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基于移动参考站的GPS动态相对定位算法研究
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摘要
相对于一个移动参考站的GPS动态相对定位简称为动对动定位,具有广泛应用,如舰队管理、战场指挥、编队飞行、运动车辆相对定位、卫对卫定轨、飞行器安全接近、载体免撞、自动驾驶等。在这些场合中难以建立不动的参考站,传统定位方法(比如雷达/激光测距),或是精度不高或是限制条件严格,不能完全满足要求。在这些应用中,物体的绝对位置重要性远小于相对位置的重要性,因此有精确已知坐标的参考站的配置不是强求的,而高的相对定位精度和可靠性是必须的。大多数相对定位方法假定参考站的精密位置是预先给定的,因此,相对定位精度主要依赖于测量误差。然而,在动对动定位中,这一先决条件是没有的,因此那些已有算法难以直接用于动对动定位,需要作适当修改,本文将对此作深入研究。
     高精度动对动定位需要使用载波相位观测值,当平台间距离很短,双差处理可以削弱相位观测值中的空间相关误差,卫星和接收机钟差可以消除掉。当残余误差很小,模糊度固定后定位精度可以达到厘米级。高精度相对定位主要地依赖于模糊度成功解算及模糊度保持为常数,然而,在动态情形下,由于接收机振荡器、遮挡和多路径等因素会引起周跳,即相位观测值的整周跳跃,周跳改变了相位观测值表达的距离值进而影响了以相位为基础的定位精度,因此,整周模糊度解算和周跳探测与修复是高精度动对动定位的核心问题。
     观测值是用来获得所需要的参数,由于观测值含有偏差和误差,为了削弱误差的影响和提高解的精度,需要有多余观测数,即实际的独立观测值数多于估计未知参数所必须的观测值数。由于误差存在使得观测值间不相容,为了消除不相容并获得待估参数,通常要应用最小二乘估计,即残差平方和加权最小原理。由于最小二乘估计仅能处理线性系统,而所需的流动站坐标未知参数包含在站星几何距离中,观测方程线性化就是GPS数据处理的基本内容。在现有的参考文献中,所给出的线性化方式可以分为两类,一是以流动站坐标为参数进行线性化,未知参数是流动站坐标改正量;另一线性化方法是以流动站到参考站的基线向量为参数,未知参数是基线向量的改正数。前一种线性化方法无疑作了三个前提假设:参考站坐标精确已知、参考站坐标与观测数据在同一坐标系、流动站近似坐标也在同一坐标系中。显然,在动对动定位中,以上假设是不存在的,因此以测站坐标为参数线性化单差、双差观测方程是不行的。后一种线性化方法在有的参考文献中介绍了很复杂的双差观测方程线性化推导过程,为此,本文给出了一种简单易行的观测方程线性化方法,在此基础上指出了动对动定位与其它定位模式在方程线性化方面的不同与相同之处。
On-the-fly GPS positioning relative to a moving reference, referred to as KINRTK in, this thesis, has many applications, such as fleet management, battlefield command, formation flying, vehicles positioning, satellite-to-satellite orbit determination, aerocraft safety approach, and others, where a static reference is difficult to establish. In this application, the absolute positions of the objects are not important but rather their relative positions, so that the configuration of the reference station with precisely known coordinates is not mandatory. High relative positioning accuracy and reliability are required. Most of the existing methods of relative positioning assume that the precise position of a reference station is given a priori. Thus, the accuracy of the relative positioning only depends on the measurement errors. However, in this research, such a precondition is not given. Therefore, those previous approaches cannot be directly used for this research. Modifications are required to process the kinematic data simultaneously. The impact of these modifications on the effectiveness of relative positioning is to be investigated in this thesis.To achieve high positioning accuracy, the double-differenced GPS carrier phase method is usually adopted. When the inter-platform distances are short, e.g., less than 10 km, double differencing can largely reduce spatially correlated errors in the carrier phase measurements. Satellite and receiver clock errors are cancelled, regardless of the inter-platform distance. When the remaining errors are small, centimeter-level accuracy relative positions can be obtained with fixed integer ambiguities. High accuracy relative positioning depends mostly on successful integer ambiguity resolution of the double-differenced carrier phase measurements. Before the carrier phase observable can be utilized as a precise range information its inherent integer cycle ambiguity must be resolved and carrier phase positioning rely on the ambiguities being constant. Unfortunately, high user dynamics, the receiver's oscillator, shadowing and multipath can cause cycle slips, i.e. jumps of the carrier phase observable by an integer multiple of wavelengths. Every cycle slip would deteriorate the high accuracy of the affected carrier phase range and also that of the position derived from such carrier phase observables. Therefore, integer ambiguity resolution and cycle slips detection and repairing are two of the crucial problems to resolve for high accuracy relative positioning.Observations are made to derive certain parameters. However, observations often contain biases and errors. To reduce the effect of the errors and assess the accuracy of the solution, redundancy is required. That is, more than the minimum number of observations is required to determine the estimated parameters. These observations must be adjusted so that the solution will be consistent with these adjusted observations. To adjust observations and to obtain the desired parameters, the method of least-squares estimation is often used. In least-squares estimation, parameters and corrected observations are derived by minimizing the weighted sum of the squared residuals. As well known, least-squares estimation can only process a linear system, while the desired parameters, rover station coordinates, are contained in the geometric range between the satellite and the receiver
    antenna. Therefore, linearization is the basic work in GPS data processing. Two modes of linearization can be found in the GPS literature. In the first approach, observation equation is linearized by rover station coordinates, whose estimated parameters are the correction to the approximated station coordinates. The other one linearizes the equations with baseline vector between rover station and the reference, whose estimated parameters are the correction to the approximated baseline vector. There are three presupposition assumptions in the former approach, i.e., known precise reference station coordinates, the coordinates and observables are in the same coordinate system, and the approximated rover station coordinates are also in the system. Obviously, these assumptions do not exist in KINRTK, and the equation must be linearized by the latter. A simple and efficient linearization method is presented, and the differences between KINRTK and other GPS positioning modes are analyzed.Most receivers attempt to keep their internal clocks synchronized to GPS Time. This is done by periodically adjusting the clock by inserting time jumps. Two typical examples of receiver clock jumps exist in different manufacturer's receivers. The first example is a millisecond jump which occurs when the clock offset becomes larger than ± 1 millisecond, the receiver corrects the clock by ± 1 millisecond. The second example is a very small clock jump which occurs every second and the jumps are often small. At the moment of the clock correction, two main effects are transferred into the code and phase observables. The effects of the geometric range corresponding to the clock jump are common to all measurements at the moment of the clock jump at one receiver. By single-differencing (SD) the measurements between satellites or double-differencing (DD) the measurements (that is, differencing between receivers followed by differencing between satellites or vice versa), the common effects can be removed. However, the effects of the geometric range rate corresponding to the jump are different for each observation. They cannot be removed by the SD or DD operation. However, like cycle slips, their effects on the code and phase observables are more or less known to users and hence it is possible to detect and remove their effects almost completely in both the measurement and parameter domains.The quality of GPS positioning is dependent on a number of factors. For attaining high-precision positioning results, we need to identify the main error sources impacting on the quality of the observations. In terms of data processing, cycle slips, receiver clock jumps and quasi-random errors are the main sources which can deteriorate the quality of the observations and subsequently, the quality of positioning results. Cycle slips are discontinuities of an integer number of cycles in the measured (integrated) carrier phase resulting from a temporary loss-of-lock in the carrier tracking loop of a GPS receiver. In this event, the integer counter is reinitialized which causes a jump in the instantaneous accumulated phase by an integer number of cycles. The detection and correction of cycle slips is needed if accurate positioning is to be carried out. Cycle slip detection and correction requires the location of the jump and the determination of its size. It can be completely removed once it is correctly detected and identified. Slip detection and repair still represents a challenge to carrier phase data processing even after years of research. For completeness, a short description of the development of strategies for detecting and determining cycle slips over the past two decades or so is presented. For the most part, techniques used in the detection and determination of cycle slips have not changed drastically since the first methods were devised in the early 1980s. The focus has always
    been on attempting to develop a reliable, somewhat automatic detection and repair procedure. All methods have the common premise that to detect a slip at least one smooth (i.e., low noise) quantity derived from the observations must be tested in some manner for discontinuities that may represent cycle slips. The derived quantities usually consist of linear combinations of the undifferenced or double-differenced L1 and L2 carrier-phase and possibly pseudorange observations. Examples of combinations useful for kinematic data are. the geometry-free phase (a scaled version of which is called the ionospheric phase delay), and widelane phase minus narrowlane pseudorange. Once the time series for the derived quantities have been produced, the cycle-slip detection process (that is, the detection of discontinuities in the time series) can be initiated. Of the various methods available, a novel approach, called Non-integer Linear Combination (NLC), is proposed.Time-relative positioning is a recently developed method for processing GPS observations. Observe first carrier phases at a station of known coordinates (a geodetic point, for example) for a short period of time (1-2 min). Preferably, the observation rate must be high—e.g., 1 s. The user then moves the receiver and the antenna quickly (e.g., 30 s) toward the station of unknown coordinates located about a hundred meters (depending on the type of transportation) away from the first one, while continuously observing carrier phases. At the second station, phase observations are recorded again for a short period of time (1-2 min). Relative positioning is then obtained by processing carrier phase observations taken at different epochs (and different stations)with a single GPS receiver. The main distinction between time-relative positioning and conventional relative positioning is that in the former there is a combination of observations taken at two different epochs and two different stations with the same receiver to detennine the position of the unknown station with respect to the known station. In other words, simultaneous observations using a second GPS receiver at a reference station are not required, unlike conventional relative positioning. The disadvantage of time-relative positioning compared to conventional relative positioning is that, since observations at both stations are not obtained simultaneously, it is also affected by the temporal "decorrelation" of errors (time variation of errors) in addition to the spatial "decorrelation" of errors also present in conventional relative positioning. In most GPS applications, regardless of surveying modes (static and kinematic) and baseline lengths (short, medium and long), the effects of the epoch-differenced biases and noise (i.e., atmospheric delay, satellite orbit bias, multipath, and receiver system noise) are more or less below a few centimetres as long as observation sampling interval is relatively short (e.g., sampling interval less than 1 minute). Based on high sampling interval assumption, time-relative positioning observation equation is further analyzed, the concept of virtual measurement is applied, which results in a robust linearization scheme. A new cycle slip detection approach based on time-relative positioning theory is studied for the first time, and valuable unrecognized knowledge of relation between satellites geometry and cycle slip detection is obtained.GPS carrier phase positioning has a higher accuracy than code positioning, assuming the integer ambiguity is correctly fixed. OTF ambiguity resolution refers to the case when the ambiguities are resolved when at least one receiver is moving, i.e., when the receiver is in kinematic mode. It differs from the static ambiguity resolution in two ways: In kinematic applications, errors of measurement cannot be reduced by time averaging because the movement of platforms can significantly change the testing environment; In kinematic
    applications, the position and velocity of the object is required for every epoch, so the batch processing cannot be adopted if real-time processing is required. Since less information is available and larger errors occur, OTF ambiguity resolution is more difficult in kinematic than in static mode. Here are some major factors affecting the OTF ambiguity resolution: Selection of observables; Inter-receiver distance; Number and geometry of satellites; Magnitude of GPS errors; Ambiguity search method; Performance required, etc. The major challenges of OTF ambiguity resolution are relative error modeling, and the efficiency and reliability of the ambiguity search technique. There are many methods that have been developed for solving On-The-Fly (OTF) ambiguity since the 1980's. Basically, they have the same strategies to fix ambiguities, namely, float ambiguity resolution, integer ambiguity searching, and the use of a distinguishing test. The float ambiguity and its variance are used to define the initial search point, and the search range of the integer candidates. Therefore, float solution is more important than anything else in ambiguity resolution. In static mode, float solution can be obtained by only processing carrier phase observables, while in the KINRTK application, although redundancy number exists with epochs increasing, no robust float solution can be achieved, and pseudo-range measurements must be added to the adjustment system.In the GPS literature there are two of the many different approaches proposed for integer ambiguity estimation, which have drawn much interest. The two approaches differ in the model used for integer ambiguity estimation. In the first approach, which is the common mode of operation for most surveying applications, an explicit use is made of the available relative receiver-satellite'geometry, named the "geometry-based" model. Integer ambiguity estimation is also possible however, when one opts for dispensing with the relative receiver-satellite geometry, and is named the "geometry-free" model. In fact from the conceptual point of view, this is the simplest approach to integer ambiguity estimation. The pseudo-range data are directly used to determine the unknown integer ambiguities of the observed phase data. Of particular interest here is the shape and orientation of the ellipsoid of standard deviation for the ambiguities. The orientation for the geometry-free model does not change as the number of epoch increases. The orientation of LI and L2 for the same satellite is exactly 37.93°, i.e., the slope is k = XLXI A.12, and the semi-minor axes for the geometry-based are equal to those of the geometry-free model, while the semi-major axes for the geometry-free model are longer than those of the geometry-based model, which means that the ellipse for the geometry-free model always contains the ellipse for the geometry-based model. The geometry is the same for every epoch solution, as long as the stochastic model remains unchanged. The orientation for the geometry-free model does not change for every epoch, while the orientation of two different satellites for the geometry-based model is closer to the axes as the number of epoch increases, which means that these two ellipses overlap each other partly. Combining these two models' advantages, a new concept for ambiguity resolution, called Dual-space Ambiguity Resolution Approach (DARA), involving a search in both spaces at the same time, is proposed.
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