The present invention relates to methods of information processing in satellite navigation systems with differential positioning of a mobile user.
Satellite navigation systems, such as GPS (USA) and GLONASS (Russia), are intended for high accuracy self-positioning of different users possessing special navigation receivers. A navigation receiver receives and processes radio signals broadcasted by satellites located within line-of-sight distance. The satellite signals comprise carrier signals that are modulated by pseudo-random binary codes, which are then used to measure the delay relative to local reference clock or oscillator. These measurements enable one to determine the so-called pseudo-ranges (γ) between the receiver and the satellites. The pseudo-ranges are different from true ranges (D, distances) between the receiver and the satellites due to variations in the time scales of the satellites and receiver and various noise sources. To produce these time scales, each satellite has its own on-board atomic clock, and the receiver has its own on-board clock, which usually comprises a quartz crystal. If the number of satellites is large enough (more than four), then the measured pseudo-ranges can be processed to determine the user location (e.g., X, Y, and Z coordinates) and to reconcile the variations in the time scales. Finding the user location by this process is often referred to as solving a navigational problem or task.
The necessity to guarantee the solution of navigational tasks with accuracy better than 10 meters, and the desire to raise the stability and reliability of measurements, have led to the development of the mode of “differential navigation ranging,” also called “differential navigation” (DN). In the DN mode, the task of finding the user position is performed relative to a Base station (Base), the coordinates of which are known with the high accuracy and precision. The Base station has a navigation receiver that receives the signals of the satellites and processes them to generate measurements. The results of these measurements enable one to calculate corrections, which are then transmitted to the user that also uses a navigation receiver. By using these corrections, the user obtains the ability to compensate for the major part of the strongly correlated errors in the measured pseudo-ranges, and to substantially improve the accuracy of his or her positioning.
Usually, the Base station is immobile during measurements. The user may be either immobile or mobile. We will call such a user “the Rover.” The location coordinates of a moving Rover are continuously changing, and should be referenced to a time scale.
Depending on the navigational tasks to be solved, different modes of operation may be used in the DN mode. They differ in the way in which the measurement results are transmitted from the Base to the Rover. In the Post-processing (PP) mode, these results are transmitted as digital recordings and go to the user after all the measurements have been finished. In the PP mode, the user reconstructs his or her location for definite time moments in the past.
Another mode is the Real-Time Processing (RTP) mode, and it provides for the positioning of the Rover receiver just during the measurements. The RTP mode uses a communication link (usually it is a radio communication link), through which all the necessary information is transmitted from the Base to the Rover receiver in digital form.
Further improvement of accuracy of differential navigation may be reached by supplementing the measurements of the pseudoranges with the measurements of the phases of the satellite carrier signals. If one measures the carrier phase of the signal received from a satellite in the Base receiver and compares it with the carrier phase of the same satellite measured in the Rover receiver, one can obtain measurement accuracy to within several percent of the carrier's wavelength, i.e., to within several centimeters.
The practical implementation of those advantages, which might be guaranteed by the measurement of the carrier phases, runs into the problem of there being ambiguities in the phase measurements.
The ambiguities are caused by two factors. First, the difference of distances ΔD from any satellite to the Base and Rover is much greater than the carrier's wavelength λ. Therefore, the difference in the phase delays of a carrier signal Δφ=ΔD/λ received by the Base and Rover receivers exceeds several cycles. Second, it is not possible to measure the integer number of cycles in Δφ from the incoming satellite signals; one can only measure the fractional part of Δφ. Therefore, it is necessary to determine the integer part of Δφ, which is called the “ambiguity”.
More precisely, we need to determine the set of all such integer parts for all the satellites being tracked, one integer part for each satellite. One has to determine this set along with other unknown values, which include the Rover's coordinates and the variations in the time scales.
In a general way, the task of generating highly-accurate navigation measurements is formulated as follows: one determines the state vector of a system, with the vector containing nΣ unknown components. Those include three Rover coordinates (usually along Cartesian axes X, Y, Z) in a given coordinate system (sometimes time derivatives of coordinates are added too); the variations of the time scales which is caused by the phase drift of the local main reference oscillator; and n integer unknown values associated with the ambiguities of the phase measurements of the carrier frequencies. The value of n is determined by the number of different carrier signals being processed, and accordingly coincides with the number of satellite channels actively functioning in the receiver. At least one satellite channel is used for each satellite whose broadcast signals are being received and processed by the receiver. Some satellites broadcast more than one code-modulated carrier signal, such as a GPS satellite that broadcasts a carrier in the L1 frequency band and a carrier in the L2 frequency band. If the receiver processes the carrier signals in both of the L1 and L2 bands, the number of satellite channels (n) increases correspondingly.
Two sets of navigation parameters are measured by the Base and Rover receivers, respectively, and are used to determine the unknown state vector. Each set of parameters includes the pseudo-range of each satellite to the receiver, and the full (complete) phase of each satellite carrier signal, the latter of which may contain ambiguities. Each pseudo-range is obtained by measuring the time delay of a code modulation signal of the corresponding satellite. The code modulation signal is tracked by a delay-lock loop (DLL) circuit in each satellite-tracking channel. The full phase of a satellite's carrier signal is tracked by phase counter (as described below) with input from a phase-lock-loop (PLL) in the corresponding satellite tracking channel (an example of which is described below in greater detail). An observation vector is generated as the collection of the measured navigation parameters for specific (definite) moments of time.
The relationship between the state vector and the observation vector is defined by a well-known system of navigation equations. Given an observation vector, the system of equations may be solved to find the state vector if the number of equations equals or exceeds the number of unknowns in the state vector. In the latter case, conventional statistical methods are used to solve the system: the least-squares method, the method of dynamic Kalman filtering, and various modifications of these methods.
Practical implementations of these methods in digital form may vary widely. In implementing or developing such a method on a processor, one usually must find a compromise between the accuracy of the results and speed of obtaining results for a given amount of processor capability, while not exceeding a certain amount of loading on the processor. The present invention is directed to novel methods and apparatuses for accelerating the obtaining of reliable estimates for the integer ambiguities at an acceptable processor load.
More particularly, the present invention is directed to novel methods and apparatuses for more quickly obtaining such estimates in floating-point form (non-integer form) which are close to the integer values. With these floating-point forms, which we call floating ambiguities, conventional methods may be used to derive the corresponding integer ambiguities.
Broadly stated, the present invention encompasses methods and apparatuses for estimating the floating ambiguities associated with the measurement of the carrier signals of a plurality of global positioning satellites, such that the floating ambiguities are preferably consist for a plurality of different time moments.
The floating ambiguities are associated with a set of phase measurements of a plurality n of satellite carrier signals made by a first navigation receiver (B) and a second navigation receiver (R) separated by a distance, wherein a baseline vector (xo,yo,zo) relates the position of the second receiver to the first receiver. Each satellite carrier signal is transmitted by a satellite and has a wavelength, and each receiver has a time clock for referencing its measurements. Any difference between the time clocks may be represented by an offset. Methods and apparatuses according to the present invention receive, for a plurality of two or more time moments j, the following inputs: a vector γjB representative of a plurality of pseudo-ranges measured by the first navigation receiver (B) and corresponding to the plurality of satellite carrier signals, a vector γjR representative of a plurality of pseudo-ranges measured by the second navigation receiver (R) and corresponding to the plurality of satellite carrier signals, a vector DjB representative of a plurality of estimated distances between the satellites and the first navigation receiver (B), a vector DJR representative of a plurality of estimated distances between the satellites and the second navigation receiver (R), a vector φjB representative of a plurality of full phase measurements of the satellite carrier signals measured by the first navigation receiver (B), a vector φjR representative of a plurality of full phase measurements of the satellite carrier signals measured by the second navigation receiver (R), and a geometric Jacobian matrix Hjγ whose matrix elements are representative of the changes in the distances between the satellites and one of the receivers that would be caused by changes in that receiver's position and time clock offset. (As used herein, the term “representative of,” as used for example used when indicating that a first entity is representative of a second entity, includes cases where the first entity is equal to the second entity, where the first entity is proportional to the second entity, and where the first entity is otherwise related to the second entity.)
The present invention may be practiced in real time, where estimates of the floating ambiguities are generated as the above satellite information is being received. The present invention may also be practiced in post-processing mode, where the floating ambiguities are estimated after all the above satellite information has been received. In the latter case, block processing according to the present invention may be done.
Preferred methods and apparatuses according to the present invention generate, for each time moment j, a vector Δγj of a plurality of range residuals of pseudo-range measurements made by the first and second navigation receivers in the form of:
Δγj=(γjR−γjB)−(DjR−DjB;
and also generate, for each time moment j, a vector Δφj of a plurality of phase residuals of full phase measurements made by the first and second navigation receivers in the form of: Δφj=(φjR−φjB)−Λ−1·(DjR−DjB),
where Λ−1 is a diagonal matrix comprising the inverse wavelengths of the satellites. In the case of real-time processing, an LU-factorization of a matrix M1, or a matrix inverse of matrix M1, is generated for a first time moment (denoted as j=1), with the matrix M1 being a function of at least Λ−1 and H1γ. Also for this initial time moment, an initial vector N1 of floating ambiguities is generated as a function of at least Δγ1, Δφ1, and the LU-factorization of matrix M1 or the matrix inverse of matrix M1. For an additional time moment j, an LU-factorization of a matrix Mj, or a matrix inverse of matrix Mj, is generated, with the matrix Mj being a function of at least Λ−1 and Hjγ. Also for an additional time moment j, a vector Nj of estimated floating ambiguities is generated as a function of at least Δγj, Δφj, and the LU-factorization or matrix Mj or the matrix inverse of matrix Mj. Exemplary forms of matrices Mj and vectors Nj are provided below. In this manner, a set of successively more accurate estimates of the floating ambiguities are generated in real-time with the vectors Nj. This method, of course, may also be practiced in a post-processing environment, where the data has been previously recorded and then processed according to the above steps.
In the post-processing environment, the following block processing approach according to the present invention may be practiced. As with above-described embodiments for real-time processing, the vectors of pseudo-range residuals Δγk and vectors of phase residuals Δφk, k=1, . . . j, are generated. Thereafter, a general matrix M is generated from the data, with M being a function of at least Λ−1 and Hkγ, for index k of Hkγ covering at least two of the time moments j, and an LU-factorization of matrix M or a matrix inverse of matrix M is generated. Thereafter, a vector N of estimated floating ambiguities is generated as a function of at least the set of range residuals Δγk, the set of phase residuals Δφk, and the LU-factorization of matrix M or the matrix inverse of matrix M.
As an advantage of the present invention, the nature of matrix M, as described in greater detail below, enables a compact way of accumulating the measured data in order to resolve the floating ambiguities. As a further advantage, forms of matrix M provide a stable manner of factorizing the matrix using previous information. In preferred embodiments, matrix M is substantially positive definite, and also preferably symmetric.
Accordingly, it is an objective of the present invention to improve the stability of generating estimates of the floating ambiguities, and a further objective to reduce the amount of computations required to generate estimates of the floating ambiguities.
This and other advantages and objectives of the present invention will become apparent to those of ordinary skill in the art in view of the following description.
Nomenclature
All vectors presented herein are in column form. The transpose of a vector or matrix is indicated by the conventional superscript “T” affixed to the end of the name of the vector or matrix. The inverse of a matrix is indicated by the conventional superscript “−” affixed to the end of the name of the matrix. For the convenience of the reader, we provide a summary notation symbols below:
Before describing the present invention, we briefly describe the structure of the satellite signals and of a typical receiver suitable for differential navigation applications. Each of the satellites radiates signals in two frequency bands: the L1 band and the L2 band. Two carrier signals are simultaneously transmitted in the L1-band; both carrier signals have the same frequency, but are shifted in phase by π/2 (90°). The first L1 carrier signal is modulated by the clear acquisition C/A-code signal and the second L1 carrier signal is modulated by the precision P-code signal. One carrier signal is transmitted in the L2 band, and uses a different frequency than the L1 carrier signals. The L2 carrier signal is modulated by the same P-code signal used to modulate the second L1 carrier signal. These carrier frequencies are between 1 GHz and 2 GHz in value. Each C/A-code signal and P-code signal comprises a repeating sequence of segments, or “chips”, where each chip is of a predetermined time period (Δ) and has a pre-selected value, which is either +1 or −1. The segment values follow a pseudo-random pattern, and thus the C/A-codes and the P-codes are called pseudo-random code signals, or PR-code signals. Additionally, before each C/A-code signal and P-code signal is modulated onto its respective carrier signal, each code signal is modulated by a low frequency (50 Hz) information signal (so-called information symbols).
The approximate distance between a satellite and a receiver is equal to the speed of light c multiplied by the transmission time it takes the satellite signal to reach the receiver. This approximate distance is called the pseudorange γ, and it can be corrected for certain errors to find a corrected distance D between the satellite and the receiver. There is a pseudorage between each visible satellite and the receiver. The transmission time from satellite to receiver is measured with the aid of clocks in the receiver and the satellite, and with the aid of several time scales (i.e., timing marks) present within the received satellite signal. The clocks in the satellites and the receiver are set to substantially the same time, but it is assumed that the receiver clock has a time offset τ because the receiver clock is based upon a quartz-crystal whereas each satellite clock is based upon a more accurate atomic reference clock. The receiver has the orbital patterns of the satellites stored in a memory, and it can determine the orbital position of the satellites based on the time of its clock. The receiver reads the timing marks on the satellite's signal, and compares them against it own clock to determine the transmission time from satellite to receiver. The satellite's low-frequency (50 Hz) information signal provides the least precise timing information, the C/A-code signal provides the next most precise timing information, and the P-code signal provides the most precise timing information. The pseudorange is determined from the low-frequency information signal and the C/A-code signal for civilian users and some military users, and is determined from the low-frequency information signal and the P-code signal for most military users. Accurate use of the P-code signal requires knowledge of a certain code signal that is only known to military users. Precision better than that provided by the P-code signal can be obtained by measuring the phase of the satellite carrier signal in a differential navigation mode using two receivers.
Referring to
Referring to
In a similar manner, the PLL has a reference carrier generator that generates a reference carrier signal that tracks the down-converter version of the satellite's carrier signal. We denote the frequency of the reference carrier signal as fNCO since the reference carrier frequency is often generated by a numerically-controlled oscillator (NCO) within the reference carrier generator. Referring to
Finally, each individual tracking channel usually comprises a search system which initially varies the reference signals to bring the PLL and DLL circuits into lock mode. The construction of this and the other above components is well known to the art, and a further detailed description thereof is not needed in order for one of ordinary skill in the art to make and use the present invention.
Brief Background on the Navigation Parameters.
Because of the time offset τ and other error effects, the pseudorange γ between a satellite and a receiver is usually not the actual distance between the satellite and the receiver. By looking at the pseudoranges of four or more satellites, there are well-known methods of estimating the time offset τ of the receiver and of accounting for some of the error effects to generate the computed distance D between the satellites and the receiver. The receiver's position may then be computed. However, because of various sources of noise and the relatively low resolution of the pseudo-random code signal, the true distances (i.e., true ranges), and receiver's position coordinates will not be exactly known, and will have errors.
In theory, more precise values for the receiver's position and clock offset could be obtained by measuring the number of carrier cycles that occur between each satellite and the receiver. The phase of the carrier of the satellite signal as transmitted by a satellite can be expressed as:
where Φ0S is an initial phase value, fS is the satellite carrier frequency, and t is the satellite's time. Because the satellite carrier frequency is generated from a very precise time base, we may assume that fS is a constant and not time dependent, and we may replace the above integral with fS·t, as we have shown in the second line in the above equation. The phase of this signal when it reaches the receiver's antenna over the range distance D(t) is denoted as φSA(t), and its value would be:
where c is the speed of light, and where τATM(t) is a delay due to anomalous atmospheric effects which occur mostly in the upper atmosphere. The number of cycles fS·τATM(t) due to the atmospheric effects cannot be predicted or determined to within an accuracy of one carrier cycle by a stand-alone receiver (i.e., cannot be determined by absolute positioning). However, the atmospheric effect can be substantially eliminated in a differential GPS mode where the phase of the satellite is measured at a rover station and a base station, ΦSA,R(t) and ΦSA,B(t) respectively, and then subtracted from one another. Over the short baseline between the rover and base stations, the atmospheric delay τATM(t) in both of these phases is equal for practical purposes, and the difference in phases is:
φSA,R(t)−φSA,B(t)=fS·DR(t)/c−fS·DB(t)/c. (4)
The terms Φ0S and fS·t have also been cancelled from the difference. In
However, the task of measuring carrier phase is not as easy as it appears. In practice, we must use non-ideal receivers to measure the phases φSA,R(t) and φSA,B(t), with each receiver having a different clock offset with respect to the GPS time, and with each receiver having phase errors occurring during the measurement process. In addition, at the present time, it is not practical to individually count the carrier cycles as they are received by the receiver's antenna since the frequency of the carrier signal is over 1 GHz. However, the PLL loop can easily track the Doppler-shift frequency fD of the carrier signal, which is in the kHz range. With a few assumptions, the phases φSA,R(t) and φSA,B(t) can be related to their respective Doppler-shift frequencies. As is known in the art, the satellite transmits at a fixed frequency of fS, but the relative motion between the satellite and receiver causes the frequency seen by the receiver to be slightly shifted from the value of fS by the Doppler frequency fD. We may write the frequency seen by the receiver's antenna as fS+fD, where fD has a positive value when the distance between the satellite and receiver's antenna is shrinking, and a negative value when the distance is increasing. Each receiver can then assume that the received phase is proportional to the predictable amount of fS·t, minus the amount fD·t due to the Doppler-shift. The Doppler amount fD·t is subtracted from fS·t because the Doppler frequency increases as the distance between the satellite and receiver's antenna decreases. The predictable amount fS·t will be the same for each receiver, but the Doppler frequencies will usually be different.
As previously mentioned with reference to
φj(Ti)=fp,nom·(Tj−Tp)−φjNCO(Tj) (5)
where fp,nom is the nominal value of the pedestal frequency, and where φjNCO(Tj) is the phase (integrated frequency) of the PLL's reference oscillator (e.g., NCO). The time moments Tj are spaced apart from each other by a time interval ΔTj, as measured by the receiver's clock, and may be express as Tj=j·ΔTj, where j is an integer. φj(Tj) is in units of cycles, and is proportional to the negative of the integrated Doppler-shift frequency. This is because φjNCO(Tj) changes value in proportional to the quantity (fp+fD)·(Tj−Tp).
While it may be possible to set φjNCO(Tp) to any value at the initial lock moment Tp, it is preferably to set φjNCO(Tp) to a value substantially equal to (fp,nom·Tp−fS·{tilde over (D)}p/c), where Tp is measured from the start of GPS time, and where {tilde over (D)}P is the approximate distance between the satellite and the receiver, as found by the pseudorange measured by the DLL, or as found by a single point positioning solution. This setting of φjNCO(Tp) is conventional and provides values of φj(Tj) for the base and rover stations which are referenced from the same starting time point.
In U.S. Pat. No. 6,268,824, which is commonly assigned with the present application, it is shown how the observable φj(Tj) is related to the distance D between the receiver and the satellite. We summarize the relationship here, neglecting the atmospheric delay τATM(tj) since this delay will be canceled out when we take the difference between receivers, and refer the reader to the patent for the derivation:
φj(Tj)=fS·Dj/c+fS·(τj−Tp)+(φ′0−Φ0S)−Nnco−ζφj (6)
where
We will now write equation (7) for the base and rover stations, adding superscripts “B” and “R” for the base and rover stations, and subscript “m” to indicate the m-th satellite signal and the m-th individual tracking channel.
φj,mB(Tj)=fS·Dj,mB/c+fS·τjB+(φ′0R−Φ0S)+NmB−ζφj,mB (8A)
φj,mR(Tj)=fS·Dj,mR/c+fS·τjR+(φ′0R−Φ0S)+NmR−ζφj,mR (8B)
For the differential navigation mode, the difference of these phases is formed:
Using Nm=(NmB−NmR) to represent the difference between the ambiguities, and using the well-known relationship fS/c=1/λm, where λm is the wavelength of the satellite carrier signal, we have:
The values for φ′0B and φ′0R can be readily determined. The values of ζφj,mB and ζφj,mR cannot be determined, but they have zero mean values (and should average to zero over time).
Now, we relate this back to the initial objective and problem that we expressed with respect to
Our Inventions Related to Ambiguity Resolution—Estimating Floating Ambiguities
Our inventions can be applied to a number of application areas. In general application areas, the rover and base stations can move with respect to one another. In one set of specific application areas, the base and rover stations are fixed to a body or vehicle (e.g., planes and ships) and separated by a fixed distance L, as shown in
((xR−xB)2+(yR−yB)2+(zR−zB)2)1/2=LRB (11)
where xR, yR, and zR, represent the rover station coordinates and where xB, yB, and zB represent the base station coordinates. The information from the constraint can be used to better estimate the Rover position relative to the Base. For this, it is preferably to form a cost penalty function mathematically equivalent to the form:
where, in preferred embodiments, the cost function F(*) will be minimized such that and its the first derivatives with respect to the rover coordinates (or alternatively the base coordinates) are reduced to values near zero:
In the preferred methods described below, the amount of weighting given to minimizing the cost function F(*) will set by a weighting parameter q (e.g., q·F(*)), with no weighting being given when q=0, and increasing degrees of weighting being given by selecting q>0. The case of setting q=0 is also equivalent to removing the constraint that the rover and base stations are separated by a fixed distance L.
The ambiguity resolution task generally comprises the following three main parts:
According to the input data, a vector of observations and a covariance matrix of measurements are formed. After that a state vector is generated, components of which are floating ambiguities, the number of which is equal to the number of satellites. On the basis of the floating ambiguity values, a search of the integer ambiguities is performed with use of a least-squares method that is modified for integer estimations.
Improvement of the floating ambiguity estimations can take place step-by-step, and the probability of correct ambiguity resolution increases step-by-step as information is accumulated. Preferred finishing of this process is registered by appearance of the signal of integer ambiguities resolution, which indicates that ambiguity resolution was performed sufficiently safely. After that, the integer ambiguities together with other input data are used for accurate determination of the base line vector. The tasks of determining the integer ambiguities and of generating the signal of integer ambiguities resolution are known to the art and do not form part of our invention. These tasks, therefore, are not described in greater detail.
Our invention is suitable for both the RTP mode and for the PP mode under movable Rover, where the Rover coordinates may be random and independent in adjacent clock moments. Our invention is also suitable for both the RTP mode and for the PP mode when both the base and rover stations are moving, where the coordinates of the stations may be random, but constrained by fixed distance LRB, in adjacent clock moments.
We start by rewriting equation (10), which has the integer ambiguities Nm in vector form:
where Λ1 is a diagonal matrix of inverse wavelengths. We note that the components of (φ′0B−φ′0R) can be selected to be integer constants, and can therefore be incorporated into the integer ambiguities N, which may be called the modified integer ambiguities N. Thus, we may simplify the above equation:
φjB(Tj)−φjR(Tj)=Λ−1·(DjB−DjR)+fS·(τjB−τjR)+N−(ζφjB−ζφjR) (14)
After this modified N are found, the “true” N may be found by subtracting (φ′0B−φ′0R) from the modified N.
As an alternative equivalent to the above, the vector (φ′0B−φ′0R) can be computed and carried over to the left-hand side of equation (14) and subtracted from (φjB(Ti)−φjR(Ti)). As such, the N that is determined will be the “true” N. Once the “true” N is found, then the underlying unknown integer number of carrier cycles Nnco may be found by negating the “true” N (i.e., multipling by −1) and then subtracting fS·Tp (Nnco=−“true” N−fS·Tp). However, for the ultimate goal of computing more accurate coordinates of the baseline, the modified ambiguities N in equation (14) can be used, and they greatly simplify the computations. Nonetheless, it will be appreciated that the present invention may be practiced by using the “true” N or Nnco in equation (14) by suitable modification of the left-hand side of equation (14), and that the appended claims cover such practices.
Our approach comprises solving the above equations (14) at a plurality of time moments jointly to find an estimation for vector N. We cannot readily find measured values for vectors τjB, τjR, ζφjB, and ζφjR, and we have some errors in the range vectors DjB nd DjR. Our approach is to represent (model) the errors in the range vectors DjB and DjR and the terms fS·(τjB−τjR)−(ζφjB−ζφjR) by the following error vector: Λ−1·Hjγ·[Δx, Δy, Δz, c·Δτ]T, where Hjγ is the Jacobian matrix (e.g., directional cosine matrix), and where [Δx, Δy, Δz, c·Δτ]T are corrections to the baseline coordinates and clock offsets of the receivers. Thus, we will model the above equation as:
(φjR−φjB)−Λ−1·(DjR−DjB)=N+Λ−1·Hjγ·[Δx, Δy, Δz, c·Δτ]T (15)
The pseudoranges will be used to estimate the vector Hjγ·[Δx, Δy, Δz, c·Δτ]T as follows:
(γjR−γjB)−(DjR−DjB)=Hjγ·[Δx, Δy, Δz, c·Δτ]T (16)
This will be done through the formation of observation vectors, state vectors, and observation matrices, and an estimation process over a plurality of time moments, as described below in greater detail. Vector N will be jointly estimated in this process.
Generation of the Vector of Observations.
A vector of observations μj is generated at each clock time moment μj=j·ΔTJ and comprises 2·n components, where n is the number of the satellite channels. The first n components are the residuals of the single differences of the Base and Rover pseudo-ranges, which we denote in vector form as Δγj:
Δγj=γj−Dj (17)
The forms represented by Equations (15)-(18) maybe represented in matrix form equivalent to:
μj=Hjμ·Aj, (19)
where vector Aj is a state vector related to observation matrix μj, and where matrix Hjμ is an observation matrix that specifies the relationship between the components of the observations vector μj and the state vector Aj. State vector vector Aj comprises (4+n) components. The first three components are increments (Δx, Δy, Δz) to the coordinates (xo, yo, zo) of the baseline vector unknown at the j-th clock moment, the fourth component is the unknown increment of the reference oscillator phases (c·Δτ). The remaining n components are the unknown floating ambiguities, different in different channels (N1, N2 . . . Nn). Matrix Hjμ comprises 2n rows and (4+n) columns, and may be divided into the following 4 parts (sub-matrices):
The first part, the left upper corner of this matrix (the first four columns by the first n rows), is occupied by the observation matrix Hjγ relating to the pseudo-range measurements, each row corresponding to one channel (from the 1-st to the n-th). For the n-th channel, the corresponding row appears like this:
[αjn, βjn, hjn, 1],
where αjn, βjn, hjn—the directional cosines of the range vector to the n-th satellite from Rover for the j-th time moment. Methods of computing directional cosines are well known to the art and a description thereof herein is not needed for one of ordinary skill in the art to make and use the present invention.
The second part of matrix Hjμ, the left lower corner (the first four columns by the last n rows), is occupied by the matrix product Λ−1·Hjγ relating to the full phase measurements, each row corresponding to one channel (from the 1-st to the n-th). For the n-th channel, the corresponding row appears like this:
[αjn/λn, βjn/λn, hjn/λn, 1/λn],
where λn is the wavelength of the carrier signal in the n-th channel.
The third part of matrix Hjμ, the right upper corner (the last n columns by the first n rows) is occupied by zeroes. And the fourth part, the right lower corner (the last n rows by the last n columns) is occupied by the elements relating to the floating ambiguities. This part represents the identity matrix In with dimensions of n×n. For the discussion that follows below, it will be convenient to identified sub-blocks of matrix Hjμ as follows Hjμ=[Qj|G], where Qj is a compound matrix formed by Hjγ and Λ as follows:
and where G is a compound matrix the zero matrix On×n and the identity matrix In as follows:
Equation (18) has 2n equations (according to the number of components of the observation vector), and may be used to determine the state vector Aj at the j-th clock moment (i.e., to determine 4+n unknown values). Solution of such a system of equations at n≧4 may be performed by the method of least squares. However, our invention relates to solving for the ambiguity vector N, which is a component of Aj, over a plurality of time moments. Before we describe that process, however, we want to first describe the groundwork of how we can integrate the minimization of the cost function F(*) for constrained distance between receivers, if used, with the solution of Equation (19), and to then describe some covariance matrices that characterize the accuracy of the measured data used to generate μj. These covariance matrices are helpful to our invention, but not strictly necessary.
The cost function F(*) may be expressed in the following form:
where:
with a zero as the four vector component. Using a second-order truncation of the Taylor series expansion, the cost function F(*) may be approximated as:
where
Because forms (21)-(23) share common variables with equation (18), the minimization of q·F(*) can be integrated with the solution of equation (18), as described below in greater detail.
Generation of the Measurements Covariance Matrix.
Measurements covariance matrix RJ is preferably formed in the following way on the basis of weight coefficients obtained in Base and Rover receivers:
The weight coefficients (Kj1γ, Kj2γ, . . . , Kjnγ) characterize the accuracy of the measurements of the residuals Δγj of the pseudo-range single differences for the corresponding satellite channels (1-st, 2-nd, . . . , n-th). The generation of the weight coefficients is not a critical part of the present invention, and one may use his particular method of weighting. We present here one of our ways, where each of these coefficients may be determined according to the weight coefficients measured in each channel by Base and Rover receivers for the pseudo-ranges, i.e., by values KjγB and KjγR.
Thus, for example, for the n-th channel:
(Kjnγ)−1=(KjnγB)−1+(KjnγR)−1,
where KjγB and KjγR are determined taking into account the measured signal-to-noise ratio in the receivers and the satellite elevation angles in the n-th channel (of Base and Rover, respectively). Specifically, for each of the receivers (no superscript used),
Kj,mγ=Zk,m2·sin(ξk,m−ξmin)·σγ2 when ξk,m>ξmin, and
Kj,mγ=0 when ξk,m≦ξmin,
where Zk,m2 is the signal strength of the m-th satellite carrier signal as received by the receiver (it has been normalized to a maximum value and made dimensionless), where ξk,m is the elevation angle of the m-th satellite as seen by the receiver, where a minimum elevation angle ξBmin at which the signal becomes visible at the receiver, where σγ2 is the variance of the code measurements (σγ≈1 m). The factor Zk,m2·sin(ξk,m−ξmin) is dimensionless.
Weight coefficients Kj1φ, Kj2φ, . . . , Kjnφ characterize the accuracy of the measurements of the residuals Δφj of the phase single differences, and are determined similarly. Here the same input data is used: the signal-to-noise ratio and the angle of elevation, but another scale for the phase measurements is considered (e.g., σφ2 instead of σγ2). Specifically, for each of the receivers (no superscript used),
Kj,mφ=Zk,m2·sin(ξk,m−ξmin)·σφ2 when ξk,m>ξmin, and
Kj,mφ=0 when ξk,m≦ξmin,
where Zk,m2, ξk,m and ξBmin are as they are above, and where σφ2 is the variance of the code measurements (σφ≈1 mm).
When the magnitudes of either of weight coefficients Kj,mγB or Kj,mγR is less than a first selected small threshold value, the value of Kj,mγ is generated as a first small number which is less than the first threshold value. This is equivalent to setting (Kj,mγ)−1 to a large number equal to the inverse of the first small number. Similarly, when the magnitudes of either of weight coefficients Kj,mφB or Kj,mφR is less than a second selected small threshold value, the value of Kj,mφ is generated as a second small number which is less than the second threshold value. This is equivalent to setting (Kj,mφ)−1 to a large number equal to the inverse of the second small number.
In some instances, satellite signals are blocked from view and should be excluded from the ambiguity resolution process. The elements of the covariance matrix Rj corresponding to these satellite signals are replaced by a very large number. The very large number is selected in advance, and has a value which exceeds by several orders of magnitude the nominal values of the covariance matrix components (Kjγ)−1 or (Kjφ)−1 encountered during operation. Consequently, in further computations, the weights of all measurements relating to these channels become so small that they do not influence the result.
As a more simple approach, but currently less preferred, one can use the following form of covariance matrix Rj, or a scaled version thereof:
This form gives an equal weighting of 1/σγ2 of to the rows of pseudorange data provided by Δγj, and an equal weighting of 1/σφ2 to the rows of phase data provided by Δφj. When a satellite is blocked from view or not visible, the elements of the covariance matrix Rj corresponding to the satellite are preferably replaced by a very large number, as described above.
Central Aspects of the Present Invention
Summarizing equation (19), the linearized measurement model at the j-th epoch takes the form:
We expect that the vector of floating ambiguities Nj will be constant in time, and therefore we will drop the subscript index j. Instead, we will denote Nj the evaluation of N obtained through the epoch from 1 to j.
Generation of the Floating Ambiguity Estimations
We create the following scalar quantity J in equation (27) which integrates the minimization of equation (26) with the minimization of the truncated cost functions Fk for the constrained distance condition (if used) according to equations (21)-(23):
As mentioned above, q is a scalar weighting factor (penalty parameter) which is equal to or greater than 0 (q≧0). We seek to minimize J in value in order to obtain ak, k=1, . . . , j and N. The minimization of scalar J essentially seeks to minimize the errors in the individual forms of ∥Hkμ·Ak−μk∥2 and conditions (11), if applicable, for data of all of the j epochs being considered, but with the constraint that floating ambiguity vector N in each individual state vector Ak be the same. The individual vectors ak are allowed to have different values. If the fixed distance constraint between rover and base stations is not considered to be present, then cost function Fk is omitted from equation (27), and all following equations based on equation (27). This may be simply done by setting weighting parameter q=0. If the fixed distance constraint is used, values for the weighting parameter q can range from approximately 0.5 to approximately 4, with a typical range being between approximately 1 and approximately 3. The best value of q often depends upon the amount of noise in the signals and the receivers, and can be found by trying several values within the above ranges (i.e., fine tuning). The inventors have found a value of q=2 to be useful for their test applications. In the case where the distance between the receivers is constrained to a fixed value, we emphasize that the use of the cost function qF is optional, and that one is not required to use it. Using the methods of the present invention without the cost function qF will still provide estimates of the floating ambiguities. The inclusion of the cost function qF generally enables more accurate estimates.
The inventors have discovered that a set of N which minimizes scalar J can be found by solving the following block linear system for the set N, which is a vector.
To the inventors' knowledge, the form of scalar J provide by equation (27) and form of the linear system provided by equation (28) are not found in the prior art. While it is preferred to use the weighting matrices R and their inverse matrices, it may be appreciated that the present invention can be practiced without them. In the latter case, each weighting matrix R may be replaced by an identity matrix of similar dimension in Equation (28) and the following equations; each inverse matrix R−1 is similarly replaced by an identity matrix.
The inventors have further constructed an inverse matrix for the block matrix on the left-hand side of the equation (28), and from this inverse matrix have found a form of N which satisfies equation (28) as follows:
where this form comprises an n×n inverse matrix multiplying an n×1 vector. In the discussion that follows, we will identify the n×n inverse matrix as M−1 and the n×1 vector as B, with N=M−1 B. The above form may be more simply expressed if we form a matrix matrix Pk for the data of the k-th time moment in the following form:
Pk=Rk−1−Ek−1Qk(QkTRk−1Qk+qSk)−1QkTRk−1
and a vector:
gk=GTRk−1Qk(QkTRk−1Qk+qSk)−1hk
With matrix Pk, equation (29) may now be written as:
We refer to Pk as a projection-like matrix for q=0 and a quasi-projection matrix for q>0. Each component matrix
is symmetric positive definite and may be inverted. Moreover, a matrix comprised of a summation of symmetric positive definite matrices is also symmetric positive definite. Thus, matrix M is symmetric positive definite and can be inverted. In preferred implementations of the present invention, the inverse of M is not directly computed. Instead, a factorization of M into a lower triangular matrix L and an upper triangular matrix U is produced as follows: M=LU. Several different factorizations are possible, and L and U are not unique for a given matrix M. The LU factorization of matrix M enables us to compute the floating ambiguities N through a sequence of forward and reverse substitutions. These substitutions are well known to the art (cf any basic text on numerical analysis or matrix computations). With symmetric positive definite matrices, one may choose L and U such that U=LT, which gives a factorization of M=LLT. This is known as the Cholesky factorization, and it generally has low error due to numerical rounding than other factorizations.
With N being generated from this form, the inventors have further found that each individual vector ak can be generated according to the following form:
ak=(QkTRk−1Qk+qSk)−1(QkTRk−1(μk−GN)−qgk). (31)
The generation of the individual vectors ak is optional to the process of generating a set of floating ambiguities N. However, when using cost function F(*) and equations (22) and (23), one can generate ak in order to update rk. The forms of N and ak which the inventors have discovered enable one to generate a vector N without having to first generate the individual vectors ak.
When using the cost function F(*), Sk and hk (and gk which is derived from hk and Sk), an estimate of the baseline vector rk at time moment “k” has to be generated. As indicated by equations (22) and (23), both Sk and hk depend upon LRB, which does not normally change, and upon rk, which can change and often does change. For generating Sk and hk, it is usually sufficient to use an estimate of rk, which we denote at rk′ and which may be provided by the user or general process that is using the present invention. As part of generating the calculated distances DkR and DkB, the user or general process uses the estimated position of the rover and the known or estimated position of the base station. An estimate rk′ can be generated by subtracting the position of the base station from the estimated position of the rover. If desired, one can refine the estimate by generating ak from equation (31), and then using the combination (rk′+ak) as a more refined estimate of rk in generating Sk and hk. To do this, one may first generate an estimate N′ to N by using equation (30) with Sk=0 and gk=0. Then equation (31) can be evaluated using N=N′, Sk=0, and gk=0 to generate refined baseline vectors rk=(rk′+ak), and initial values of Sk′, hk′, and gk′. Equation (30) is then again evaluated using the initial values Sk′, hk′, and gk′ for Sk, hk, and gk, respectively. The process may be repeated again. To speed convergence, one can consider using prior values of Sk′ and gk′ in generating ak for k>1 as follows:
ak=(QkTRk−1Qk+qSk-1)−1(QkTRk−1(μk−GN′)−qgk-1).
First Exemplary Set of Method Implementations of the Present Invention
The inventors have discovered a number of ways to employ the form of N provided by Equation (30). For post-processing application, the satellite data may be collected for a plurality j of time moments, the matrices Rk and Qk (and optionally Sk) and the vectors μk (and optionally hk and gk) for each k-th time moment may then be computed, and the n×n inverse matrix M−1 and the n×1 vector B may then be generated and thereafter multiplied together to generate the vector N. The plurality of time moments may be spaced apart from one another by equal amounts of time or by unequal amounts of time. As indicated above, instead of generating the inverse matrix M−1, one may generate the LU factorization of M and perform the forward and reverse substitutions. The factorization-substitution process is faster than generating the inverse matrix, and more numerically stable than most matrix inversion processes. If necessary, Equations (30) and (31) may be iterated as described above until convergence for significantly nonlinear dependency of quantities in equations (22) and (23) on the Rover position.
For real-time applications, M−1 and B may be initially computed at a first time moment from a first set of data (e.g., R1, Q1, μ1, R2, Q2, μ2) and then recomputed at subsequent time moments when additional data becomes available. For instance, we can initially compute M and B based on l time moments k=1 to k=l as follows:
where the subscript “l” has been used with Ml and Bl to indicate that they are based on the l time moments k=1 to k=l. The floating ambiguity may then be computed from Nl=[Ml−1]·Bl, using matrix inversion or LU-factorization and substitution. Data from the next time moment l+1 can then be used to generate the updated quantities Ml+1 and Bl+1 as follows using the previously computed quantities Ml and Bl:
Ml+1=Ml+GTPl+1G (31C)
Bl+1=Bl+GTPl+1μl+1+qgl+1, (31D)
With an updated set of floating ambiguities being computed from Nl+1=[Ml+1]−1 Bl+1, using matrix inversion or LU-factorization and substitution. It may be appreciated that the above forms of Ml+1 and Bl+1 may be employed recursively (e.g., iteratively) in time to compute updated floating ambiguities Nl+1 from previously-computed values of the quantities Ml and Bl as satellite data is collected. The recursion may be done with each recursive step adding data from one epoch, or with each recursive step adding data from multiple epochs, such as provided by the following forms:
where Ml and Bl are based upon j time moments, and Mm and Bm are based on these time moments plus the time moments l+1 through to m, where m>l+1. While these recursion methods are preferably applied to real-time applications, it may be appreciated that they may be equally used in post processing applications. Furthermore, while one typically arranges the time moments such that each time moment k+1 occurs after time moment k, it may be appreciated that other ordering of the data may be used, particularly for post processing applications.
The steps of the above method are generally illustrated in a flow diagram 40 shown in
It may be appreciated that the above steps may be performed other sequences than that specifically illustrated in
The above method may be carried out on the exemplary apparatus 100 shown in
Data processor 110 may be configured to implement the above-described method embodiments, such as exemplified by the steps in
Computer program produce 60 comprises five instruction sets. Instruction Set #1 directs data processor 110 to receive the measured data from data portal 120. The measured data from portal 120 may be loaded into data memory 114 by Instruction Set #1. As another implementation, the data may be loaded into memory 114 by subsequent instruction sets as the data is needed. In the latter case, Instruction Set #1 can take the form of a low-level I/O routine that is called by the other instruction sets as needed. As such, data portal 120 and data processor 110 under the direction of instruction set #1 provide means for receiving the measured data for apparatus 100. Instruction Set #2 directs data processor to generate, for each time moment j, a vector Δγj of a plurality of range residuals of pseudo-range measurements made by the first and second navigation receivers in the form of: Δγj=(γjR−γjB)−(DjR−DjB). As such, data processor 110 under the direction of instruction set #2 provides means for generating the range residuals Δγj for apparatus 100. Instruction Set #3 directs data processor 110 to generate, for each time moment j, a vector Δφj of a plurality of phase residuals of full phase measurements made by the first and second navigation receivers in the form of: Δφj=(φjR−φjB)−Λ−1·(DjR−DjB), where Λ−1 is a diagonal matrix comprising the inverse wavelengths of the satellites. As such, data processor 110 under the direction of instruction set #3 provides apparatus 100 with means for generating the phase residuals Δφj. The residuals may be stored in data memory 114.
Instruction Set #4 directs data processor 110 to generate an LU-factorization of matrix M or a matrix inverse of matrix M, the matrix M being a function of at least Λ−1 and Hkγ, for index k of Hγ covering at least two of the time moments j. Exemplary forms of matrix M have been provided above. Matrix M and its LU-factorization or inverse may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #4 provide apparatus 100 with means for generating matrix M and its LU-factorization or inverse. Finally, instruction Set #5 directs data processor 110 to generate a vector N of estimated floating ambiguities as a function of at least the set of range residuals Δγk, the set of phase residuals Δφk, and the LU-factorization of matrix M or the matrix inverse of matrix M. Exemplary forms of vector N have been provided above. Vector N may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #5 provide apparatus 100 with means for generating an vector N, which is an estimate of the floating ambiguities.
The resulting estimates provided by vector N may be outputted on keyboard/display 115, or may be provided to the more general process through data portal 120 or by other transfer means (such as by memory 114 if data processor 110 is also used to implement the more general process).
Second Exemplary Set of Method Implementations of the Present Invention
The inventors have developed additional recursive methods that are generally better suited to real-time applications. The second exemplary set of methods generally facilitate implementations which require less memory storage space and fewer computations. We previously defined a projection-like matrix Pk for the data of the k-th time moment as follows:
Pk=Rk−1−Rk−1Qk(QkTRk−1Qk+qSk)−1QkTRk−1. (32)
Equation (32) was then applied to the form of equation (30) to provide the form:
where M and B are identified in the forms of:
The forms of equations (33B) can be expressed in the following recursion form:
Mj=Mj−1+GTPjG and Bj=Bj−1+GTPjμj+qgj (34)
Then
Nj=(Mj−1+GTPjG)−1(Bj−1+GTPjμj+qgj) (35A)
noting that Nj=[Mj]−1 Bj for the data from time moments 1 through j, we can write Nj−1=[Mj−1]−1 Bj−1 for the data from time moments 1 through j−1. The latter can be rearranged as Mj−1 Nj−1=Bj−1 and used to substitute for the term Bj−1 in equation (35A) to provide:
Nj=(Mj−1+GTPjG)−1(Mj−1Nj−1+GTPjμj+qgj) (35B)
To equation (35B), we now add and subtract the term GT Pj G Nj−1 from the second bracketed quantity to obtain:
Nj=(Mj−1+GTPjG)−1(Mj−1Nj−1+GTPjGNj−1−GTPjGNj−1+GTPjμj+qgj) (35C)
Noting that the first two terms of the second bracketed quantity can be factored as (Mj−1+GTPjG) Nj−1 and that the factor (Mj−1+GTPjG) is the inverse of the first bracketed quantity in equation (35C), it can be seen that the first bracketed quantity multiplied onto (Mj−1+GTPjG) Nj−1 is simply Nj−1. Therefore, equation (35C) can be simplified as:
Nj=Nj−1+(Mj−1+GTPjG)−1(−GTPjGNj−1+GTPjμj+qgj) (35D)
The second bracketed quantity of equation (35D) can be further simplified as:
Nj=Nj−1+(Mj−1+GTPjG)−1(GTPj(μj−GNj−1)+qgj) (35E)
Using equation (34) this becomes:
Nj=Nj−1+Mj−1(GTPj(μj−GNj−1)+qgj) (36)
With this, the following recursive method may be used in a real time application:
(5A) Generate an LU-factorization of Mk, where Mk is in a form equivalent to Mk=Mk−1+GTPkG. Exemplary ways of generating LU factorizations are described in greater detail below.
During the first few recursion steps, matrix Mk may be ill-conditioned, and thus the generation of the LU factorization or inverse of Mk may incur some rounding errors. This problem can be mitigated by using Rk=I during the few recursions, or using an Rk with more equal weightings between the psuedorange and phase data, and then switching a desired form for Rk.
The steps of the above method are generally illustrated in a flow diagram 70 shown in
At step 74, the method generates, for time moment j=1, an LU-factorization of a matrix M1 or a matrix inverse of matrix M1, the matrix M1 being a function of at least Λ−1 and Hlγ. Any of the forms for M described above may be used. At step 75, the method generates, for time moment j=1, a vector N1 as a function of at least Δγ1, Δφ1, and the LU-factorization of matrix M1 or the matrix inverse of matrix M1. At step 76, the method generates, for an additional time moment j≠1, an LU-factorization of a matrix Mj or a matrix inverse of matrix Mj, the matrix Mj being a function of at least Λ−1 and Hjγ. At step 77, the method generates, for an additional time moment j≠1, a vector Nj as a function of at least Δγj, Δφj, and the LU-factorization or matrix Mj or the matrix inverse of matrix Mj. At step 78, the estimated ambiguity vector Nj is reported. If the estimated ambiguity vector has not achieved sufficient accuracy, as set by the user, steps 76 and 77 are repeated, with steps 76-78 forming a loop. If the estimated ambiguity vector has achieved a sufficient degree of accuracy, or it steps 76-78 have been repeated for a maximum number of times set by the user, the process is ended. If the cost function F(*) is included, then step 76 may include the generation of ak for refined estimates of rk, as indicated above.
It may be appreciated that the above steps may be performed other sequences than that specifically illustrated in
The above method embodiments may be carried out on the exemplary apparatus 100 shown in
Computer program produce 80 comprises eight instruction sets. Instruction Set #1 directs data processor 110 to receive the measured data from data portal 120. The measured data from portal 120 may be loaded into data memory 114 by Instruction Set #1. As another implementation, the data may be loaded into memory 114 by subsequent instruction sets as the data is needed. In the latter case, Instruction Set #1 can take the form of a low-level I/O routine that is called by the other instruction sets as needed. As such, data portal 120 and data processor 110 under the direction of instruction set #1 provide means for receiving the measured data for apparatus 100. Instruction Set #2 directs data processor to generate, for each time moment j, a vector Δγj of a plurality of range residuals of pseudo-range measurements made by the first and second navigation receivers in the form of: Δγj=(γjR−γjB)−(DjR−DjB). As such, data processor 110 under the direction of instruction set #2 provides means for generating the range residuals Δγj for apparatus 100. Instruction Set #3 directs data processor 110 to generate, for each time moment j, a vector Δφj of a plurality of phase residuals of full phase measurements made by the first and second navigation receivers in the form of: Δφj=(φjR−φjB)−Λ−1·(DjR−DjB), where Λ−1 is a diagonal matrix comprising the inverse wavelengths of the satellites. As such, data processor 110 under the direction of instruction set #3 provides apparatus 100 with means for generating the phase residuals Δφj. The residuals may be stored in data memory 114.
Instruction Set #4 directs data processor 110 to generate, for time moment j=1, an LU-factorization of a matrix M1 or a matrix inverse of matrix M1, the matrix M1 being a function of at least Λ−1 and H1 and H1γ. Exemplary forms of matrix M1 have been provided above. Matrix M1 and its LU-factorization or inverse may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #4 provide apparatus 100 with means for generating matrix M1 and its LU-factorization or inverse. Instruction Set #5 directs the data processor 110 to generate, for time moment j=1, an estimated ambiguity vector N1 as a function of at least Δγ1, Δφ1, and the LU-factorization of matrix M1 or the matrix inverse of matrix M1. Exemplary forms of vector N1 have been provided above. Vector N1 may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #5 provide apparatus 100 with means for generating an vector N1, which is an estimate of the floating ambiguities.
Instruction Set #6 directs data processor 110 to generate, for one or more additional time moments j≠1, an LU-factorization of a matrix Mj or a matrix inverse of matrix Mj, the matrix Mj being a function of at least Λ−1 and Hjγ. Exemplary forms of matrix Mj have been provided above. Matrix Mj and its LU-factorization or inverse may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #6 provide apparatus 100 with means for generating matrix Mj and its LU-factorization or inverse. Because of their similar operations, Instruction Set #6 may share or duplicate portions of Instruction Set #4. Instruction Set #7 directs the data processor 110 to generate, for one or more additional time moments j≠1, a vector Nj as a function of at least Δγj, Δφj, and the LU-factorization or matrix Mj or the matrix inverse of matrix Mj. Exemplary forms of vector Nj have been provided above. Vector Nj may be stored in data memory 114. As such, data processor 110 under the direction of instruction set #7 provide apparatus 100 with means for generating an vector Nj, which is an estimate of the floating ambiguities. Because of their similar operations, Instruction Set #7 may share or duplicate portions of Instruction Set #5.
Instruction Set #8 directs the data processor 110 to report vector Nj as having estimates of the floating ambiguities, and to repeat Instruction Sets #6 and #7 if vector does not have sufficient (or desired) accuracy, or if it is desired to keep the process going even through sufficient accuracy has been reached. The resulting estimates provided by vector N may be outputted on keyboard/display 115, or may be provided to the more general process through data portal 120 or by other transfer means (such as by memory 114 if data processor 110 is also used to implement the more general process).
Give the detailed description of the present Specification, it is well within the ability of one skilled in the GPS art to construct all of the above Instruction Sets without undue experimentation, and a detailed code listing thereof is not needed for one of ordinary skill in the art to make and use the present invention.
Methods of LU-Factorization of Matrix M
First Method.
We now discuss methods of LU-factorization for matrix M. The factorization methods may be used in any of the above steps or computer instruction sets where an LU-factorization is generated or where an inverse matrix is generated, such as in step (5A) described above, and also used in step (5B) to construct an inverse matrix for M, although such is computationally costly. In one approach of LU-factorization, the matrix Mk−1 from the previous iteration is retained for the current iteration, and GT Pk G from the current iteration is added to it to form the matrix Mk for the current iteration of step (5B). Then, any LU-factorization method may be used to find a lower triangular matrix Lk and an upper triangular matrix Uk which satisfies Mk=Lk Uk. Since Mk is symmetric positive definite, the Cholesky method may be used. This method has good numerical stability, and generates upper triangular matrix Uk such that it equals the transpose of lower triangular matrix Lk: Uk=LkT. With this factorization, Mk=Lk LkT. The standard Cholesky method requires a square-root operation for each row of the matrix (n rows requires n square-root operations). Such operations may be difficult or time consuming to perform on mid-range processor chips. A modification of the Cholesky method developed by Wilkinson and Reinsch may be used to avoid these square-root operations. In this method, the factorization of Mk={tilde over (L)}D{tilde over (L)}T is used, where D is a diagonal matrix. We refer readers who are not familiar with this area of the art to the following references for further information:
Instead of using the modified Cholesky method, the following method developed by the inventors may be used. The inventors currently prefer this method. Given that we have generated the previous factorization Mk−1=Lk−1Lk−1T, we generate a factorization TkTkT for the quantitiy GTPkG as follows: TkTkT=GTPkG. Later, we will describe how this factorization TkTkT may be generated. Using TkTkT=GTPkG, the factorization LkLkT of Mk may be written as:
LkLkT=Lk−1Lk−1T+TkTkT. (37)
It is known in the matrix computation art that the product of two n×n matrices X and Y is equal to the sum of the outer products of the columns of these matrices, as specified below:
where {x1, x2, . . . , xn} are the columns of matrix X, and where {y1, y2, . . . , yn} are the columns of matrix Y. The inventors have applied this general knowledge to their development of the invention to recognize that
where {tk,1, tk,2, . . . , tk,n} are the columns of matrix Tk. Each outer product tk,stk,sT is an n×n matrix of rank one. It is known from the article entitled “Methods for Modifying Matrix Factorizations” by P. E. Gill, G. H. Golub, W. Murray, and M. A. Saunders (Mathematics of Computation, Vol. 28, No. 126, April 1974, pp. 505-535) that when a rank-one matrix of the form z zT is added to a symmetric positive definite matrix A, a previously computed Cholesky factorization of matrix A may be modified with a relatively few number of computations (much less than the number of computations need to generate a factorization of A+zzT). The inventors have further recognized that performing n such rank-one modifications on the previous factorization Lk−1Lk−1T for Mk−1 using z zT=tk,stk,sT for s=1 to s=n would also require less computations and would have better accuracy that a new factorization for Mk.
Let us illustrate this approach by first defining a set of intermediate factorization matrices {tilde over (L)}1, {tilde over (L)}2, . . . , {tilde over (L)}n, each of which has the same dimensions as Lk−1 and Lk. We now go through a sequence of n rank-one modifications which will sequentially generate the matrices {tilde over (L)}1 through {tilde over (L)}n, with the last matrix {tilde over (L)}n being in a form which is substantially equal to the desired factorization Lk. The first rank-one modification starts with any of the matrices tk,stk,sT. Without loss of generality, we will start with s=1 in order to simplify the presentation. We then write:
{tilde over (L)}1{tilde over (L)}1T=Lk−1Lk−1T+tk,1tk,1T (40)
which can be factored as:
{tilde over (L)}1{tilde over (L)}1T=Lk−1(I+c1c1T)Lk−T, (41)
where vectors c1 and tk,1 are related to one another as follows: Lk−1Tc1=tk,1. Vector c1 is readily obtained from vector tk,1 with a forward substitution process with the previously computed matrix Lk−1, since Lk−1, is lower triangular. Then, the above reference by Gill, et al. teaches how to readily obtain a Cholesky factorization of (I+c1c1T), which we denote here as {overscore (L)}1{overscore (L)}1T. The reader is referred to that reference, as well any other references teaching such factorizations, for the implementation details. From this it can be seen that the form of equation (35) becomes:
{tilde over (L)}1{tilde over (L)}1T=Lk−1({overscore (L)}1{overscore (L)}1T)Lk−1T, (42)
and thus {tilde over (L)}1=Lk−1{overscore (L)}1. The multiplication of two lower triangular matrices is relatively easy to perform and computationally inexpensive.
We now perform the second rank-one modification using rank-one modification the matrix tk,2tk,2T (s=2) in a similar manner by writing:
{tilde over (L)}2{tilde over (L)}2T={tilde over (L)}1{tilde over (L)}1T+tk,2tk,2T (43)
which can be factored as:
{tilde over (L)}2 {tilde over (L)}2T={tilde over (L)}1(I+c2c2T){tilde over (L)}1T, (44)
where vector C2 is generated from tk,2 by forward substitution according to: {tilde over (L)}1c2=tk,2. A Cholesky factorization of (I+c2c2T) is then obtained, which we denote here as {overscore (L)}2{overscore (L)}2T. Thus, {tilde over (L)}2={tilde over (L)}1{overscore (L)}2. The recursion process continues in this manner until {tilde over (L)}n is computed. The following recursion sequence can be used:
Close examination of the second method shows that the following more compact recursion sequence may be used:
The previously-described main instruction sets that generate LU factorizations of matrix M can be constructed to include instructions that direct data processor 110 to carry out the above forms steps of factorizing matrix M under the above second and third methods. Specifically, there would be a first subset of instructions that direct the data processor to generate an LU-factorization of matrix Mj−1 in a form equivalent to Lj−1 Lj−1T wherein Lj−1 is a low-triangular matrix and Lj−1T is the transpose of Lj−1. In addition, there would be a second subset of instructions that direct the data processor to generate a factorization of GT Pj G in a form equivalent to TjTjT=GTPjG, where TjT is the transpose of Tj (examplary methods for this are described below). There would also be a third subset of instructions that direct the data processor to generate an LU-factorization of matrix Mj in a form equivalent to Lj LjT from a plurality n of rank-one modifications of matrix Lj−1, as described above, each rank-one modification being based on a respective column of matrix Tj, where n is the number of rows in matrix Mj. The combination of these subsets of instructions and data processor 110 provides apparatus 100 with means for performing the above tasks.
Generation of Matrix Tk
The last two factorization methods requires finding TkTkT=GTPkG so that the column vectors tk,s may be used. One can use the Cholesky factorization method to generate Tk since GTPkG is symmetric positive definite (we call this the first method of generating matrix Tk). The above second subset of instructions be constructed to include further instructions that direct data processor 110 to carry out the any form of Cholesky factorization of GTPkG. to generate Tk. The combination of these further instructions and data processor 110 provides apparatus 100 with means for generate matrix Tj from a Cholesky factorization of GTPjG. However, the inventors have developed the following more efficient second method of generation of matrix Tk. It must be noted that this second method of generation of matrix Tk is applicable if the penalty parameter q related to the constant distance constraints defined by equation (11), and appearing starting with the Equation (27), is set to zero. In other words, the second method of generating matrix Tk described below is applicable if the constant distant constraints are not used.
The Second Method of Generating Matrix Tk
The second method is based on a novel block Householder transformation of the matrix GTPkG which the inventors have developed. This method is based on constraining the weighting matrices Rγ and Rφ to the following forms that are based on a common weighing matrix W:
where σγ and σφ are scalar parameters selected by the user, and where λGPS2 is either the L1-band wavelength or the L2-band wavelength of the GPS system. If all the wavelengths in Λ are the same, the above forms reduce to:
With W, σγ, σφ, λGPS2, Rγ and Rφ selected, the following steps are employed to generate matrix Tk
The above second subset of instructions be constructed to include further instructions that direct data processor 110 to carry out the above four general step under this second method of generating matrix Tk. The combination of these further instructions and data processor 110 provides apparatus 100 with means for generate matrix Tj.
While the present invention has been particularly described with respect to the illustrated embodiments, it will be appreciated that various alterations, modifications and adaptations may be made based on the present disclosure, and are intended to be within the scope of the present invention. While the invention has been described in connection with what is presently considered to be the most practical and preferred embodiments, it is to be understood that the present invention is not limited to the disclosed embodiments but, on the contrary, is intended to cover various modifications and equivalent arrangements included within the scope of the appended claims.
APPENDIX A—Derivation of the Second Method of Generating Matrix T.
To simplify the presentation of this derivation, we take the case of where the measurements are provided in only one GPS frequency band (e.g., L1-band). Generalization to two-band data and multiband data (GLONASS) is straight-forward matter. First, let us relate the range weighting matrix (Rγ)−1 and the phase weighting matrix (Rφ)−1 to a common weight matrix W and two scalar parameters σγ and σφ as follows:
where W is a diagonal positive definite n×n matrix. We now want to look at the block factorization of the component (QkTRk−1Qk)−1, which is part of Pk=Rk−1−Rk−1Qk(QkTRk−1Qk)−1QkTRk−1. To simplify the presentation, we are going to omit the time-moment subscript “k” and the pseudorange superscript “γ” from our notation for
matrix component (QkTRk−1Qk)−1 as follows:
With the condition that the measurement data is within one signal band, all of the wavelengths are the same (for the purposes of determining the floating ambiguity), and the diagonal wavelength matrix Λ may be replaced by the identity matrix I multiplied by the scalar wavelength value λ: Λ=λI. This leads to the simplification:
The quantity
may be represented a single scalar value b
and the above may be further simplified as:
(QTR−1Q)−1=σφ2b(HTWH)−1.
The matrix W is diagonal positive definite so we can write W=W1/2W1/2. Then we have
Denoting the matrix product W1/2H more simply as {tilde over (H)} (i.e., W1/2H={tilde over (H)}), the above form can be rewritten as:
We now generate reduced forms for {tilde over (H)} and {tilde over (H)}T. We apply the Householder transformation to matrix {tilde over (H)}T, which is indicated by Householder matrix SHH:
{tilde over (H)}TSHH={tilde over (V)}=[V|O4×(n−4)],
where matrix V is a lower diagonal 4×4 matrix. Matrix S is an n×n matrix, and is an orthogonal (so that SHHSHHT=In) since it is a Householder matrix. Multiplying both sides of the above equation by SHHT, and using the fact that SHHSHHT=In, we can find that:
{tilde over (H)}T[V|O4×(n−4)]SHHT={tilde over (V)}SHHT.
Then, by the transpose rule, we can find {tilde over (H)}=SHH{tilde over (V)}T. We now substitute these reduced forms for {tilde over (H)} and {tilde over (H)}T in the prior equation for GTPG, and perform the following sequence of substitutions, expansions, and regroupings:
Finally, we obtain
In the case when we use both GPS and GLONASS measurements, take matrices (Rγ)−1 and (Rφ)−1 in the form
where λ is the GPS wave length, then all the above reasoning hold including the formula for T. However the value
close to 1 (but always less than 1), so
is a small value, the operation of taking a square root does not reduce accuracy.
This method of generating the matrix T may be extended to L1 and L2 band measurements. Let
where λ1 and λ2 are the wavelengths of GPS L1 and L2 bands, respectively, and W is the weighing matrix, as above. Then
Matrix Q thus takes the form
so that
where b is defined as
Note that in this case the matrix G takes the form
As in the case of L1 measurements, denote W1/2H={tilde over (H)}, and, implementing Householder transformation:
{tilde over (H)}TSHH={tilde over (V)}=[V|O4×(n−4)], that is
H=SHH{tilde over (V)}T, {tilde over (H)}T={tilde over (V)}SHHT,
we obtain:
Matrix K has the following structure:
The Cholesky factorization of matrix K: K={tilde over (K)}{tilde over (K)}T may be obtained using finite formula:
Thus, for matrix T, where GPGT=TTT, we may write
where sub-matrixces A11, A21, and A22 are as follows: