CN107421550B - An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging - Google Patents
An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging Download PDFInfo
- Publication number
- CN107421550B CN107421550B CN201710611461.6A CN201710611461A CN107421550B CN 107421550 B CN107421550 B CN 107421550B CN 201710611461 A CN201710611461 A CN 201710611461A CN 107421550 B CN107421550 B CN 107421550B
- Authority
- CN
- China
- Prior art keywords
- earth
- time
- noise
- satellite
- state
- Prior art date
- Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
- Active
Links
- 238000000034 method Methods 0.000 title claims abstract description 70
- 238000005259 measurement Methods 0.000 claims abstract description 95
- 238000004422 calculation algorithm Methods 0.000 claims abstract description 52
- 238000001914 filtration Methods 0.000 claims abstract description 45
- 239000011159 matrix material Substances 0.000 claims description 83
- 230000003044 adaptive effect Effects 0.000 claims description 49
- 230000001133 acceleration Effects 0.000 claims description 21
- 238000004364 calculation method Methods 0.000 claims description 21
- 238000005070 sampling Methods 0.000 claims description 19
- PEDCQBHIVMGVHV-UHFFFAOYSA-N Glycerine Chemical compound OCC(O)CO PEDCQBHIVMGVHV-UHFFFAOYSA-N 0.000 claims description 18
- 230000008569 process Effects 0.000 claims description 10
- 230000005484 gravity Effects 0.000 claims description 6
- 230000007704 transition Effects 0.000 claims description 4
- 230000001174 ascending effect Effects 0.000 claims description 2
- 238000006243 chemical reaction Methods 0.000 claims description 2
- 230000010354 integration Effects 0.000 claims description 2
- 230000006735 deficit Effects 0.000 abstract 1
- 230000002950 deficient Effects 0.000 description 6
- 230000000694 effects Effects 0.000 description 5
- 238000004088 simulation Methods 0.000 description 5
- 238000010586 diagram Methods 0.000 description 3
- 230000009471 action Effects 0.000 description 2
- 230000008859 change Effects 0.000 description 2
- 230000007423 decrease Effects 0.000 description 2
- 238000005516 engineering process Methods 0.000 description 2
- 238000009499 grossing Methods 0.000 description 2
- 239000000523 sample Substances 0.000 description 2
- 230000002123 temporal effect Effects 0.000 description 2
- 230000015572 biosynthetic process Effects 0.000 description 1
- 238000012937 correction Methods 0.000 description 1
- 230000001934 delay Effects 0.000 description 1
- 230000003111 delayed effect Effects 0.000 description 1
- 238000011161 development Methods 0.000 description 1
- 238000011156 evaluation Methods 0.000 description 1
- 125000001475 halogen functional group Chemical group 0.000 description 1
- 230000006872 improvement Effects 0.000 description 1
- 230000001788 irregular Effects 0.000 description 1
- 230000007774 longterm Effects 0.000 description 1
- 238000012423 maintenance Methods 0.000 description 1
- 238000000691 measurement method Methods 0.000 description 1
- 239000000203 mixture Substances 0.000 description 1
- 239000002245 particle Substances 0.000 description 1
- 230000000737 periodic effect Effects 0.000 description 1
- 230000003094 perturbing effect Effects 0.000 description 1
- 238000012805 post-processing Methods 0.000 description 1
- 238000012545 processing Methods 0.000 description 1
- 238000004445 quantitative analysis Methods 0.000 description 1
- 238000011160 research Methods 0.000 description 1
- 238000007619 statistical method Methods 0.000 description 1
- 238000012546 transfer Methods 0.000 description 1
Images
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01C—MEASURING DISTANCES, LEVELS OR BEARINGS; SURVEYING; NAVIGATION; GYROSCOPIC INSTRUMENTS; PHOTOGRAMMETRY OR VIDEOGRAMMETRY
- G01C21/00—Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00
- G01C21/24—Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00 specially adapted for cosmonautical navigation
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01C—MEASURING DISTANCES, LEVELS OR BEARINGS; SURVEYING; NAVIGATION; GYROSCOPIC INSTRUMENTS; PHOTOGRAMMETRY OR VIDEOGRAMMETRY
- G01C21/00—Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00
- G01C21/02—Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00 by astronomical means
Landscapes
- Engineering & Computer Science (AREA)
- Radar, Positioning & Navigation (AREA)
- Remote Sensing (AREA)
- Physics & Mathematics (AREA)
- Astronomy & Astrophysics (AREA)
- Automation & Control Theory (AREA)
- General Physics & Mathematics (AREA)
- Other Investigation Or Analysis Of Materials By Electrical Means (AREA)
- Position Fixing By Use Of Radio Waves (AREA)
Abstract
Description
技术领域technical field
本发明属于地球卫星星座的自主定轨领域,具体来说,是一种仅利用地球-拉格朗日(Lagrange)联合星座内的星间测距信息,基于自适应滤波实现地球卫星星座自主定轨的方法。The invention belongs to the field of autonomous orbit determination of earth satellite constellations, in particular, it is a method for realizing autonomous determination of earth satellite constellations based on adaptive filtering only by using inter-satellite ranging information in an earth-Lagrange joint constellation. rail method.
背景技术Background technique
近几十年来,卫星导航在国民经济和军事斗争领域中发挥着越来越重要的作用,提高卫星自主运行能力对于减轻地面测控负担、降低卫星运行费用、提高卫星生存能力和扩展航天器的应用潜力等方面具有重要意义。卫星的自主定轨技术是实现卫星自主控制的前提,对保障其自主运行发挥着至关重要的作用,也成为当今卫星导航与控制技术的发展趋势。In recent decades, satellite navigation has played an increasingly important role in the national economy and military struggle. Improving the autonomous operation of satellites is important for reducing the burden of ground measurement and control, reducing satellite operating costs, improving satellite survivability and expanding the application of spacecraft. potential, etc. are of great significance. The satellite's autonomous orbit determination technology is the premise of realizing the autonomous control of the satellite, which plays a vital role in ensuring its autonomous operation, and has also become the development trend of today's satellite navigation and control technology.
目前星座的自主定轨方法主要分为各卫星独立自主定轨和星座整体自主定轨两类方法。前者是通过卫星上搭载的各种惯性器件、星敏感器和导航接收机等获取卫星相对于其他自然天体或者导航星的距离、方向等信息来对自身位置进行在线估计,系统构成简单,运算量小,但其定轨精度受到自然天体表面的不规则程度以及敏感器的测量精度等因素的限制,单独使用难以达到导航级别应用的精度;后者则是充分利用星座内部各卫星间的相对测量信息来实现星座的整网定轨,短弧段定轨精度高,但存在着“亏秩”问题,即仅利用星间相对测量信息无法确定星座在惯性空间中的整体性方向旋转,造成星座卫星的长弧段定轨精度随时间增长而逐步下降。为了解决“亏秩”问题,国外有学者指出当星座或卫星编队所处的引力场高度不对称时,便会由轨道的“唯一性”引入绝对信息,从而解决星座整体旋转的不可观问题。研究发现,在众多非对称摄动引力场中,第三体引力的相对强度最大,特别是在L1和L2两个Lagrange点附近区域,因此通过联合地球卫星星座和Lagrange点星座进行联合自主定轨可以解决“亏秩”问题。利用此种自主定轨方法可以大大降低航天器自主导航系统的复杂性,减少导航测量设备,提高自主定轨精度。同时,Lagrange导航星座还可以作为深空探测导航基站,为其他深空探测器提供导航信息,从而有效解决地面深空探测网在深空导航精度、实时性、安全性等方面存在的问题,因此研究地球-Lagrange联合星座的自主定轨具有重大意义。At present, the autonomous orbit determination methods of the constellation are mainly divided into two types: the independent orbit determination of each satellite and the overall autonomous orbit determination of the constellation. The former uses various inertial devices, star sensors and navigation receivers on the satellite to obtain information such as the distance and direction of the satellite relative to other natural celestial bodies or navigation stars to estimate its own position online. The system has a simple structure and requires less computation. It is small, but its orbit determination accuracy is limited by factors such as the irregularity of the surface of natural celestial bodies and the measurement accuracy of sensors. It is difficult to achieve the accuracy of navigation-level applications when used alone; the latter makes full use of the relative measurement between satellites in the constellation. The orbit determination of the constellation is based on information to realize the whole network orbit determination of the constellation. The orbit determination of the short arc segment has high accuracy, but there is a problem of "deficient rank", that is, only the relative measurement information between the satellites cannot determine the overall direction of the constellation in the inertial space. The orbit determination accuracy of the long arc segment decreases gradually with the increase of time. In order to solve the problem of "deficient rank", some foreign scholars have pointed out that when the gravitational field in which the constellation or satellite formation is located is highly asymmetric, absolute information will be introduced from the "uniqueness" of the orbit, thereby solving the unobservable problem of the overall rotation of the constellation. The study found that among many asymmetric perturbation gravitational fields, the relative strength of the third body gravitational force is the largest, especially in the area near the two Lagrange points L 1 and L 2 , so joint autonomy is carried out through the joint Earth satellite constellation and the Lagrange point constellation. Orbit determination can solve the "deficient rank" problem. Using this method of autonomous orbit determination can greatly reduce the complexity of the spacecraft's autonomous navigation system, reduce the number of navigation and measurement equipment, and improve the accuracy of autonomous orbit determination. At the same time, the Lagrange navigation constellation can also be used as a deep space exploration navigation base station to provide navigation information for other deep space probes, thereby effectively solving the problems of the ground deep space exploration network in deep space navigation accuracy, real-time, security, etc. Therefore, It is of great significance to study the autonomous orbit determination of the combined Earth-Lagrange constellation.
目前,国内外关于地球-Lagrange联合星座的自主定轨方法中主要以批处理算法、扩展卡尔曼滤波(Extend Kalman Filter,EKF)算法和无迹卡尔曼滤波(Unscented KalmanFilter,UKF)算法等常规算法为基础。但是,批处理算法往往用于事后处理,不适用于实时定轨;常规的EKF和UKF算法虽然采用了便于实时计算的递推形式,但往往要求系统噪声和测量噪声的先验信息已知,否则将造成系统性能下降甚至引起滤波发散。由于在轨卫星的实际受力情况复杂,特别是Lagrange卫星,难以获得较为精确的噪声统计特性,而且卫星轨道维持的机动等导致的不规律建模误差也会造成统计特性的改变,使得先验信息失去意义,因此研究能够根据测量信息序列自适应调整的自主导航算法对于提高自主定轨系统的鲁棒性,保证自主定轨精度有着重要意义。At present, the autonomous orbit determination methods for the Earth-Lagrange joint constellation at home and abroad mainly use conventional algorithms such as batch algorithm, Extended Kalman Filter (EKF) algorithm and Unscented Kalman Filter (UKF) algorithm. as the basis. However, batch processing algorithms are often used for post-processing and are not suitable for real-time orbit determination. Although conventional EKF and UKF algorithms use a recursive form that is convenient for real-time calculation, they often require prior information of system noise and measurement noise to be known. Otherwise, the system performance will be degraded and even filter divergence will be caused. Due to the complexity of the actual force of the satellites in orbit, especially the Lagrange satellites, it is difficult to obtain more accurate noise statistical characteristics, and irregular modeling errors caused by the maneuvers of satellite orbit maintenance will also cause changes in statistical characteristics, making the priori The information is meaningless, so the research on the autonomous navigation algorithm that can be adaptively adjusted according to the measurement information sequence is of great significance to improve the robustness of the autonomous orbit determination system and ensure the accuracy of the autonomous orbit determination.
发明内容SUMMARY OF THE INVENTION
本发明为了解决上述问题,提出一种基于星间测距的地球-Lagrange联合星座自主定轨方法,该方法仅利用星间链路获取的星-星距离测量信息,利用自适应非线性滤波(Adaptive Nonlinear Filter,ANF)算法,采用集中式结构融合有效测量信息,实现地球-Lagrange联合星座中各个卫星位置和速度的解算。该星座定轨方法首先采用集中式结构建立地球-Lagrange联合星座自主定轨的系统模型,其中地球导航卫星的状态方程主要基于地心惯性直角坐标系下的受摄二体问题动力学模型来建立,Lagrange导航卫星的状态方程主要基于质心会合坐标系下的圆型限制性三体问题动力学模型来建立,测量方程采用地心惯性直角坐标系下的星间距离测量模型;然后,采用自适应非线性滤波算法对有效测量信息进行融合实现地球-Lagrange联合星座的自主定轨;最后以3颗中地球轨道(MEO)卫星和2颗Lagrange卫星组成的联合星座为例验证方法的有效性。In order to solve the above-mentioned problems, the present invention proposes a method for autonomous orbit determination of the Earth-Lagrange joint constellation based on inter-satellite ranging. The Adaptive Nonlinear Filter, ANF) algorithm adopts a centralized structure to fuse the effective measurement information to realize the calculation of the position and velocity of each satellite in the Earth-Lagrange joint constellation. The constellation orbit determination method first adopts a centralized structure to establish the system model of the Earth-Lagrange joint constellation autonomous orbit determination, in which the state equation of the earth navigation satellite is mainly established based on the received two-body problem dynamics model in the geocentric inertial rectangular coordinate system. , the state equation of the Lagrange navigation satellite is mainly established based on the dynamic model of the circular restricted three-body problem in the center of mass rendezvous coordinate system, and the measurement equation adopts the inter-satellite distance measurement model in the geocentric inertial rectangular coordinate system; The nonlinear filtering algorithm fuses the effective measurement information to realize the autonomous orbit determination of the Earth-Lagrange joint constellation. Finally, a joint constellation composed of three medium earth orbit (MEO) satellites and two Lagrange satellites is used as an example to verify the effectiveness of the method.
一种基于星间测距的地球-Lagrange联合星座自主定轨方法,具体包括以下几个步骤:An Earth-Lagrange joint constellation autonomous orbit determination method based on inter-satellite ranging, which specifically includes the following steps:
步骤一:在集中式结构下,建立地球-Lagrange联合星座自主定轨系统的状态方程;Step 1: Under the centralized structure, establish the state equation of the Earth-Lagrange joint constellation autonomous orbit determination system;
步骤二:在集中式结构下,建立地球-Lagrange联合星座自主定轨系统的测量方程;Step 2: Under the centralized structure, establish the measurement equation of the Earth-Lagrange joint constellation autonomous orbit determination system;
步骤三:在集中式结构下,根据上述建立的地球-Lagrange联合星座自主定轨系统模型,确定实现轨道参数估计的滤波方法;Step 3: Under the centralized structure, according to the above established model of the Earth-Lagrange joint constellation autonomous orbit determination system, determine a filtering method for realizing orbit parameter estimation;
步骤四:在集中式结构下,基于选定滤波算法的地球-Lagrange联合星座自主定轨方法的具体实现。Step 4: Concrete realization of the Earth-Lagrange joint constellation autonomous orbit determination method based on the selected filtering algorithm under the centralized structure.
本发明的优点在于:The advantages of the present invention are:
(1)通过引入Lagrange卫星为系统提供绝对信息,有效解决“亏秩”问题,提高了地球-Lagrange联合星座长期自主定轨精度;(1) By introducing Lagrange satellites to provide absolute information for the system, the problem of "deficient rank" is effectively solved, and the long-term autonomous orbit determination accuracy of the Earth-Lagrange joint constellation is improved;
(2)仅利用星间测距信息,减轻了系统设备的复杂性;(2) Only the inter-satellite ranging information is used to reduce the complexity of the system equipment;
(3)Lagrange导航星座对地球导航星座的覆盖率高,提高了自主定轨精度;(3) The Lagrange navigation constellation has a high coverage rate of the earth navigation constellation, which improves the accuracy of autonomous orbit determination;
(4)利用自适应非线性滤波算法在线实时估计系统噪声的统计特性,提高了自主定轨的滤波算法精度和稳定性,从而提高自主定轨精度。(4) Using the adaptive nonlinear filtering algorithm to estimate the statistical characteristics of the system noise online in real time, the accuracy and stability of the filtering algorithm for autonomous orbit determination are improved, thereby improving the accuracy of autonomous orbit determination.
附图说明Description of drawings
图1为基于星间测距的地球-Lagrange联合星座自主定轨系统构成示意图;Figure 1 is a schematic diagram of the composition of the Earth-Lagrange joint constellation autonomous orbit determination system based on inter-satellite ranging;
图2为基于星间测距的地球-Lagrange联合星座自主定轨方法结构图;Fig. 2 is the structure diagram of the method for autonomous orbit determination of the Earth-Lagrange joint constellation based on inter-satellite ranging;
图3为基于自适应非线性滤波的自主导航算法流程图;3 is a flowchart of an autonomous navigation algorithm based on adaptive nonlinear filtering;
图4为实施例系统精度随bQ、bC、bq变化趋势图;Fig. 4 is the variation trend diagram of the system accuracy of the embodiment with b Q , b C , and b q ;
图5为实施例GNSS卫星的位置误差曲线图。FIG. 5 is a position error graph of an embodiment GNSS satellite.
具体实施方式Detailed ways
下面将结合附图和实施例对本发明作进一步的详细说明。The present invention will be further described in detail below with reference to the accompanying drawings and embodiments.
本发明是一种基于星间测距的地球-Lagrange联合星座自主定轨方法,其系统构成见图1,图中显示该联合星座定轨系统由地球导航星座及其星间链路测距、Lagrange导航星座及其星间链路测距以及两星座卫星间的星间链路测距构成,其中地球导航星座由m颗中/高轨卫星组成,编号依次为1,2,…,i,…m;Lagrange导航星座由n颗运行在L1和L2点附近Halo周期轨道上的卫星组成,编号依次为1,2,…,k,…n。一种基于星间测距的地球-Lagrange联合星座自主定轨方法的基本实现过程参见图2,图中显示该定轨方法的基本实现过程主要包括测量信息获取和星座轨道参数估计。其中获取的测量信息包括地球导航星座内部的星间距离测量信息、Lagrange导航星座内部的星间距离测量信息以及地球导航卫星和Lagrange导航卫星间的距离测量信息三类距离测量信息;在进行星座轨道参数估计时,①基于地球卫星和Lagrange卫星的简化轨道动力学模型建立联合星座定轨系统的状态方程,②建立三类距离测量信息的测量方程,③利用由状态方程和测量方程构成的系统模型,采用合适的自适应非线性滤波算法,实现轨道参数的估计;最后,输出估计得到的星座中卫星的位置和速度。在地心惯性坐标系和质心会和坐标系下,采用直角坐标描述法(即用位置和速度分量来表示卫星当前的运行状态),利用自适应非线性滤波估计方法,结合根据轨道动力学方程和测量信息建立的系统模型,实现地球-Lagrange联合星座的自主定轨,具体步骤为:The present invention is an autonomous orbit determination method based on inter-satellite ranging based on the Earth-Lagrange joint constellation, and its system structure is shown in Figure 1. The figure shows that the joint constellation orbit determination system consists of the earth navigation constellation and its inter-satellite link ranging, The Lagrange navigation constellation and its inter-satellite link ranging, as well as the inter-satellite link ranging between the two constellations of satellites, consist of the earth navigation constellation consisting of m medium/high-orbit satellites, numbered 1,2,...,i, ...m; the Lagrange Navigation Constellation consists of n satellites operating in Halo periodic orbits near L 1 and L 2 , numbered 1, 2, ..., k, ... n in order. Figure 2 shows the basic implementation process of an Earth-Lagrange joint constellation autonomous orbit determination method based on inter-satellite ranging, which shows that the basic implementation process of the orbit determination method mainly includes measurement information acquisition and constellation orbit parameter estimation. The acquired measurement information includes three types of distance measurement information: the inter-satellite distance measurement information within the Earth Navigation Constellation, the inter-satellite distance measurement information within the Lagrange Navigation Constellation, and the distance measurement information between the Earth Navigation Satellite and the Lagrange Navigation Satellite; In parameter estimation, ① the state equation of the joint constellation orbit determination system is established based on the simplified orbital dynamics model of the Earth satellite and the Lagrange satellite, ② the measurement equation of the three types of distance measurement information is established, and ③ the system model composed of the state equation and the measurement equation is used. , using a suitable adaptive nonlinear filtering algorithm to estimate the orbit parameters; finally, output the estimated position and velocity of the satellites in the constellation. Under the geocentric inertial coordinate system and the center of mass meeting coordinate system, the Cartesian coordinate description method is used (that is, the current operating state of the satellite is represented by the position and velocity components), and the adaptive nonlinear filtering estimation method is used. The system model established with the measurement information realizes the autonomous orbit determination of the Earth-Lagrange joint constellation. The specific steps are:
步骤一:在集中式结构下,建立地球-Lagrange联合星座自主定轨系统的状态方程;Step 1: Under the centralized structure, establish the state equation of the Earth-Lagrange joint constellation autonomous orbit determination system;
准确的系统模型是保障星座运行状态参数估计精度的主要因素之一。本发明基于卫星轨道动力学模型来建立系统状态方程。An accurate system model is one of the main factors to ensure the accuracy of constellation operating state parameter estimation. The present invention establishes the system state equation based on the satellite orbit dynamics model.
(1)地球导航卫星轨道动力学模型(1) Earth Navigation Satellite Orbit Dynamics Model
地球导航卫星主要是中高轨卫星,受到地球的质心引力作用远大于其他作用力,一般采用受摄二体问题动力学模型。为了满足计算高效和高精度的要求,根据摄动力影响大小来选择主要摄动项建模。对于中、高轨卫星来说,在诸多摄动项中,地球非球形对称带来的摄动影响可达104米级,其中3阶以上引力场摄动影响与J2项相比小很多,可以忽略;日月引力摄动影响可达103米级;太阳光压摄动影响可达102米级;而潮汐、相对论效应和反照光压摄动等其他摄动的影响在10-1米级以下,可以忽略;同时高轨处大气密度甚微,大气阻力摄动影响可以忽略。因此,本发明主要考虑了地球质心引力以及J2项和日、月引力三种主要摄动力构成的轨道动力学模型来建立系统状态方程。Earth navigation satellites are mainly medium and high-orbit satellites, and the gravitational force of the earth's center of mass is far greater than other forces. Generally, the dynamic model of the received two-body problem is adopted. In order to meet the requirements of computational efficiency and high precision, the main perturbation term is selected according to the influence of the perturbation force. For medium- and high-orbit satellites, among many perturbation terms, the perturbation effect caused by the non-spherical symmetry of the earth can reach the order of 10 4 meters, of which the perturbation effect of the gravitational field of order 3 and above is much smaller than that of the J 2 term. , can be neglected; the influence of sun-moon gravitational perturbation can reach 10 3 meters; the influence of solar light pressure perturbation can reach 10 2 meters ; Below 1 meter level, it can be ignored; at the same time, the atmospheric density at high orbit is very small, and the influence of atmospheric resistance perturbation can be ignored. Therefore, the present invention mainly considers the orbital dynamics model composed of the earth's centroid gravitational force and the J 2 term and three main perturbing forces of sun and moon gravitational force to establish the system state equation.
在地心直角惯性坐标系下,结合轨道动力学模型建立对联合星座中待测地球卫星i进行定轨的状态方程如下:In the earth-centered rectangular inertial coordinate system, combined with the orbital dynamics model, the state equation for orbit determination of the earth satellite i to be measured in the joint constellation is established as follows:
式中,待测地球卫星i对应的状态向量为这里[xEi,yEi,zEi]T和分别为该地球卫星的位置矢量和速度矢量。FE为系统状态函数,WEi(t)为系统噪声,满足均值为qEi(t),方差为QEi(t)的高斯白噪声。式(1)可以进一步详细写为:In the formula, the state vector corresponding to the earth satellite i to be measured is where [x Ei , y Ei , z Ei ] T and are the position vector and velocity vector of the earth satellite, respectively. F E is the system state function, W Ei (t) is the system noise, satisfying the Gaussian white noise with mean value q Ei (t) and variance Q Ei (t). Equation (1) can be further written as:
其中,和为x、y、z三轴速度噪声分量,和是x、y、z三轴加速度等效噪声分量,包括未建模摄动项和噪声项;和分别为地球卫星i对应的已建模速度矢量和加速度矢量,其中加速度主要考虑地球中心引力加速度a0,Ei、J2摄动项加速度和日月引力摄动加速度aMS,Ei,具体表达式如下:in, and is the three-axis velocity noise component of x, y, and z, and is the equivalent noise component of the x, y, and z three-axis acceleration, including the unmodeled perturbation term and noise term; and are the modeled velocity vector and acceleration vector corresponding to the earth satellite i respectively, in which the acceleration mainly considers the acceleration of the earth's center gravitational acceleration a 0, Ei , J 2 perturbation term and the sun-moon gravitational perturbation acceleration a MS,Ei , the specific expression is as follows:
1)本发明考虑的卫星i的地球中心引力加速度a0,Ei满足:1) the earth center gravitational acceleration a 0 of the satellite i considered by the present invention, Ei satisfies:
式中,为待测卫星i的地心距,μ为地球质量ME与引力常数G的乘积,即地球引力常数。In the formula, is the geocentric distance of the satellite i to be measured, and μ is the product of the earth's mass ME and the gravitational constant G, that is, the earth's gravitational constant.
2)J2摄动项加速度满足:2) J 2 perturbation term acceleration Satisfy:
式中,Re为地球赤道半径,J2为二阶带谐系数。In the formula, Re is the equatorial radius of the earth, and J 2 is the second-order harmonic coefficient.
3)日月引力引起的摄动加速度aMS,Ei满足:3) The perturbation acceleration a MS,Ei caused by the gravity of the sun and the moon satisfies:
式中,(xS,yS,zS)和(xM,yM,zM)分别为太阳和月球在地心直角惯性坐标系下的三维位置坐标,和分别为卫星i到太阳和月球的距离,和分别为地心到太阳和月球的距离,μS和μM分别为太阳引力常数和月球引力常数。where (x S , y S , z S ) and (x M , y M , z M ) are the three-dimensional position coordinates of the sun and the moon in the earth-centered rectangular inertial coordinate system, respectively, and are the distances from satellite i to the sun and the moon, respectively, and are the distances from the center of the earth to the sun and the moon, respectively, and μ S and μ M are the solar gravitational constant and the lunar gravitational constant, respectively.
(2)Lagrange导航卫星轨道动力学模型(2) Lagrange Navigation Satellite Orbit Dynamics Model
与地球导航卫星不同,Lagrange卫星运行在地月系Lagrange点附近,受到的地球中心引力作用和月球中心引力作用量级相近,所以在描述其运动时,本发明采用圆型限制性三体模型。Different from the earth navigation satellite, the Lagrange satellite operates near the Lagrange point of the Earth-Moon system, and the magnitude of the central gravitational action of the Earth and the central gravitational action of the moon is similar, so when describing its motion, the present invention adopts a circular restricted three-body model.
在质心会合坐标系下,结合轨道动力学模型可建立对Lagrange星座中待测月球卫星k进行定轨的状态方程如下:In the center-of-mass rendezvous coordinate system, combined with the orbital dynamics model, the equation of state for orbit determination of the lunar satellite k to be measured in the Lagrange constellation can be established as follows:
式中,待测Lagrange月球卫星k对应的状态向量为这里[xLk,yLk,zLk]T和分别为该星的无量纲位置矢量和速度矢量,其特征质量、特征长度和特征时间如式(7)所示,其中ME和MM分别为地球质量和月球质量,L为地月距离。FL为系统状态函数,WLk(t)为系统噪声,满足均值为qLk(t),方差为QLk(t)的高斯白噪声。In the formula, the state vector corresponding to the Lagrange lunar satellite k to be tested is where [x Lk , y Lk , z Lk ] T and are the dimensionless position vector and velocity vector of the star, respectively, and its characteristic mass, characteristic length and characteristic time are shown in Equation (7), where M E and M M are the mass of the earth and the moon, respectively, and L is the distance between the earth and the moon. FL is the system state function, and W Lk (t) is the system noise, satisfying the Gaussian white noise with mean value q Lk (t) and variance Q Lk (t).
式(6)可以进一步详细写为:Equation (6) can be further written as:
其中为Lagrange卫星k对应的已建模速度矢量,μ0=MM/(MM+ME),ΔE,Lk、ΔM,Lk分别为Lagrange卫星k的地心距和月心距,和为Lagrange卫星k的x、y、z三轴速度噪声分量,和是Lagrange卫星k的x、y、z三轴加速度等效噪声分量,包括未建模摄动项和噪声项。in is the modeled velocity vector corresponding to the Lagrange satellite k, μ 0 =M M /(M M +M E ), Δ E,Lk , Δ M,Lk are the geocentric and lunar distances of the Lagrange satellite k, respectively, and is the x, y, and z three-axis velocity noise components of the Lagrange satellite k, and is the equivalent noise component of the x, y, and z three-axis acceleration of the Lagrange satellite k, including the unmodeled perturbation term and the noise term.
(3)地球-Lagrange联合星座自主定轨系统的状态方程(3) State equation of the Earth-Lagrange joint constellation autonomous orbit determination system
假设整个自主定轨系统包含m颗地球卫星和n颗Lagrange卫星。根据上述单颗卫星定轨的状态方程(1)和(6),建立集中式结构的星座定轨状态方程如下:It is assumed that the entire autonomous orbit determination system includes m Earth satellites and n Lagrange satellites. According to the state equations (1) and (6) of the above single satellite orbit determination, the state equation of the constellation orbit determination with a centralized structure is established as follows:
即:which is:
式中,为状态向量,F为整个星座定轨系统的状态函数矢量,W(t)表示均值为q(t),方差为Q(t)的系统噪声。In the formula, is the state vector, F is the state function vector of the entire constellation orbit determination system, W(t) represents the system noise with mean q(t) and variance Q(t).
步骤二:在集中式结构下,建立地球-Lagrange联合星座自主定轨系统的测量方程;Step 2: Under the centralized structure, establish the measurement equation of the Earth-Lagrange joint constellation autonomous orbit determination system;
地球-Lagrange联合星座自主定轨系统所用到的观测信息只有星间距离测量,但由于两类卫星的动力学模型是在不同坐标系中建立的,所以整个星座的星间距离测量模型被分为三类:The observation information used by the Earth-Lagrange joint constellation autonomous orbit determination system is only the inter-satellite distance measurement, but since the dynamic models of the two types of satellites are established in different coordinate systems, the inter-satellite distance measurement models of the entire constellation are divided into Three categories:
(1)地球导航卫星间的星间距离测量模型(1) Inter-satellite distance measurement model between earth navigation satellites
对于地球导航卫星,记卫星i和卫星j之间的距离观测量为ρEi,Ej,则有:For earth navigation satellites, denote the observed distance between satellite i and satellite j as ρ Ei,Ej , then we have:
ρEi,Ej=hE(XEi,XEj)+vEi,Ej,i≠j (11)ρ Ei,Ej =h E (X Ei ,X Ej )+v Ei,Ej , i≠j (11)
其中vEi,Ej为卫星i和卫星j之间的距离等效测量噪声,包括建模误差和量测噪声。in v Ei,Ej is the distance equivalent measurement noise between satellite i and satellite j, including modeling error and measurement noise.
(2)Lagrange导航卫星间的星间距离测量模型(2) Inter-satellite distance measurement model between Lagrange navigation satellites
记Lagrange卫星i和j之间的距离观测量为ρLi,Lj,有:Denote the observed distance between Lagrange satellites i and j as ρ Li,Lj , we have:
ρLi,Lj=hL(XLi,XLj)+vLi,Lj,i≠j (12)ρ Li,Lj =h L (X Li ,X Lj )+v Li,Lj , i≠j (12)
其中vLi,Lj为Lagrange卫星i和j之间的距离等效测量噪声,包括建模误差和量测噪声。in v Li, Lj is the distance equivalent measurement noise between Lagrange satellites i and j, including modeling error and measurement noise.
(3)地球导航卫星和Lagrange卫星间的测量模型(3) Measurement model between earth navigation satellites and Lagrange satellites
为了表示GNSS卫星i和Lagrange卫星k之间的距离关系,需要将两颗卫星的位置参数放在同一坐标系中表示,则有:In order to represent the distance relationship between the GNSS satellite i and the Lagrange satellite k, the position parameters of the two satellites need to be represented in the same coordinate system, as follows:
其中,是Lagrange卫星在地心惯性坐标系中的位置向量,它是关于Lagrange卫星在质心会合坐标系中的状态向量XLk中的无量纲位置向量[xLk,yLk,zLk]T的函数,其转换关系为:in, is the position vector of the Lagrange satellite in the geocentric inertial coordinate system, which is a function of the dimensionless position vector [x Lk , y Lk , z Lk ] T in the state vector X Lk of the Lagrange satellite in the center of mass rendezvous coordinate system, Its conversion relationship is:
其中,R表示由质心会合坐标系到地心惯性坐标系的旋转矩阵,表达式如下:Among them, R represents the rotation matrix from the convergent coordinate system of the center of mass to the inertial coordinate system of the earth's center, and the expression is as follows:
其中uM=ωM+θM,iM、ΩM、ωM和θM分别表示月球绕地轨道的轨道倾角、升交点赤经、近地点幅角以及真近点角。where u M = ω M + θ M , i M , Ω M , ω M and θ M represent the orbital inclination of the moon's orbit around the Earth, the right ascension of the ascending node, the argument of perigee and the true perigee angle, respectively.
(4)地球-Lagrange联合星座自主定轨系统的测量方程(4) Measurement equation of the Earth-Lagrange joint constellation autonomous orbit determination system
根据上述测量方程(11)、(12)和(13),建立集中式结构的星座定轨测量方程如下:According to the above measurement equations (11), (12) and (13), the constellation orbit determination measurement equation with a centralized structure is established as follows:
Z(t)=h[X(t),t]+V(t) (16)Z(t)=h[X(t),t]+V(t) (16)
即:which is:
其中V(t)为零均值,方差为R(t)的等效测量噪声。式(17)给出的是一般情况下的观测方程,在实际应用时,某些距离测量量会受到地球或者月球的遮挡等因素的影响而出现不可测的情况,这时需要从式(17)中将相应的测距信息剔除。where V(t) is zero mean and the variance is the equivalent measurement noise of R(t). Equation (17) gives the observation equation in general. In practical application, some distance measurements will be affected by factors such as the occlusion of the earth or the moon, resulting in unmeasurable situations. ), the corresponding ranging information will be eliminated.
步骤三:根据上述建立的基于星间距离测量的地球-Lagrange联合星座自主定轨系统模型,确定实现轨道参数估计的滤波方法;Step 3: According to the above-established Earth-Lagrange joint constellation autonomous orbit determination system model based on inter-satellite distance measurement, determine a filtering method for realizing orbit parameter estimation;
该非线性系统的状态需要采用非线性滤波方法来估计。常规的非线性滤波方法,如EKF、UKF、容积滤波和粒子滤波等,在噪声的先验统计信息精确已知的情况下可以获得较为理想的结果。但是在本系统中,等效系统噪声Wk除了包含未建模误差之外,还包含滤波算法中的离散化误差(和线性化误差),这使得噪声具有时变非高斯统计特性,且难以准确获取。为此,一般在应用这些非线性滤波算法时,通常将噪声近似为平稳随机白噪声序列,即认为Qk≡Q,并根据经验来确定Q。为了保证在整个滤波过程中状态估计误差能收敛到稳定值,Q的取值往往偏大,即满足Q≥max{Qk},这使得系统性能难以达到最优。The state of the nonlinear system needs to be estimated using nonlinear filtering methods. Conventional nonlinear filtering methods, such as EKF, UKF, volumetric filtering and particle filtering, can achieve ideal results when the prior statistical information of noise is accurately known. However, in this system, the equivalent system noise Wk not only contains the unmodeled error, but also contains the discretization error (and linearization error) in the filtering algorithm, which makes the noise have time-varying non-Gaussian statistical characteristics, and it is difficult to Accurately obtain. For this reason, when applying these nonlinear filtering algorithms, the noise is usually approximated as a stationary random white noise sequence, that is, Q k ≡ Q, and Q is determined empirically. In order to ensure that the state estimation error can converge to a stable value during the entire filtering process, the value of Q is often too large, that is, to satisfy Q≥max {Qk}, which makes it difficult to achieve optimal system performance.
为了解决这一问题,本发明在常规非线性滤波算法的基础上,结合Sage-Husa自适应算法的思想对系统噪声的统计特性进行在线估计和修正,以提高滤波的精度和稳定性。考虑到工程实用性,本发明采用自适应EKF方法或自适应Sigma点卡尔曼滤波(SigmaPoints Kalman Filter,SPKF)方法,实现卫星轨道参数估计。In order to solve this problem, the present invention, based on the conventional nonlinear filtering algorithm, combines the idea of Sage-Husa adaptive algorithm to estimate and correct the statistical characteristics of the system noise online, so as to improve the filtering accuracy and stability. Considering the practicality of the project, the present invention adopts the adaptive EKF method or the adaptive Sigma Points Kalman Filter (SPKF) method to realize the estimation of satellite orbit parameters.
第一,当系统对运算速度要求较高或系统存储空间较小时,采用自适应EKF方法对经过离散化后的非线性系统进行状态估计。自适应EKF的基本思想是利用泰勒级数展开的方法对连续非线性的状态方程和观测方程进行离散化和线性化处理,然后在经典卡尔曼滤波的基础上,通过时变噪声统计估值器,实时估计和修正系统噪声和观测噪声的统计特性,再进行状态估计。具体步骤如下:First, when the system has high requirements on the operation speed or the system storage space is small, the adaptive EKF method is used to estimate the state of the discretized nonlinear system. The basic idea of the adaptive EKF is to use the Taylor series expansion method to discretize and linearize the continuous nonlinear state equation and observation equation, and then use the time-varying noise statistical estimator on the basis of the classical Kalman filter. , estimate and correct the statistical characteristics of system noise and observation noise in real time, and then perform state estimation. Specific steps are as follows:
(1)时间更新(1) Time update
计算一步预测状态:Compute the one-step predicted state:
式中,为k时刻的系统噪声均值的估计值,为利用动力学方程进行的状态一步递推,一种方法是通过离散化和线性化后的方程(19)计算得到,其中为k时刻的状态估计,为(k+1)时刻的一步预测状态估计,Δt为积分步长;另一种方法是通过4阶Runge-Kutta(RK4)方法直接对连续状态方程(9)数值积分计算得到。In the formula, is the estimated value of the mean value of the system noise at time k, For the one-step recurrence of states using the kinetic equation, one method is computed by discretizing and linearizing equation (19), where is the state estimate at time k, is the one-step predicted state estimation at (k+1) time, and Δt is the integration step size; another method is to directly numerically integrate the continuous state equation (9) by the fourth-order Runge-Kutta (RK4) method.
计算状态转移矩阵:Compute the state transition matrix:
式中,Φk+1/k为从k时刻到(k+1)时刻的状态转移矩阵。In the formula, Φ k+1/k is the state transition matrix from time k to time (k+1).
计算一步预测误差协方差矩阵:Compute the one-step forecast error covariance matrix:
式中,Pk+1/k为一步预测状态的误差协方差矩阵,Pk为k时刻估计状态的误差协方差矩阵,为k时刻系统噪声方差阵的估计值。In the formula, P k+1/k is the error covariance matrix of the one-step prediction state, P k is the error covariance matrix of the estimated state at time k, is the estimated value of the system noise variance matrix at time k.
考虑到滤波初始的一段时间内系统状态估计误差尚未收敛且用于估计系统噪声的样本较少,此时估计的噪声统计特性波动较大且不够准确,将使滤波收敛较慢,严重时甚至导致滤波发散。因此在滤波初始的一段时间内(0~T),本算法并不将估计的噪声统计特性应用于时间更新过程,而是采用噪声的先验统计信息,此时的时间更新算法如下:Considering that the system state estimation error has not converged in the initial period of filtering and there are few samples used to estimate the system noise, the estimated noise statistical characteristics fluctuate greatly and are not accurate enough at this time, which will make the filtering converge slowly, and even lead to severe cases. Filter divergence. Therefore, during the initial period of filtering (0~T), this algorithm does not apply the estimated noise statistical characteristics to the time update process, but uses the prior statistical information of the noise. The time update algorithm at this time is as follows:
(2)测量更新:(2) Measurement update:
计算增益矩阵:Calculate the gain matrix:
式中,Kk+1为(k+1)时刻的增益矩阵,为基于一步预测状态估计计算的观测向量h的Jacobian矩阵,Rk+1为(k+1)时刻测量噪声协方差阵。In the formula, K k+1 is the gain matrix at time (k+1), is a state estimation based on one-step prediction The Jacobian matrix of the calculated observation vector h, R k+1 is the measurement noise covariance matrix at the time (k+1).
计算新息向量:Compute the innovation vector:
式中υk+1为(k+1)时刻的新息向量,Zk+1为(k+1)时刻的测量向量。In the formula, υ k+1 is the innovation vector at time (k+1), and Z k+1 is the measurement vector at time (k+1).
计算状态估计值:Compute the state estimate:
计算状态估计误差协方差阵:Compute the state estimation error covariance matrix:
计算系统噪声统计特性的估计值:Compute an estimate of the noise statistics of the system:
其中,in,
式中0<bq<1,0<bQ<1,0<bC<1分别为计算q、Q、C的遗忘因子。随着k的增大, 和的值分别趋向于(1-bq)、(1-bQ)和(1-bC),因此bq、bQ和bC越大,当前信息的比重越小。侧重于跟踪系统噪声均值q的变化,取值过大会使偏小,取值过小则会引起滤波发散;侧重于平滑的取值,取值过小平滑效果较差,取值过大则使偏小,增大了滤波发散的风险;用来跟踪方差C的变化,取值过小会使估值的波动变大,取值过大则会使跟踪产生延迟。In the formula, 0<b q <1, 0<b Q <1, and 0<b C <1 are the forgetting factors for calculating q, Q, and C, respectively. As k increases, and The values of are tending to (1-b q ), (1-b Q ) and (1-b C ) respectively, so the larger b q , b Q and b C are, the smaller the weight of current information is. Focus on tracking the change of the system noise mean q, if the value is too large, it will make the If the value is too small, it will cause filter divergence; focus on smoothness The value of , if the value is too small, the smoothing effect is poor, and if the value is too large, the It is too small, which increases the risk of filter divergence; It is used to track the change of variance C. If the value is too small, the fluctuation of the valuation will increase, and if the value is too large, the tracking will be delayed.
在实际应用时,虽然式(29)和(30)的计算具有一定的平滑作用,但仍然会出现负定的情况,为了保证滤波的稳定,在负定的情况下对式(29)中的项的对角线元素取绝对值,非对角线元素取0来近似处理。In practical applications, although the calculations of equations (29) and (30) have a certain smoothing effect, there will still be In the case of negative definite, in order to ensure the stability of filtering, in the case of negative definite The diagonal elements of the item take the absolute value, and the off-diagonal elements take 0 for approximation.
第二,当系统更注重精度指标,而对运算速度和占用存储空间无特别限制时,采用自适应的Sigma点Kalman滤波(Sigma Points Kalman Filter,SPKF)方法对连续非线性系统进行状态估计。自适应SPKF的基本思想是将根据确定性采样策略得到的Sigma采样点经非线性函数直接传递,然后在经典卡尔曼滤波算法框架的基础上,通过时变噪声统计估值器,实时估计和修正系统噪声和观测噪声的统计特性,再进行状态估计。具体步骤如下:Second, when the system pays more attention to the accuracy index, and there is no special restriction on the operation speed and occupied storage space, the adaptive Sigma Points Kalman Filter (SPKF) method is used to estimate the state of the continuous nonlinear system. The basic idea of adaptive SPKF is to directly transfer the Sigma sampling points obtained according to the deterministic sampling strategy through a nonlinear function, and then, on the basis of the classical Kalman filter algorithm framework, through the time-varying noise statistical estimator, real-time estimation and correction Statistical characteristics of system noise and observation noise, and then state estimation. Specific steps are as follows:
1)选择Sigma点采样策略1) Select the Sigma point sampling strategy
目前常用的Sigma点采样策略有对称采样、单形采样、中心差分采样和容积采样等多种采样方式。选择一种采样策略,计算SPKF的权系数Wi m、Wi c,其中i=0,1,…,L,L为由具体的采样策略决定的采样点个数,Wi m用于均值估计,Wi c用于方差估计。At present, the commonly used Sigma point sampling strategies include symmetric sampling, simplex sampling, central difference sampling and volume sampling. Select a sampling strategy and calculate the weight coefficients W i m and W i c of SPKF, where i =0,1,...,L, L is the number of sampling points determined by the specific sampling strategy, and Wi m is used for the mean value estimate, W ic is used for variance estimation.
2)时间更新:2) Time update:
根据1)中选择的采样策略以及k时刻的状态估计值和估计误差协方差Pk计算k时刻的Sigma点集χi,k(i=0,1,…,L)。According to the sampling strategy selected in 1) and the state estimate value at time k and the estimated error covariance P k to calculate the Sigma point set χ i,k (i=0,1,...,L) at time k.
计算Sigma点的一步预测值:Calculate the one-step predicted value of the Sigma point:
χi,k+1/k=F[χi,k,k],i=0,1,…,L (34)χ i,k+1/k =F[χ i,k ,k], i=0,1,...,L (34)
其中,χi,k为第i个Sigma点在k时刻的值,χi,k+1/k为第i个Sigma点在k+1时刻的一步预测值。Among them, χ i,k is the value of the i-th Sigma point at time k, and χ i,k+1/k is the one-step prediction value of the i-th Sigma point at
计算一步预测状态:Compute the one-step predicted state:
式中,为k时刻的系统噪声均值的估计值,为(k+1)时刻的一步预测状态估计。In the formula, is the estimated value of the mean value of the system noise at time k, is the one-step predicted state estimate at time (k+1).
计算状态一步预测误差协方差矩阵:Compute the state one-step prediction error covariance matrix:
式中,Pk+1/k为一步预测状态的误差协方差矩阵,为k时刻系统噪声方差阵的估计值;In the formula, P k+1/k is the error covariance matrix of the one-step prediction state, is the estimated value of the system noise variance matrix at time k;
在滤波初始的时间0~T内,采用噪声的先验统计信息,时间更新如下:Within the
3)测量更新:3) Measurement update:
根据1)中选择的采样策略以及和Pk+1/k更新Sigma点集;According to the sampling strategy selected in 1) and Update the Sigma point set with P k+1/k ;
估计测量值:Estimated measurements:
γi,k+1/k=h(χi,k+1/k) (39)γ i, k+1/k = h(χ i, k+1/k ) (39)
其中γi,k+1/k为由第i个Sigma点计算的第(k+1)时刻测量向量的估计值,为第(k+1)时刻测量向量的加权估计值。where γ i,k+1/k is the estimated value of the measurement vector at the (k+1)th time calculated by the i-th Sigma point, is the weighted estimate of the measurement vector at the (k+1)th time.
计算增益矩阵:Calculate the gain matrix:
其中,Rk+1为(k+1)时刻测量噪声协方差阵,Py,k+1/k为第(k+1)时刻测量向量估计值的协方差,Pxy,k+1/k为第(k+1)时测量向量估计值与状态一步预测值的协方差,Kk+1为(k+1)时刻的增益矩阵。Among them, R k+1 is the measurement noise covariance matrix at the time (k+1), P y,k+1/k is the covariance of the estimated value of the measurement vector at the (k+1)th time, P xy,k+1/ k is the covariance between the estimated value of the measurement vector and the state one-step predicted value at the (k+1)th time, and K k+1 is the gain matrix at the (k+1) time.
计算新息向量:Compute the innovation vector:
式中υk+1为(k+1)时刻的新息向量,Zk+1为(k+1)时刻的测量向量;where υ k+1 is the innovation vector at (k+1) time, and Z k+1 is the measurement vector at (k+1) time;
计算(k+1)时刻的状态估计值 Calculate the state estimate at time (k+1)
计算(k+1)时刻的状态估计误差协方差阵Pk+1:Calculate the state estimation error covariance matrix P k+1 at time (k+1):
4)计算系统噪声统计特性的估计值:4) Calculate the estimated value of the statistical characteristics of the system noise:
其中,in,
式中0<bq<1,0<bQ<1,0<bC<1分别为计算q、Q、C的遗忘因子。In the formula, 0<b q <1, 0<b Q <1, and 0<b C <1 are the forgetting factors for calculating q, Q, and C, respectively.
当出现负定的情况时,对式(48)中的项的对角线元素取绝对值,非对角线元素取0。when it appears In the case of negative definiteness, for Eq. (48) The diagonal elements of the item take the absolute value, and the off-diagonal elements take 0.
步骤四:在集中式结构下,基于选定滤波方法的地球-Lagrange联合星座自主定轨算法的具体实现;Step 4: Concrete realization of the Earth-Lagrange joint constellation autonomous orbit determination algorithm based on the selected filtering method under the centralized structure;
根据本发明提出的自适应非线性滤波算法实现地球-Lagrange联合星座自主定轨算法的流程图参见图4,具体过程如下:The flowchart of realizing the autonomous orbit determination algorithm of the Earth-Lagrange joint constellation according to the adaptive nonlinear filtering algorithm proposed by the present invention is shown in Figure 4, and the specific process is as follows:
具体过程如下:The specific process is as follows:
(1)数据初始化;(1) Data initialization;
初始化的参数包括:k=0,滤波步长h,噪声切换参数T,初始状态初始误差协方差阵P0、初始系统噪声均值初始系统噪声方差阵测量噪声方差阵R以及遗忘因子bq、bQ、bC;The initialized parameters include: k=0, filter step size h, noise switching parameter T, initial state Initial error covariance matrix P 0 , initial system noise mean Initial system noise variance matrix Measure the noise variance matrix R and forgetting factors b q , b Q , b C ;
其中,噪声切换参数T为时间更新算法中噪声统计特性切换的时间节点:当k<T时,使用噪声的先验统计特性进行时间更新;当k≥T时,使用估计的噪声统计特性进行时间更新;初始状态初始误差协方差阵P0、初始系统噪声方差阵根据需要确定;初始系统噪声均值取零;测量噪声方差阵R根据测量设备的性能确定;遗忘因子bq、bQ取值介于0.99~1.0之间,bC取值介于0.9~0.99之间;Among them, the noise switching parameter T is the time node for switching the statistical characteristics of noise in the time update algorithm: when k<T, use the prior statistical characteristics of noise for time update; when k≥T, use the estimated statistical characteristics of noise to perform time update update; initial state Initial error covariance matrix P 0 , initial system noise variance matrix Determined as needed; initial system noise mean Take zero; the measurement noise variance matrix R is determined according to the performance of the measurement equipment; the forgetting factors b q and b Q are between 0.99 and 1.0, and the value of b C is between 0.9 and 0.99;
(2)如果采用自适应EKF算法,直接转到(4);如果采用自适应SPKF算法,转到(3);(2) If the adaptive EKF algorithm is adopted, go directly to (4); if the adaptive SPKF algorithm is adopted, go to (3);
(3)根据选择的Sigma点采样策略计算权系数Wi m、Wi c;(3) Calculate the weight coefficients W i m and W i c according to the selected Sigma point sampling strategy;
(4)如果k<T,采用噪声的先验统计特性进行时间更新,转到(5);否则采用估计的噪声统计特性进行时间更新,转到(6);(4) If k<T, use the priori statistical characteristics of noise to perform time update, and go to (5); otherwise, use the estimated noise statistical characteristics to perform time update, and go to (6);
(5)采用噪声的先验统计特性的时间更新;完成后转到(7);(5) Time update using a priori statistical characteristics of noise; go to (7) after completion;
利用k时刻的状态估计及误差协方差阵Pk作为k时刻的状态初值及误差协方差阵,依次计算状态一步预测值及预测误差协方差矩阵Pk+1/k,实现自适应Kalman滤波估计方法的时间更新。当采用自适应EKF算法时,计算公式分别为式(22)和式(23);当采用自适应SPKF算法时,计算公式分别为式(37)和(38);Using state estimation at time k and the error covariance matrix P k as the initial state value and the error covariance matrix at time k, and calculate the state one-step prediction value in turn and the prediction error covariance matrix P k+1/k , to realize the time update of the adaptive Kalman filter estimation method. When the adaptive EKF algorithm is adopted, the calculation formulas are formula (22) and formula (23) respectively; when the adaptive SPKF algorithm is adopted, the calculation formulas are formulas (37) and (38) respectively;
(6)采用估计的噪声统计特性的时间更新;(6) Using the time update of the estimated noise statistics;
利用k时刻的状态估计及误差协方差阵Pk作为k时刻的状态初值及误差协方差阵,依次计算状态一步预测值及预测误差协方差矩阵Pk+1/k,实现自适应Kalman滤波估计方法的时间更新。当采用自适应EKF算法时,计算公式分别为式(18)和式(21);当采用自适应SPKF算法时,计算公式分别为式(35)和(36);Using state estimation at time k and the error covariance matrix P k as the initial state value and the error covariance matrix at time k, and calculate the state one-step prediction value in turn and the prediction error covariance matrix P k+1/k , to realize the time update of the adaptive Kalman filter estimation method. When the adaptive EKF algorithm is used, the calculation formulas are formula (18) and formula (21) respectively; when the adaptive SPKF algorithm is used, the calculation formulas are formulas (35) and (36) respectively;
(7)测量更新;(7) Measurement update;
依次计算(k+1)时刻的增益矩阵Kk+1、新息矩阵υk+1、状态估计值及误差协方差矩阵Pk+1,实现自适应Kalman滤波的测量更新。当采用自适应EKF算法时,计算公式分别为式(24)~(27);当采用自适应SPKF算法时,计算公式分别为式(43)~(46);Calculate the gain matrix K k+1 , the innovation matrix υ k+1 , and the state estimation value at (k+1) time in turn and the error covariance matrix P k+1 to realize the measurement update of the adaptive Kalman filter. When the adaptive EKF algorithm is adopted, the calculation formulas are respectively equations (24) to (27); when the adaptive SPKF algorithm is adopted, the calculation formulas are respectively equations (43) to (46);
(8)估计系统噪声统计特性;(8) Estimate the statistical characteristics of system noise;
依次计算系统噪声的均值估计值和协方差估计值当采用自适应EKF算法时,计算公式分别为式(28)和(29);当采用自适应SPKF算法时,计算公式分别为式(47)和(48);Calculate the mean estimate of the system noise in turn and covariance estimates When the adaptive EKF algorithm is used, the calculation formulas are formulas (28) and (29) respectively; when the adaptive SPKF algorithm is used, the calculation formulas are formulas (47) and (48) respectively;
(9)判断滤波过程是否结束;如需继续进行滤波,k=k+1,并返回到(4)。(9) Determine whether the filtering process is over; if it is necessary to continue filtering, k=k+1, and return to (4).
本发明首先研究仅利用星间距离测量时存在的“亏秩”问题,引入Lagrange卫星来提供绝对基准;然后在集中式结构下,采用自适应非线性滤波估计方法,实现地球-Lagrange联合星座的自主定轨。The present invention firstly studies the problem of "deficient rank" when only using inter-satellite distance measurement, and introduces Lagrange satellites to provide an absolute reference; Autonomous track.
本发明提出的一种基于星间测距的地球-Lagrange联合星座自主定轨方法,该方法首先在集中式结构下建立地球-Lagrange联合星座的状态方程;然后建立地球-Lagrange联合星座的测量方程;最后采用自适应非线性滤波方法实现地球-Lagrange联合的自主定轨。A method for autonomous orbit determination of the Earth-Lagrange joint constellation based on inter-satellite ranging proposed by the present invention firstly establishes the state equation of the Earth-Lagrange joint constellation under a centralized structure; then establishes the measurement equation of the Earth-Lagrange joint constellation ; Finally, an adaptive nonlinear filtering method is used to realize the autonomous orbit determination of the Earth-Lagrange joint.
实施例:Example:
以某地球-Lagrange星座为例,该星座由3颗MEO卫星和2颗Lagrange卫星构成。MEO卫星编号为E1~E3;Lagrange卫星编号为L1~L2。在仿真中发现,MEO星座中各卫星的定轨精度近似,Lagrange星座中各卫星的定轨精度也近似,因此文中仅以编号为E1的MEO卫星和编号为L1的Lagrange卫星为例进行说明。Take an Earth-Lagrange constellation as an example, the constellation consists of 3 MEO satellites and 2 Lagrange satellites. The MEO satellites are numbered E 1 to E 3 ; the Lagrange satellites are numbered L 1 to L 2 . In the simulation, it is found that the orbit determination accuracy of each satellite in the MEO constellation is similar, and the orbit determination accuracy of each satellite in the Lagrange constellation is also similar. Therefore, only the MEO satellite numbered E 1 and the Lagrange satellite numbered L 1 are used as examples in this paper. illustrate.
仿真条件:Simulation conditions:
采用STK来模拟星座实际运行情况,产生星座运行过程中的标称轨道数据,。STK is used to simulate the actual operation of the constellation, and to generate the nominal orbit data during the operation of the constellation.
(1)标称数据生成参数设置(1) Nominal data generation parameter setting
仿真时间为2016年1月1日12:00:00—2016年6月28日12:00:00,历时180d,步长T=1s。地球卫星的轨道动力学模型采用高精度轨道预报模型(The High-precision orbitpropagator,HPOP),其中地球模型采用WGS84-EGM96模型,考虑21×21阶非球形摄动;其他摄动项包括太阳引力、月球引力、太阳光压(光压系数Cr=1.0)和大气阻力(大气阻力系数Cd=2.2);卫星截面积与卫星质量之比S/m=0.02m2/kg。Lagrange卫星的轨道动力学模型采用圆型限制性三体问题模型。The simulation time is from 12:00:00 on January 1, 2016 to 12:00:00 on June 28, 2016, which lasted 180d, and the step size was T=1s. The orbital dynamics model of the earth satellite adopts the high-precision orbit propagator (HPOP), in which the earth model adopts the WGS84-EGM96 model, which considers 21×21 order aspheric perturbations; other perturbation terms include solar gravity, Lunar gravity, solar light pressure (light pressure coefficient C r =1.0) and atmospheric drag (atmospheric drag coefficient C d =2.2); the ratio of satellite cross-sectional area to satellite mass S/m=0.02m 2 /kg. The orbital dynamics model of the Lagrange satellite adopts a circular restricted three-body problem model.
(2)基本滤波参数设置(2) Basic filter parameter settings
地球卫星的状态方程同样采用受摄二体问题模型,但摄动项仅考虑J2项和日月引力;Lagrange卫星的状态方程采用圆型限制性三体问题模型,滤波周期T=100s。The state equation of the earth satellite also adopts the received two-body problem model, but the perturbation term only considers the J2 term and the gravitational force of the sun and the moon; the state equation of the Lagrange satellite adopts the circular restricted three-body problem model, and the filter period T=100s.
在集中式结构下,地球-Lagrange联合星座自主定轨的系统噪声方差阵初值为Q0=diag([QE1,0 QE2,0 QE3,0 QL1,0 QL2,0]),其中 σLx0=σLy0=σLz0=10-10[L],测量噪声方差阵为σEi,Ej=σEi,Lk=σLk,Ll=5m;初始状态估计误差协方差阵P0=diag([PE1,0 PE2,0 PE3,0 PL1,0 PL2,0]),Under the centralized structure, the initial value of the system noise variance matrix for autonomous orbit determination of the Earth-Lagrange joint constellation is Q 0 =diag([Q E1,0 Q E2,0 Q E3,0 Q L1,0 Q L2,0 ]) ,in σ Lx0 =σ Ly0 =σ Lz0 =10 −10 [L], The measurement noise variance matrix is σ Ei,Ej =σ Ei,Lk =σ Lk,Ll =5m; initial state estimation error covariance matrix P 0 =diag([P E1,0 P E2,0 P E3,0 P L1,0 P L2,0 ]),
其中σEx,0=σEy,0=σEz,0=1m,σLx,0=σLy,0=σLz,0=1m, in σ Ex,0 =σ Ey,0 =σ Ez,0 =1m, σ Lx,0 =σ Ly,0 =σ Lz,0 =1m,
(3)评估方法(3) Evaluation method
因为实际系统中的系统状态和估计误差均为随机量,所以在得到各个仿真时刻的估计误差后,采用统计方法(计算误差数据的均方根误差)来评估星座中卫星的绝对定轨和相对定位的效果。采用滤波估计收敛后的估计状态作为样本来统计误差。均方根误差计算公式如下:Because the system state and estimation error in the actual system are both random quantities, after obtaining the estimation error at each simulation time, a statistical method (calculating the root mean square error of the error data) is used to evaluate the absolute orbit determination and relative relative orbit determination of the satellites in the constellation. positioning effect. The estimated state after the convergence of the filter estimation is used as a sample to calculate the error. The formula for calculating the root mean square error is as follows:
其中,为第i时刻的估计值,Xi为第i时刻的真值,n为数据总数。in, is the estimated value at the i-th moment, X i is the true value at the i-th moment, and n is the total number of data.
为了便于量化分析,这里分别以三轴位置误差的平方和和三轴速度误差的平方和作为卫星定轨的距离误差和速率误差,其均方根误差的计算公式如下:In order to facilitate quantitative analysis, the sum of squares of three-axis position errors and the sum of squares of three-axis velocity errors are used as the distance error and rate error of satellite orbit determination. The calculation formula of the root mean square error is as follows:
卫星距离估计误差:Satellite distance estimation error:
卫星速率估计误差:Satellite rate estimation error:
实施方式:集中式地球-Lagrange联合星座自主定轨系统模型的状态向量由五星的位置、速度构成,采用星间距离测量方式,重点研究自适应EKF对定轨精度的提高。Implementation: The state vector of the centralized Earth-Lagrange joint constellation autonomous orbit determination system model is composed of the positions and speeds of five stars, and the inter-satellite distance measurement method is used, focusing on the improvement of the orbit determination accuracy of the adaptive EKF.
步骤一:建立地球-Lagrange联合星座自主定轨系统的状态方程Step 1: Establish the state equation of the Earth-Lagrange joint constellation autonomous orbit determination system
在地心直角惯性坐标系下,地球导航卫星i的状态向量为其中[xEi,yEi,zEi]T和分别为该星的位置矢量和速度矢量,结合轨道动力学模型式(1)可建立卫星Ei定轨的状态方程:In the earth-centered rectangular inertial coordinate system, the state vector of the earth navigation satellite i is where [x Ei , y Ei , z Ei ] T and are the position vector and velocity vector of the satellite, respectively, combined with the orbital dynamics model formula (1), the state equation of the satellite Ei orbit determination can be established:
式中,卫星Ei的地球中心引力、J2摄动力和日月引力引起的加速度分别为a0,Ei、aJ2,Ei和aMS,Ei,具体定义参见式(3)~式(5)。WEi(t)表示卫星Ei的系统噪声,包含未建模摄动,满足E[WEi(t)]=0,E[WEi(t)WEi(τ)]=QEi(t)δ(t-τ),δ(t-τ)是狄拉克函数,即 In the formula, the acceleration caused by the earth's center gravity, J 2 perturbation force and sun-moon gravity of satellite Ei are a 0,Ei , a J2,Ei and a MS,Ei , respectively. For the specific definitions, please refer to equations (3) to (5) . W Ei (t) represents the system noise of satellite Ei, including unmodeled perturbation, satisfying E[W Ei (t)]=0, E[W Ei (t)W Ei (τ)]=Q Ei (t) δ(t-τ), δ(t-τ) is the Dirac function, that is
Lagrange卫星k对应的状态向量为其中[xLk,yLk,zLk]T和分别为该星的无量纲位置矢量和速度矢量,结合轨道动力学模型式(6)可建立卫星Lk定轨的状态方程:The state vector corresponding to the Lagrange satellite k is where [x Lk , y Lk , z Lk ] T and are the dimensionless position vector and velocity vector of the star, respectively. Combined with the orbital dynamics model formula (6), the state equation for the orbit determination of the satellite L k can be established:
式中,WLk(t)表示卫星Ei的系统噪声,包含未建模摄动,满足E[WLk(t)]=0,E[WLk(t)WLk(τ)]=QLk(t)δ(t-τ)。In the formula, W Lk (t) represents the system noise of satellite Ei, including unmodeled perturbation, satisfying E[W Lk (t)]=0, E[W Lk (t)W Lk (τ)]=Q Lk (t)δ(t-τ).
根据上述单颗卫星的状态方程,可以建立集中式结构的五星星座状态方程如下:According to the state equation of the above single satellite, the state equation of the five-star constellation with a centralized structure can be established as follows:
式中,为包含星座中五颗卫星所有状态的状态向量,W(t)表示系统噪声,满足E[W(t)]=q(t),E[W(t)W(τ)]=Q(t)δ(t-τ)。In the formula, is the state vector containing all states of the five satellites in the constellation, W(t) represents the system noise, which satisfies E[W(t)]=q(t), E[W(t)W(τ)]=Q(t )δ(t-τ).
步骤二:建立地球-Lagrange联合星座自主定轨系统的测量方程Step 2: Establish the measurement equation of the Earth-Lagrange joint constellation autonomous orbit determination system
在集中式结构下,五星星座采用星间链路测量的测量方程如下:Under the centralized structure, the measurement equation of the five-star constellation using the inter-satellite link measurement is as follows:
式中,hE为三颗地球卫星间的测量方程,hEL为地球卫星和Lagrange卫星间的测量方程,hL为两颗Lagrange卫星间的测量方程,参见式(11)~式(13)。In the formula, h E is the measurement equation between the three Earth satellites, h EL is the measurement equation between the Earth satellite and the Lagrange satellite, and h L is the measurement equation between the two Lagrange satellites, see equations (11) to (13) .
V(t)=[ΔEi,Ej…ΔEi,Lk…ΔLk,Ll…]T为经过电离层、对流层延迟等误差补偿之后残余的伪距观测噪声向量,为零均值、标准差为R(t)的白噪声。V(t)=[ ΔEi,Ej … ΔEi,Lk … ΔLk,Ll …] T is the residual pseudorange observation noise vector after error compensation such as ionospheric and tropospheric delays, with zero mean and standard deviation R (t) white noise.
步骤三:在集中式结构下,根据上述建立的地球-Lagrange联合星座自主定轨系统模型,确定实现轨道参数估计的滤波方法。Step 3: Under the centralized structure, according to the above established model of the Earth-Lagrange joint constellation autonomous orbit determination system, determine a filtering method for realizing orbit parameter estimation.
本例要求算法的计算速度快和计算资源需求少,因此采用自适应EKF算法。In this example, the algorithm requires fast calculation speed and less computing resource requirements, so the adaptive EKF algorithm is adopted.
步骤四:在集中式结构下,采用自适应EKF估计方法实现地球-Lagrange五星星座联合自主定轨,并仿真分析地球-Lagrange五星星座联合自主定轨的性能。Step 4: Under the centralized structure, the adaptive EKF estimation method is used to realize the joint autonomous orbit determination of the Earth-Lagrange five-star constellation, and the performance of the joint autonomous orbit determination of the Earth-Lagrange five-star constellation is simulated and analyzed.
结合地球-Lagrange五星星座集中式联合自主定轨流程图(图4)和发明内容步骤四,采用自适应EKF估计方法实现地球-Lagrange五星星座联合自主定轨。Combined with the Earth-Lagrange five-star constellation centralized joint autonomous orbit determination flowchart (Fig. 4) and the fourth step of the invention, the adaptive EKF estimation method is used to realize the Earth-Lagrange five-star constellation joint autonomous orbit determination.
(1)数据初始化。初始化的参数包括:k=0,滤波步长h=100s,阈值T=(10天×86400s/天)/100s,初始状态初始误差协方差阵P0、初始系统噪声均值初始系统噪声方差阵测量噪声方差阵R=5m以及遗忘因子bq=0.9999、bQ=0.9999、bC=0.90。(1) Data initialization. The initialized parameters include: k=0, filter step size h=100s, threshold T=(10 days×86400s/day)/100s, initial state Initial error covariance matrix P 0 , initial system noise mean Initial system noise variance matrix Measurement noise variance matrix R=5m and forgetting factors b q =0.9999, b Q =0.9999, b C =0.90.
注:因为bq取值过小将引起滤波发散,所以这里取一个较大值作为初始值,先调节bQ和bC到最佳值,最后调节bq。Note: Because the value of b q is too small, it will cause filter divergence, so a larger value is taken as the initial value here, first adjust b Q and b C to the best value, and finally adjust b q .
(2)如果k<T,则采用噪声的先验统计特性进行时间更新,转到(3);否则采用估计的噪声统计特性进行时间更新,转到(4)。(2) If k<T, use the prior statistical characteristics of noise to perform time update, and go to (3); otherwise, use the estimated noise statistical characteristics to perform time update, and go to (4).
(3)采用噪声的先验统计特性的时间更新。利用k时刻的状态估计及误差协方差阵Pk作为k时刻的状态初值及误差协方差阵,根据式(22)和式(23)分别计算状态一步预测值及预测误差协方差矩阵Pk+1/k,实现自适应EKF估计方法的时间更新。转到(5)。(3) Temporal update using a priori statistical properties of noise. Using state estimation at time k and the error covariance matrix P k as the initial state value and the error covariance matrix at time k, and calculate the state one-step predicted value according to Equation (22) and Equation (23) respectively and the prediction error covariance matrix P k+1/k to realize the time update of the adaptive EKF estimation method. Go to (5).
(4)采用估计的噪声统计特性的时间更新。利用k时刻的状态估计及误差协方差阵Pk作为k时刻的状态初值及误差协方差阵,根据式(18)和式(21)分别计算状态一步预测值及预测误差协方差矩阵Pk+1/k,实现自适应EKF估计方法的时间更新。(4) Temporal update with estimated noise statistics. Using state estimation at time k and the error covariance matrix P k as the initial state value and the error covariance matrix at time k, and calculate the state one-step predicted value according to Equation (18) and Equation (21) respectively and the prediction error covariance matrix P k+1/k to realize the time update of the adaptive EKF estimation method.
(5)自适应EKF测量更新。根据式(24)~(27)依次计算(k+1)时刻的增益矩阵Kk+1、新息矩阵υk+1、状态估计值及误差协方差矩阵Pk+1,实现EKF的测量更新。(5) Adaptive EKF measurement update. Calculate the gain matrix K k+1 , the innovation matrix υ k+1 , and the state estimation value at the time (k+1) sequentially according to equations (24) to (27). and the error covariance matrix P k+1 to realize the measurement update of the EKF.
(6)估计系统噪声统计特性。根据式(28)和(29)分别计算系统噪声的均值估计值和协方差估计值 (6) Estimate the statistical characteristics of the system noise. Calculate the mean estimated value of system noise according to equations (28) and (29) respectively and covariance estimates
(7)判断滤波过程是否结束。如需继续进行滤波,k=k+1,并返回到(2)。(7) Determine whether the filtering process is over. To continue filtering, k=k+1, and return to (2).
步骤五:调节遗忘因子bQ、bC、bq。Step 5: Adjust forgetting factors b Q , b C , b q .
结合发明内容步骤三中关于三个遗忘因子的作用以及步骤四中给出的遗忘因子的大致范围,依次调节bQ、bC、bq,重复执行步骤三中滤波过程,使系统达到相对最优,具体调节步骤如下:Combined with the functions of the three forgetting factors in step 3 of the invention and the approximate range of the forgetting factors given in step 4, adjust b Q , b C , b q in turn, and repeat the filtering process in step 3, so that the system reaches the relative maximum. Excellent, the specific adjustment steps are as follows:
(1)固定bQ=0.9999、bq=0.9999,逐渐增大bC,根据滤波结果确定bC的最佳取值,记为 (1) Fix b Q = 0.9999, b q = 0.9999, increase b C gradually, and determine the optimal value of b C according to the filtering result, denoted as
(2)固定bq=0.9999,逐渐减小bQ,根据滤波结果确定bQ的最佳取值,记为 (2) Fixed b q =0.9999, gradually reduce b Q , determine the optimal value of b Q according to the filtering result, denoted as
(3)固定逐渐减小bq,根据滤波结果确定bq的最佳取值,记为 (3) Fixed Decrease b q gradually, and determine the optimal value of b q according to the filtering result, denoted as
系统精度随bQ、bC、bq变化趋势图如图4所示,据图可确定最优遗忘因子组合为:bq=0.9993、bQ=0.9997、bC=0.96。Figure 4 shows the variation trend of system accuracy with b Q , b C , and b q . According to the figure, it can be determined that the optimal forgetting factor combination is: b q =0.9993, b Q =0.9997, and b C =0.96.
本发明在分析仅利用星间距离测量时存在的“亏秩”问题的基础上,引入Lagrange卫星以提供绝对基准;然后在集中式结构下,采用自适应EKF估计方法,实现了地球-Lagrange联合星座的自主定轨。On the basis of analyzing the "deficient rank" problem when only using inter-satellite distance measurement, the present invention introduces Lagrange satellites to provide an absolute reference; then, under the centralized structure, an adaptive EKF estimation method is adopted to realize the Earth-Lagrange joint The autonomous orbit of the constellation.
在星间测距误差为零均值,标准差为5m的情况下,得到以下仿真结果:When the inter-satellite ranging error is zero mean and the standard deviation is 5m, the following simulation results are obtained:
由于星座中三颗MEO卫星的定轨精度类似,因此以卫星E1为例,其x、y、z三轴定轨距离误差分别为7.78m,7.60m和10.06m,其误差曲线如图5所示,距离估计误差为14.81m;x、y、z三轴定轨速度误差分别为1.43×10-3m/s,3.92×10-3m/s和4.74×10-3m/s,速度估计误差为6.31×10-3m/s。同样,两颗Lagrange的定轨精度类似,以卫星L1为例,其x、y、z三轴定轨距离误差分别为2.66m,3.60m和3.39m,距离估计误差为5.62m;x、y、z三轴定轨速度误差分别为2.11×10-5m/s,1.64×10-5m/s和1.48×10-5m/s,速度估计误差为3.06×10-5m/s。Since the orbit determination accuracy of the three MEO satellites in the constellation is similar, taking satellite E1 as an example, the orbit determination distance errors of the x, y and z axes are 7.78m, 7.60m and 10.06m respectively. The error curves are shown in Figure 5. The distance estimation error is 14.81m; the orbit determination speed errors of the x, y, and z axes are 1.43×10 -3 m/s, 3.92×10 -3 m/s and 4.74×10 -3 m/s, respectively. The estimated error is 6.31×10 -3 m/s. Similarly, the orbit determination accuracy of the two Lagranges is similar. Taking satellite L1 as an example, the orbit determination distance errors of the x, y and z axes are 2.66m, 3.60m and 3.39m respectively, and the distance estimation error is 5.62m; The orbit determination velocity errors of the three axes and z are 2.11×10 -5 m/s, 1.64×10 -5 m/s and 1.48×10 -5 m/s respectively, and the velocity estimation error is 3.06×10 -5 m/s.
验证了本发明方法的有效性。The effectiveness of the method of the present invention is verified.
Claims (4)
Priority Applications (1)
Application Number | Priority Date | Filing Date | Title |
---|---|---|---|
CN201710611461.6A CN107421550B (en) | 2017-07-25 | 2017-07-25 | An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging |
Applications Claiming Priority (1)
Application Number | Priority Date | Filing Date | Title |
---|---|---|---|
CN201710611461.6A CN107421550B (en) | 2017-07-25 | 2017-07-25 | An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging |
Publications (2)
Publication Number | Publication Date |
---|---|
CN107421550A CN107421550A (en) | 2017-12-01 |
CN107421550B true CN107421550B (en) | 2020-08-28 |
Family
ID=60431049
Family Applications (1)
Application Number | Title | Priority Date | Filing Date |
---|---|---|---|
CN201710611461.6A Active CN107421550B (en) | 2017-07-25 | 2017-07-25 | An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging |
Country Status (1)
Country | Link |
---|---|
CN (1) | CN107421550B (en) |
Families Citing this family (14)
Publication number | Priority date | Publication date | Assignee | Title |
---|---|---|---|---|
CN108287334A (en) * | 2018-02-06 | 2018-07-17 | 西安四方星途测控技术有限公司 | Spin satellite attitude estimation method and system based on RCS measurement data |
CN109031349B (en) * | 2018-04-20 | 2022-04-08 | 南京航空航天大学 | An intelligent autonomous operation system for GEO satellites |
CN109752006B (en) * | 2018-11-23 | 2022-09-09 | 中国西安卫星测控中心 | Method for using incomplete external measurement data in real-time filtering |
CN109682383B (en) * | 2018-11-23 | 2022-11-04 | 中国西安卫星测控中心 | A real-time filtering positioning method using deep space three-way measurement distance and data |
CN109933847B (en) * | 2019-01-30 | 2022-09-16 | 中国人民解放军战略支援部队信息工程大学 | An Improved Active Segment Ballistic Estimation Algorithm |
CN109917431B (en) * | 2019-04-02 | 2021-03-23 | 中国科学院空间应用工程与技术中心 | A method for autonomous navigation of GNSS satellites using DRO orbit and inter-satellite measurement |
CN109975839B (en) * | 2019-04-10 | 2023-04-07 | 华砺智行(武汉)科技有限公司 | Joint filtering optimization method for vehicle satellite positioning data |
CN110793528B (en) * | 2019-09-27 | 2021-04-13 | 西安空间无线电技术研究所 | Low-orbit satellite-based anchoring-based Beidou navigation constellation autonomous orbit determination method |
CN111522036B (en) * | 2020-04-30 | 2022-07-26 | 中国科学院微小卫星创新研究院 | Satellite-usable Beidou satellite centralized constellation autonomous navigation system and navigation method |
CN111947667B (en) * | 2020-06-24 | 2022-08-12 | 火眼位置数智科技服务有限公司 | Low-orbit satellite real-time high-precision orbit determination method based on kinematics and dynamics combination |
CN112504281B (en) * | 2020-11-16 | 2023-06-27 | 中国人民解放军63921部队 | Spacecraft orbit determination method based on Beidou inter-satellite unidirectional link |
CN113008243B (en) * | 2021-02-23 | 2024-03-19 | 重庆两江卫星移动通信有限公司 | Autonomous orbit determination method and system for low orbit satellite constellation |
CN113204917B (en) * | 2021-04-25 | 2021-12-07 | 中国科学院国家空间科学中心 | Space-based optical angle measurement arc section initial orbit determination method for GEO target and correlation method |
CN115113646B (en) * | 2022-07-07 | 2025-02-14 | 上海交通大学 | Satellite formation flat root state continuous estimation method and system based on Kalman filter |
Family Cites Families (6)
Publication number | Priority date | Publication date | Assignee | Title |
---|---|---|---|---|
US9091552B2 (en) * | 2011-10-25 | 2015-07-28 | The Boeing Company | Combined location and attitude determination system and methods |
US9057780B2 (en) * | 2013-04-18 | 2015-06-16 | California Institute Of Technology | Real-time and post-processed orbit determination and positioning |
US9939260B2 (en) * | 2014-08-28 | 2018-04-10 | The Boeing Company | Satellite transfer orbit search methods |
CN105716612B (en) * | 2016-02-29 | 2017-05-10 | 武汉大学 | A design method of strapdown inertial navigation system simulator |
CN106338753B (en) * | 2016-09-22 | 2019-03-12 | 北京航空航天大学 | A Geosynchronous Orbit Constellation Orbit Determination Method Based on Ground Station/Inter-satellite Link/GNSS Joint Measurement |
CN106885577B (en) * | 2017-01-24 | 2020-01-21 | 南京航空航天大学 | Autonomous orbit determination method for Lagrange navigation satellite |
-
2017
- 2017-07-25 CN CN201710611461.6A patent/CN107421550B/en active Active
Non-Patent Citations (1)
Title |
---|
"导航卫星自主导航关键技术研究";肖寅;《中国博士学位论文全文数据库(电子期刊)》;20160115;正文第24-29页 * |
Also Published As
Publication number | Publication date |
---|---|
CN107421550A (en) | 2017-12-01 |
Similar Documents
Publication | Publication Date | Title |
---|---|---|
CN107421550B (en) | An Earth-Lagrange Joint Constellation Autonomous Orbit Determination Method Based on Inter-satellite Ranging | |
CN109917431B (en) | A method for autonomous navigation of GNSS satellites using DRO orbit and inter-satellite measurement | |
CN106338753B (en) | A Geosynchronous Orbit Constellation Orbit Determination Method Based on Ground Station/Inter-satellite Link/GNSS Joint Measurement | |
CN101216319B (en) | Low orbit satellite multi-sensor fault tolerance autonomous navigation method based on federal UKF algorithm | |
CN109592079A (en) | A kind of spacecraft coplanar encounter of limiting time becomes rail strategy and determines method | |
CN111552003B (en) | Asteroid gravitational field full-autonomous measurement system and method based on ball satellite formation | |
CN107797130A (en) | Low orbit spacecraft multiple spot multi-parameter track upstream data computational methods | |
CN106643744B (en) | A kind of remote lunar surface lander precision positioning method that tracing mode is relayed based on quadruple pass | |
CN108844536A (en) | A kind of earth-magnetism navigation method based on measurement noise covariance matrix estimation | |
CN105138005B (en) | A kind of Relative Orbit Elements based on interstellar distance determine method | |
CN111522036B (en) | Satellite-usable Beidou satellite centralized constellation autonomous navigation system and navigation method | |
CN105487405B (en) | Low tracking Gravisat semi-physical system | |
CN112161632B (en) | An Initial Positioning Method of Satellite Formation Based on Relative Position Vector Measurement | |
CN110816896B (en) | Satellite on-satellite simple orbit extrapolation method | |
CN1995915A (en) | Deep space probe UPF celestial self-navigation method based on starlight angle | |
CN111125874A (en) | High-precision rail measurement forecasting method for movable platform | |
CN104864875B (en) | A kind of spacecraft autonomic positioning method based on non-linear H ∞ filtering | |
CN115314101B (en) | A Fast Modeling Method for LEO Communication Satellite Constellation Based on Parallel Computing | |
CN108959665B (en) | Method and system for generating orbital prediction error empirical model suitable for low-orbit satellites | |
CN104408326B (en) | A kind of appraisal procedure to survey of deep space independent navigation filtering algorithm | |
CN107036595A (en) | Deformation of hull angular estimation method based on interacting multiple model filters | |
CN114675276B (en) | Space target radar track improvement method and device | |
Liuqing et al. | An autonomous navigation study of Walker constellation based on reference satellite and inter-satellite distance measurement | |
CN107830856A (en) | Towards the sun TDOA method for measurement and Combinated navigation method of formation flight | |
Olson | Sequential estimation methods for small body optical navigation |
Legal Events
Date | Code | Title | Description |
---|---|---|---|
PB01 | Publication | ||
PB01 | Publication | ||
SE01 | Entry into force of request for substantive examination | ||
GR01 | Patent grant | ||
GR01 | Patent grant |