CN107144283A - A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe - Google Patents

A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe Download PDF

Info

Publication number
CN107144283A
CN107144283A CN201710527892.4A CN201710527892A CN107144283A CN 107144283 A CN107144283 A CN 107144283A CN 201710527892 A CN201710527892 A CN 201710527892A CN 107144283 A CN107144283 A CN 107144283A
Authority
CN
China
Prior art keywords
mrow
msub
mfrac
mover
deep space
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.)
Pending
Application number
CN201710527892.4A
Other languages
Chinese (zh)
Inventor
刘宇
阳光
王卫华
苏枫
秦长涛
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
Shanghai Aerospace Control Technology Institute
Original Assignee
Shanghai Aerospace Control Technology Institute
Priority date (The priority date 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 date listed.)
Filing date
Publication date
Application filed by Shanghai Aerospace Control Technology Institute filed Critical Shanghai Aerospace Control Technology Institute
Priority to CN201710527892.4A priority Critical patent/CN107144283A/en
Publication of CN107144283A publication Critical patent/CN107144283A/en
Pending legal-status Critical Current

Links

Classifications

    • GPHYSICS
    • G01MEASURING; TESTING
    • 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
    • G01C21/24Navigation; Navigational instruments not provided for in groups G01C1/00 - G01C19/00 specially adapted for cosmonautical navigation

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)
  • Navigation (AREA)

Abstract

The present invention is disclosed the invention provides a kind of high considerable degree optical pulsar hybrid navigation method for deep space probe, and it is included:Step 1:Observations of pulsar equation is mixed with optical observation equation, mixing observational equation is set up;Step 2:Using many body gravity models of deep space probe, inertial position and speed using detector set up detector's status equation as quantity of state;Step 3:Construct EKF and optimal estimation calculating is carried out to the state of detector, obtain Position And Velocity under accurate detector inertial system.The method of the present invention overcomes the problem of inertial navigation accumulated error is big, solve the problem of pulsar navigation ornamental is weak, it greatly strengthen the ornamental of navigation system, greatly reduce the convergence time of navigation system, and navigation accuracy is effectively raised, it can be directly used for the autonomous control of deep space probe.

Description

A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe
Technical field
The present invention relates to deep space probe air navigation aid, and in particular to a kind of high considerable degree optics for deep space probe Pulsar hybrid navigation method, it comprehensively utilizes the angular observation information and pulsar of the celestial body apart from observation information, in terms of Calculate the main precision navigation information of deep space probe.
Background technology
Ground based radio navigation limited ability in the distribution of tracking telemetry and command station, device the factor such as distance constraint, it is difficult to for deep spy Survey device and affordable high-precision real-time navigation information is provided.Traditional inertial navigation is not suitable for making due to error accumulation effect For main navigation means.The Optical autonomous navigation of single goal is simultaneously non-fully considerable, and it is difficult to be generalized to whole mission phase in addition. X-ray pulsar navigation technology has that independence is strong, anti-interference is good, can support the spies such as the full mission phase of deep space probe Point.But the X-ray signal of pulsar is very weak, more feasible sensor scheme is only capable of tracking 1~2 navigation pulsar simultaneously, The orbit information of detector can only be determined using Dynamic orbit determination method.Due to only having 1 vector, system is caused locally can not See.
The content of the invention
It is an object of the invention to provide a kind of air navigation aid, it has high ornamental, can be used for survey of deep space.
In order to achieve the above object, mixed the invention provides a kind of high considerable degree optical pulsar for deep space probe Air navigation aid is closed, this method comprises the following steps:
Step 1:During deep space probe is close to big celestial body, introduce to the optical observation amount of neighbouring celestial body as supplement, Observations of pulsar equation is mixed with optical observation equation, mixing observational equation is set up;
Step 2:Using many body gravity models of deep space probe, inertial position and speed using detector are built as quantity of state Vertical detector's status equation;
Step 3:According to the observational equation of step 1 and the state equation of step 2, construction EKF is to detector State carry out optimal estimation calculating, obtain Position And Velocity under accurate detector inertial system;Wherein, EKF Equation be:
K (k)=P (k, k-1) HT(k) [H (k) P (k, k-1) HT(k)+R(k)]-1
P (k, k-1)=Φ (k, k-1) P (k-1) ΦT(k, k-1)+Q (k-1)
Wherein, initial value isP (0,0)=Var { x (0) }=Px(0), in formula,Known state model Covariance matrix E [w (k) w (k) of noiseT]=Q, covariance matrix E [v (k) v (k) of measurement model noiseT]=R, w represent system Model error, v represents measurement noise, and k represents current step number, and x represents quantity of state, and μ represents gravitational constant, and X represents discrete state Amount, T represents discrete periodic, and I represents unit matrix, and Z represents discrete observation amount, and t represents the time..
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, described pulse Star observational equation is:
In formula, ΔΦiThe observation phase difference of pulse signal,For the unit direction vector of pulse direction of visual lines, λ is navigation The distance propagated in pulse signal a cycle, Δ Ni is pulse period complete cycle difference, Δ x be spacecraft and sun barycenter it Between distance, i represents pulsar sequence number.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, described optics Observational equation is:
Wherein, p, 1 is coordinate of the photocentre of target celestial body in camera image plane, and unit is millimeter, RcIFor camera coordinates It is the pose transformation matrix of relative inertness coordinate system, x, y, z is position of the detector under Mars J2000 inertial coodinate systems.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, RcIIt is to utilize phase The posture for the body coordinate system relative inertness coordinate system that machine coordinate system opposing body Conversion Matrix of Coordinate and star sensor are determined Transition matrix is determined.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, described mixing Observational equation:
Z=h (X)+v;Wherein, z represents p, l, △ φi;V is measurement noise.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, in step 2, visit Surveying device state equation is:
Wherein, state variable The position vector of detector is represented,Represent the speed arrow of detector Amount;W is system model error, ax ay azFor projection of the solar gravitation perturbation under Mars inertial system, x, y, z is that detector exists Position under Mars J2000 inertial coodinate systems,Wherein, centered on GM celestial body gravitational constant;R is flight Position vector of the device in inertial system;P is perturbative force.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, r calculation formula It is as follows:
Wherein, rpFor the position vector of the relatively large celestial body barycenter of detector;μM、μS、μE、μJBe followed successively by big celestial body, the sun, The gravitational constant of ball, Jupiter;rMp,rSp,rEp,rJpIt is followed successively by the position vector of big celestial body, the sun, the earth, Jupiter to detector; rMS,rME,rMJFor position vector between two days bodies, drawn by the DE405 ephemeris in U.S. jet laboratory (JPL), subscript M is represented Big celestial body, under
Mark S represents the sun, and subscript E represents the earth, and subscript J represents Jupiter.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, in step 3, structure The method for making EKF is included:
Step 3.1, state equation discretization first to step 2, and surroundingLinearisation,Nearby expand into two Rank Taylor series;
Step 3.2, by the observational equation discretization of step one, andLinearisation nearby.
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, step 3.1 is handled Second order Taylor series afterwards are:
Above-mentioned is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, wherein, step 3.2 is handled Equation afterwards is:
The method that the present invention is provided overcomes the problem of inertial navigation accumulated error is big, solves pulsar navigation ornamental Weak the problem of, the ornamental of navigation system is greatly strengthen, greatly reduce the convergence time of navigation system, and effectively improve Navigation accuracy, can be directly used for the autonomous control of deep space probe.
Brief description of the drawings
Fig. 1 is hybrid measurement scheme schematic diagram of the present invention;
Fig. 2 is implementation result figure of the invention.
Embodiment
Technical scheme is described further below in conjunction with drawings and examples.
As shown in figure 1, be the optical pulsar hybrid measurement scheme schematic diagram of the present invention, wherein, SSB refers to solar system matter (Solar System Barycenter, it is the coordinate origin in figure to the heart, and the r of deep space probe is that the relative point is calculated ), pulsar 1 and pulsar 2 are used for the observations of pulsar for nearly celestial body (such as Mars), and deep space probe is close to big celestial body When, introduce and supplement is used as to the optical observation amount of neighbouring celestial body.
Optical pulsar of the present invention mixes high considerable deep space air navigation aid, and its step is as follows:
Step one:During detector is close to big celestial body, introduces to the optical observation amount of neighbouring celestial body as supplement, set up Mix observational equation;
Observations of pulsar equation is mixed with optical observation equation.Burst length model can typically be expressed as pulse signal Total phase to the function of time.Total phase of burst length model can be expressed as a fractional part plus a complete cycle Number, i.e.,
Φ (t)=Ψ (T)+N (t)
In formula, Φ (t) is total phase, and Ψ (T) is fractional part, and N (t) is integer part.Integer multiples are small plus observation Number fractional phase just directly reflects detector to the distance of reference frame.
Δ ρ represents the distance component along pulsar direction of visual lines spacecraft (deep space probe) and sun barycenter, i tables in formula Show pulsar sequence number, λiBy the distance propagated in the navigation pulse signal a cycle of i-th of pulsar,For observation arteries and veins Rush arrival time and forecast the difference of pulse arrival time, △ ΦiThe observation phase difference of pulse signal, Δ NiFor pulse period complete cycle Difference,For the unit direction vector of pulse direction of visual lines, Δ x is the distance between spacecraft and sun barycenter (equivalent to Fig. 1 In r, it is but consistent with state quantity symbol X for convenience here, so having used Δ x).It is rewritten into matrix form:
The direct observed quantity of optical navigation camera is the picpointed coordinate of Mars central point, is not considering electromagnetism and light distortion In the case of, it is considered to by the use of the goal pels coordinate given by camera as observed quantity, it can be expressed as:
Wherein p, l are coordinate of the photocentre of target celestial body in camera image plane, and unit is millimeter, and RcI is camera coordinates It is the pose transformation matrix of relative inertness coordinate system, RcI can utilize camera coordinates system opposing body's Conversion Matrix of Coordinate Rcb The pose transformation matrix RbI of the body coordinate system relative inertness coordinate system determined with star sensor determines that x, y, z exists for detector Position under Mars J2000 inertial coodinate systems.
The mixing observational equation that can determine system with reference to equation (1) and (2) is:
Z=h (X)+v.
Wherein z is p, l, △ φi, v is measurement noise, and X represents quantity of state.
Step 2:Using many body gravity models of deep space probe, inertial position and speed using detector are built as quantity of state Vertical detector's status equation.
The motion of deep space probe is by center gravitation (Section 1 on the right of following formula equal sign) and each perturbative force synergy Result.Its stress is as follows:
In formula centered on GM celestial body gravitational constant;R is position vector of the aircraft in inertial system, and R represents its mould (scalar);P be perturbative force for the deep space probe close to big celestial body, detector can be set up by gravitation body greatly centered on celestial body The equation of motion.Consider big celestial body gravitation, solar gravitation, terrestrial gravitation, Jupiter gravitation herein, due to apart from big celestial body farther out, Therefore other Perturbation Effects such as big celestial body gravitation aspherical can not be considered, kinetics equation is set up as follows:
In formula, rpFor the position vector of the relatively large celestial body barycenter of detector;μM、μS、μE、μJBe followed successively by big celestial body, the sun, The gravitational constant of ball, Jupiter;rMp,rSp,rEp,rJpIt is followed successively by the position vector of big celestial body, the sun, the earth, Jupiter to detector; rMS,rME,rMJFor position vector between two days bodies, drawn by JPL DE405 ephemeris, subscript M represents big celestial body, subscript S is represented The sun, subscript E represents the earth, and subscript J represents Jupiter.
The Position And Velocity vector of selection detector is used as state variableObtained according to dynamics of orbits model It is to system state equation
W is system model error, a in formulax ay azPerturbed projection under Mars inertial system for solar gravitation, x, y, z It is meant that position of the detector under Mars J2000 inertial coodinate systems.
Step 3:Optimal estimation is carried out to the state of detector using EKF (EKF), accurately visited Survey Position And Velocity under device inertial system;
The new state equation and new observational equation being augmented more than, are extended the design of Kalman's optimal estimation algorithm: For continuous system described above, the state equation discretization that first need to be set up step 2, and surroundLinearisation, ExistNearby expand into second order Taylor series:
The mixing observational equation discretization that step one is set up, andNearby linearly turn to:
In formula, H represents 1 rank of series expansion.
Covariance matrix E [w (k) w (k) of known state plant noiseT]=Q, the covariance matrix E [v of measurement model noise (k)v(k)T]=R, then EKF recurrence equation is:
K (k)=P (k, k-1) HT(k)[H(k)P(k,k-1)HT(k)+R(k)]-1
P (k, k-1)=Φ (k, k-1) P (k-1) ΦT(k,k-1)+Q(k-1)
Initial value isP (0,0)=Var { x (0) }=Px(0), in formula,
Choose an imaginary mars exploration task, when detector is close to Mars, to deep space optical guidance (OpN), three kinds of air navigation aids of optical pulsar hybrid navigation method (OPHN) of single pulsar navigation (PN) and the present invention Tested, as a result as shown in Figure 2.Use as we can clearly see from the figure after the present invention, the convergence time of navigation algorithm is by original Carry out reducing for tens of hours in a few hours, while navigation accuracy is also carried by original more than 10 best kms for simple pulsar navigation Height arrives thousands of rice.
From Observability Analysis, using the observation program of single goal, single goal optical navigation method (OpN) simultaneously can not See, optical guidance precision finally dissipates gradually with the time;The ornamental of pulse star air navigation aid (PN) is with detector position In right amount with the relation of observed pulsar vector and and change, therefore its ornamental is unstable.
In mathematical simulation, restrained during the navigation accuracy of pulse star air navigation aid, when and dissipate.Precision is distributed in several Ten arrive hundreds of kms, and convergence process therein is also in or so tens of hours.And by the angular surveying of optical target and pulsar Time measurement be combined after, the ornamental of hybrid navigation method is greatly improved.Using the navigation system of OPHN methods whole Close to Mars process, single convergence is embodied, navigation accuracy just quickly converges to km magnitude after a few hours.Easily see To OPHN, either convergence or precision are all substantially better than OpN and PN.
In summary, the present invention is when deep space probe is close to big celestial body, angle of the optical guidance sensor to the celestial body Spend observed quantity and introduce navigation system, rebuild the observational equation mixed with pulsar distance observation, substantially increased and lead The ornamental of boat system, so that between the convergence for substantially reducing navigation system is received, and improve the precision of navigation system.
Although present disclosure is discussed in detail by above preferred embodiment, but it should be appreciated that above-mentioned Description is not considered as limitation of the present invention.After those skilled in the art have read the above, for the present invention's A variety of modifications and substitutions all will be apparent.Therefore, protection scope of the present invention should be limited to the appended claims.

Claims (10)

1. a kind of high considerable degree optical pulsar hybrid navigation method for deep space probe, it is characterised in that this method bag Include following steps:
Step 1:During deep space probe is close to big celestial body, introduce to the optical observation amount of neighbouring celestial body as supplement, by arteries and veins Rush star observational equation to mix with optical observation equation, set up mixing observational equation;
Step 2:Using many body gravity models of deep space probe, the inertial position and speed using detector are set up and visited as quantity of state Survey device state equation;
Step 3:According to the observational equation of step 1 and the state equation of step 2, shape of the construction EKF to detector State carries out optimal estimation calculating, obtains Position And Velocity under accurate detector inertial system;Wherein, the side of EKF Cheng Wei:
<mrow> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>,</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>=</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>+</mo> <mi>f</mi> <mo>&amp;lsqb;</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>,</mo> <msub> <mi>t</mi> <mrow> <mi>k</mi> <mo>-</mo> <mn>1</mn> </mrow> </msub> <mo>&amp;rsqb;</mo> <mi>T</mi> <mo>+</mo> <mi>A</mi> <mo>&amp;lsqb;</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>&amp;rsqb;</mo> <mi>f</mi> <mo>&amp;lsqb;</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>,</mo> <msub> <mi>t</mi> <mrow> <mi>k</mi> <mo>-</mo> <mn>1</mn> </mrow> </msub> <mo>&amp;rsqb;</mo> <mfrac> <msup> <mi>T</mi> <mn>2</mn> </msup> <mn>2</mn> </mfrac> </mrow>
<mrow> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>)</mo> </mrow> <mo>=</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>,</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>+</mo> <mi>K</mi> <mrow> <mo>(</mo> <mi>k</mi> <mo>)</mo> </mrow> <mo>{</mo> <mi>Z</mi> <mrow> <mo>(</mo> <mi>k</mi> <mo>)</mo> </mrow> <mo>-</mo> <mi>h</mi> <mo>&amp;lsqb;</mo> <mover> <mi>x</mi> <mo>^</mo> </mover> <mrow> <mo>(</mo> <mi>k</mi> <mo>,</mo> <mi>k</mi> <mo>-</mo> <mn>1</mn> <mo>)</mo> </mrow> <mo>,</mo> <mi>k</mi> <mo>&amp;rsqb;</mo> <mo>}</mo> </mrow>
K (k)=P (k, k-1) HT(k) [H (k) P (k, k-1) HT(k)+R(k)]-1
P (k, k-1)=Φ (k, k-1) P (k-1) ΦT(k, k-1)+Q (k-1)
Wherein, initial value isP (0,0)=Var { x (0) }=Px(0), in formula,Known state model Covariance matrix E [w (k) w (k) T]=Q of noise, covariance matrix E [v (k) v (k) of measurement model noiseT]=R, w represent system Model error, v represents measurement noise, and k represents current step number, and x represents quantity of state, and μ represents gravitational constant, and X represents discrete state Amount, T represents discrete periodic, and I represents unit matrix, and Z represents discrete observation amount, and t represents the time.
2. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 1 It is, described observations of pulsar equation is:
In formula, △ ΦiThe observation phase difference of pulse signal,For the unit direction vector of pulse direction of visual lines, λ is navigation pulse The distance propagated in signal a cycle, Δ NiFor pulse period complete cycle difference, Δ x is between spacecraft and sun barycenter Distance, i represents pulsar sequence number.
3. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 2 It is, described optical observation equation is:
<mrow> <mi>p</mi> <mo>=</mo> <mi>f</mi> <mfrac> <mrow> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>1</mn> <mo>,</mo> <mn>1</mn> <mo>)</mo> </mrow> <mi>x</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>1</mn> <mo>,</mo> <mn>2</mn> <mo>)</mo> </mrow> <mi>y</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>1</mn> <mo>,</mo> <mn>3</mn> <mo>)</mo> </mrow> <mi>z</mi> </mrow> <mrow> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>1</mn> <mo>)</mo> </mrow> <mi>x</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>2</mn> <mo>)</mo> </mrow> <mi>y</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>3</mn> <mo>)</mo> </mrow> <mi>z</mi> </mrow> </mfrac> </mrow>
<mrow> <mi>l</mi> <mo>=</mo> <mi>f</mi> <mfrac> <mrow> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>2</mn> <mo>,</mo> <mn>1</mn> <mo>)</mo> </mrow> <mi>x</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>2</mn> <mo>,</mo> <mn>2</mn> <mo>)</mo> </mrow> <mi>y</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>2</mn> <mo>,</mo> <mn>3</mn> <mo>)</mo> </mrow> <mi>z</mi> </mrow> <mrow> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>1</mn> <mo>)</mo> </mrow> <mi>x</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>2</mn> <mo>)</mo> </mrow> <mi>y</mi> <mo>+</mo> <msub> <mi>R</mi> <mrow> <mi>c</mi> <mi>I</mi> </mrow> </msub> <mrow> <mo>(</mo> <mn>3</mn> <mo>,</mo> <mn>3</mn> <mo>)</mo> </mrow> <mi>z</mi> </mrow> </mfrac> </mrow>
Wherein, p, l are coordinate of the photocentre of target celestial body in camera image plane, and unit is millimeter, RcIFor camera coordinates system phase To the pose transformation matrix of inertial coodinate system, x, y, z is position of the detector under Mars J2000 inertial coodinate systems.
4. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 3 It is, RcIIt is that the body coordinate system determined using camera coordinates system opposing body Conversion Matrix of Coordinate and star sensor is used to relatively Property coordinate system pose transformation matrix determine.
5. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 3 It is, described mixing observational equation:
Z=h (X)+v;Wherein, z represents p, l, △ φi;V is measurement noise.
6. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 1 It is, in step 2, detector's status equation is:
<mrow> <mover> <mi>X</mi> <mo>&amp;CenterDot;</mo> </mover> <mo>=</mo> <mfenced open = "[" close = "]"> <mtable> <mtr> <mtd> <mo>-</mo> <mfrac> <mi>&amp;mu;</mi> <msup> <mi>r</mi> <mn>3</mn> </msup> </mfrac> <mi>x</mi> <mo>+</mo> <msub> <mi>a</mi> <mi>x</mi> </msub> </mtd> </mtr> <mtr> <mtd> <mrow> <mo>-</mo> <mfrac> <mi>&amp;mu;</mi> <msup> <mi>r</mi> <mn>3</mn> </msup> </mfrac> <mi>y</mi> <mo>+</mo> <msub> <mi>a</mi> <mi>y</mi> </msub> </mrow> </mtd> </mtr> <mtr> <mtd> <mrow> <mo>-</mo> <mfrac> <mi>&amp;mu;</mi> <msup> <mi>r</mi> <mn>3</mn> </msup> </mfrac> <mi>z</mi> <mo>+</mo> <msub> <mi>a</mi> <mi>z</mi> </msub> </mrow> </mtd> </mtr> </mtable> </mfenced> <mo>+</mo> <mi>w</mi> <mo>,</mo> </mrow>
Wherein, state variable The position vector of detector is represented,Represent the velocity of detector;W is System model error, axayazFor projection of the solar gravitation perturbation under Mars inertial system, x, y, z is detector in Mars J2000 Position under inertial coodinate system,Wherein, centered on GM celestial body gravitational constant;R is aircraft in inertia Position vector in system;P is perturbative force.
7. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 6 It is, r calculation formula is as follows:
<mrow> <msub> <mover> <mi>r</mi> <mo>&amp;CenterDot;&amp;CenterDot;</mo> </mover> <mi>p</mi> </msub> <mo>=</mo> <mo>-</mo> <msub> <mi>&amp;mu;</mi> <mi>M</mi> </msub> <mfrac> <msub> <mi>r</mi> <mrow> <mi>M</mi> <mi>p</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>M</mi> <mi>p</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>-</mo> <msub> <mi>&amp;mu;</mi> <mi>S</mi> </msub> <mo>&amp;lsqb;</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>S</mi> <mi>p</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>S</mi> <mi>p</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>M</mi> <mi>S</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>M</mi> <mi>S</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>&amp;rsqb;</mo> <mo>-</mo> <msub> <mi>&amp;mu;</mi> <mi>E</mi> </msub> <mo>&amp;lsqb;</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>E</mi> <mi>p</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>E</mi> <mi>p</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>M</mi> <mi>E</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>M</mi> <mi>E</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>&amp;rsqb;</mo> <mo>-</mo> <msub> <mi>&amp;mu;</mi> <mi>J</mi> </msub> <mo>&amp;lsqb;</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>J</mi> <mi>p</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>J</mi> <mi>p</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>r</mi> <mrow> <mi>M</mi> <mi>J</mi> </mrow> </msub> <msubsup> <mi>r</mi> <mrow> <mi>M</mi> <mi>J</mi> </mrow> <mn>3</mn> </msubsup> </mfrac> <mo>&amp;rsqb;</mo> <mo>,</mo> </mrow>
Wherein, rpFor the position vector of the relatively large celestial body barycenter of detector;μM、μS、μE、μJBe followed successively by big celestial body, the sun, the earth, The gravitational constant of Jupiter;rMp,rSp,rEp,rJpIt is followed successively by the position vector of big celestial body, the sun, the earth, Jupiter to detector;rMS, rME,rMJFor position vector between two days bodies, drawn by JPL DE405 ephemeris, subscript M represents big celestial body, subscript S is represented too Sun, subscript E represents the earth, and subscript J represents Jupiter.
8. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 1 It is, in step 3, the method for construction EKF is included:
Step 3.1, state equation discretization first to step 2, and surroundingLinearisation,Nearby expand into second order safe Strangle series;
Step 3.2, by the observational equation discretization of step one, andLinearisation nearby.
9. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 8 It is, the second order Taylor series after step 3.1 processing are:
10. it is used for the high considerable degree optical pulsar hybrid navigation method of deep space probe, its feature as claimed in claim 8 It is, the equation after step 3.2 processing is:
CN201710527892.4A 2017-06-30 2017-06-30 A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe Pending CN107144283A (en)

Priority Applications (1)

Application Number Priority Date Filing Date Title
CN201710527892.4A CN107144283A (en) 2017-06-30 2017-06-30 A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe

Applications Claiming Priority (1)

Application Number Priority Date Filing Date Title
CN201710527892.4A CN107144283A (en) 2017-06-30 2017-06-30 A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe

Publications (1)

Publication Number Publication Date
CN107144283A true CN107144283A (en) 2017-09-08

Family

ID=59784607

Family Applications (1)

Application Number Title Priority Date Filing Date
CN201710527892.4A Pending CN107144283A (en) 2017-06-30 2017-06-30 A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe

Country Status (1)

Country Link
CN (1) CN107144283A (en)

Cited By (7)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN108761386A (en) * 2018-05-24 2018-11-06 西安石油大学 A kind of communication and navigation integration differential pulse localization method based on X-ray
CN110146093A (en) * 2019-06-19 2019-08-20 北京理工大学 Binary asteroid detection independently cooperates with optical navigation method
CN110174850A (en) * 2019-04-30 2019-08-27 上海卫星工程研究所 Angle measurement test the speed Integrated Navigation Semi-physical Simulation verifying system and method
CN111947668A (en) * 2020-08-26 2020-11-17 中南大学 Online estimation-based angle measurement/distance measurement combined navigation method for wooden star detector
CN112082560A (en) * 2020-08-07 2020-12-15 上海航天控制技术研究所 Mars braking strategy online formulation method based on autonomous navigation
CN113091731A (en) * 2021-03-03 2021-07-09 北京控制工程研究所 Spacecraft autonomous navigation method based on star sight relativistic effect
CN114485678A (en) * 2021-12-31 2022-05-13 上海航天控制技术研究所 Heaven and earth integrated lunar surface landing navigation method

Citations (8)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN102879014A (en) * 2012-10-24 2013-01-16 北京控制工程研究所 Optical imaging autonomous navigation semi-physical simulation testing system for deep space exploration proximity process
CN103017772A (en) * 2012-11-30 2013-04-03 北京控制工程研究所 Optical and pulsar fusion type self-navigating method based on observability analysis
CN103234538A (en) * 2013-04-07 2013-08-07 北京理工大学 Autonomous navigation method for planet in final approaching section
CN103954279A (en) * 2014-05-19 2014-07-30 武汉科技大学 Doppler differential velocity model and method for combined navigation by using doppler differential velocity model and X-ray pulsar
CN104567880A (en) * 2014-12-23 2015-04-29 北京理工大学 Mars ultimate approach segment autonomous navigation method based on multi-source information fusion
CN105509750A (en) * 2015-11-27 2016-04-20 上海卫星工程研究所 Astronomical velocity measurement and ground radio combined Mars acquisition phase navigation method
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
CN107421533A (en) * 2017-06-22 2017-12-01 北京航空航天大学 A kind of deep space probe X-ray pulsar TOA/DTOA Combinated navigation methods

Patent Citations (8)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN102879014A (en) * 2012-10-24 2013-01-16 北京控制工程研究所 Optical imaging autonomous navigation semi-physical simulation testing system for deep space exploration proximity process
CN103017772A (en) * 2012-11-30 2013-04-03 北京控制工程研究所 Optical and pulsar fusion type self-navigating method based on observability analysis
CN103234538A (en) * 2013-04-07 2013-08-07 北京理工大学 Autonomous navigation method for planet in final approaching section
CN103954279A (en) * 2014-05-19 2014-07-30 武汉科技大学 Doppler differential velocity model and method for combined navigation by using doppler differential velocity model and X-ray pulsar
CN104567880A (en) * 2014-12-23 2015-04-29 北京理工大学 Mars ultimate approach segment autonomous navigation method based on multi-source information fusion
CN105509750A (en) * 2015-11-27 2016-04-20 上海卫星工程研究所 Astronomical velocity measurement and ground radio combined Mars acquisition phase navigation method
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
CN107421533A (en) * 2017-06-22 2017-12-01 北京航空航天大学 A kind of deep space probe X-ray pulsar TOA/DTOA Combinated navigation methods

Non-Patent Citations (2)

* Cited by examiner, † Cited by third party
Title
王卫华: "非线性滤波技术及其在深空探测自主导航中的应用", 《中国优秀硕士学位论文全文数据库工程科技II辑》 *
王超: "一种基于X射线脉冲星的自主导航算法研究", 《中国优秀硕士学位论文全文数据库工程科技II辑》 *

Cited By (10)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN108761386A (en) * 2018-05-24 2018-11-06 西安石油大学 A kind of communication and navigation integration differential pulse localization method based on X-ray
CN110174850A (en) * 2019-04-30 2019-08-27 上海卫星工程研究所 Angle measurement test the speed Integrated Navigation Semi-physical Simulation verifying system and method
CN110146093A (en) * 2019-06-19 2019-08-20 北京理工大学 Binary asteroid detection independently cooperates with optical navigation method
CN112082560A (en) * 2020-08-07 2020-12-15 上海航天控制技术研究所 Mars braking strategy online formulation method based on autonomous navigation
CN112082560B (en) * 2020-08-07 2022-09-27 上海航天控制技术研究所 Mars braking strategy online formulation method based on autonomous navigation
CN111947668A (en) * 2020-08-26 2020-11-17 中南大学 Online estimation-based angle measurement/distance measurement combined navigation method for wooden star detector
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
CN113091731A (en) * 2021-03-03 2021-07-09 北京控制工程研究所 Spacecraft autonomous navigation method based on star sight relativistic effect
CN114485678A (en) * 2021-12-31 2022-05-13 上海航天控制技术研究所 Heaven and earth integrated lunar surface landing navigation method
CN114485678B (en) * 2021-12-31 2023-09-12 上海航天控制技术研究所 Navigation method for land, ground and lunar landing

Similar Documents

Publication Publication Date Title
CN107144283A (en) A kind of high considerable degree optical pulsar hybrid navigation method for deep space probe
CN102175241B (en) Autonomous astronomical navigation method of Mars probe in cruise section
CN103063217B (en) Deep space detector astronomy/radio combination navigation method based on ephemeris correction
CN103674032B (en) Merge the autonomous navigation of satellite system and method for pulsar radiation vector timing observation
Deng et al. Interplanetary spacecraft navigation using pulsars
CN102879014B (en) Optical imaging autonomous navigation semi-physical simulation testing system for deep space exploration proximity process
CN102538819B (en) Autonomous navigation semi-physical simulation test system based on biconical infrared and star sensors
CN105509750B (en) A kind of astronomy test the speed combined with terrestrial radio Mars capture section air navigation aid
CN104848862B (en) The punctual method and system in a kind of ring fire detector precision synchronous location
CN104165640A (en) Near-space missile-borne strap-down inertial navigation system transfer alignment method based on star sensor
CN105203101A (en) Deep space explorer acquisition phase celestial navigation method based on target object ephemeris correction
CN104457705B (en) Deep space target celestial body based on the autonomous optical observation of space-based just orbit determination method
CN105160125B (en) A kind of simulating analysis of star sensor quaternary number
CN101354251B (en) Method for determining deep space detector equivalent transfer orbit
Burton et al. Online attitude determination of a passively magnetically stabilized spacecraft
CN107655485A (en) A kind of cruise section independent navigation position deviation modification method
CN108548542A (en) A kind of LEO based on atmospheric drag acceleration analysis determines method
CN103591956B (en) A kind of deep space probe autonomous navigation method based on Analysis on Observability
CN110304279A (en) A kind of mass center on-orbit calibration compensation method of electric propulsion satellite
Kai et al. Performance enhancement of X-ray pulsar navigation using autonomous optical sensor
Wang et al. Absolute navigation for Mars final approach using relative measurements of X-ray pulsars and Mars orbiter
CN103047986B (en) A kind of large-scale space-time and in-orbit dynamic effect analogy method
CN103512574A (en) Optical guidance method for deep space probe based on minor planet sequence image
CN107727102A (en) Astronomy test the speed combined with terrestrial radio Mars capture section air navigation aid
CN103017773B (en) A kind of based on catalog of celestial bodies region feature and natural satellite road sign around section air navigation aid

Legal Events

Date Code Title Description
PB01 Publication
PB01 Publication
SE01 Entry into force of request for substantive examination
SE01 Entry into force of request for substantive examination
WD01 Invention patent application deemed withdrawn after publication
WD01 Invention patent application deemed withdrawn after publication

Application publication date: 20170908