CN107024211B - A kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method - Google Patents

A kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method Download PDF

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CN107024211B
CN107024211B CN201710478722.1A CN201710478722A CN107024211B CN 107024211 B CN107024211 B CN 107024211B CN 201710478722 A CN201710478722 A CN 201710478722A CN 107024211 B CN107024211 B CN 107024211B
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arrival time
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宁晓琳
桂明臻
吴伟仁
房建成
刘刚
孙晓函
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Beijing University of Aeronautics and Astronautics
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    • G01CMEASURING DISTANCES, LEVELS OR BEARINGS; SURVEYING; NAVIGATION; GYROSCOPIC INSTRUMENTS; PHOTOGRAMMETRY OR VIDEOGRAMMETRY
    • G01C21/00Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00
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Abstract

The present invention relates to a kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation methods.The state model of spacecraft is established according to dynamics of orbits first, it is utilized respectively angle measurement sensor again and obtains starlight angular distance measurement, pulse arrival time measurement is obtained using X-ray pulsar detector, astronomical doppler velocity measurement is obtained using spectrometer, establishes starlight angular distance measurement model, differential pulse arrival time measurement model and difference astronomy doppler velocity measurement model respectively according to these measurements later.The position and speed of UKF filtering estimation spacecraft is used after discretization.The invention belongs to Spacecraft Autonomous Navigation field, estimated accuracy of the present invention is high, has important practical significance to Spacecraft Autonomous Navigation.

Description

A kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method
Technical field
The invention belongs to Spacecraft Autonomous Navigation fields, are related to a kind of based on starlight angular distance, differential pulse arrival time, difference Divide the celestial self-navigation method of the measurements such as astronomical doppler velocity.
Background technique
China's plan emits a Mars probes in the year two thousand twenty, therefore mars exploration will attract more and more concerns. For deep space exploration task, navigation accuracy has an important influence the success or failure of task.Mainly pass through ground observing and controlling at present It stands and provides navigation information for spacecraft.With the increase of distance between spacecraft and the earth, signal is carried out by ground control station The round trip time delay of transmission will be increasing.In addition, day, which insults, will cause signal interruption.Therefore, it is necessary to improve the certainly leading of spacecraft Boat ability.
The autonomous navigation method that can be used for deep space probe mainly has astronomical angle measurement air navigation aid, X-ray pulsar ranging Air navigation aid and astronomical Doppler range rate measurement air navigation aid.Astronomical angle measurement air navigation aid passes through measurement spacecraft and nearly celestial body and navigation Angle between fixed star obtains the location information of spacecraft.But the navigation accuracy of this method is with spacecraft and nearly celestial body Between distance increase and decline.X-ray pulsar range-finding navigation can provide high-precision location information, and navigation accuracy not by The influence of position between spacecraft and celestial body.But since the signal of X-ray pulsar is fainter, it usually needs by longer The epoch of time folds to obtain measurement.In addition, pulsar turning error and satellite atomic clock clock deviation will affect navigation essence Degree.Astronomical Doppler range rate measurement navigation obtains spacecraft by measurement spectrum frequency displacement as caused by radial motion between spacecraft and fixed star Velocity information.But this method can not provide location information, and the dynamic change of stellar spectrum will affect its navigation essence Degree.
Summary of the invention
The present invention proposes a kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method, utilizes starlight angle Absolute location information is provided away from measurement, is missed using time difference X-ray pulsar pulse arrival time measurement attenuation systems The influence of difference, provides relative position information, weakens stellar spectrum dynamic using time difference astronomy doppler velocity measurement and becomes The influence of change, provides velocity information.Three kinds of measurements are filtered by UKF and are combined, provide high-precision lead for deep space probe Boat information.
The technical solution adopted by the present invention to solve the technical problems are as follows: the state of spacecraft is established according to dynamics of orbits Model, obtains starlight angular distance measurement using angle measurement sensor, obtains pulse arrival time amount using X-ray pulsar detector Measurement obtains astronomical doppler velocity measurement using spectrometer, establishes starlight angular distance respectively according to these measurements and measure mould Type, differential pulse arrival time measurement model and difference astronomy doppler velocity measurement model.Estimated after discretization using UKF filtering Count the position and speed of spacecraft.
Specifically includes the following steps:
1. establishing the System State Model based on dynamics of orbits
It in the sports immunology of Mars Approach phase is using the sun as center celestial body to be taken the photograph Three-Body Model by spacecraft, by other Disturbance is considered as process noise.Kinetic model at solar core inertial coodinate system (J2000.0) is writeable are as follows:
Wherein | | | | indicate 2 norms of vector, | | | |3Indicate | | | | cube, r and v be spacecraft relatively too The position and speed of sun.μsAnd μmIt is the gravitational constant of the sun and Mars, r respectivelymIt is position vector of the Mars with respect to the sun, rsm =r-rmIt is position vector of the spacecraft with respect to Mars.W is process noise caused by various disturbances.State mould can be obtained by above formula Type is as follows:
Wherein quantity of state X=[r, v]TThe position for being spacecraft under sun inertial coodinate system and speed,For quantity of state X Derivative,For moment t'sF (X (t), t) is mission nonlinear continuous state transfer function, and w is process noise, w (t) w for being moment t.
2. judging whether there is pulse arrival time measurement
Due to pulse signal need observation cycle it is longer, solid with starlight angular distance measurement and astronomy doppler velocity measurement Amount is compared, and the sampling period of pulse arrival time measurement is longer.Therefore, with starlight angular distance measurement and astronomical doppler velocity The sampling period of measurement is as filtering cycle.When filtered time instant does not have pulse arrival time measurement, to by state model And the system model that starlight angular distance measurement model, difference astronomy doppler velocity measurement model are constituted is used to by UKF filtering Posteriority state estimation and posteriori error covariance of the spacecraft with respect to the sun under property system.When filtered time instant has pulse arrival time When measurement, to by state model and starlight angular distance measurement model, difference astronomy doppler velocity measurement model, differential pulse to The system model constituted up to measuring time value model is estimated by the posteriority state that UKF filters the opposite sun of spacecraft under acquisition inertial system Meter and posteriori error covariance.
3. establishing the measurement model of starlight angular distance
The starlight angular distance between spacecraft and phobos, Deimos and its background fixed star is obtained using angle measurement sensor, with this A little starlight angular distances establish measurement model as measurement:
Wherein αp1And αp2It is the starlight angular distance between spacecraft and phobos and two background fixed stars, α respectivelyd1And αd2Respectively It is the starlight angular distance between spacecraft and Deimos and two background fixed stars, rsp、rsdIt is phobos, Deimos respectively relative to boat The position vector of its device, s1、s2It is the direction vector of two fixed stars under inertial system, r respectivelyp、rdIt is phobos, Deimos respectively Position vector relative to the sun.
Using these starlight angular distances as measurement Z1=[αp1p2d1d2]T, starlight angular distance measurement model can be established Expression formula:
Z1=[αp1p2d1d2]T=h1[X(t),t]+v1(t) (4)
Wherein h1() indicates the non-linear continuous measurement function of starlight angular distance, v1(t) amount of t moment starlight angular distance is indicated Survey noise.
4. establishing the measurement model of difference astronomy doppler velocity
Solar spectrum frequency displacement is obtained using spectrometer, and radial velocity of the spacecraft with respect to the sun is obtained according to frequency displacement, with This establishes measurement model as measurement:
Wherein vrIndicate radial velocity measurement of the spacecraft with respect to the sun, vrtIndicate radial speed of the spacecraft with respect to the sun Spend true value, υpIndicate the disturbance term as caused by solar spectrum frequency fluctuation, υmIndicate that astronomical doppler velocity measures noise.
Establish the measurement model of difference astronomy doppler velocity:
Wherein vr(t) and vrIt (t-1) is the radial velocity measurement of t moment and t-1 moment spacecraft with respect to the sun respectively, vrt(t) and vrtIt (t-1) is the radial velocity true value of t moment and t-1 moment spacecraft with respect to the sun, υ respectivelyp(t) and υp(t- It 1) is disturbance term caused by t moment and t-1 moment solar spectrum frequency fluctuation, υ respectivelym(t) and υm(t-1) be respectively t moment and The measurement noise at t-1 moment, △ υp(t)=υp(t)-υpIt (t-1) is υ after differencepResidual error, △ υm(t)=υm(t)-υm(t-1) It is υ after differencemResidual error.
Using difference astronomy doppler velocity as measurement Z2=[vr(t)-vr(t-1)] difference astronomy Doppler can, be established The expression formula of velocity measurement model:
Z2=[vr(t)-vr(t-1)]=h2[X(t),X(t-1)]+v2(t) (7)
Wherein h2() indicates the non-linear continuous measurement function of difference astronomy doppler velocity, v2(t) indicate that t moment is poor Divide the error in measurement of astronomical doppler velocity.With the posteriority state estimation at t-1 momentInstead of X (t-1), then difference arteries and veins The expression formula being flushed to up to measuring time value model is writeable are as follows:
Z2=h2[X(t),t]+v2(t) (8)
5. establishing the measurement model of differential pulse arrival time
Pulse arrival time measurement is obtained using X-ray pulsar detector, using pulse arrival time as measurement Establish measurement model:
Wherein tbIndicate that pulsar pulse reaches the time of solar system mass center, tSCIndicate that pulsar pulse reaches spacecraft Time, rSIndicate that position vector of the spacecraft with respect to solar system mass center, c indicate that the light velocity, n indicate side of the pulsar under inertial system To vector, D0Pulsar is indicated to the distance of solar system mass center, b indicates position vector of the solar system mass center with respect to the sun.
Establish the measurement model of differential pulse arrival time:
Wherein τ (t) indicates the differential pulse arrival time of t moment, tb(t) and tb(t-1) when respectively indicating t moment and t-1 Carve the time that pulsar pulse reaches solar system mass center, tSC(t) and tSC(t-1) t moment and t-1 moment pulsar are respectively indicated The time of pulse arrival spacecraft.
Using differential pulse arrival time as measurement Z3=[τ (t)] can establish differential pulse arrival time measurement model Expression formula:
Z3=[τ (t)]=h3[X(t),X(t-1)]+v3(t) (11)
Wherein h3() indicates the non-linear continuous measurement function of differential pulse arrival time, v3(t) t moment difference is indicated The measurement noise of pulse arrival time.With the posteriority state estimation at t-1 momentInstead of X (t-1), then differential pulse arrives Expression formula up to measuring time value model is writeable are as follows:
Z3=h3[X(t),t]+v3(t) (12)
6. carrying out discretization
When filtered time instant does not have pulse arrival time measurement, if the measurement Z of navigation system at this time12=[Z1,Z2]T, Measure noise v12=[v1,v2]T, Navigation System Model are as follows:
Wherein h12() indicates the non-linear continuous measurement function of navigation system when no pulse arrival time measurement.It is right Formula (13) carries out discretization:
Wherein XkAnd Z12kThe quantity of state of etching system and system when without pulse arrival time measurement when respectively indicating k Measurement, F (Xk-1, k-1) be f (X (t), t) it is discrete after nonlinear state transfer function, H12(Xk, k) and it is h12[X (t), t] from Non-linear measurement function after dispersion, WkAnd V12kRespectively indicate w (t) and v12(t) equivalent noise after discrete.
When filtered time instant has pulse arrival time measurement, if the measurement Z=[Z of navigation system at this time1,Z2,Z3]T, Measure noise v=[v1,v2,v3]T, Navigation System Model are as follows:
Wherein h () indicates the non-linear continuous measurement function of navigation system when pulse arrival time measurement.To formula (15) discretization is carried out:
Wherein ZkIndicate the measurement of etching system when k, H (Xk, k) be h [X (t), t] it is discrete after non-linear measurement function, VkIndicate the equivalent noise after v (t) is discrete.
7. carrying out the position and speed estimation that UKF filtering obtains spacecraft
When filtered time instant does not have pulse arrival time measurement, UKF is passed through to the system model formula (14) after discretization Be filtered obtain inertial system under spacecraft with respect to the sun posteriority state estimationAnd posteriori error association side DifferenceWhereinRespectively position of the kth moment spacecraft with respect to the sun, speed Posterior estimator.When filtered time instant has arteries and veins It is flushed to up to when time quantum measurement, acquisition is filtered by UKF to the system model formula (16) after discretizationAndIt willAndOutput, while these estimated values are returned into filter, for obtaining the output at k+1 moment.
The principle of the present invention is: obtaining observable Space Vehicle position information completely using starlight angular distance, but precision is not high. The pulse arrival time measurement obtained using the front and back moment obtains differential pulse arrival time by difference, weakens pulsar angle The influence of location error and satellite atomic clock clock deviation to navigation accuracy, obtains high-precision location information.It is obtained using the front and back moment The astronomical doppler velocity measurement obtained obtains difference astronomy doppler velocity by difference, weakens stellar spectrum dynamic change pair The influence of navigation accuracy obtains high-precision velocity information.The state model that spacecraft is established according to dynamics of orbits, builds respectively Vertical starlight angular distance measurement model, differential pulse arrival time measurement model and difference astronomy doppler velocity measurement model, it is discrete It filters to obtain the high-precision position and speed of spacecraft using UKF after change.
The advantages of the present invention over the prior art are that: (1) it realizes and navigates to the high-precision independent of spacecraft.(2) sharp High-precision location information is obtained with differential pulse arrival time.(3) it is obtained using difference astronomy doppler velocity high-precision Velocity information.
Detailed description of the invention
Fig. 1 is deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method flow chart in the present invention.
Fig. 2 is culminant star optic angle of the present invention away from measurement model schematic diagram.
Fig. 3 is X-ray pulsar range-finding navigation schematic illustration in the present invention.
Specific embodiment
Fig. 1 gives deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method system flow chart.Here By taking mars exploration Approach phase as an example, the specific implementation process that the present invention will be described in detail:
1. establishing the System State Model based on dynamics of orbits
It in the sports immunology of Mars Approach phase is using the sun as center celestial body to be taken the photograph Three-Body Model by spacecraft, by other Disturbance is considered as process noise.Kinetic model at solar core inertial coodinate system (J2000.0) is writeable are as follows:
Wherein | | | | indicate 2 norms of vector, | | | |3Indicate | | | | cube, r and v be spacecraft relatively too The position and speed of sun.μsAnd μmIt is the gravitational constant of the sun and Mars, r respectivelymIt is position vector of the Mars with respect to the sun, rsm =r-rmIt is position vector of the spacecraft with respect to Mars.W is process noise caused by various disturbances.State mould can be obtained by above formula Type is as follows:
Wherein quantity of state X=[r, v]TThe position for being spacecraft under sun inertial coodinate system and speed,For quantity of state X Derivative,For moment t'sF (X (t), t) is mission nonlinear continuous state transfer function, and w is process noise, w (t) For the w of moment t.
2. judging whether there is pulse arrival time measurement
Due to pulse signal need observation cycle it is longer, solid with starlight angular distance measurement and astronomy doppler velocity measurement Amount is compared, and the sampling period of pulse arrival time measurement is longer.Therefore, with starlight angular distance measurement and astronomical doppler velocity The sampling period of measurement is as filtering cycle.When filtered time instant does not have pulse arrival time measurement, to by state model And the system model that starlight angular distance measurement model, difference astronomy doppler velocity measurement model are constituted is used to by UKF filtering Posteriority state estimation and posteriori error covariance of the spacecraft with respect to the sun under property system.When filtered time instant has pulse arrival time When measurement, to by state model and starlight angular distance measurement model, difference astronomy doppler velocity measurement model, differential pulse to The system model constituted up to measuring time value model is estimated by the posteriority state that UKF filters the opposite sun of spacecraft under acquisition inertial system Meter and posteriori error covariance.
3. establishing the measurement model of starlight angular distance
The starlight angular distance between spacecraft and phobos, Deimos and its background fixed star is obtained using angle measurement sensor, with this A little starlight angular distances establish measurement model as measurement.Fig. 2 gives starlight angular distance measurement model schematic diagram.Wherein rsp、rsdPoint It is not the position vector of phobos, Deimos relative to spacecraft, s1、s2It is the direction vector of two fixed stars under inertial system respectively, rp、rdIt is the position vector of phobos, Deimos relative to the sun respectively.Starlight angular distance measurement model is writeable are as follows:
Wherein αp1And αp2It is the starlight angular distance between spacecraft and phobos and two background fixed stars, α respectivelyd1And αd2Respectively It is the starlight angular distance between spacecraft and Deimos and two background fixed stars.Using these starlight angular distances as measurement Z1=[αp1, αp2d1d2]T, the expression formula of starlight angular distance measurement model can be established:
Z1=[αp1p2d1d2]T=h1[X(t),t]+v1(t) (4)
Wherein h1() indicates the non-linear continuous measurement function of starlight angular distance, v1(t) amount of t moment starlight angular distance is indicated Survey noise.
4. establishing the measurement model of difference astronomy doppler velocity
Solar spectrum frequency displacement is obtained using spectrometer, and radial velocity of the spacecraft with respect to the sun is obtained according to frequency displacement, with This establishes measurement model as measurement:
Wherein vrIndicate radial velocity measurement of the spacecraft with respect to the sun, vrtIndicate radial speed of the spacecraft with respect to the sun Spend true value, υpIndicate the disturbance term as caused by solar spectrum frequency fluctuation, υmIndicate that astronomical doppler velocity measures noise.
Establish the measurement model of difference astronomy doppler velocity:
Wherein vr(t) and vrIt (t-1) is the radial velocity measurement of t moment and t-1 moment spacecraft with respect to the sun respectively, vrt(t) and vrtIt (t-1) is the radial velocity true value of t moment and t-1 moment spacecraft with respect to the sun, υ respectivelyp(t) and υp(t- It 1) is disturbance term caused by t moment and t-1 moment solar spectrum frequency fluctuation, υ respectivelym(t) and υm(t-1) be respectively t moment and The measurement noise at t-1 moment, △ υp(t)=υp(t)-υpIt (t-1) is υ after differencepResidual error, △ υm(t)=υm(t)-υm(t-1) It is υ after differencemResidual error.
Using difference astronomy doppler velocity as measurement Z2=[vr(t)-vr(t-1)] difference astronomy Doppler can, be established The expression formula of velocity measurement model:
Z2=[vr(t)-vr(t-1)]=h2[X(t),X(t-1)]+v2(t) (7)
Wherein h2() indicates the non-linear continuous measurement function of difference astronomy doppler velocity, v2(t) indicate that t moment is poor Divide the error in measurement of astronomical doppler velocity.With the posteriority state estimation at t-1 momentInstead of X (t-1), then difference arteries and veins The expression formula being flushed to up to measuring time value model is writeable are as follows:
Z2=h2[X(t),t]+v2(t) (8)
5. establishing the measurement model of differential pulse arrival time
Fig. 3 gives X-ray pulsar range-finding navigation schematic illustration.Wherein tSCAnd tbRespectively indicate i-th pulsar Pulse reaches the time of spacecraft and solar system mass center (SSB), and n is the direction vector of lower i-th pulsar of day heart inertial system, rS Position vector for detector with respect to solar system mass center, is represented by rS=r-b, b are position vector of the SSB with respect to the sun, c table Show the light velocity.As can be seen from Figure, c (tb-tSC) it is believed that rSProjection on n.Consider relativistic effect and geometric effect, time Transformation model may be expressed as:
Wherein D0Pulsar is indicated to the distance of solar system mass center, equation the right first item is what geometric distance generated Doppler delay, Section 2 indicate that X-ray reaches time delay caused by the solar system in parallel, usually first two are referred to as Roemer delay, Section 3 indicate the time delay that bending of light generates under solar gravitation field action, and referred to as Shapiro prolongs Late.
Establish the measurement model of differential pulse arrival time:
Wherein τ (t) indicates the differential pulse arrival time of t moment, tb(t) and tb(t-1) when respectively indicating t moment and t-1 Carve the time that pulsar pulse reaches solar system mass center, tSC(t) and tSC(t-1) t moment and t-1 moment pulsar are respectively indicated The time of pulse arrival spacecraft.
Using differential pulse arrival time as measurement Z3=[τ (t)] can establish differential pulse arrival time measurement model Expression formula:
Z3=[τ (t)]=h3[X(t),X(t-1)]+v3(t) (11)
Wherein h3() indicates the non-linear continuous measurement function of differential pulse arrival time, v3(t) t moment difference is indicated The measurement noise of pulse arrival time.With the posteriority state estimation at t-1 momentInstead of X (t-1), then differential pulse arrives Expression formula up to measuring time value model is writeable are as follows:
Z3=h3[X(t),t]+v3(t) (12)
6. carrying out discretization
When filtered time instant does not have pulse arrival time measurement, if the measurement Z of navigation system at this time12=[Z1,Z2]T, Measure noise v12=[v1,v2]T, Navigation System Model are as follows:
Wherein h12() indicates the non-linear continuous measurement function of navigation system when no pulse arrival time measurement.It is right Formula (13) carries out discretization:
Wherein XkAnd Z12kThe quantity of state of etching system and system when without pulse arrival time measurement when respectively indicating k Measurement, F (Xk-1, k-1) be f (X (t), t) it is discrete after nonlinear state transfer function, H12(Xk, k) and it is h12[X (t), t] from Non-linear measurement function after dispersion, WkAnd V12kRespectively indicate w (t) and v12(t) equivalent noise after discrete.
When filtered time instant has pulse arrival time measurement, if the measurement Z=[Z of navigation system at this time1,Z2,Z3]T, Measure noise v=[v1,v2,v3]T, Navigation System Model are as follows:
Wherein h () indicates the non-linear continuous measurement function of navigation system when pulse arrival time measurement.To formula (15) discretization is carried out:
Wherein ZkIndicate the measurement of etching system when k, H (Xk, k) be h [X (t), t] it is discrete after non-linear measurement function, VkIndicate the equivalent noise after v (t) is discrete.
7. carrying out the position and speed estimation that UKF filtering obtains spacecraft
System model after discretization is filtered by UKF, specific step is as follows.
A. init state amountWith State error variance battle array P0
In formula,It is the estimated value of the 0th moment (initial time) Space Vehicle position and speed, X0It is the 0th moment spacecraft The true value of position and speed.
B. sigma sampled point is chosen
InA series of sampled points are nearby chosen, the mean value and covariance of these sample points are respectivelyWith State variable is 6 × 1 dimensions, then choosing 13 sample pointsAnd its weight w0,w1…,w12It is as follows respectively:
Wherein τ indicates zooming parameter,Indicate the i-th row or column of sqrtm of making even.
C. it transmits sigma sampled point and obtains prior estimate and prior uncertainty covariance
The one-step prediction of each sampled pointAre as follows:
Merge allObtain prior state estimationAre as follows:
Prior uncertainty covarianceAre as follows:
In formula, QkFor k moment state model noise covariance battle array.
D. it measures and updates
According to measurement equation, each sampled point is calculatedPrediction measurementWhen filtered time instant does not have pulse arrival When time quantum measures:
When filtered time instant has pulse arrival time measurement:
Merge allIt obtains prediction and measures YkAre as follows:
It calculates prediction and measures covariance Pyy,kAnd cross covariance Pxy,k:
Wherein RkThe measurement noise covariance battle array of etching system when for k.Calculate filtering gain KkAre as follows:
Calculate posteriority state estimation
Calculate posteriori error covariance
It willAndOutput, while these estimated values are returned into filter, for obtaining the output at k+1 moment.
The content that description in the present invention is not described in detail belongs to the prior art well known to professional and technical personnel in the field.

Claims (1)

1. a kind of deep space probe angle measurement/differential speed measuring/difference ranges Combinated navigation method, it is characterised in that: dynamic according to track Mechanics establishes the state model of spacecraft, obtains starlight angular distance measurement using angle measurement sensor, is detected using X-ray pulsar Device obtains pulse arrival time measurement, astronomical doppler velocity measurement is obtained using spectrometer, according to these measurements point Starlight angular distance measurement model, differential pulse arrival time measurement model and difference astronomy doppler velocity measurement model are not established; The position and speed of UKF filtering estimation spacecraft is used after discretization;Specifically includes the following steps:
1. establishing the System State Model based on dynamics of orbits
In the sports immunology of Mars Approach phase it is using the sun as center celestial body to be taken the photograph Three-Body Model by spacecraft, other is disturbed It is considered as process noise;Kinetic model under solar core inertial coodinate system is writeable are as follows:
Wherein | | | | indicate 2 norms of vector, | | | |3Indicate | | | | cube, r and v are position of the spacecraft with respect to the sun It sets and speed;μsAnd μmIt is the gravitational constant of the sun and Mars, r respectivelymIt is position vector of the Mars with respect to the sun, rsm=r-rm It is position vector of the spacecraft with respect to Mars;W is process noise caused by various disturbances;State model can be obtained by above formula such as Under:
Wherein quantity of state X=[r, v]TThe position for being spacecraft under sun inertial coodinate system and speed,For leading for quantity of state X Number,For moment t'sF (X (t), t) is mission nonlinear continuous state transfer function, and w is process noise, and w (t) is The w of moment t;
2. judging whether there is pulse arrival time measurement
Since the observation cycle that pulse signal needs is longer, Gu with starlight angular distance measurement and astronomical doppler velocity measurement phase Than the sampling period of pulse arrival time measurement is longer;Therefore, it is measured with starlight angular distance measurement and astronomical doppler velocity The sampling period of amount is as filtering cycle;When filtered time instant does not have pulse arrival time measurement, to by state model and star Optic angle is filtered by UKF away from the system model that measurement model, difference astronomy doppler velocity measurement model are constituted and obtains inertial system Posteriority state estimation and posteriori error covariance of the lower spacecraft with respect to the sun;When filtered time instant has pulse arrival time measurement When amount, when to being reached by state model and starlight angular distance measurement model, difference astronomy doppler velocity measurement model, differential pulse Between measurement model constitute system model by UKF filtering obtain inertial system under spacecraft relatively the sun posteriority state estimation with And posteriori error covariance;
3. establishing the measurement model of starlight angular distance
The starlight angular distance between spacecraft and phobos, Deimos and its background fixed star is obtained using angle measurement sensor, with these stars Optic angle is away from establishing measurement model as measurement:
Wherein αp1And αp2It is the starlight angular distance between spacecraft and phobos and two background fixed stars, α respectivelyd1And αd2It is boat respectively Starlight angular distance between its device and Deimos and two background fixed stars, rsp、rsdIt is phobos, Deimos respectively relative to spacecraft Position vector, s1、s2It is the direction vector of two fixed stars under inertial system, r respectivelyp、rdIt is that phobos, Deimos are opposite respectively In the position vector of the sun;
Using these starlight angular distances as measurement Z1=[αp1p2d1d2]T, the expression of starlight angular distance measurement model can be established Formula:
Z1=[αp1p2d1d2]T=h1[X(t),t]+v1(t) (4)
Wherein h1() indicates the non-linear continuous measurement function of starlight angular distance, v1(t) indicate that the measurement of t moment starlight angular distance is made an uproar Sound;
4. establishing the measurement model of difference astronomy doppler velocity
Solar spectrum frequency displacement is obtained using spectrometer, and radial velocity of the spacecraft with respect to the sun is obtained according to frequency displacement, is made with this Measurement model is established for measurement:
Wherein vrIndicate radial velocity measurement of the spacecraft with respect to the sun, vrtIndicate that spacecraft is true with respect to the radial velocity of the sun Real value, υpIndicate the disturbance term as caused by solar spectrum frequency fluctuation, υmIndicate that astronomical doppler velocity measures noise;
Establish the measurement model of difference astronomy doppler velocity:
Wherein vr(t) and vrIt (t-1) is the radial velocity measurement of t moment and t-1 moment spacecraft with respect to the sun, v respectivelyrt(t) And vrtIt (t-1) is the radial velocity true value of t moment and t-1 moment spacecraft with respect to the sun, υ respectivelyp(t) and υp(t-1) divide It is not disturbance term caused by t moment and t-1 moment solar spectrum frequency fluctuation, υm(t) and υmIt (t-1) is t moment and t-1 respectively The measurement noise at moment, Δ υp(t)=υp(t)-υpIt (t-1) is υ after differencepResidual error, Δ υm(t)=υm(t)-υm(t-1) it is υ after differencemResidual error;
Using difference astronomy doppler velocity as measurement Z2=[vr(t)-vr(t-1)] difference astronomy doppler velocity can, be established The expression formula of measurement model:
Z2=[vr(t)-vr(t-1)]=h2[X(t),X(t-1)]+v2(t) (7)
Wherein h2() indicates the non-linear continuous measurement function of difference astronomy doppler velocity, v2(t) t moment difference day is indicated The error in measurement of literary doppler velocity;With the posteriority state estimation at t-1 momentInstead of X (t-1), then differential pulse arrives Expression formula up to measuring time value model is writeable are as follows:
Z2=h2[X(t),t]+v2(t) (8)
5. establishing the measurement model of differential pulse arrival time
Pulse arrival time measurement is obtained using X-ray pulsar detector, is established using pulse arrival time as measurement Measurement model:
Wherein tbIndicate that pulsar pulse reaches the time of solar system mass center, tSCIndicate pulsar pulse reach spacecraft when Between, rSIndicate that position vector of the spacecraft with respect to solar system mass center, c indicate that the light velocity, n indicate direction of the pulsar under inertial system Vector, D0Pulsar is indicated to the distance of solar system mass center, b indicates position vector of the solar system mass center with respect to the sun;
Establish the measurement model of differential pulse arrival time:
Wherein τ (t) indicates the differential pulse arrival time of t moment, tb(t) and tb(t-1) t moment and t-1 moment arteries and veins are respectively indicated Rush the time that star pulse reaches solar system mass center, tSC(t) and tSC(t-1) t moment and t-1 moment pulsar pulse are respectively indicated Reach the time of spacecraft;
Using differential pulse arrival time as measurement Z3=[τ (t)], can establish the table of differential pulse arrival time measurement model Up to formula:
Z3=[τ (t)]=h3[X(t),X(t-1)]+v3(t) (11)
Wherein h3() indicates the non-linear continuous measurement function of differential pulse arrival time, v3(t) t moment differential pulse is indicated The measurement noise of arrival time;With the posteriority state estimation at t-1 momentInstead of X (t-1), then when differential pulse reaches Between measurement model expression formula it is writeable are as follows:
Z3=h3[X(t),t]+v3(t) (12)
6. carrying out discretization
When filtered time instant does not have pulse arrival time measurement, if the measurement Z of navigation system at this time12=[Z1,Z2]T, measure Noise v12=[v1,v2]T, Navigation System Model are as follows:
Wherein h12() indicates the non-linear continuous measurement function of navigation system when no pulse arrival time measurement;To formula into Row discretization:
Wherein XkAnd Z12kWhen respectively indicating k the quantity of state of etching system and when without pulse arrival time measurement system measurement Amount, F (Xk-1, k-1) be f (X (t), t) it is discrete after nonlinear state transfer function, H12(Xk, k) and it is h12[X (t), t] discretization Non-linear measurement function afterwards, WkAnd V12kRespectively indicate w (t) and v12(t) equivalent noise after discrete;
When filtered time instant has pulse arrival time measurement, if the measurement Z=[Z of navigation system at this time1,Z2,Z3]T, measure Noise v=[v1,v2,v3]T, Navigation System Model are as follows:
Wherein h () indicates the non-linear continuous measurement function of navigation system when pulse arrival time measurement;Formula is carried out Discretization:
Wherein ZkIndicate the measurement of etching system when k, H (Xk, k) be h [X (t), t] it is discrete after non-linear measurement function, VkTable Show the equivalent noise after v (t) is discrete;
7. carrying out the position and speed estimation that UKF filtering obtains spacecraft
When filtered time instant does not have pulse arrival time measurement, the system model formula after discretization is filtered by UKF Posteriority state estimation of the spacecraft with respect to the sun under acquisition inertial systemAnd posteriori error covarianceIts InRespectively position of the kth moment spacecraft with respect to the sun, speed Posterior estimator;When filtered time instant has pulse arrival Between measurement when, acquisition is filtered by UKF to the system model formula after discretizationAndIt willAndOutput, together When by these estimated values return filter, for obtaining the output at k+1 moment.
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* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
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CN111551172B (en) * 2020-05-13 2022-05-10 北京航空航天大学 Lunar probe angle measurement/time differential distance/speed combined navigation method
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CN111947668B (en) * 2020-08-26 2022-03-18 中南大学 Online estimation-based angle measurement/distance measurement combined navigation method for wooden star detector
CN113551667B (en) * 2021-07-21 2024-05-24 北京航空航天大学 Spacecraft inertia/star starlight vector/solar Doppler speed combined navigation method
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Citations (9)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN101672651A (en) * 2009-09-25 2010-03-17 北京航空航天大学 Autonomous astronomical navigation method of spark detector based on improved MMUPF filtering method
CN101692001A (en) * 2009-09-25 2010-04-07 北京航空航天大学 Autonomous celestial navigation method for deep space explorer on swing-by trajectory
CN101876710A (en) * 2010-04-29 2010-11-03 北京航空航天大学 Real-time satellite signal simulator based device for synchronously increasing and decreasing visible satellites and construction method thereof
CN103148856A (en) * 2013-03-04 2013-06-12 北京航空航天大学 Swing-by probe autonomous celestial navigation method based on adaptive scale change
CN104006813A (en) * 2014-04-03 2014-08-27 中国人民解放军国防科学技术大学 Pulsar/starlight angle combination navigation method of high orbit satellite
CN105203101A (en) * 2015-09-02 2015-12-30 北京航空航天大学 Deep space explorer acquisition phase celestial navigation method based on target object ephemeris correction
CN106017480A (en) * 2016-05-20 2016-10-12 武汉科技大学 Deeply-integrated navigation method for acquisition phase of deep space exploration
CN106204629A (en) * 2016-08-17 2016-12-07 西安电子科技大学 Space based radar and infrared data merge moving target detection method in-orbit
CN106767845A (en) * 2017-02-20 2017-05-31 中国人民解放军国防科学技术大学 Spacecraft air navigation aid based on earth rail ground moon libration point Heterogeneous constellation high

Patent Citations (9)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN101672651A (en) * 2009-09-25 2010-03-17 北京航空航天大学 Autonomous astronomical navigation method of spark detector based on improved MMUPF filtering method
CN101692001A (en) * 2009-09-25 2010-04-07 北京航空航天大学 Autonomous celestial navigation method for deep space explorer on swing-by trajectory
CN101876710A (en) * 2010-04-29 2010-11-03 北京航空航天大学 Real-time satellite signal simulator based device for synchronously increasing and decreasing visible satellites and construction method thereof
CN103148856A (en) * 2013-03-04 2013-06-12 北京航空航天大学 Swing-by probe autonomous celestial navigation method based on adaptive scale change
CN104006813A (en) * 2014-04-03 2014-08-27 中国人民解放军国防科学技术大学 Pulsar/starlight angle combination navigation method of high orbit satellite
CN105203101A (en) * 2015-09-02 2015-12-30 北京航空航天大学 Deep space explorer acquisition phase celestial navigation method based on target object ephemeris correction
CN106017480A (en) * 2016-05-20 2016-10-12 武汉科技大学 Deeply-integrated navigation method for acquisition phase of deep space exploration
CN106204629A (en) * 2016-08-17 2016-12-07 西安电子科技大学 Space based radar and infrared data merge moving target detection method in-orbit
CN106767845A (en) * 2017-02-20 2017-05-31 中国人民解放军国防科学技术大学 Spacecraft air navigation aid based on earth rail ground moon libration point Heterogeneous constellation high

Non-Patent Citations (6)

* Cited by examiner, † Cited by third party
Title
A Novel Differential Doppler Measurement-Aided Autonomous Celestial Navigation Method for Spacecraft During Approach Phase;XIAOLIN NING等;《IEEE TRANSACTIONS ON AEROSPACE AND ELECTROINC SYSTEMS》;20170430;第53卷(第2期);587-597 *
Observability analysis of autonomous navigation for deep space exploration with LOSTOAvelocity measurements;Xin Ma等;《IEEE》;20161231;1-9 *
基于X射线脉冲星的航天器自主导航方法研究;刘劲;《中国博士学位论文全文数据库工程科技II辑》;20110915(第9期);C032-8 *
基于星光多普勒的脉冲星脉冲到达时间补偿;刘劲;《华中科技大学学报(自然科学版)》;20140131;第42卷(第1期);129-132 *
脉冲多普勒导引头角跟踪系统建模与仿真技术研究;王刚;《中国优秀硕士学位论文全文数据库工程科技II辑》;20060715(第7期);C032-20 *
行星际间飞行的自主导航方法研究;何赟晟;《中国优秀硕士学问论文全文数据库工程科技II辑》;20120715(第7期);C031-416 *

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