner on GPS Technology Development

    Locata's new VRay Orb 80 switching antenna.
    Locata’s new VRay Orb 80 switching antenna.

    The Air Force Institute of Technology (AFIT) and Locata Corporation have signed a Co-operative Research & Development Agreement (CRADA) to build and demonstrate new Locata multipath mitigation technology for use in GPS receivers. This cooperation is expected to leverage many years of proprietary Locata ground-based technology development to bring completely new capabilities to satellite-based GPS receivers, AFIT said.

    The Air Force Institute of Technology, or AFIT, is the Air Force’s graduate school of engineering and management as well as its institution for technical professional continuing education.

    The CRADA is specifically directed to evaluate Locata’s patented correlator and switching antenna technologies for use in positioning receivers running at GPS frequencies. Locata’s engineers will transfer knowledge and experience they have gained with existing Locata commercial systems to help AFIT design and build an initial multi-element GPS-based switching antenna prototype which is based on Locata’s patents. This will ensure AFIT researchers and engineers can familiarize themselves with the new antenna’s characteristics, and provide AFIT with an essential platform to develop GPS-specific versions of Locata’s correlator and switching algorithms. When built, AFIT intends to use its GPS receiver and the prototype switching antenna to physically demonstrate the feasibility of using Locata technology to improve GPS receiver performance.

    An animation was created specifically to explain RF problems created by multipath and Locata’s VRay solution. The animation shows the first proof-of-concept 2D, 64-element antenna Locata’s engineers prototyped in 2011.

    After initial prototypes are built, AFIT plans to design and test several other GPS-based versions of Locata’s switching antenna array to assess how Locata’s commercial antennas can be adapted to use cases which are of particular interest to the military. Designs already discussed with Locata include stand-alone antennas, arrays conformal to a vehicle’s frame (such as a Humvee’s roof or aircraft fuselage), and a version built into helmets.

    As a first step in implementing this CRADA collaboration, AFIT personnel visited Locata’s head office the week of April 29 for a detailed, wide-ranging introduction to the design fundamentals for this new type of antenna. Locata hosted AFIT’s John Raquet, Peter Collins and Jason Barhorst (see picture) in multiple engineering meetings where Locata’s current production version antenna was revealed for the first time, and then closely analyzed. AFIT and Locata engineers then workshopped the modification and design choices required to integrate Locata design into a GPS form-factor.

    “If this CRADA is successful, Locata’s technology could enable a significantly improved technical performance and reduction in the cost of multiple-element GPS antennas,” said John Raquet, director, Advanced Navigation Technology Center, AFIT. “This will enable much wider adoption of the technology, resulting in more reliable GPS positioning for more users. We are excited to investigate this technology advance for the benefits it will potentially bring to American warfighters.”

    “We are incredibly proud to once again be involved in a CRADA with the Air Force Institute of Technology, developing on the cutting-edge of navigation technology,” said Nunzio Gambale, CEO and co-founder, Locata Corporation. “Our previous LocataNet partnership with Dr. Raquet and his world-class AFIT researchers quickly taught us why this team is renown throughout the industry. The AFIT engineers bring an exceptional skill base to this important integration of Locata technology into GPS receivers. I’m certain that our collaboration, along with access to the USAF’s unmatched prototyping and testing capabilities, will deliver ground-breaking functionality for future GPS devices.”

    AFIT expects at least one master’s degree to be awarded for the research tasks involved in the CRADA. Work against the approved CRADA project plan will commence immediately, and involve several other participants providing admin and lab support to AFIT and Locata. The final report produced by this CRADA will include results and measured performance of the Locata-enhanced GPS receiver and other design considerations gleaned from AFIT’s experience with the new Locata antenna and correlators.

     AFIT-Locata Kick-off Meeting. This is the first picture ever released by Locata which shows their radically new switching antenna, a design that AFIT will now modify for use with GPS receivers. Pictured (L-R): Dr. Steve Hewitson & Ian Sainsbery (Locata engineers); Jason Barhorst (AFIT); David Small (Locata technology inventor), Nunzio Gambale (Locata CEO), Dr. John Raquet (Director, Advanced Navigation Technology Center, AFIT), Dr. Peter Collins (AFIT), Dr. Trevor Hobbs (Locata Director of R&D).
    AFIT-Locata Kick-off Meeting: This is the first picture ever released by Locata which shows their radically new switching antenna, a design that AFIT will now modify for use with GPS receivers. Pictured (L-R): Dr. Steve Hewitson & Ian Sainsbery (Locata engineers); Jason Barhorst (AFIT); David Small (Locata technology inventor), Nunzio Gambale (Locata CEO), Dr. John Raquet (Director, Advanced Navigation Technology Center, AFIT), Dr. Peter Collins (AFIT), Dr. Trevor Hobbs (Locata Director of R&D).
  • Panasonic Offers Durable Antennas for Wireless

    Panasonic Offers Durable Antennas for Wireless

    The VIC100 Series antenna by Panasonic

    The VIC100 Series antenna by Panasonic is an active L1 GPS antenna designed for timing and synchronization. It offers immunity to noise and interference, and secure performance by attenuating noise and interference near the GPS L1 frequency through triple-filtering design.

    The VIC100 Series is housed in a waterproof enclosure designed for excellent performance under severe environmental conditions. Its shape prevents accumulation of snow and ice, eliminating problems with bird perching and enhanced immunity to lightning surge.

  • Tallysman Introduces Dual-Frequency Antenna Series

    Tallysman Introduces Dual-Frequency Antenna Series

    TW3802 Shown with flat radome.  Conical radome also available.
    TW3802 Shown with flat radome. Conical radome also available.

    Tallysman Wireless Inc. has added the dual-frequency TW3800 series to its high-quality precision line of antenna products.

    The TW3800 series antennas feature a circular stacked patch antenna for improved axial ratio, yet are small and light, and have the extended bandwidth required for L1/L2 GPS & G1/G2 GLONASS, the company said. The operating voltage range is from +2.5 to 16 VDC. The antennas have a temperature compensated LNAs and operate from -40 to +85o C to provide reliable performance in most any environment. The TW3800 is packaged in a through hole mount making it suitable for mobile applications.

    The TW380x is suited for many applications, including:

    • Anti-jamming GPS
    • Mission-critical GPS timing
    • Military and security
    • Network timing and synchronization
    • Precise tracking
    • High signal availability

    The TW3805 is the OEM version of the TW3802, and can be custom tuned to provide optimal performance inside virtually any housing, Tallysman said.

    “The circular patch design of the TW380X antennas permits precision custom tuning with excellent axial ratios.”  said Gyles Panther, president of Tallysman Wireless. “This flexibility, combined with the very wide operating voltage enables this antenna to work with virtually any receiver on the market.”

    The Tallysman TW3805HR antenna.
    The Tallysman TW3805HR antenna.

     

  • Lockheed Martin Delivers Antenna Assemblies for First GPS III Satellite

    Lockheed Martin has completed and is preparing to install the navigation, communication, and hosted payload antenna assemblies for the first satellite of the next-generation GPS III.

    Seven antenna assemblies, produced at Lockheed Martin’s Newtown, Pennsylania, facility were delivered to the company’s GPS III Processing Facility (GPF) near Denver, Colorado, on June 14.  The antennas will be installed on the first GPS III space vehicle (SV01), which Lockheed Martin will deliver to the U.S. Air Force on schedule, “flight-ready,” in 2014.

    The new antennas for GPS III SV01 will provide the satellite’s capability to send and/or receive data for Earth-coverage and military Earth-coverage navigation; a UHF crosslink for inter-satellite data transfer; telemetry, tracking and control for satellite-ground communications; and data acquisition and communication for the nuclear detection system hosted payload. The antenna designs enable three to eight times greater anti-jamming signal power to be broadcast to military users across the globe when compared to previous GPS generations.

    “These antennas on the next generation of GPS III satellites will transmit data utilized by more than one billion users with navigation, positioning and timing needs,” explained Keoki Jackson, vice president of Lockheed Martin’s Navigation Systems mission area. “We have become reliant on GPS for providing signals that affect everything from cell phones and wristwatches, to shipping containers and commercial air traffic, to ATMs and financial transactions worldwide.”

    GPS III is a critically important program for the Air Force, affordably replacing aging GPS satellites in orbit, while improving capability to meet the evolving demands of military, commercial and civilian users. GPS III satellites will deliver three times better accuracy, include enhancements which extend spacecraft life 25 percent further than the prior GPS block, and a new civil signal designed to be interoperable with international global navigation satellite systems.

    The production of the first GPS III satellite continues on schedule. Recent testing of the SV 01 bus — the portion of the space vehicle that carries mission payloads and hosts them in orbit — assured that all bus subsystems are functioning normally and that they are ready for final integration with the satellite’s navigation payload.
    This milestone follows February’s successful initial power on of the SV01 spacecraft bus, which demonstrated  the electrical-mechanical integration, validated the satellite’s interfaces and led the way for functional electrical hardware-software integration testing.

    Lockheed Martin is under contract for production of the first four GPS III satellites (SV01-04), and has received advanced procurement funding for long-lead components for the fifth, sixth, seventh and eighth satellites (SV05-08).

    The GPS III team is led by the Global Positioning Systems Directorate at the U.S. Air Force Space and Missile Systems Center. Lockheed Martin is the GPS III prime contractor with teammates ITT Exelis, General Dynamics, Infinity Systems Engineering, Honeywell, ATK and other subcontractors. Air Force Space Command’s 2nd Space Operations Squadron (2SOPS), based at Schriever Air Force Base, Colorado, manages and operates the GPS constellation for both civil and military users.

  • Innovation: GNSS Spoofing Detection

    Innovation: GNSS Spoofing Detection

    Correlating Carrier Phase with Rapid Antenna Motion

    By Mark L. Psiaki with Steven P. Powell and Brady W. O’Hanlon

    GPS World photo
    INNOVATION INSIGHTS by Richard Langley

    IT’S A HOSTILE (ELECTRONIC) WORLD OUT THERE, PEOPLE. Our wired and radio-based communication systems are constantly under attack from evil doers. We are all familiar with computer viruses and worms hiding in malicious software or malware distributed over the Internet or by infected USB flash drives. Trojan horses are particularly insidious. These are programs concealing harmful code that can lead to many undesirable effects such as deleting a user’s files or installing additional harmful software. Such programs pass themselves off as benign, just like the “gift” the Greeks delivered to the Trojans as reported in Virgil’s Aeneid. This was a very early example of spoofing. Spoofing of Internet Protocol (IP) datagrams is particularly prevalent. They contain forged source IP addresses with the purpose of concealing the identity of the sender or impersonating another computing system.

    To spoof someone or something is to deceive or hoax, passing off a deliberately fabricated falsehood made to masquerade as truth. The word “spoof” was introduced by the English stage comedian Arthur Roberts in the late 19th century. He invented a game of that name, which involved trickery and nonsense. Now, the most common use of the word is as a synonym for parody or satirize — rather benign actions. But it is the malicious use of spoofing that concerns users of electronic communications.

    And it is not just wired communications that are susceptible to spoofing. Communications and other services using radio waves are, in principle, also spoofable. One of the first uses of radio-signal spoofing was in World War I when British naval shore stations sent transmissions using German ship call signs. In World War II, spoofing became an established military tactic and was extended to radar and navigation signals. For example, German bomber aircraft navigated using radio signals transmitted from ground stations in occupied Europe, which the British spoofed by transmitting similar signals on the same frequencies. They coined the term “meaconing” for the interception and rebroadcast of navigation signals (meacon = m(islead)+(b)eacon).

    Fast forward to today. GPS and other GNSS are also susceptible to meaconing. From the outset, the GPS P code, intended for use by military and other so-called authorized users, was designed to be encrypted to prevent straightforward spoofing. The anti-spoofing is implemented using a secret “W” encryption code, resulting in the P(Y) code. The C/A code and the newer L2C and L5 codes do not have such protection; nor, for the most part, do the civil codes of other GNSS. But, it turns out, even the P(Y) code is not fully protected from sophisticated meaconing attacks.

    So, is there anything that military or civil GNSS users can do, then, to guard against their receivers being spoofed by sophisticated false signals? In this month’s column, we take a look at a novel, yet relatively easily implemented technique that enables users to detect and sequester spoofed signals. It just might help make it a safer world for GNSS positioning, navigation, and timing.


    “Innovation” is a regular feature that discusses advances in GPS technology andits applications as well as the fundamentals of GPS positioning. The column is coordinated by Richard Langley of the Department of Geodesy and Geomatics Engineering, University of New Brunswick. He welcomes comments and topic ideas. To contact him, see the “Contributing Editors” section on page 4.

    The radionavigation community has known about the dangers of GNSS spoofing for a long time, as highlighted in the 2001 Volpe Report (see Further Reading). Traditional receiver autonomous integrity monitoring (RAIM) had been considered a good spoofing defense. It assumes a dumb spoofer whose false signal produces a random pseudorange and large navigation solution residuals. The large errors are easy to detect, and given enough authentic signals, the spoofed signal(s) can be identified and ignored.

    That spoofing model became obsolete at The Institute of Navigation’s GNSS 2008 meeting. Dr. Todd Humphreys introduced a new receiver/spoofer that could simultaneously spoof all signals in a self-consistent way undetectable to standard RAIM techniques. Furthermore, it could use its GNSS reception capabilities and its known geometry relative to the victim to overlay the false signals initially on top of the true ones. Slowly it could capture the receiver tracking loops by raising the spoofer power to be slightly larger than that of the true signals, and then it could drag the victim receiver off to false, but believable, estimates of its position, time, or both.

    Two of the authors of this article contributed to Humphreys’ initial developments. There was no intention to help bad actors deceive GNSS user equipment (UE). Rather, our goal was to field a formidable “Red Team” as part of a “Red Team/Blue Team” (foe/friend) strategy for developing advanced “Blue Team” spoofing defenses.

    This seemed like a fun academic game until mid-December 2011, when news broke that the Iranians had captured a highly classified Central Intelligence Agency drone, a stealth Lockheed Martin RQ-170 Sentinel, purportedly by spoofing its GPS equipment. Given our work in spoofing and detection, this event caused quite a stir in our Cornell University research group, in Humphreys’ University of Texas at Austin group, and in other places. The editor of this column even got involved in our extensive e-mail correspondence. Two key questions were: Wouldn’t a classified spy drone be equipped with a Selective Availability Anti-Spoofing Module (SAASM) receiver and, therefore, not be spoofable? Isn’t it difficult to knit together a whole sequence of false GPS position fixes that will guide a drone to land in a wrong location? These issues, when coupled with apparent inconsistencies in the Iranians’ story and visible damage to the drone, led us to discount the spoofing claim.

    Developing a New Spoofing Defense

    My views about the Iranian claims changed abruptly in mid-April 2012. Todd Humphreys phoned me about an upcoming test of GPS jammers, slated for June 2012 at White Sands Missile Range (WSMR), New Mexico. The Department of Homeland Security (DHS) had already spent months arranging these tests, but Todd revealed something new in that call: He had convinced the DHS to include a spoofing test that would use his latest “Red Team” device. The goal would be to induce a small GPS-guided unmanned aerial vehicle (UAV), in this case a helicopter, to land when it was trying to hover. “Wow”, I thought. “This will be a mini-replication of what the Iranians claimed to have done to our spy drone, and I’m sure that Todd will pull it off. I want to be there and see it.” Cornell already had plans to attend to test jammer tracking and geolocation, but we would have to come a day early to see the spoofing “fun” — if we could get permission from U.S. Air Force 746th Test Squadron personnel at White Sands.

    The implications of the UAV test bounced around in my head that evening and the next morning on my seven-mile bike commute to work. During that ride, I thought of a scenario in which the Iranians might have mounted a meaconing attack against a SAASM-equipped drone. That is, they might possibly have received and re-broadcast the wide-band P(Y) code in a clever way that could have nudged the drone off course and into a relatively soft landing on Iranian territory.

    In almost the next moment, I conceived a defense against such an attack. It involves small antenna motions at a high frequency, the measurement of corresponding carrier-phase oscillations, and the evaluation of whether the motions and phase oscillations are more consistent with spoofed signals or true signals. This approach would yield a good defense for civilian and military receivers against both spoofing and meaconing attacks. The remainder of this article describes this defense and our efforts to develop and test it.

    It is one thing to conceive an idea, maybe a good idea. It is quite another thing to bring it to fruition. This idea seemed good enough and important enough to “birth” the conception. The needed follow-up efforts included two parts, one theoretical and the other experimental.

    The theoretical work involved the development of signal models, hypothesis tests, analyses, and software. It culminated in analysis and truth-model simulation results, which showed that the system could be very practical, using only centimeters of motion and a fraction of a second of data to reliably differentiate between spoofing attacks and normal GNSS operation.

    Theories and analyses can contain fundamental errors, or overlooked real-world effects can swamp the main theoretical effect. Therefore, an experimental prototype was quickly conceived, developed, and tested. It consisted of a very simple antenna-motion system, an RF data-recording device, and after-the-fact signal processing. The signal processing used Matlab to perform the spoofing detection calculations after using a C-language software radio to perform standard GPS acquisition and tracking.

    Tests of the non-spoofed case could be conducted anywhere outdoors. Our initial tests occurred on a Cornell rooftop in Ithaca, New York. Tests of the spoofed case are harder. One cannot transmit live spoofing signals except with special permission at special times and in special places, for example, at WSMR in the upcoming June tests. Fortunately, the important geometric properties of spoofed signals can be simulated by using GPS signal reception at an outdoor antenna and re-radiation in an anechoic chamber from a single antenna. Such a system was made available to us by the NASA facility at Wallops Island, Virginia, and our simulated spoofed-case testing occurred in late April of last year. All of our data were processed before mid-May, and they provided experimental confirmation of our system’s efficacy. The final results were available exactly three busy weeks after the initial conception.

    Although we were convinced about our new system, we felt that the wider GNSS community would like to see successful tests against live-signal attacks by a real spoofer. Therefore, we wanted very much to bring our system to WSMR for the June 2012 spoofing attack on the drone. We could set up our system near the drone so that it would be subject to the same malicious signals, but without the need to mount our clumsy prototype on a compact UAV helicopter. We were concerned, however, about the possibility of revealing our technology before we had been able to apply for patent protection. After some hesitation and discussions with our licensing and technology experts, we decided to bring our system to the WSMR test, but with a physical cover to keep it secret. The cover consisted of a large cardboard box, large enough to accommodate the needed antenna motions. The WSMR data were successfully collected using this method. Post-processing of the data demonstrated very reliable differentiation between spoofed and non-spoofed cases under live-signal conditions, as will be described in subsequent sections of this article.

    System Architecture and Prototype

    The components and geometry of one possible version of this system are shown in FIGURE 1. The figure shows three of the GNSS satellites whose signals would be tracked in the non-spoofed case: satellites j-1, j, and j+1. It also shows the potential location of a spoofer that could send false versions of the signals from these same satellites. The spoofer has a single transmission antenna. Satellites j-1, j, and j+1 are visible to the receiver antenna, but the spoofer could “hijack” the receiver’s tracking loops for these signals so that only the false spoofed versions of these signals would be tracked by the receiver.

    Figure 1. Spoofing detection antenna articulation system geometry relative to base mount, GNSS satellites, and potential spoofer.
    Figure 1. Spoofing detection antenna articulation system geometry relative to base mount, GNSS satellites, and potential spoofer. Photo: Mark L. Psiaki with Steven P. Powell and Brady W. O’Hanlon

    The receiver antenna mount enables its phase center to be moved with respect to the mounting base. In Figure 1, this motion system is depicted as an open kinematic chain consisting of three links with ball joints. This is just one example of how a system can be configured to allow antenna motion. Spoofing detection can work well with just one translational degree of freedom, such as a piston-like up-and-down motion that could be provided by a solenoid operating along the za articulation axis. It would be wise to cover the motion system with an optically opaque radome, if possible, to prevent a spoofer from defeating this system by sensing the high-frequency antenna motions and spoofing their effects on carrier phase.

    Suppose that the antenna articulation time history in its local body-fixed (xa, ya, za) coordinate system is ba(t). Then the received carrier phases are sensitive to the projections of this motion onto the line-of-sight (LOS) directions of the received signals. These projections are along  Eq-rj1Eq-rj, and  Eq-r-j+1 in the non-spoofed case, with Eq-rj  being the known unit direction vector from the jth GNSS satellite to the nominal antenna location. In the spoofed case, the projections are all along Eq-rsp, regardless of which signal is being spoofed, with Eq-rsp being the unknown unit direction vector from the spoofer to the victim antenna. Thus, there will be differences between the carrier-phase responses of the different satellites in the non-spoofed case, but these differences will vanish in the spoofed case. This distinction lies at the heart of the new spoofing detection method. Given that a good GNSS receiver can easily distinguish quarter-cycle carrier-phase variations, it is expected that this system will be able to detect spoofing using antenna motions as small as 4.8 centimeters, that is, a quarter wavelength of the GPS L1 signal.

    The UE receiver and spoofing detection block in Figure 1 consists of a standard GNSS receiver, a means of inputting the antenna motion sensor data, and additional signal processing downstream of the standard GNSS receiver operations. The latter algorithms use as inputs the beat carrier-phase measurements from a standard phase-locked loop (PLL).

    It may be necessary to articulate the antenna at a frequency nearly equal to the bandwidth of the PLL (say, at 1 Hz or higher). In this case, special post-processing calculations might be required to reconstruct the high-frequency phase variations accurately before they can be used to detect spoofing. The needed post-processing uses the in-phase and quadrature accumulations of a phase discriminator to reconstruct the noisy phase differences between the true signal and the PLL numerically controlled oscillator (NCO) signal. These differences are added to the NCO phases to yield the full high-bandwidth variations.

    We implemented the first prototype of this system with one-dimensional antenna motion by mounting its patch antenna on a cantilevered beam. It is shown in FIGURE 2. Motion is initiated by pulling on the string shown in the upper left-hand part of the figure. Release of the string gives rise to decaying sinusoidal oscillations that have a frequency of about 2 Hz.

    Figure 2. Antenna articulation system for first prototype spoofing detector tests: a cantilevered beam that allows single-degree-of-freedom antenna phase-center vibration along a horizontal axis. Photo: Mark L. Psiaki with Steven P. Powell and Brady W. O’Hanlon
    Figure 2. Antenna articulation system for first prototype spoofing detector tests: a cantilevered beam that allows single-degree-of-freedom antenna phase-center vibration along a horizontal axis. Photo: Mark L. Psiaki with Steven P. Powell and Brady W. O’Hanlon

    The remainder of the prototype system consisted of a commercial-off-the-shelf RF data recording device, off-line software receiver code, and off-line spoofing detection software. The prototype system lacked an antenna motion sensor. We compensated for this omission by implementing additional signal-processing calculations. They included off-line parameter identification of the decaying sinusoidal motions coupled with estimation of the oscillations’ initial amplitude and phase for any given detection.

    This spoofing detection system is not the first to propose the use of antenna motion to uncover spoofing, and it is related to techniques that rely on multiple antennas. The present system makes three new contributions to the art of spoofing detection: First, it clearly explains why the measured carrier phases from a rapidly oscillating antenna provide a good means to detect spoofing. Second, it develops a precise spoofing detection hypothesis test for a moving-antenna system. Third, it demonstrates successful spoofing detection against live-signal attacks by a “Humphreys-class” spoofer.

    Signal Model Theory and Verification

    The spoofing detection test relies on mathematical models of the response of beat carrier phase to antenna motion. Reasonable models for the non-spoofed and spoofed cases are, respectively:

    Eq-1b  (1a)

    Eq-1a(1b)

    where Eq-0jk is the received (negative) beat carrier phase of the authentic or spoofed satellite-j signal at the kth sample time Eq-tjmk . The three-by-three direction cosines matrix A is the transformation from the reference system, in which the direction vectors Eq-rj  and Eq-rsp are defined, to the local body-axis system, in which the antenna motion ba(t) is defined. λ is the nominal carrier wavelength. The terms involving the unknown polynomial coefficients Eq-Bj0, Eq-Bj1 , and Eq-Bj2 model other low-frequency effects on carrier phase, including satellite motion, UE motion if its antenna articulation system is mounted on a vehicle, and receiver clock drift. The term Eq-nj0k is the receiver phase noise. It is assumed to be a zero-mean, Gaussian, white-noise process whose variance depends on the receiver carrier-to-noise-density ratio and the sample/accumulation frequency.

    If the motion of the antenna is one-dimensional, then ba(t) takes the form Eq-ba1, with Eq-ba being the articulation direction in body-axis coordinates and ra(t) being a known scalar antenna deflection amplitude time history. If one defines the articulation direction in reference coordinates as Eq-ra , then the carrier-phase models in Equations (1a) and (1b) become

    Eq-2a   (2a)

    Eq-2b  (2b)

    There is one important feature of these models for purposes of spoofing detection. In the non-spoofed case, the term that models the effects of antenna motion varies between GPS satellites because the Eq-rj direction vector varies with j. The spoofed case lacks variation between the satellites because the one spoofer direction Eq-rsp replaces Eq-rj for all of the spoofed satellites. This becomes clear when one compares the first terms on the right-hand sides of Eqsuations (1a) and (1b) for the 3-D motion case and on the right-hand sides of Equations (2a) and (2b) for the 1-D case.

    The carrier-phase time histories in FIGURES 3 and 4 illustrate this principle. These data were collected at WSMR using the prototype antenna motion system of Figure 2. The carrier-phase time histories have been detrended by estimating the Eq-Bj0, Eq-Bj1 , and Eq-Bj2 coefficients in Equations (2a) and (2b) and subtracting off their effects prior to plotting. In Figure 3, all eight satellite signals exhibit similar decaying sinusoid time histories, but with differing amplitudes and some of them with sign changes. This is exactly what is predicted by the 1-D non-spoofed model in Equation (2a). All seven spoofed signals in Figure 4, however, exhibit identical decaying sinusoidal oscillations because the Eq-rsp-tra term in Equation (2b) is the same for all of them.

    Figure 3. Detrended carrier-phase data from multiple satellites for a typical non-spoofed case using a 1-D antenna articulation system.
    Figure 3. Detrended carrier-phase data from multiple satellites for a typical non-spoofed case using a 1-D antenna articulation system.

     

    Figure 4. Multiple satellites’ detrended carrier-phase data for a typical spoofed case using a 1-D antenna articulation system.
    Figure 4. Multiple satellites’ detrended carrier-phase data for a typical spoofed case using a 1-D antenna articulation system.

    As an aside, an interesting feature of Figure 3 is its evidence of the workings of the prototype system. The ramping phases of all the signals from t = 0.4 seconds to t = 1.4 seconds correspond to the initial pull on the string shown in Figure 2, and the steady portion from t = 1.4 seconds to t = 2.25 seconds represents a period when the string was held fixed prior to release.

    Spoofing Detection Hypothesis Test

    A hypothesis test can precisely answer the question of which model best fits the observed data: Does carrier-phase sameness describe the data, as in Figure 4? Then the receiver is being spoofed. Alternatively, is carrier-phase differentness more reasonable, as per Figure 3? Then the signals are trustworthy.

    A hypothesis test can be developed for any batch of carrier-phase data that spans a sufficiently rich antenna motion profile ba(t) or ρa(t). The profile must include high-frequency motions that cannot be modeled by the  Eq-Bj0, Eq-Bj1 , and Eq-Bj2quadratic polynomial terms in Equations (1a)-(2b); otherwise the detection test will lose all of its power. A motion profile equal to one complete period of a sine wave has the needed richness.

    Suppose one starts with a data batch that is comprised of carrier-phase time histories for L different GNSS satellites: Eq-0jk for samples k = 1, …, Mj and for satellites j = 1,…, L. A standard hypothesis test develops two probability density functions for these data, one conditioned on the null hypothesis of no spoofing, H0, and the other conditioned on the hypothesis of spoofing, H1.  The Neyman-Pearson lemma (see Further Reading) proves that the optimal hypothesis test statistic equals the ratio of these two probability densities. Unfortunately, the required probability densities depend on additional unknown quantities. In the 1-D motion case, these unknowns include the Eq-Bj0, Eq-Bj1 , and Eq-Bj2 coefficients, the dot product Eq-rsp-tra, and the direction Eq-tra  if one assumes that the UE attitude is unknown. A true Neyman-Pearson test would hypothesize a priori distributions for these unknown quantities and integrate their dependencies out of the two joint probability distributions. Our sub-optimum test optimally estimates relevant unknowns for each hypothesis based on the carrier-phase data, and it uses these estimates in the Neyman-Pearson probability density ratio. Although sub-optimal as a hypothesis test, this approach is usually effective, and it is easier to implement than the integration approach in the present case.

    Consider the case of 1-D antenna articulation and unknown UE attitude. Maximum-likelihood calculations optimally estimate the nuisance parameters  Eq-Bj0, Eq-Bj1 , and Eq-Bj2  for j = 1, …, L for both hypotheses along with the unit vector Eq-tra for the non-spoofed hypothesis, or the scalar dot product Eq-nsix for the spoofed hypothesis. The estimation calculations for each hypothesis minimize the negative natural logarithm of the corresponding conditional probability density. Because  Eq-Bj0, Eq-Bj1 , and Eq-Bj2 enter the resulting cost functions quadratically, their optimized values can be computed as functions of the other unknowns, and they can be substituted back into the costs. This part of the calculation amounts to a batch high-pass filter of both the antenna motion and the carrier-phase response.

    The remaining optimization problems take, under the non-spoofed hypothesis, the form:

    find:      Eq-tra    (3a)

    to minimize:       Eq-Jnonsp  (3b)

    subject to:             Eq-rasmall   (3c)

    and, under the spoofed hypothesis, the form:

    find:      η    (4a)

    to minimize:   Eq-Jspn      (4b)

    subject to:     Eq-111 .   (4c)

    The coefficient Eq-rj44 is a function of the deflections Eq-Pat for k = 1, …, Mj, and the non-homogenous term Eq-zj4 is derived from the jth phase time history Eq-0jk for k = 1, …, Mj. These two quantities are calculated during the  Eq-Bj0, Eq-Bj1, Eq-Bj2 optimization. The constraint in Equation (3c) forces the estimate of the antenna articulation direction to be unit-normalized. The constraint in Eq. (4c) ensures that η is a physically reasonable dot product.

    The optimization problems in Equations (3a)-(3c) and (4a)-(4c) can be solved in closed form using techniques from the literature on constrained optimization, linear algebra, and matrix factorization. The optimal estimates of Eq-tra and η can be used to define a spoofing detection statistic that equals the natural logarithm of the Neyman-Pearson ratio:

    Eq-y-small(5)

    It is readily apparent that γ constitutes a reasonable test statistic: If the signal is being spoofed so that carrier-phase sameness is the best model, then ηopt will produce a small value of  Eq-Jsp-nbecause the spoofed-case cost function in Equation (4b) is consistent with carrier-phase sameness. The value of Eq-Jnonsp-r, however, will not be small because the plurality of  Eq-rj directions in Equation (3b) precludes the possibility that any Eq-tra estimate will yield a small non-spoofed cost. Therefore, γ will tend to be a large negative number in the event of spoofing because Eq-Jnonsp-r >> Eq-Jsp-n is likely. In the non-spoofed case, the opposite holds true: Eq-ropt  will yield a small value of Eq-Jnonsp-r, but no estimate of η will yield a small Eq-jspn2, and γ will be a large positive number because  Eq-Jnonsp-r<< Eq-Jsp-n.

    Therefore, a sensible spoofing detection test employs a detection threshold γth somewhere in the neighborhood of zero. The detection test computes a γ value based on the carrier-phase data, the antenna articulation time history, and the calculations in Equations (3a)-(5). It compares this γ to γth. If γγth, then the test indicates that there is no spoofing. If γ < γth, then a spoofing alert is issued.

    The exact choice of γth is guided by an analysis of the probability of false alarm. A false alarm occurs if a spoofing attack is declared when there is no spoofing. The false-alarm probability is determined as a function of γth by developing a γ probability density function under the null hypothesis of no spoofing p(γ|H0). The probability of false alarm equals the integral of p(γ|H0) from γ = Eq-infinity to γ = γth. This integral relationship can be inverted to determine the γth threshold that yields a given prescribed false-alarm probability

    A complication arises because p(γ|H0) depends on unknown parameters, Eq-tra  in the case of an unknown UE attitude and 1-D antenna motion. Although sub-optimal, a reasonable way to deal with the dependence of p(γ|Eq-tra,H0) on Eq-tra is to use the worst-case Eq-tra for a given γth. The worst-case articulation direction Eq-rawc maximizes the p(γ|Eq-tra,H0) false-alarm integral. It can be calculated by solving an optimization problem. This analysis can be inverted to pick γth so that the worst-case probability of false alarm equals some prescribed value. For most actual Eq-tra values, the probability of false alarm will be lower than the prescribed worst case.

    Given γth, the final needed analysis is to determine the probability of missed detection. This analysis uses the probability density function of g under the spoofed hypothesis, p(γ|η,H1). The probability of missed detection is the integral of this function from γ = γth to γ = +Eq-infinity2. The dependence of p(γ|η,H1) on the unknown dot product η can be handled effectively, though sub-optimally, by determining the worst-case probability of false alarm. This involves an optimization calculation, which finds the worst-case dot product ηwc that maximizes the missed-detection probability integral. Again, most actual η values will yield lower probabilities of missed detection.

    Note that the above-described analyses rely on approximations of the probability density functions p(γ|Eq-tra,H0) and p(γ|η,H1). The best approximations include dominant Gaussian terms plus small chi-squared or non-central chi-squared terms. It is difficult to analyze the chi-squared terms rigorously. Their smallness, however, makes the use of Gaussian approximations reasonable.

    We have developed and evaluated several alternative formulations of this spoofing detection method. One is the case of full 3-D ba(t) antenna motion with unknown UE attitude. The full direction cosines matrix A is estimated in the modified version of the non-spoofed optimal fit calculations of Equations (3a)-(3c), and the full spoofing direction vector Eq-bsp is estimated in the modified version of Equations (4a)-(4c). A different alternative allows the 1-D motion time history ρa(t) to have an unknown amplitude-scaling factor that must be estimated. This might be appropriate for a UAV drone with a wing-tip-mounted antenna if it induced antenna motions by dithering its ailerons. In fixed-based applications, as might be used by a financial institution, a cell-phone tower, or a power-grid monitor, the attitude would be known, which would eliminate the need to estimate Eq-tra or A for the non-spoofed case.

    Test Results

    The initial tests of our concept involved generation of simulated truth-model carrier-phase data Eq-0jk using simulated Eq-Bj0, Eq-Bj1 , and Eq-Bj2 polynomial coefficients, simulated satellite LOS direction vectors Eq-rj for the non-spoofed cases, a simulated true spoofer LOS direction Eq-rsp for the spoofed cases, and simulated antenna motions parameterized by Eq-tra and ρa(t). Monte-Carlo analysis was used to generate many different batches of phase data with different random phase noise realizations in order to produce simulated histograms of the p(γ|Eq-tra, H0) and p(γ|η,H1) probability density functions  that are used in false-alarm and missed-detection analyses.

    The truth-model simulations verified that the system is practical. A representative calculation used one cycle of an 8-Hz 1-D sinusoidal antenna oscillation with a peak-to-peak amplitude of 4.76 centimeters (exactly 1/4 of the L1 wavelength). The accumulation frequency was 1 kHz so that there were Mj = 125 carrier-phase measurements per satellite per data batch. The number of satellites was L = 6, their Eq-rj LOS vectors were distributed to yield a geometrical dilution of precision of 3.5, and their carrier-to-noise-density ratios spanned the range 38.2 to 44.0 dB-Hz. The worst-case probability of a spoofing false alarm was set at 10-5 and the corresponding worst-case probability of missed detection was 1.2 ´ 10-5. Representative non-worst-case probabilities of false alarm and missed detection were, respectively, 1.7 ´ 10-9 and 1.1 ´ 10-6. These small numbers indicate that this is a very powerful test. Ten-thousand run Monte-Carlo simulations of the spoofed and non-spoofed cases verified the reasonableness of these probabilities and the reasonableness of the p(γ|Eq-tra, H0) and p(γ|η,H1) Gaussian approximations that had been used to derive them.

    The live-signal tests bore out the truth-model simulation results. The only surprise in the live-signal tests was the presence of significant multipath, which was evidenced by received carrier amplitude oscillations that correlated with the antenna oscillations and whose amplitudes and phases varied among the different received GPS signals. As a verification that these oscillations were caused by multipath, the only live-signal data set without such amplitude oscillations was the one taken in the NASA Wallops anechoic chamber, where one would not expect to find multipath. The multipath, however, seems to have negligible impact on the efficacy of this spoofing detection system.

    FIGURES 5 and 6 show the results of typical non-spoofed and spoofed cases from WSMR live-signal tests that took place on the evening of June 19–20, 2012. Each plot shows the spoofing detection statistic γ on the horizontal axis and various related probability density functions on the vertical axis. This statistic has been calculated using a modified test that includes the estimation of two additional unknowns: an antenna articulation scale factor f and a timing bias t0 for the decaying sinusoidal oscillation eq-pa. The damping ratio ζ and the undamped natural frequency wn are known from prior system identification tests.

    Figure 5. Spoofing detection statistic, threshold, and related probability density functions for a typical non-spoofed case with live data.
    Figure 5. Spoofing detection statistic, threshold, and related probability density functions for a typical non-spoofed case with live data.

     

    Figure 6. Performance of a typical spoofed case with live data: spoofing detection statistic, threshold, and related probability density functions.
    Figure 6. Performance of a typical spoofed case with live data: spoofing detection statistic, threshold, and related probability density functions.

    The vertical dashed black line in each plot shows the actual value of γ as computed from the GPS data. There are three vertical dash-dotted magenta lines that lie almost on top of each other. They show the worst-case threshold values γth as computed for the optimal and ±2σ estimates of t0: t0opt, t0opt+2σt0opt, and t0opt-2σt0opt. They have been calculated for a worst-case probability of false alarm equal to 10-6. An ad hoc method of compensating for the prototype system’s t0 uncertainty is to use the left-most vertical magenta line as the detection threshold γth. The vertical dashed black line lies very far to the right of all three vertical dash-dotted magenta lines in Figure 5, which indicates a successful determination that the signals are not being spoofed. In Figure 6, the situation is reversed. The vertical dashed black line lies well to the left of the three vertical dash-dotted magenta lines, and spoofing is correctly and convincingly detected.

    These two figures also plot various relevant probability density functions. Consistent with the consideration of three possible values of the t0 motion timing estimate, these are plotted in triplets. The three dotted cyan probability density functions represent the worst-case non-spoofed situation, and the dash-dotted red probability functions represent the corresponding worst-case spoofed situations. Obviously, there is sufficient separation between these sets of probability density functions to yield a powerful detection test, as evidenced by the ability to draw the dash-dotted magenta detection thresholds in a way that clearly separates the red and cyan distributions. Further confirmation of good detection power is provided by the low worst-case probabilities of false alarm and missed detection, the latter metric being 1.6 ´ 10-6 for the test in Figure 5 and 7 ´ 10-8 for Figure 6.

    The solid-blue distributions on the two plots correspond to the ηopt estimate and the spoofed assumption, which is somewhat meaningless for Figure 5, but meaningful for Figure 6. The dashed-green distributions are for the Eq-tra estimate under the non-spoofed assumption. The wide separations between the blue distributions and the green distributions in both figures clearly indicate that the worst-case false-alarm and missed-detection probabilities can be very conservative.

    The detection test results in Figures 5 and 6 have been generated using the last full oscillation of the respective carrier-phase data, as in Figures 3 and 4, but applied to different data sets. In Figure 3, the last full oscillation starts at t = 3.43 seconds, and it starts at t = 2.11 seconds in Figure 4. The peak-to-peak amplitude of each last full oscillation ranged from 4-6 centimeters, and their periods were shorter than 0.5 seconds. It would have been possible to perform the detections using even shorter data spans had the mechanical oscillation frequency of the cantilevered antenna been higher.

    Conclusions

    In this article, we have presented a new method to detect spoofing of GNSS signals. It exploits the effects of intentional high-frequency antenna motion on the measured beat carrier phases of multiple GNSS signals. After detrending using a high-pass filter, the beat carrier-phase variations can be matched to models of the expected effects of the motion. The non-spoofed model predicts differing effects of the antenna motion for the different satellites, but the spoofed case yields identical effects due to a geometry in which all of the false signals originate from a single spoofer transmission antenna. Precise spoofing detection hypothesis tests have been developed by comparing the two models’ ability to fit the measured data.

    This new GNSS spoofing detection technique has been evaluated using both Monte-Carlo simulation and live data. Its hypothesis test yields theoretical false-alarm probabilities and missed-detection probabilities on the order of 10-5 or lower when working with typical numbers and geometries of available GPS signals and typical patch-antenna signal strengths. The required antenna articulation deflections are modest, on the order of 4-6 centimeters peak-to-peak, and detection intervals less than 0.5 seconds can suffice.

    A set of live-signal tests at WSMR evaluated the new technique against a sophisticated receiver/spoofer, one that mimics all visible signals in a way that foils standard RAIM techniques. The new system correctly detected all of the attacks. These are the first known practical detections of live-signal attacks mounted against a civilian GNSS receiver by a dangerous new generation of spoofers.

    Future Directions

    This work represents one step in an on-going “Blue Team” effort to develop better defenses against new classes of GNSS spoofers. Planned future improvements include 1) the ability to use electronically synthesized antenna motion that eliminates the need for moving parts, 2) the re-acquisition of true signals after detection of spoofing, 3) the implementation of real-time prototypes using software radio techniques, and 4) the consideration of “Red-Team” counter-measures to this defense  and how the “Blue Team” could combat them; counter-measures such as high-frequency phase dithering of the spoofed signals or coordinated spoofing transmissions from multiple locations.

    Acknowledgments

    The authors thank the following people and organizations for their contributions to this effort:  The NASA Wallops Flight Facility provided access to their anechoic chamber. Robert Miceli, a Cornell graduate student, helped with data collection at that facility. Dr. John Merrill and the Department of Homeland Security arranged the live-signal spoofing tests. The U.S. Air Force 746th Test Squadron hosted the live-signal spoofing tests at White Sands Missile Range. Prof. Todd Humphreys and members of his University of Texas at Austin Radionavigation Laboratory provided live-signal spoofing broadcasts from their latest receiver/spoofer.

    Manufacturers

    The prototype spoofing detection data capture system used an Antcom Corp. (www.antcom.com) 2G1215A L1/L2 GPS antenna. It was connected to an Ettus Research (www.ettus.com) USRP (Universal Software Radio Peripheral) N200 that was equipped with the DBSRX2 daughterboard.


    MARK L. PSIAKI is a professor in the Sibley School of Mechanical and Aerospace Engineering at Cornell University, Ithaca, New York. He received a B.A. in physics and M.A. and Ph.D. degrees in mechanical and aerospace engineering from Princeton University, Princeton, New Jersey. His research interests are in the areas of GNSS technology, applications, and integrity, spacecraft attitude and orbit determination, and general estimation, filtering, and detection.

    STEVEN P. POWELL is a senior engineer with the GPS and Ionospheric Studies Research Group in the Department of Electrical and Computer Engineering at Cornell University. He has M.S. and B.S. degrees in electrical engineering from Cornell University. He has been involved with the design, fabrication, testing, and launch activities of many scientific experiments that have flown on high altitude balloons, sounding rockets, and small satellites. He has designed ground-based and space-based custom GPS receiving systems primarily for scientific applications.

    BRADY W. O’HANLON is a graduate student in the School of Electrical and Computer Engineering at Cornell University. He received a B.S. in electrical and computer engineering from Cornell University. His interests are in the areas of GNSS technology and applications, GNSS security, and GNSS as a tool for space weather research.

    VIDEO

    Here is a video of Cornell University’s antenna articulation system for the team’s first prototype spoofing detector tests.

    FURTHER READING

    • The Spoofing Threat and RAIM-Resistant Spoofers

    “Status of Signal Authentication Activities within the GNSS Authentication and User Protection System Simulator (GAUPSS) Project” by O. Pozzobon, C. Sarto, A. Dalla Chiara, A. Pozzobon, G. Gamba, M. Crisci, and R.T. Ioannides, in Proceedings of ION GNSS 2012, the 25th International Technical Meeting of The Institute of Navigation, Nashville, Tennessee, September 18–21, 2012, pp. 2894-2900.

    Assessing the Spoofing Threat” by T.E. Humphreys, P.M. Kintner, Jr., M.L. Psiaki, B.M. Ledvina, and B.W. O’Hanlon in GPS World, Vol. 20, No. 1, January 2009, pp. 28-38.

    Vulnerability Assessment of the Transportation Infrastructure Relying on the Global Positioning System – Final Report. John A. Volpe National Transportation Systems Center, Cambridge, Massachusetts, August 29, 2001.

    Moving-Antenna and Multi-Antenna Spoofing Detection

    Robust Joint Multi-Antenna Spoofing Detection and Attitude Estimation by Direction Assisted Multiple Hypotheses RAIM” by M. Meurer, A. Konovaltsev, M. Cuntz, and C. Hattich, in Proceedings of ION GNSS 2012, the 25th International Technical Meeting of The Institute of Navigation, Nashville, Tennessee, September 18–21, 2012, pp. 3007-3016.

    “GNSS Spoofing Detection for Single Antenna Handheld Receivers” by J. Nielsen, A. Broumandan, and G. Lachapelle in Navigation, Vol. 58, No. 4, Winter 2011, pp. 335-344.

    Alternate Spoofing Detection Strategies

    “Who’s Afraid of the Spoofer? GPS/GNSS Spoofing Detection via Automatic Gain Control (AGC)” by D.M. Akos, in Navigation, Vol. 59, No. 4, Winter 2012-2013, pp. 281-290.

    “Civilian GPS Spoofing Detection based on Dual-Receiver Correlation of Military Signals” by M.L. Psiaki, B.W. O’Hanlon, J.A. Bhatti, D.P. Shepard, and T.E. Humphreys in Proceedings of ION GNSS 2011, the 24th International Technical Meeting of The Institute of Navigation, Portland, Oregon, September 19–23, 2011, pp. 2619-2645.

    Statistical Hypothesis Testing

    Fundamentals of Statistical Signal Processing, Volume II: Detection Theory by S. Kay, published by Prentice Hall, Upper Saddle River, New Jersey,1998.

    An Introduction to Signal Detection and Estimation by H.V. Poor, 2nd edition, published by Springer-Verlag, New York, 1994.

  • FICOSA Integrates OriginGPS Antenna Module in Telematic Unit

    FICOSA demonstrated a telematic unit integrating a multi-service antenna module for positioning and satellite navigation supporting all the geographic positioning standards at the 2013 Mobile World Congress in Barcelona in February.

    The major advantage of this technological innovation is that the proposed multi-channel GPS/Galileo/GLONASS/BeiDou/QZSS receiver allows tracking across all the different navigation and positioning satellite standards worldwide, so that automakers can  the having to manage different variants of in-vehicle telematic units (iVTUs) depending on the geographical market. iVTUs are needed for emergency call function, fleet management, and other functions. It incorporates an OriginGPS antenna.

    The new module is a complete system-in-package featuring miniature surface mount device technology footprint designed to commit unique integration features for high volume, low power and cost-sensitive applications.

    In addition, the reduced size of the receiver module makes the most of a stacked-up in board integration through miniaturized integrated circuits and surface mount devices, allows an aggressive reduction of the iVTU packaging, which is advantageous for the OEM for car assembly, iVTU localization inside the vehicle, and weight reduction.

    The innovation represents the result of the international collaboration between FICOSA and OriginGPS. “We view the telematics market as a growing market and it is our privilege to cooperate and partner with Ficosa and its excellent engineering team,” said Haim Goldberger, CEO and founder of OriginGPS.

    “In FICOSA, innovation and technology are two main tools for our future and working with OriginGPS is a great issue,” said Jose María Forcadell, Advanced Communications Business Unit Director at FICOSA.

  • Signal Decoding with Conventional Receiver and Antenna

    Signal Decoding with Conventional Receiver and Antenna

    A Case History Using the New Galileo E6-B/C Signal

    By Sergei Yudanov, JAVAD GNSS

    A method of decoding an unknown pseudorandom noise code uses a conventional GNSS antenna and receiver with modified firmware. The method was verified using the signals from the Galileo In-Orbit Validation satellites.

    Decoding an unknown GNSS pseudorandom noise (PRN) code can be rather easily done using a high-gain steerable dish antenna as was used, for example, in determine the BeiDou-M1 broadcast codes before they were publicly announced. The signal-to-noise ratio within one chip of the code is sufficient to determine its sign. This article describes a method of getting this information using a conventional GNSS antenna and receiver with modified firmware. The method was verified using the signals from the Galileo In-Orbit Validation (IOV) satellites. In spite of the fact that only pilot signal decoding seems to be possible at first glance, it is shown that in practice data signals can also be decoded.

    Concept

    The idea is to do coherent accumulation of each chip of an unknown signal during a rather long time interval. The interval may be as long as a full satellite pass; for medium Earth orbits, this could be up to six hours. One of the receiver’s channels is configured in the same way as for signal tracking. The I and Q signal components are accumulated during one chip length in the digital signal processor, and these values are added to an array cell, referenced by chip number, by the processor. Only a limited amount of information need be known about the signal: its RF frequency; the expected chip rate; the expected total code length; and the modulation method.

    The decoding of binary-phase-shift-keying (BPSK) signals (as most often used) is the subject of this article. It appears that the decoding of more complicated signals is possible too, but this should be proved. A limitation of this method (in common with that of the dish method) is the maximum total code length that can be handled: for lengths greater than one second and bitrates higher than 10,000 kilobits per second, the receiver’s resources may not be sufficient to deal with the signal.

    Reconstructing the Signal’s Phase

    This method requires coherency. During the full accumulation period, the phase difference between the real signal phase and the phase of the signal generated by the receiver’s channel should be much less than one cycle of the carrier frequency. Depending on the GNSS’s available signals, different approaches may be used. The simplest case is reconstruction of a third signal while two other signals on different frequencies are of known structure and can be tracked.

    The main (and possibly the only significant) disturbing factor is the ionosphere. The ionospheric delay (or, more correctly, the variation of ionospheric delay) is calculated using the two known tracked signals, then the phase of the third signal, as affected by the ionosphere, is predicted.

    The final formula (the calculations are trivial and are widely available in the literature) is:

    Y-Eq1

    where:
    φ1 , f1 are the phase and frequency of the first signal in cycles and Hz, respectively
    φ2 , f2   are the phase and frequency of the second signal in cycles and Hz, respectively
    φ3 , f3   are the phase and frequency of the third signal in cycles and Hz, respectively.

    It was confirmed that for all pass periods (elevation angles less than 10 degrees were not tested), the difference between the calculated phase and real phase was always less than one-tenth of a cycle. GPS Block IIF satellites PRN 1 and PRN 25 were used to prove this: the L1 C/A-code and L5 signals were used as the first and second signals, with the L2C signal as the third unknown.

    If two known signals are not available, and the ionospheric delay cannot be precisely calculated, it is theoretically possible to obtain an estimate of the delay from one or more neighboring satellites with two signals available. Calculations and estimations should be carried out to investigate the expected precision.

    The Experiment

    The Galileo E6-B/C signal as currently transmitted by the IOV satellites was selected for the experiment, as its structure has not been published. The E6 signal has three components: E6-A, E6-B and E6-C. The E6-A component is part of the Galileo Public Regulated Service, while the two other components will serve the Galileo Commercial Service. The E6-B component carries a data signal, while the E6-C component is a pilot signal.

    From open sources, it is known that the carrier frequency of the E6 signal is 1278.75 MHz and that the E6-B and E6-C components use BPSK modulation at 5,115 chips per millisecond with a primary code length of one millisecond. E6-B’s data rate is 1,000 bits per second and the total length of the pilot code is 100 milliseconds (a secondary code of 100 bits over 100 milliseconds is also present in the E6-C signal, which aids in signal acquisition).

    A slightly modified commercial high-precision multi-GNSS receiver, with the E6 band and without the GLONASS L2 band, was used for this experiment. The receiver was connected to a conventional GNSS antenna, placed on a roof and was configured as described above. The E1 signal was used as the first signal and E5a as the second signal. The E6 code tracking (using 5,115 chip values of zero) was 100 percent guided from the E1 code tracking (the changing of the code delay in the ionosphere was ignored). The E6 phase was guided from E1 and E5a using the above equation. Two arrays for 511,500 I and Q samples were organized in firmware. The integration period was set to one chip (200 nanoseconds).

    Galileo IOV satellite PRN 11 (also variously known as E11, ProtoFlight Model and GSAT0101) was used initially, and the experiment started when the satellite’s elevation angle was about 60 degrees and lasted for only about 30 minutes. Then the I and Q vectors were downloaded to a PC and analyzed.

    Decoding of Pilot Signal (E6-C)

    Decoding of the pilot signal is made under the assumption that any possible influence of the data signal is small because the number of ones and zeros of E6-B in each of 511,500 chips of the 100-millisecond integration interval is about the same. First, the secondary code was obtained. Figure 1 shows the correlation of the first 5,115 chips with 5,115 chips shifted by 0 to 511,500 chips. Because the initial phase of the E6 signal is unknown, two hypotheses for computing the amplitude or signal level were checked: [A] = [I] + [Q] and [A] = [I] – [Q], and the combination with the higher correlation value was selected for all further analysis.

    Y-Fig1
    Figure 1. Un-normalized autocorrelation of E6-C signal chips.

    In Figure 1, the secondary code is highly visible: we see a sequence of 100 positive and negative correlation peaks (11100000001111 …; interpreting the negative peaks as zeros).This code is the exact complement (all bits reversed) of the published E5a pilot secondary code for this satellite. More will be said about the derived codes and their complements later. It appears that, for all of the IOV satellites, the E6-C secondary codes are the same as the E5a secondary codes.

    After obtaining the secondary code, it is possible to coherently add all 100 milliseconds of the integration interval with the secondary code sign to increase the energy in each chip by 100 times. Proceeding, we now have 5,115 chips of the pilot signal ­— the E6-C primary code.

    To understand the correctness of the procedure and to check its results, we need to confirm that there is enough signal energy in each chip. To this end, a histogram of the pilot signal chip amplitudes can be plotted (see Figure 2). We see that there is nothing in the middle of the plot. This means that all 5,115 chips are correct, and there is no chance that even one bit is wrong.

    Y-Fig2
    Figure 2. Histogram of pilot signal chip amplitude in arbitrary units.

    But there is one effect that seems strange at first glance: instead of two peaks we have four (two near each other). We will shortly see that this phenomenon results from the influence of the E6-B data signal and it may be decoded also.

    Decoding the Data Signal

    The presence of four peaks in the histogram of Figure 2 was not understood initially, so a plot of all 511,500 signal code chips was made (see Figure 3).
    Interestingly, each millisecond of the signal has its own distribution, and milliseconds can be found where the distribution is close to that when two signals with the same chip rate are present. In this case, there should be three peaks in the energy (signal strength) spectrum: –2E, 0, and +2E, where E is the energy of one signal (assuming the B and C signals have the same strength).

    Figure 3. Plot of 511,500 signal code chip amplitudes in arbitrary units.
    Figure 3. Plot of 511,500 signal code chip amplitudes in arbitrary units.

    One such time interval (starting at millisecond 92 and ending at millisecond 97) is shown in Figure 4. The middle of the plot (milliseconds 93 to 96) shows the described behavior. Figure 5 is a histogram of signal code chip amplitude for the signal from milliseconds 93 to 96.

    Figure 4  Plot of signal code chip amplitude in arbitrary units from milliseconds 93 to 96.
    Figure 4. Plot of signal code chip amplitude in arbitrary units from milliseconds 93 to 96.

    Then we collect all such samples (milliseconds) with the same data sign together to increase the signal level. Finally, 5,115 values are obtained. Their distribution is shown in Figure 6.

    The central peak is divided into two peaks (because of the presence of the pilot signal), but a gap between the central and side peaks (unlike the case of Figure 5) is achieved. This allows us to get the correct sign of all data signal chips. Subtracting the already known pilot signal chips, we get the 5,115 chips of the data signal — the E6-B primary code. This method works when there are at least some samples (milliseconds) where the number of chips with the same data bit in the data signal is significantly more than half.

    Y-Fig5
    Figure 5. Histogram of signal code chip amplitude.
    Figure 6  Histogram of the signed sum of milliseconds chip amplitude with a noticeable presence of the data signal.
    Figure 6. Histogram of the signed sum of milliseconds chip amplitude with a noticeable presence of the data signal.
    Proving the Codes

    The experimentally determined E6-B and E6-C primary codes and the E6-C secondary codes for all four IOVsatellites (PRNs 11, 12, 19, and 20) were put in the receiver firmware. The receiver was then able to autonomously track the E6-B and E6-C signals of the satellites.

    Initial decoding of E6-B navigation data has been performed. It appears that the data has the same preamble (the 16-bit synchronization word) as that given for the E6-B signal in the GIOVE Interface Control Document (ICD). Convolutional encoding for forward error correction is applied as described in the Galileo Open Service ICD, and 24-bit cyclic redundancy check error detection (CRC-24) is used. At the time of the analysis, all four IOV satellites transmitted the same constant navigation data message.

    Plots of PRN 11 E6 signal tracking are shown in Figure 7 and in Figure 8. The determined codes may be found at env-gpsworld-integration.kinsta.cloud/galileo-E6-codes. Some of these codes may be the exact complement of the official codes since the code-determination technique has a one-half cycle carrier-phase ambiguity resulting in an initial chip value ambiguity. But from the point of view of receiver tracking, this is immaterial.

    Figure 7  Signal-to-noise-density ratio of E1 (red), E5a (magenta), E5b (blue), and E6 (green) code tracking of Galileo IOV satellite PRN 11 on December 21–22, 2012.
    Figure 7. Signal-to-noise-density ratio of E1 (red), E5a (magenta), E5b (blue), and E6 (green) code tracking of Galileo IOV satellite PRN 11 on December 21–22, 2012.
    Figure 8  Pseudorange minus carrier phase (in units of meters) of E1 (red), E5a (magenta), E5b (blue), and E6 (green) code tracking of Galileo IOV satellite PRN 11 on December 21–22, 2012.
    Figure 8. Pseudorange minus carrier phase (in units of meters) of E1 (red), E5a (magenta), E5b (blue), and E6 (green) code tracking of Galileo IOV satellite PRN 11 on December 21–22, 2012.
    Acknowledgments

    Special thanks to JAVAD GNSS’s DSP system developers. The system is flexible so it allows us to do tricks like setting the integration period to one chip, and powerful enough to be able to do required jobs within a 200-nanosecond cycle. This article was prepared for publication by Richard Langley.

    Manufacturers

    A JAVAD GNSS TRE-G3T-E OEM receiver, a modification of the TRE-G3T receiver, was used in the experiment, connected to a conventional JAVAD GNSS antenna. Plots of E6 code tracking of all four IOV satellites may be found on the company’s website.


    Sergei Yudanov is a senior firmware developer at JAVAD GNSS, Moscow.

  • Innovation: Getting Control

    Innovation: Getting Control

    Off-the-Shelf Antennas for Controlled-Reception-Pattern Antenna Arrays

    By Yu-Hsuan Chen, Sherman Lo, Dennis M. Akos, David S. De Lorenzo, and Per Enge

    GPS World photo
    INNOVATION INSIGHTS by Richard Langley

    THE ANTENNA IS A CRITICAL COMPONENT OF ANY GNSS RECEIVING EQUIPMENT. It must be carefully designed for the frequencies and structures of the signals to be acquired and tracked. Important antenna properties include polarization, frequency coverage, phase-center stability, multipath suppression, the antenna’s impact on receiver sensitivity, reception or gain pattern, and interference handling. While all of these affect an antenna’s performance, let’s just look at the last two here.

    The gain pattern of an antenna is the spatial variation of the gain, or ratio of the power delivered by the antenna for a signal arriving from a particular direction compared to that delivered by a hypothetical isotropic reference antenna. Typically, for GNSS antennas, the reference antenna is also circularly polarized and the gain is then expressed in dBic units.

    An antenna may have a gain pattern with a narrow central lobe or beam if it is used for communications between two fixed locations or if the antenna can be physically steered to point in the direction of a particular transmitter. GNSS signals, however, arrive from many directions simultaneously, and so most GNSS receiving antennas tend to be omni-directional in azimuth with a gain roll-off from the antenna boresight to the horizon.

    While such an antenna is satisfactory for many applications, it is susceptible to accidental or deliberate interference from signals arriving from directions other than those of GNSS signals. Interference effects could be minimized if the gain pattern could be adjusted to null-out the interfering signals or to peak the gain in the directions of all legitimate signals. Such a controlled-reception-pattern antenna (CRPA) can be constructed using an array of antenna elements, each one being a patch antenna, say, with the signals from the elements combined before feeding them to the receiver. The gain pattern of the array can then be manipulated by electronically adjusting the phase relationship between the elements before the signals are combined. However, an alternative approach is to feed the signals from each element to separate banks of tracking channels in the receiver and form a beam-steering vector based on the double-difference carrier-phase measurements from pairs of elements that is subsequently used to weight the signals from the elements before they are processed to obtain a position solution. In this month’s column, we learn how commercial off-the-shelf antennas and a software-defined receiver can be used to design and test such CRPA arrays.


    “Innovation” features discussions about advances in GPS technology, its applications, and the fundamentals of GPS positioning. The column is coordinated by Richard Langley, Department of Geodesy and Geomatics Engineering, University of New Brunswick. To contact him with topic ideas, email him at lang @ unb.ca.


    Signals from global navigation satellite systems are relatively weak and thus vulnerable to deliberate or unintentional interference. An electronically steered antenna array system provides an effective approach to mitigate interference by controlling the reception pattern and steering the system’s beams or nulls. As a result, so-called controlled-reception-pattern-antenna (CRPA) arrays have been deployed by organizations such as the U.S. Department of Defense, which seeks high levels of interference rejection.

    Our efforts have focused on developing a commercially viable CRPA system using commercial off-the-shelf (COTS) components to support the needs of Federal Aviation Administration (FAA) alternative position navigation and timing (APNT) efforts. In 2010, we implemented a seven-element, two-bit-resolution, single-beam and real-time CRPA software receiver. In 2011, the receiver was upgraded to support all-in-view, 16-bit-resolution with four elements.

    Even though we can implement these CRPA software receivers in real time, the performance of anti-interference is highly dependent on the antenna array layout and characteristics of the antenna elements. Our beamforming approach allows us to use several COTS antennas as an array rather than a custom-designed and fully calibrated antenna. The use of COTS antennas is important, as the goal of our effort is to develop a CRPA for commercial endeavors — specifically for robust timing for the national airspace. Hence, it is important to study the geometry layout of the individual antennas of the array to assess the layouts and to determine how antenna performance affects the array’s use.

    In our work, we have developed a procedure for calculating the electrical layouts of an antenna array by differential carrier-phase positioning. When compared to the physical layout, the results of electrical layouts can be used to determine the mutual coupling effect of each combination. Using the electrical layout, the resultant gain patterns can be calculated and used to see the beamwidth and the side-lobe issue. This is important as these factors have significant effects on anti-interference performance. This study focuses on understanding the performance effects of geometry and developing a method for describing the best geometry.

    We adopted three models of COTS antenna and two possible layouts for a four-element array. Then, signal collection hardware consisting of four Universal Software Radio Peripheral (USRP) software-defined radios and one host personal computer was assembled to collect array data sets for each layout/antenna combination. Our developed CRPA software receiver was used to process all data sets and output carrier-phase measurements.

    In this article, we will present the pattern analysis for the two selected layouts and describe how we collected the experimental data. We’ll then show the results of calculating the electrical spacing for the layouts are compare them to the physical layouts. Lastly, we’ll show the resulting patterns, discuss the antenna mutual coupling effects, and give our conclusions.

    Antenna Array Pattern Analysis

    Pattern is defined as the directional strength of a radio-frequency signal viewed from the antenna. The pattern of an antenna array is the product of the isotropic array factor and the isolated element pattern. We assume that the pattern of each element is identical and only consider the isotropic array factor. FIGURE 1 shows the coordination of an antenna array. The first element is set as a reference position. The x-axis is the east direction, the y-axis is the north direction, and the z-axis is the up direction. The baseline vector of the ith antenna is given by I-pi and I-r is the unit vector to the satellite.

    I-Fig1
    Figure 1. Antenna array geometry and direction of satellite. Array elements are identified as E#1, E#2, E#3, and E#4.

    The isotropic array factor is given by

    I-Eq1   (1)

    where λ is wavelength, and Ai is a complex constant. Currently, we only implement a four-element-array CRPA software receiver in real time. Hence, we analyze two kinds of layout of half-wavelength four-element arrays: a symmetrical Y array and a square array. Each antenna is separated from its nearest neighbor by a half wavelength. FIGURE 2 shows photos of the two layouts. FIGURE 3 shows the physical layouts.

    I-Fig2
    Figure 2. Photos of antenna arrays (left: Y array; right: square array).
    I-Fig3top
    Figure 3A. Physical layout of antenna arrays (Y array).
    I-Fig3bottom
    Figure 3B. Physical layout of antenna arrays (square array).

    The antenna patterns towards an elevation angle of 90 degrees, computed using equation 1 and the design layouts, are shown in FIGURE 4. One of the key characteristics of a pattern is the beamwidth, which is defined as the angle with 3-dB loss. FIGURE 5 shows the patterns in elevation angle where the beamwidth of the Y layout is 74 degrees and 86 degrees for the square layout. A narrow beamwidth will benefit anti-interference performance particularly if the interference is close to the direction of a target satellite.

    I-Fig4
    Figure 4. Patterns of antenna arrays (left: Y array; right: square array).
    FIGURE 5 Pattern beamwidths of Y and square arrays (3 dB beamwidth shown).
    Figure 5. Pattern beamwidths of Y and square arrays (3 dB beamwidth shown).
    Specifications of COTS Antennas

    Typically, the COTS antenna selection is determined by high gain and great out-of-band rejection. TABLE 1 shows the specifications of the three antenna models used in this article. These antennas are all patch antennas. The antennas are equipped with surface-acoustic-wave filters for rejecting out-of-band signals. A three-stage low noise amplifier with over 30 dB gain is also embedded in each antenna.

    I-T1
    Table 1. Specifications of COTS antennas used.
    Signal Collection Hardware and Experimental Setup

    The hardware used to collect the antenna array datasets is shown in FIGURE 6 with block-diagram representation in FIGURE 7. The hardware includes a four-element antenna array, four USRP2 software radio systems and one host computer. The signal received from the COTS antenna passes to a USRP2 board equipped with a 800–2300 MHz DBSRX2 programmable mixing and down-conversion daughterboard. The individual USRP2 boards are synchronized by a 10-MHz external common clock generator and a pulse-per-second (PPS) signal. The USRP2s are controlled by the host computer running the Ubuntu distribution of Linux. The open-source GNU Radio software-defined radio block is used to configure USRP2s and collect datasets. All USRP2s are configured to collect the L1 (1575.42 MHz) signal. The signals are converted to near zero intermediate frequency (IF) and digitized to 14-bit complex outputs (I and Q).

    I-Fig7
    Figure 6. Photo of the signal collection hardware.
    I-Fig6
    Figure 7. Block diagram of the signal collection hardware.

    The sampling rate is set as 4 MHz. The host computer uses two solid state drives for storing data sets. For our study, a 64-megabytes per second data transfer rate is needed. The fast solid state drives are especially useful when using high bandwidth signals such as L5, which will require an even higher data streaming rate (80 megabytes per second per channel).

    To compare the physical and electrical layouts of the antenna arrays, we set up the signal collection hardware to record six data sets for the two layouts and the three antenna models as shown in TABLE 2. All of the data sets were five minutes long to obtain enough carrier-phase measurements for positioning.

    I-T2
    Table 2. Experimental setups.
    Logging Carrier-Phase Measurements

    To calculate the precise spacing between the antenna elements, hundreds of seconds of carrier-phase measurements from each element are needed. The collected data sets were provided by our in-house-developed CRPA software receiver. The receiver was developed using Visual Studio under Windows. Most of source code is programmed using C++. Assembly language is used to program the functions with high computational complexity such as correlation operations. The software architecture of the receiver is depicted in FIGURE 8. This architecture exploits four sets of 12 tracking channels in parallel to process each IF signal from an antenna element. Each channel is dedicated to tracking the signal of a single satellite. The tracking channels output carrier-phase measurements to build the steering vectors for each satellite. The Minimum Variance Distortionless Response (MVDR) algorithm was adopted for adaptively calculating the weights for beamforming. Here, there are 12 weight sets, one for each satellite in a tracking channel, for the desired directions of satellites.

    Figure 8. Block diagram of the software architecture.
    Figure 8. Block diagram of the software architecture.

    Using the pre-correlation beamforming approach, the weights are multiplied with IF data and summed over all elements to form 12 composite signals. These signals are then processed by composite tracking channels. Finally, positioning is performed if pseudoranges and navigation messages are obtained from these channels. FIGURE 9 is the graphical user interface (GUI) of the CRPA software receiver. It consists of the channel status of all channels, carrier-phase differences, positioning results, an east-north (EN) plot, a sky plot, a carrier-to-noise-density (C/N0) plot and the gain patterns of the array for each tracked satellite. In the figure, the CRPA software receiver is tracking 10 satellites and its positioning history is shown in the EN plot. The beamforming channels have about 6 dB more gain in C/N0 than the channels of a single element. In each pattern, the direction with highest gain corresponds to the direction of the satellite. While the CRPA software receiver is running, the carrier-phase measurements of all elements and the azimuth and elevation angle of the satellites are logged every 100 milliseconds. Each data set in Table 2 was processed by the software receiver to log the data.

    FIGURE 9 Screenshot of the controlled-reception-pattern-antenna software-receiver graphical user interface.
    Figure 9. Screenshot of the controlled-reception-pattern-antenna software-receiver graphical user interface.
    Electrical Layout of Antenna Array – Procedure

    The procedure of calculating the electrical layout of an antenna array is depicted in FIGURE 10. The single-difference integrated carrier phase (ICP) between the signals of an element, i, and a reference element, j, is represented as:

    I-Eq2   (2)

    where rkij is differential range toward the kth satellite between the ith and jth antenna elements (a function of the baseline vector between the ith and jth elements), δLij is the cable-length difference between the ith and jth antenna elements, Nkij is the integer associated with Φkij , εkij and  is the phase error. The double-difference ICP between the kth satellite and reference satellite l is represented as:
    I-Eq3   (3)

    The cable-length difference term is subtracted in the double difference. Since the distances between the antenna elements are close to one wavelength, equation (3) can be written as:
    I-Eq4   (4)

    where i-rk is the unit vector to satellite k, pij is the baseline vector between the ith and jth elements. By combining all the double-difference measurements of the ijth pair of elements, the observations equation can be represented as:
    I-Eq5      (5)

    From the positioning results of composite channels, the azimuth and elevation angle of satellites are used to manipulate matrix G. To solve equation (5), the LAMBDA method was adopted to give the integer vector N. Then, pij  is solved by substituting N into equation (5). Finally, the cable-length differences are obtained by substituting the solutions of N and pij into equation (2).

    This approach averages the array pattern across all satellite measurements observed during the calibration period.

    FIGURE 10 Procedure for calculating antenna-array electrical spacing.
    Figure 10. Procedure for calculating antenna-array electrical spacing.
    Electrical Layout of Antenna Array – Results

    Using the procedure in the previous section, all electrical layouts of the antenna array were calculated and are shown in FIGURES 11 and 12. We aligned the vectors from element #1 to element #2 for all layouts. TABLE 3 lists the total differences between the physical and electrical layouts. For the same model of antenna, the Y layout has less difference than the square layout. And, in terms of antenna model, antenna #1 has the least difference for both Y and square layouts. We could conclude that the mutual coupling effect of the Y layout is less than that of the square layout, and that antenna #1 has the smallest mutual coupling effect among all three models of antenna for these particular elements and observations utilized.

    FIGURE 11 Results of electrical layout using three models of antenna compared to the physical layout for the Y array.
    Figure 11. Results of electrical layout using three models of antenna compared to the physical layout for the Y array.
    I-Fig12
    Figure 12. Results of electrical layout using three models of antenna compared to physical layout for the square array.
    Table 3. Total differences between physical and electrical layouts.
    Table 3. Total differences between physical and electrical layouts.

    To compare the patterns of all calculated electrical layouts, we selected two specific directions: an elevation angle of 90 degrees and a target satellite, WAAS GEO PRN138, which was available for all data sets. The results are shown in FIGURES 13 and 14, respectively. From Figure 13, the beamwidth of the Y layout is narrower than that of the square layout for all antenna models. When compared to Figure 5, this result confirms the validity of our analysis approach. But, in Figure 14, a strong sidelobe appears at azimuth -60º in the pattern of Y layout for antenna #2. If there is some interference located in this direction, the anti-interference performance of the array will be limited. This is due to a high mutual coupling effect of antenna #2 and only can be seen after calculating the electrical layout.

    I-Fig13
    Figure 13. Patterns of three models of antenna and two layouts toward an elevation angle of 90 degrees.
    I-Fig14
    Figure 14. Patterns of three models of antenna and two layouts toward the WAAS GEO satellite PRN138.
    Conclusions

    The results of our electrical layout experiment show that the Y layout has a smaller difference with respect to the physical layout than the square layout. That implies that the elements of the Y layout have less mutual coupling. For the antenna selection, arrays based on antenna model #1 showed the least difference between electrical and physical layout. And its pattern does not have a high grating lobe in a direction other than to the target satellite.

    The hardware and methods used in this article can serve as a testing tool for any antenna array. Specifically, our methodology, which can be used to collect data, compare physical and electrical layouts, and assess resultant antenna gain patterns, allows us to compare the performances of different options and select the best antenna and layout combination. Results can be used to model mutual coupling and the overall effect of layout and antenna type on array gain pattern and overall CRPA capabilities. This procedure is especially important when using COTS antennas to assemble an antenna array and as we increase the number of antenna elements and the geometry possibilities of the array.

    Acknowledgments

    The authors gratefully acknowledge the work of Dr. Jiwon Seo in building the signal collection hardware. The authors also gratefully acknowledge the Federal Aviation Administration Cooperative Research and Development Agreement 08-G-007 for supporting this research. This article is based on the paper “A Study of Geometry and Commercial Off-The-Shelf (COTS) Antennas for Controlled Reception Pattern Antenna (CRPA) Arrays” presented at ION GNSS 2012, the 25th International Technical Meeting of the Satellite Division of The Institute of Navigation, held in Nashville, Tennessee, September 17–21, 2012.

    Manufacturers

    The antennas used to construct the arrays are Wi-Sys Communications Inc., now PCTEL, Inc. models WS3978 and WS3997 and PCTEL, Inc. model 3978D-HR. The equipment used to collect data sets includes Ettus Research LLC model USRP2 software-defined radios and associated DBSRX2 daughterboards.


    Yu-Hsuan Chen is a postdoctoral scholar in the GNSS Research Laboratory at Stanford University, Stanford, California.

    Sherman Lo is a senior research engineer at the Stanford GNSS Research Laboratory.

    Dennis M. Akos is an associate professor with the Aerospace Engineering Science Department in the University of Colorado at Boulder with visiting appointments at Luleå Technical University, Sweden, and Stanford University.

    David S. De Lorenzo is a principal research engineer at Polaris Wireless, Mountain View, California, and a consulting research associate to the Stanford GNSS Research Laboratory.

    Per Enge is a professor of aeronautics and astronautics at Stanford University, where he is the Kleiner-Perkins Professor in the School of Engineering. He directs the GNSS Research Laboratory.

    FURTHER READING

    • Authors’ Publications

    “A Study of Geometry and Commercial Off-The-Shelf (COTS) Antennas for Controlled Reception Pattern Antenna (CRPA) Arrays” by Y.-H. Chen in Proceedings of ION GNSS 2012, the 25th International Technical Meeting of The Institute of Navigation, Nashville, Tennessee, September 17–21, 2012, pp. 907–914 (ION Student Paper Award winner).

    “A Real-Time Capable Software-Defined Receiver Using GPU for Adaptive Anti-Jam GPS Sensors” by J. Seo, Y.-H. Chen, D.S. De Lorenzo, S. Lo, P. Enge, D. Akos, and J. Lee in Sensors, Vol. 11, No. 9, 2011, pp. 8966–8991, doi: 10.3390/s110908966.

    “Real-Time Software Receiver for GPS Controlled Reception Pattern Array Processing” by Y.-H. Chen, D.S. De Lorenzo, J. Seo, S. Lo, J.-C. Juang, P. Enge, and D.M. Akos in Proceedings of ION GNSS 2010, the 23rd International Technical Meeting of The Institute of Navigation, Portland, Oregon, September 21–24, 2010, pp. 1932–1941.

    “A GNSS Software Receiver Approach for the Processing of Intermittent Data” by Y.-H. Chen and J.-C. Juang in Proceedings of ION GNSS 2007, the 20th International Technical Meeting of The Institute of Navigation, Fort Worth, Texas, September 25–28, 2007, pp. 2772–2777.

    • Controlled-Reception-Pattern Antenna Arrays

    “Anti-Jam Protection by Antenna: Conception, Realization, Evaluation of a Seven-Element GNSS CRPA” by F. Leveau, S. Boucher, E. Goron, and H. Lattard in GPS World, Vol. 24, No. 2, February 2013, pp. 30–33.

    “Development of Robust Safety-of-Life Navigation Receivers” by M.V.T. Heckler, M. Cuntz, A. Konovaltsev, L.A. Greda, A. Dreher, and M. Meurer in IEEE Transactions on Microwave Theory and Techniques, Vol. 59, No. 4, April 2011, pp. 998–1005, doi: 10.1109/TMTT.2010.2103090.

    Phased Array Antennas, 2nd Edition, by R. C. Hansen, published by John Wiley & Sons, Inc., Hoboken, New Jersey, 2009.

    • Antenna Principles

    “Selecting the Right GNSS Antenna” by G. Ryley in GPS World, Vol. 24, No. 2, February 2013, pp. 40–41 (in PDF of 2013 Antenna Survey.)

    GNSS Antennas: An Introduction to Bandwidth, Gain Pattern, Polarization, and All That” by G.J.K. Moernaut and D. Orban in GPS World, Vol. 20, No. 2, February 2009, pp. 42–48.

    A Primer on GPS Antennas” by R.B. Langley in GPS World, Vol. 9, No. 7, July 1998, pp. 50-54.

    • Software-Defined Radios for GNSS

    “A USRP2-based Reconfigurable Multi-constellation Multi-frequency GNSS Software Receiver Front End” by S. Peng and Y. Morton in GPS Solutions, Vol. 17, No. 1, January 2013, pp. 89-102.

    Software GNSS Receiver: An Answer for Precise Positioning Research” by T. Pany, N. Falk, B. Riedl, T. Hartmann, G. Stangl, and C. Stöber in GPS World, Vol. 23, No. 9, September 2012, pp. 60–66.

    Simulating GPS Signals: It Doesn’t Have to Be Expensive” by A. Brown, J. Redd, and M.-A. Hutton in GPS World, Vol. 23, No. 5, May 2012, pp. 44–50.

    Digital Satellite Navigation and Geophysics: A Practical Guide with GNSS Signal Simulator and Receiver Laboratory by I.G. Petrovski and T. Tsujii with foreword by R.B. Langley, published by Cambridge University Press, Cambridge, U.K., 2012.

    “A Real-Time Software Receiver for the GPS and Galileo L1 Signals” by B.M. Ledvina, M.L. Psiaki, T.E. Humphreys, S.P. Powell, and P.M. Kintner, Jr. in Proceedings of ION GNSS 2006, the 19th International Technical Meeting of The Institute of Navigation, Fort Worth, Texas, September 26–29, 2006, pp. 2321–2333.

  • Taoglas Launches GPS/GLONASS Passive Flexible Loop Antenna

    Taoglas_passive_antennaTaoglas USA, Inc., provider of antenna solutions to the M2M and connected device market, has launched the FXP.611 Cloud, a GPS/GLONASS flexible loop antenna that the company says outperforms most active patch antennas with an efficiency of 80 percent and a peak gain of 3 dBi across the GPS and GLONASS bands (1575 to 1610Mhz).

    This antenna can resist external detuning effects due to dual resonance and has a small form factor of 38 x 37 x 0.1 millimeters. At less than half the cost of heavy active patch antennas, this peel and stick, flexible loop antenna is suitable for any GPS/GLONASS M2M device, Taoglas said.

    “We’ve been blown away by the performance of this linear polarized A-GPS GLONASS antenna,” said Dermot O’Shea, director at Taoglas. “Before we developed the FXP.611 Cloud, we had only seen this kind of performance from active patch antennas. We ran a drive test in downtown San Diego and were surprised by the real-time performance and first time to fix from cold-start of this passive loop, particularly in urban canyons where you expect active patches to out perform.”

    Original equipment manufacturers will find the FXP.611 suitable for assisted GPS/GLONASS applications for industrial handheld devices, tablets and smartphones. According to Taoglas, the patent-pending FXP.611 Cloud antenna

    • eliminates the need for a filter or low noise amplifier (LNA), and can connect directly to a module or to a connector on a board.
    • offers a “peel and stick” mounting with 3M tape that can be attached to plastic device housings freeing up board space.
    • costs half the price of active patch antennas.
    • incorporates a detuning design with dual resonance.
    • radiates power uniformly with an omnidirectional design, making it suitable for use in devices that have fixed positions.

    The FXP.611 Cloud antenna is available for purchase immediately from Taoglas by contacting [email protected] and online later in the first quarter of 2013 with Taoglas distributors.

  • Raytheon UK Wins Contract for GPS Anti-Jam System

    Raytheon UK has been awarded a significant contract by the UK Ministry of Defence for delivery of a new GPS anti-jam antenna land system. The contract is for an undisclosed number of advanced systems for deployment in operational theaters spanning multiple vehicle platforms. This UOR (Urgent Operational Requirement) contract is the first award for Raytheon’s GPS Anti-Jam (AJ) Land product family.

    “Raytheon UK has a track record of on-time delivery for GPS AJ systems, having delivered over 7,000 units for air and naval capabilities in the UK and U.S., said Bob Delorge, chief executive, Raytheon UK. “Many of the military platforms used in operations are protected by the proven Raytheon GPS anti-jam technology, and the first order for our Land GPS AJ product family marks a significant success.”

    The contract will see the deployment of the systems under a very short timescale, with final delivery of the capability expected to be completed six months from contract award.

    Raytheon UK is a subsidiary of Raytheon Company. It is a prime contractor and major supplier to the UK Ministry of Defence. Raytheon UK also designs, develops and manufactures a range of high-technology electronic systems and software at facilities in Harlow, Glenrothes, Uxbridge, Waddington and Broughton.

  • u-blox Introduces Small Multi-GNSS Module with Built-in Antenna

    u-blox, the Swiss positioning and wireless module and chip company, announces UC530M, a tiny parallel GPS/GLONASS module with built-in antenna. The antenna module can be embedded in space-restricted environments because of its tiny footprint of 9.6 x 14.0 x 1.95 millimeters. The highly integrated SMT design reduces the need for external components and minimizes manufacturing costs, u-blox said.

    “Location-aware functionality in ever-smaller consumer and industrial devices is a clear market trend. This presents an increasing challenge to OEMs,” said Thomas Nigg, vice president of product marketing at u-blox. “Manufacturers are confronted with the difficult task of providing fast and accurate positioning in compact devices, while time-to-market and price pressure call for minimal R&D effort and low cost. The new UC530M is built to address these requirements: a complete low-power, high performance multi-GNSS receiver with integrated antenna. The module is easy to integrate in a wide variety of devices cost-effectively.”

    With high sensitivity, -165 dBm in tracking, and very low power consumption, typically only 66 mW average power consumption, the UC530M can be directly connected to a lithium battery, eliminating costly voltage regulators. Advanced low-power modes are also supported along with three days self-assistance support. Additional functionality includes a logger function which stores location information in internal memory. With a typical log interval of 15 seconds, log capacity can be up to 16 hours.

    The integrated antenna of the UC530M exhibits significantly better radiation efficiency than small patch antennas, and performs well against larger and heavier patch antennas. Its circular radiation pattern brings flexibility to hardware designs, u-blox said. The optional connectivity to an external antenna extends the applicability of the module to a wider range of devices from handheld computers to asset tracking systems. The module is drop-in compatible with the UC530 GPS antenna module announced in June 2012.

    Engineering samples of the UC530M modules are available in December 2012.

  • Topcon’s MG-A8 Antenna Designed for Accurate Maritime Applications

    Topcon Positioning Systems announces the MG-A8 antenna for navigation and precise positioning in marine applications. According to Topcon, the new MG-A8 marine antenna provides exemplary GNSS signal tracking while not being susceptible to signal jamming from other sources, such as Inmarsat communications.

    The MG-A8 antenna can be used in DGPS mode for meter-level navigation purposes but can also be used for RTK centimeter level positioning in areas where there is a network of reference stations available to support this level of precision. With its RTK capabilities, the MG-A8 is a “preferred solution for applications such as dredging in inland river channels and waterways,” said Tom Morris, TPS senior product development manager.

    “This antenna is designed with challenging marine applications in mind.  It is accurate, rugged, reliable and affordable.”