CN106325099B - A kind of spacecraft real-time track improved method based on pseudo- relative motion - Google Patents

A kind of spacecraft real-time track improved method based on pseudo- relative motion Download PDF

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CN106325099B
CN106325099B CN201610606257.0A CN201610606257A CN106325099B CN 106325099 B CN106325099 B CN 106325099B CN 201610606257 A CN201610606257 A CN 201610606257A CN 106325099 B CN106325099 B CN 106325099B
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周敬
李明涛
高东
郑建华
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National Space Science Center of CAS
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Abstract

本发明提供了一种基于伪相对运动的航天器实时轨道改进方法,本发明通过分别求解无/有摄动条件下的航天器相对运动动力学模型,得到无/有摄动条件下相对运动解析表达式,并与轨道漂移数据相对应,运用傅里叶变换方法处理轨道漂移数据,解算得到航天器初始位置误差和速度误差,最后便可以反演得到航天器实时位置矢量和速度矢量。利用上述方法可以在初始定轨技术的基础上将定轨精度提高将近一个量级;并具有普遍适应性,利用CW方程及考虑摄动下的改进方程实现圆/近圆航天器轨道改进,也可利用Lawden方程及其考虑摄动下的变形实现椭圆航天器轨道改进。

The present invention provides a real-time trajectory improvement method for spacecraft based on pseudo-relative motion. The present invention obtains the relative motion analysis under the condition of no/with perturbation by separately solving the relative motion dynamics model of the spacecraft under the condition of no/with perturbation Expression, and corresponding to the orbital drift data, use the Fourier transform method to process the orbital drift data, solve the initial position error and velocity error of the spacecraft, and finally obtain the real-time position vector and velocity vector of the spacecraft. Using the above method can improve the orbit determination accuracy by nearly an order of magnitude on the basis of the initial orbit determination technology; and it has universal adaptability, using the CW equation and the improved equation considering the perturbation to realize the improvement of the circular/near-circular spacecraft orbit, and also The improvement of the elliptical spacecraft orbit can be realized by using the Lawden equation and its deformation considering the perturbation.

Description

一种基于伪相对运动的航天器实时轨道改进方法A real-time trajectory improvement method for spacecraft based on pseudo-relative motion

技术领域technical field

本发明属于航天器轨道确定领域,具体涉及一种基于伪相对运动的航天器实时轨道改进方法。The invention belongs to the field of orbit determination of spacecraft, in particular to a method for improving real-time orbit of spacecraft based on pseudo relative motion.

背景技术Background technique

航天器轨道确定就是对含有测量误差的航天器运动状态数据,使用统计学原理对航天器轨道进行估值的过程。通过轨道确定可以得到航天器在过去、当前和未来一段时间内任一时刻的运动状态。Spacecraft orbit determination is the process of estimating the spacecraft orbit using statistical principles for the spacecraft motion state data that contains measurement errors. Through orbit determination, the motion state of the spacecraft at any time in the past, current and future period can be obtained.

根据是否采用航天器所受摄动力的力学模型及与力学模型的关系,可以将定轨方法分为运动学定轨、动力学定轨和简化动力学定轨;根据数据处理策略可以分为批处理法和序贯递推法;根据弧段的长度可以分为短弧段法和长弧段法;根据积分方法可以分为单步法和多步法。According to whether to use the mechanical model of the perturbed force of the spacecraft and the relationship with the mechanical model, the orbit determination method can be divided into kinematic orbit determination, dynamic orbit determination and simplified dynamic orbit determination; according to the data processing strategy, it can be divided into batch Processing method and sequential recursion method; according to the length of the arc, it can be divided into short arc method and long arc method; according to the integration method, it can be divided into single-step method and multi-step method.

目前,常用的航天器定轨方法是最小二乘估计方法和各种形式的卡尔曼滤波方法。最小二乘估计方法需要在迭代过程中存储大量的数据以供下次迭代使用;卡尔曼滤波方法会由于数据可观测性差、初轨差、测量数据强非线性等造成滤波定轨结果发散;此外,最小二乘估计方法和卡尔曼滤波方法还存在因可观性造成的法方程矩阵和协方差矩阵病态这一数值问题。At present, the commonly used spacecraft orbit determination methods are the least square estimation method and various forms of Kalman filter methods. The least squares estimation method needs to store a large amount of data in the iterative process for the next iteration; the Kalman filter method will cause divergence of the filter orbit determination results due to poor data observability, initial orbit difference, and strong nonlinearity of the measurement data; in addition , the least squares estimation method and the Kalman filter method also have the numerical problem that the normal equation matrix and the covariance matrix are ill-conditioned due to observability.

由于上述传统轨道确定方法的测量精度是有限的,在观测数据精度没有大幅度改进的情况下,无法使得轨道确定精度得到进一步的提高,因此,需要研究新型的轨道改进方法以提高轨道确定的精度。Since the measurement accuracy of the above-mentioned traditional orbit determination methods is limited, the accuracy of orbit determination cannot be further improved without a substantial improvement in the accuracy of observation data. Therefore, it is necessary to study new orbit improvement methods to improve the accuracy of orbit determination .

发明内容Contents of the invention

本发明的目的在于,为解决现有航天器轨道确定方法的测量精度低的技术问题,提供一种基于伪相对运动的航天器实时轨道改进方法。The object of the present invention is to provide a method for improving real-time orbit of spacecraft based on pseudo relative motion in order to solve the technical problem of low measurement accuracy of existing spacecraft orbit determination methods.

为实现上述目的,本发明提供的一种基于伪相对运动的航天器实时轨道改进方法,包括:In order to achieve the above object, a method for improving real-time orbit of spacecraft based on pseudo-relative motion provided by the present invention includes:

步骤1)将航天器的测量轨道作为参考轨道,以初始时刻测量轨道确定的航天器初始状态作为预报轨道的起点,并依据轨道动力学模型生成该预报轨道;Step 1) taking the measured orbit of the spacecraft as the reference orbit, taking the initial state of the spacecraft determined by the measured orbit at the initial moment as the starting point of the predicted orbit, and generating the predicted orbit according to the orbital dynamics model;

步骤2)将预报轨道与测量轨道之间的差值作为轨道漂移数据,并以该轨道漂移数据所形成的轨迹定义为航天器的伪相对运动;Step 2) using the difference between the predicted orbit and the measured orbit as the orbital drift data, and defining the trajectory formed by the orbital drift data as the pseudo-relative motion of the spacecraft;

步骤3)分别求解无、有摄动条件下伪相对运动的动力学模型,得到无、有摄动条件下伪相对运动的解析表达式,运用傅里叶变换方法处理轨道漂移数据后,以解算得到的解析表达式反演出航天器的初始状态误差的估计值;Step 3) Solve the dynamic model of pseudo relative motion under the condition of no perturbation and presence of perturbation respectively, obtain the analytical expression of pseudo relative motion under the condition of no perturbation and presence of perturbation, and use the Fourier transform method to process the orbital drift data to solve The calculated analytical expression is used to invert the estimated value of the initial state error of the spacecraft;

步骤4)利用初始状态误差的估计值与参考轨道的初始状态误差值之差,作为航天器轨道改进值。Step 4) Use the difference between the estimated value of the initial state error and the initial state error value of the reference orbit as the spacecraft orbit improvement value.

作为上述技术方案的进一步改进,所述步骤3)中的无摄动条件下伪相对运动的解析表达式为:As a further improvement of the above-mentioned technical solution, the analytical expression of the pseudo-relative motion under the condition of no perturbation in the step 3) is:

其中,n为轨道平均角运动,即参考轨道角频率,t表示时间,各参数及其关系设置为:Among them, n is the average angular motion of the orbit, that is, the reference orbital angular frequency, t represents the time, and the parameters and their relationships are set as:

其中,(x0,y0,z0)表示三轴初始位置误差,表示三轴初始速度误差;Among them, (x 0 , y 0 , z 0 ) represents the three-axis initial position error, Indicates the three-axis initial velocity error;

运用傅里叶变换方法处理轨道漂移数据,解算得到常值项xc yc、长期项3xcnt/2和周期项csin(nt+φ)中的各系数xc,b,yc,c,φ,并利用上述解析表达式进行反演,得到初始状态误差的估计值 Using the Fourier transform method to process the orbital drift data, the constant value term x c y c , the long-term term 3x c nt/2 and the periodic term are obtained Each coefficient x c ,b, in csin(nt+φ) y c ,c,φ, and use the above analytic expression to invert to get the initial state error estimated value of

作为上述技术方案的进一步改进,所述步骤3)中的有摄动条件下伪相对运动的解析表达式为:As a further improvement of the above-mentioned technical solution, the analytical expression of the pseudo-relative motion under the perturbation condition in the step 3) is:

其中,各参数及其关系设置为:Among them, the parameters and their relationships are set as:

其中,n为轨道平均角运动,即参考轨道角频率,t表示时间,u为地球引力系数,rref为参考轨道地心距,iref为参考轨道倾角,J2为第二带谐项,Re为地球半径,n1、n2、n3、n4、n5分别为相对运动中各周期分量的角频率;Among them, n is the average orbital angular motion, that is, the reference orbital angular frequency, t is the time, u is the gravitational coefficient of the earth, rref is the reference orbital center distance, iref is the reference orbital inclination, J2 is the second harmonic term, R e is the radius of the earth, n 1 , n 2 , n 3 , n 4 , n 5 are the angular frequencies of each periodic component in relative motion;

运用傅里叶变换方法处理轨道漂移数据,解算得到常值项A3,A7、长期项A6t和周期项A1cos(n1t+θ1),A2cos(n2t+θ2),A4cos(n3t+θ3),A5cos(n4t+θ4),A8sin(n5t+θ5)中的各系数A11,A22,A3,A43,A54,A6,A7,A85,并利用上述解析表达式进行反演,得到初始状态误差的估计值 Using the Fourier transform method to process the orbital drift data, the constant value items A 3 , A 7 , the long-term item A 6 t and the periodic item A 1 cos(n 1 t+θ 1 ), A 2 cos(n 2 t +θ 2 ), A 4 cos(n 3 t+θ 3 ), A 5 cos(n 4 t+θ 4 ), A 8 sin(n 5 t+θ 5 ), A 1 , θ 1 , A 2 , θ 2 , A 3 , A 4 , θ 3 , A 5 , θ 4 , A 6 , A 7 , A 8 , θ 5 , and use the above analytical expressions to perform inversion to obtain the initial state error estimated value of

本发明的一种基于伪相对运动的航天器实时轨道改进方法的优点在于:The advantage of a kind of spacecraft real-time track improvement method based on pseudo-relative motion of the present invention is:

1、高定轨精度,可以在初始定轨技术的基础上将定轨精度提高将近一个量级;1. High orbit determination accuracy, which can improve the orbit determination accuracy by nearly an order of magnitude on the basis of the initial orbit determination technology;

2、实时性,可以对时间逆向积分,得到当前时刻航天器的位置矢量和速度矢量;2. Real-time, it can reversely integrate time to obtain the position vector and velocity vector of the spacecraft at the current moment;

3、普遍适应性,利用CW方程及考虑摄动下的改进方程实现圆/近圆航天器轨道改进,也可利用Lawden方程及其考虑摄动下的变形实现椭圆航天器轨道改进。3. Universal adaptability, use the CW equation and the improved equation considering perturbation to realize the improvement of circular/near-circular spacecraft orbit, and also use the Lawden equation and its deformation considering perturbation to realize the improvement of elliptical spacecraft orbit.

附图说明Description of drawings

图1为本发明的一种基于伪相对运动的航天器实时轨道改进方法流程图。Fig. 1 is a flow chart of a real-time orbit improvement method for a spacecraft based on pseudo relative motion in the present invention.

图2为本发明实施例中示出的航天器伪相对运动的轨迹示意图。Fig. 2 is a schematic diagram of the trajectory of the pseudo relative motion of the spacecraft shown in the embodiment of the present invention.

图3为本发明实施例中航天器轨道径向漂移数据及傅里叶变换处理得到的幅频曲线。Fig. 3 is an amplitude-frequency curve obtained by processing radial drift data of spacecraft orbit and Fourier transform in an embodiment of the present invention.

图4为本发明实施例中航天器轨道迹向漂移数据及傅里叶变换处理得到的幅频曲线。Fig. 4 is an amplitude-frequency curve obtained by processing spacecraft trajectory drift data and Fourier transform in an embodiment of the present invention.

图5为本发明实施例中航天器轨道法向漂移数据及傅里叶变换处理得到的幅频曲线。Fig. 5 is an amplitude-frequency curve obtained by processing normal drift data of spacecraft orbit and Fourier transform in an embodiment of the present invention.

具体实施方式Detailed ways

下面结合附图和实施例对本发明所述的一种基于伪相对运动的航天器实时轨道改进方法进行详细说明。A method for improving real-time orbit of a spacecraft based on pseudo-relative motion according to the present invention will be described in detail below in conjunction with the accompanying drawings and embodiments.

本发明提供的一种基于伪相对运动的航天器实时轨道改进方法,它能够实现初始轨道确定条件下的航天器轨道改进。The invention provides a method for improving the real-time orbit of a spacecraft based on pseudo relative motion, which can realize the improvement of the orbit of the spacecraft under the condition of determining the initial orbit.

本发明通过分别求解无/有摄动条件下的航天器相对运动动力学模型,得到无/有摄动条件下相对运动解析表达式,并与轨道漂移数据相对应,运用傅里叶变换方法解算得到航天器初始位置误差和速度误差,最后便可以反演得到航天器实时位置矢量和速度矢量。The present invention obtains the analytical expression of relative motion under the condition of no/with perturbation by separately solving the relative motion dynamics model of the spacecraft under the condition of no/with perturbation, and corresponds to the orbital drift data, and uses the Fourier transform method to solve The initial position error and velocity error of the spacecraft are calculated, and finally the real-time position vector and velocity vector of the spacecraft can be obtained by inversion.

具体地,一种基于伪相对运动的航天器实时轨道改进方法,其包括如下步骤:Specifically, a method for improving real-time orbit of a spacecraft based on pseudo-relative motion, comprising the steps of:

①借鉴航天器编队飞行的思想,将航天器的测量轨道(初定轨轨道)作为参考轨道,基于初定轨状态的预报轨道作为对应的“伪卫星”的轨道,由于测量轨道和预报轨道偏差较小,两者之差可以理解为一种相对运动,即伪相对运动;①Referring to the idea of spacecraft formation flight, the spacecraft's measurement orbit (preliminary orbit orbit) is used as the reference orbit, and the predicted orbit based on the initial orbit status is used as the corresponding "pseudo-satellite" orbit. Due to the deviation between the measured orbit and the predicted orbit Small, the difference between the two can be understood as a kind of relative motion, that is, pseudo relative motion;

②将初始时刻初定轨确定的航天器初始状态作为预报轨道的起点,依据轨道动力学模型,生成一条预报轨道,将预报轨道与测量轨道做差,即为轨道漂移数据;②The initial state of the spacecraft determined by the initial orbit determination at the initial moment is used as the starting point of the predicted orbit, and a predicted orbit is generated according to the orbital dynamics model, and the difference between the predicted orbit and the measured orbit is the orbit drift data;

③分别求解无、有摄动条件下伪相对运动的动力学模型,在不考虑摄动力情况下,当航天器参考轨道为近地圆/近圆轨道时,参考轨道和预报轨道之间的相对运动满足CW方程,即③ Solve the dynamic model of pseudo-relative motion under the conditions of no perturbation and presence of perturbation respectively. Without considering the perturbation force, when the reference orbit of the spacecraft is a near-earth circular/near-circular orbit, the relative relationship between the reference orbit and the predicted orbit The motion satisfies the CW equation, namely

其中,(x0,y0,z0)表示三轴初始位置误差,表示三轴初始速度误差(在参考轨道的轨道坐标系上),n为轨道平均角运动,即参考轨道角频率,t表示时间,这些量均为理论已知量;Among them, (x 0 , y 0 , z 0 ) represents the three-axis initial position error, Indicates the three-axis initial velocity error (on the orbital coordinate system of the reference orbit), n is the average angular motion of the orbit, that is, the angular frequency of the reference orbit, and t represents the time, and these quantities are all theoretically known quantities;

将CW方程转化为常值项、周期项和长期项组合的形式,即Transform the CW equation into the form of a combination of constant term, periodic term and long-term term, namely

其中各参数及其关系设置如下:The parameters and their relationships are set as follows:

④参考轨道和预报轨道之间的轨道漂移数据满足上述CW方程,运用傅里叶变换方法处理该轨道漂移数据,解算得到常值项xc yc、长期项3xcnt/2和周期项csin(nt+φ)系数xc,b,yc,c,φ,并利用式(3)进行反演,得到初始状态误差的估计值 ④ The orbital drift data between the reference orbit and the predicted orbit satisfies the above CW equation, and the Fourier transform method is used to process the orbital drift data, and the constant item x c y c , the long-term item 3x c nt/2 and the periodic item are obtained by solving csin(nt+φ) coefficient x c ,b, y c , c, φ, and use formula (3) to invert to get the initial state error estimated value of

⑤反演得到的初始状态误差的估计值与初始状态误差之差,即为基于伪相对运动的航天器实时轨道改进精度值;⑤ Estimated value of initial state error obtained by inversion error from the initial state The difference is the improved accuracy value of the real-time orbit of the spacecraft based on pseudo-relative motion;

由于所述的预报轨道是时间正向积分得到的,最后得到的当前时刻前的某一时刻的卫星轨道状态;同样地方式,如果将轨道动力学模型进行时间逆向积分,便可得到当前时刻状态为初始值的预报轨道。如果将预报轨道的起点放在当前时刻之前的某一时刻,最后利用上述步骤①-⑤得到的是那一时刻的轨道状态改进精度值;同理,如果将预报轨道的起点放在当前时刻,最后得到的便是当前时刻的轨道状态改进精度值,从而实现了航天器轨道的实时改进。Since the predicted orbit is obtained by time forward integration, the satellite orbit state at a certain moment before the current moment is finally obtained; in the same way, if the orbit dynamics model is time-reversely integrated, the current moment state can be obtained is the predicted orbit of the initial value. If the starting point of the predicted orbit is placed at a certain moment before the current moment, the last step ①-⑤ above is used to obtain the improved accuracy value of the orbital state at that moment; similarly, if the starting point of the predicted orbit is placed at the current moment, The final result is the improved accuracy value of the orbit state at the current moment, thus realizing the real-time improvement of the orbit of the spacecraft.

⑥在考虑J2摄动情况下,航天器的伪相对运动动力学模型表示为:⑥ Considering the J2 perturbation, the pseudo-relative dynamics model of the spacecraft is expressed as:

其中,分别为三轴运动量的二阶导数,表示动力学过程。in, Respectively are the second derivatives of the three-axis motion, representing the dynamic process.

其中各参数及其关系设置如下:The parameters and their relationships are set as follows:

其中,n为轨道平均角运动,t表示时间,u为地球引力系数,rref为参考轨道地心距,iref为参考轨道倾角,J2为第二带谐项,Re为地球半径。Among them, n is the average orbital angular motion, t is time, u is the gravitational coefficient of the earth, r ref is the reference orbit geocentric distance, i ref is the reference orbit inclination, J 2 is the second harmonic term, R e is the radius of the earth.

由于J2摄动下航天器的地心距和轨道倾角变化量很小,并考虑到实际工程应用,假设航天器参考轨道为圆轨道,轨道倾角为28.5°、轨道高度为500km时,J2摄动下的地心距的变化范围为4.48km,相对变化量为0.065%;轨道倾角的变化范围为0.03°,相对变化量为0.11%。,为得到J2摄动下相对运动解析形式,合理假设航天器地心距和轨道倾角为常量,具体值分别取为参考轨道平均半长轴和平均轨道倾角,便得到J2摄动下航天器伪相对运动动力学方程:Due to the small changes in the distance from the center of the earth and the orbital inclination of the spacecraft under the J2 perturbation, and considering the practical engineering application, assuming that the reference orbit of the spacecraft is a circular orbit, the orbital inclination is 28.5°, and the orbital altitude is 500km, the J2 perturbation The variation range of the earth center distance below is 4.48km, and the relative variation is 0.065%; the variation range of the orbital inclination is 0.03°, and the relative variation is 0.11%. , in order to obtain the analytical form of relative motion under J2 perturbation, it is reasonable to assume that the spacecraft's center distance and orbital inclination are constant, and the specific values are respectively taken as the average semi-major axis of the reference orbit and the average orbital inclination, then the spacecraft pseudo Relative motion dynamic equation:

其中各参数及其关系设置如下:The parameters and their relationships are set as follows:

求解可得伪相对运动解析表达式为:The analytical expression of the pseudo-relative motion can be obtained as follows:

需要说明的是,z轴相对运动分量与xy平面相对运动分量解耦、z轴相对运动实现非超越化需要更多的假设条件、且z轴相对运动定轨精度对整体定轨精度影响很小,因此,z轴相对运动直接取为CW方程中z轴运动形式,即It should be noted that the decoupling of the z-axis relative motion component from the xy-plane relative motion component, and the realization of non-transcendence of the z-axis relative motion requires more assumptions, and the z-axis relative motion orbit determination accuracy has little effect on the overall orbit determination accuracy , therefore, the z-axis relative motion is directly taken as the z-axis motion form in the CW equation, namely

其中:in:

将公式(9)转化为常值项、周期项、长期项组合的形式:Transform formula (9) into the form of constant value item, periodic item, and long-term item combination:

其中:in:

其中,n为轨道平均角运动,即参考轨道角频率,t表示时间,u为地球引力系数,rref为参考轨道地心距,iref为参考轨道倾角,J2为第二带谐项,Re为地球半径,n1、n2、n3、n4、n5分别为相对运动中各周期分量的角频率;Among them, n is the average orbital angular motion, that is, the reference orbital angular frequency, t is the time, u is the gravitational coefficient of the earth, rref is the reference orbital center distance, iref is the reference orbital inclination, J2 is the second harmonic term, R e is the radius of the earth, n 1 , n 2 , n 3 , n 4 , n 5 are the angular frequencies of each periodic component in relative motion;

⑦在J2摄动下参考轨道与预报轨道之间的轨道漂移数据满足上述运动形式,同样运用傅里叶变换方法处理伪相对运动轨道漂移数据,得到常值项A3,A7、长期项A6t和周期项A1cos(n1t+θ1),A2cos(n2t+θ2),A4cos(n3t+θ3),A5cos(n4t+θ4),A8sin(n5t+θ5)中的各系数A11,A22,A3,A43,A54,A6,A7,A85,并利用公式(12)进行反向解算,得到初始状态误差的估计值 ⑦ Under J2 perturbation, the orbit drift data between the reference orbit and the predicted orbit satisfies the above motion form, and the Fourier transform method is also used to process the pseudo relative motion orbit drift data, and the constant items A 3 , A 7 and the long-term item A 6 t and periodic terms A 1 cos(n 1 t+θ 1 ), A 2 cos(n 2 t+θ 2 ), A 4 cos(n 3 t+θ 3 ), A 5 cos(n 4 t+θ 3 4 ), each coefficient A 1 , θ 1 , A 2 , θ 2 , A 3 , A 4 , θ 3 , A 5 , θ 4 , A 6 , A 7 in A 8 sin(n 5 t+θ 5 ) ,A 85 , and use the formula (12) to carry out the reverse solution to get the initial state error estimated value of

⑧解算得到的初始状态误差的估计值与初始状态误差之差,即为J2摄动下基于伪相对运动的航天器实时轨道改进精度值;⑧ The estimated value of the initial state error obtained from the solution error from the initial state The difference is the improved precision value of the real-time orbit of the spacecraft based on pseudo-relative motion under J2 perturbation;

另外,在同时考虑J2摄动和大气阻力摄动情况下,近地航天器轨道因大气阻力摄动引起的位置偏差仅为几米至几十米量级,因此在航天器轨道确定中不必再求解大气阻力摄动下的航天器伪相对运动方程,直接使用J2摄动下的航天器伪相对运动方程(公式9)对航天器轨道进行确定便可,轨道改进精度基本不受影响。In addition, considering J2 perturbation and atmospheric drag perturbation at the same time, the position deviation of near-Earth spacecraft orbit due to atmospheric drag perturbation is only on the order of a few meters to tens of meters, so it is not necessary to solve The pseudo-relative motion equation of the spacecraft under the perturbation of atmospheric drag can be directly used to determine the orbit of the spacecraft using the pseudo-relative motion equation of the spacecraft under the J2 perturbation (Formula 9), and the accuracy of the orbit improvement is basically not affected.

实施例一Embodiment one

如图1所示,记在初始时刻t0,航天器的真实位置位于A点,初定轨(测量轨道)确定航天器位于B点,由于初定轨误差的存在,实际位置A与测量位置B并不重合,记初定轨误差为(在参考轨道的轨道坐标系上,为假设已知量),此亦为航天器初始状态误差,将此状态误差在时间、空间上进行延伸,即将预报轨道和测量轨道做差,得到一段时间内的轨道漂移数据,亦即为此段时间内的状态漂移量。由于状态漂移量相对状态量为小量,则预报轨道和测量轨道之间的偏差可以看作一种相对运动,且满足一定的规律。As shown in Figure 1, recorded at the initial time t 0 , the real position of the spacecraft is at point A, and the initial orbit (measurement orbit) determines that the spacecraft is at point B. Due to the existence of the initial orbit error, the actual position A and the measured position B does not coincide, and the initially determined orbit error is (On the orbital coordinate system of the reference orbit, it is assumed to be a known quantity), this is also the initial state error of the spacecraft, and this state error is extended in time and space, that is, to make a difference between the predicted orbit and the measured orbit, and obtain a period of time The orbital drift data in , that is, the amount of state drift within this period of time. Since the state drift is small relative to the state quantity, the deviation between the predicted orbit and the measured orbit can be regarded as a kind of relative motion, which satisfies a certain law.

(1)情形一:在不考虑外界摄动力的情况下,处理步骤如下:(1) Situation 1: Without considering the external perturbation force, the processing steps are as follows:

①航天器轨道为近地圆/近圆轨道,则参考轨道和预报轨道之间的相对运动满足CW方程,即①The orbit of the spacecraft is a near-earth circular/near-circular orbit, then the relative motion between the reference orbit and the predicted orbit satisfies the CW equation, that is,

②CW运动方程中包含常值项、周期项、长期项,对CW运动方程进行整理可得:②The CW motion equation contains constant value term, periodic term and long-term term. After sorting out the CW motion equation, we can get:

其中各参数及其关系设置如下:The parameters and their relationships are set as follows:

③对获得的、满足上述CW方程形式的轨道状态漂移数据进行傅里叶变换处理:③ Perform Fourier transform processing on the obtained orbital state drift data satisfying the above CW equation form:

F{af1(t)+bf2(t)}=aF1(w)+bF2(w)F{af 1 (t)+bf 2 (t)}=aF 1 (w)+bF 2 (w)

得到相应的幅频响应曲线;Get the corresponding amplitude-frequency response curve;

④根据幅频响应曲线,提取相应的频率、幅值、相位信息,傅里叶变换处理X轴轨道漂移数据,得到xc,b,n,傅里叶变换处理Y轴漂移数据得到yc,处理Z轴,得到c,φ。利用此信息对初始状态偏差进行辨识,即可得到辨识结果即初始状态误差的估计值,两者之差即为轨道改进精度值。④ According to the amplitude-frequency response curve, extract the corresponding frequency, amplitude, and phase information, and process the X-axis orbital drift data by Fourier transform to obtain x c , b, n, the Fourier transform processes the Y-axis drift data to obtain y c , and processes the Z-axis to obtain c, φ. Use this information to bias the initial state Identify and get the identification result That is, the estimated value of the initial state error, and the difference between the two is the orbit improvement accuracy value.

(2)情形二:在考虑外界摄动力的情况下,对于近地航天器,其外界摄动力主要是J2摄动和大气阻力摄动。处理步骤如下:(2) Scenario 2: In the case of considering the external perturbation force, for the near-Earth spacecraft, the external perturbation force is mainly J2 perturbation and atmospheric resistance perturbation. The processing steps are as follows:

①首先仅考虑J2摄动,此种情况下航天器伪相对运动动力学方程表示为:① Firstly, only the J2 perturbation is considered. In this case, the dynamic equation of the pseudo-relative motion of the spacecraft is expressed as:

其中各参数及其关系设置如下:The parameters and their relationships are set as follows:

其中,rref为参考星的实时地心距,iref为参考星的实时轨道倾角。Among them, r ref is the real-time geocentric distance of the reference star, and i ref is the real-time orbit inclination of the reference star.

②在J2摄动下,上式中航天器地心距和轨道倾角呈现正弦振荡趋势,导致上式微分方程为一超越方程,无法得到解析解形式,但地心距和轨道倾角变化幅值相比其平均值为小量,因此可以在满足精度的前提下合理假设地心距和轨道倾角为恒定值,其值大小由平均轨道根数求得:②Under the J2 perturbation, the earth center distance and orbit inclination of the spacecraft in the above formula show a sinusoidal oscillation trend, so the differential equation in the above formula is a transcendental equation, and the form of analytical solution cannot be obtained, but the change amplitude of the earth center distance and orbit inclination is similar It is smaller than its average value, so it can be reasonably assumed that the earth center distance and orbital inclination angle are constant values under the premise of satisfying the accuracy, and its value is obtained from the average orbital element:

由此,在J2摄动下航天器伪相对运动动力学方程由超越方程转化为非超越方程。Therefore, under the J2 perturbation, the dynamic equation of the pseudo-relative motion of the spacecraft is transformed from a transcendental equation to a non-transcendental equation.

此时,在J2摄动条件下伪相对运动的解析表达式为:At this time, the analytical expression of the pseudo-relative motion under the J2 perturbation condition is:

③对满足上述运动方程形式的轨道状态漂移数据进行傅里叶变换处理:③ Perform Fourier transform processing on the orbital state drift data satisfying the above motion equation:

F{af1(t)+bf2(t)}=aF1(w)+bF2(w)F{af 1 (t)+bf 2 (t)}=aF 1 (w)+bF 2 (w)

④对初始状态误差进行辨识,得辨识结果即初始状态误差的估计值,两者之差即为航天器轨道改进精度值。④ For the initial state error Identify and get the result That is, the estimated value of the initial state error, and the difference between the two is the improved accuracy value of the spacecraft orbit.

另外,在同时考虑J2摄动和大气阻力摄动情况下,对于常规外形航天器,大气阻力摄动只与航天器面质比、轨道高度有较大关系。在500km的轨道高度下,运行两个周期,大气阻力摄动仅会产生10米左右的位置误差,当轨道高度增加时,大气阻力摄动影响量级呈指数递减,并且大气阻力只对航天器迹向相对运动产生影响,对径向、法向相对运动影响很小,并且引入大气模型会增加计算量,因此可以不考虑大气阻力的影响,直接将J2摄动下的伪相对运动方程作为同时考虑J2摄动和大气阻力摄动时的相对运动方程,然后利用傅里叶变换方法对摄动情况下的相对运动数据处理,最终实现航天器的轨道改进。In addition, considering the J2 perturbation and the atmospheric drag perturbation at the same time, for a spacecraft with a conventional shape, the atmospheric drag perturbation only has a greater relationship with the spacecraft's area-to-mass ratio and orbital altitude. At an orbital altitude of 500km, after two cycles of operation, the atmospheric drag perturbation will only produce a position error of about 10 meters. When the orbital altitude increases, the magnitude of the influence of the atmospheric drag perturbation decreases exponentially, and the atmospheric drag only affects the spacecraft The impact on the relative motion in the track direction has little effect on the relative motion in the radial and normal directions, and the introduction of the atmospheric model will increase the amount of calculation. Therefore, the pseudo relative motion equation under the J2 perturbation can be directly used as the simultaneous Consider the relative motion equation of J2 perturbation and atmospheric drag perturbation, and then use the Fourier transform method to process the relative motion data in the perturbation case, and finally realize the orbit improvement of the spacecraft.

如表1所示,本实施例所选取的航天器的初始状态矢量、初始状态误差及利用本发明的方法反演得到的初始误差的数据分别为:As shown in Table 1, the initial state vector and initial state error of the spacecraft selected in this embodiment and the data of the initial error obtained by inversion using the method of the present invention are respectively:

表1 仿真初始数据和仿真结果Table 1 Simulation initial data and simulation results

图3即为相应的航天器轨道径向漂移数据及傅里叶变换处理得到的幅频曲线;由幅频响应曲线中的前2个峰值和起始点,可以提取得到三组频率、幅值和相位信息A1,n11,A2,n22,A3Figure 3 is the amplitude-frequency curve obtained from the corresponding spacecraft orbit radial drift data and Fourier transform processing; from the first two peaks and the starting point in the amplitude-frequency response curve, three groups of frequency, amplitude and Phase information A 1 , n 1 , θ 1 , A 2 , n 2 , θ 2 , A 3 .

图4即为相应的航天器轨道迹向漂移数据及傅里叶变换处理得到的幅频曲线;由幅频响应曲线中的前2个峰值和起始点,可以提取得到三组频率、幅值和相位信息A4,n33,A5,n44,A6,A7Figure 4 is the amplitude-frequency curve obtained from the corresponding spacecraft track drift data and Fourier transform processing; from the first two peaks and the starting point in the amplitude-frequency response curve, three groups of frequency, amplitude and Phase information A 4 , n 3 , θ 3 , A 5 , n 4 , θ 4 , A 6 , A 7 .

图5即为相应的航天器轨道法向漂移数据及傅里叶变换处理得到的幅频曲线。由幅频响应曲线中的第1个峰值处,可以提取得到一组频率、幅值和相位信息A8,n55Figure 5 is the amplitude-frequency curve obtained from the corresponding spacecraft orbital normal drift data and Fourier transform processing. A set of frequency, amplitude and phase information A 8 , n 5 , θ 5 can be extracted from the first peak in the amplitude-frequency response curve.

将图3至图5提取到的频率、幅值和相位信息整合在一起,最后利用公式(12)进行反向计算,便可以得到初始状态误差的估计值(即表1中傅里叶变换反演位置误差和傅里叶变换反演速度误差),此估计值与初始状态误差(即表1中初始航天器位置误差和初始航天器速度误差)之差即为基于伪相对运动的航天器实时轨道改进精度。Integrating the frequency, amplitude and phase information extracted from Fig. 3 to Fig. 5, and finally using the formula (12) for reverse calculation, the estimated value of the initial state error can be obtained (that is, the Fourier transform inversion position error and the Fourier transform inversion velocity error in Table 1), this estimated value is different from the initial state error (That is, the difference between the initial spacecraft position error and the initial spacecraft velocity error in Table 1) is the improved accuracy of the real-time orbit of the spacecraft based on pseudo relative motion.

最后所应说明的是,以上实施例仅用以说明本发明的技术方案而非限制。尽管参照实施例对本发明进行了详细说明,本领域的普通技术人员应当理解,对本发明的技术方案进行修改或者等同替换,都不脱离本发明技术方案的精神和范围,其均应涵盖在本发明的权利要求范围当中。Finally, it should be noted that the above embodiments are only used to illustrate the technical solutions of the present invention rather than limit them. Although the present invention has been described in detail with reference to the embodiments, those skilled in the art should understand that modifications or equivalent replacements to the technical solutions of the present invention do not depart from the spirit and scope of the technical solutions of the present invention, and all of them should be included in the scope of the present invention. within the scope of the claims.

Claims (3)

1.一种基于伪相对运动的航天器实时轨道改进方法,其特征在于,包括:1. A real-time orbit improvement method for spacecraft based on pseudo-relative motion, characterized in that it comprises: 步骤1)将航天器的测量轨道作为参考轨道,以初始时刻测量轨道确定的航天器初始状态作为预报轨道的起点,并依据轨道动力学模型生成该预报轨道;Step 1) taking the measured orbit of the spacecraft as the reference orbit, taking the initial state of the spacecraft determined by the measured orbit at the initial moment as the starting point of the predicted orbit, and generating the predicted orbit according to the orbital dynamics model; 步骤2)将预报轨道与测量轨道之间的差值作为轨道漂移数据,并以该轨道漂移数据所形成的轨迹定义为航天器的伪相对运动;Step 2) using the difference between the predicted orbit and the measured orbit as the orbital drift data, and defining the trajectory formed by the orbital drift data as the pseudo-relative motion of the spacecraft; 步骤3)分别求解无、有摄动条件下伪相对运动的动力学模型,得到无、有摄动条件下伪相对运动的解析表达式,运用傅里叶变换方法处理轨道漂移数据后,以解算得到的解析表达式反演出航天器的初始状态误差的估计值;Step 3) Solve the dynamic model of pseudo relative motion under the condition of no perturbation and presence of perturbation respectively, obtain the analytical expression of pseudo relative motion under the condition of no perturbation and presence of perturbation, and use the Fourier transform method to process the orbital drift data to solve The calculated analytical expression is used to invert the estimated value of the initial state error of the spacecraft; 步骤4)利用初始状态误差的估计值与参考轨道的初始状态误差值之差,作为航天器轨道改进值。Step 4) Use the difference between the estimated value of the initial state error and the initial state error value of the reference orbit as the spacecraft orbit improvement value. 2.根据权利要求1所述的基于伪相对运动的航天器实时轨道改进方法,其特征在于,2. the spacecraft real-time orbit improvement method based on pseudo-relative motion according to claim 1, is characterized in that, 所述步骤3)中的无摄动条件下伪相对运动的解析表达式为:The analytical expression of pseudo-relative motion under the condition of no perturbation in described step 3) is: 其中,n为轨道平均角运动,即参考轨道角频率,t表示时间,各参数及其关系设置为:Among them, n is the average angular motion of the orbit, that is, the reference orbital angular frequency, t represents the time, and the parameters and their relationships are set as: 其中,(x0,y0,z0)表示三轴初始位置误差,表示三轴初始速度误差;Among them, (x 0 , y 0 , z 0 ) represents the three-axis initial position error, Indicates the three-axis initial velocity error; 运用傅里叶变换方法处理轨道漂移数据,解算得到常值项xc yc、长期项3xcnt/2和周期项csin(nt+φ)中的各系数xc,b,yc,c,φ,并利用上述解析表达式进行反演,得到初始状态误差的估计值 Using the Fourier transform method to process the orbital drift data, the constant value term x c y c , the long-term term 3x c nt/2 and the periodic term are obtained Each coefficient x c ,b, in csin(nt+φ) y c ,c,φ, and use the above analytic expression to invert to get the initial state error estimated value of 3.根据权利要求1所述的基于伪相对运动的航天器实时轨道改进方法,其特征在于,3. the spacecraft real-time orbit improvement method based on pseudo-relative motion according to claim 1, is characterized in that, 所述步骤3)中的有摄动条件下伪相对运动的解析表达式为:The analytical expression of pseudo-relative motion under the perturbation condition in described step 3) is: 其中,各参数及其关系设置为:Among them, the parameters and their relationships are set as: 其中,n为轨道平均角运动,即参考轨道角频率,t表示时间,u为地球引力系数,rref为参考轨道地心距,iref为参考轨道倾角,J2为第二带谐项,Re为地球半径,n1、n2、n3、n4、n5分别为相对运动中各周期分量的角频率;(x0,y0,z0)表示三轴初始位置误差,表示三轴初始速度误差;Among them, n is the average orbital angular motion, that is, the reference orbital angular frequency, t is the time, u is the gravitational coefficient of the earth, rref is the reference orbital center distance, iref is the reference orbital inclination, J2 is the second harmonic term, R e is the radius of the earth, n 1 , n 2 , n 3 , n 4 , and n 5 are the angular frequencies of each periodic component in the relative motion, respectively; (x 0 , y 0 , z 0 ) represent the three-axis initial position error, Indicates the three-axis initial velocity error; 运用傅里叶变换方法处理轨道漂移数据,解算得到常值项A3,A7、长期项A6t和周期项A1cos(n1t+θ1),A2cos(n2t+θ2),A4cos(n3t+θ3),A5cos(n4t+θ4),A8sin(n5t+θ5)中的各系数A11,A22,A3,A43,A54,A6,A7,A85,并利用上述解析表达式进行反演,得到初始状态误差的估计值 Using the Fourier transform method to process the orbital drift data, the constant value items A 3 , A 7 , the long-term item A 6 t and the periodic item A 1 cos(n 1 t+θ 1 ), A 2 cos(n 2 t +θ 2 ), A 4 cos(n 3 t+θ 3 ), A 5 cos(n 4 t+θ 4 ), A 8 sin(n 5 t+θ 5 ), A 1 , θ 1 , A 2 , θ 2 , A 3 , A 4 , θ 3 , A 5 , θ 4 , A 6 , A 7 , A 8 , θ 5 , and use the above analytical expressions to perform inversion to obtain the initial state error estimated value of
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