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104 results about "X-ray pulsar" patented technology

X-ray pulsars or accretion-powered pulsars are a class of astronomical objects that are X-ray sources displaying strict periodic variations in X-ray intensity. The X-ray periods range from as little as a fraction of a second to as much as several minutes.

Navigation satellite autonomous navigation system and method based on X-ray pulsar

InactiveCN101038169AHigh precision autonomous navigationStable periodicityInstruments for comonautical navigationNavigation by astronomical meansFault toleranceInformation processing
A autonomous navigation system of a navigational satellite based on X radial pulse satellite includes: an X radial detector, an atomic clock group on the satellite, a planet of our solar system parameter database, an X radial pulsar module and a characteristic parameter database, a computer on the satellite, a strap-down inertial navigation system SINS and an autonomous navigation algorithm module library; in the autonomous navigation method, the X radial photons radiated from the pulsar are used as the input of the external information; the pulse arrival time TOA and the angular position information are obtained; data is processed through a autonomous navigation filter; and the navigational parameters such as the position, the speed, the time and the pose of the navigational satellite; the navigational telegraph text and the control command are generated independently, and the independent running of the navigational satellite is realized. The present invention has the advantages of providing a long time and a high degree of accuracy autonomous navigation, and providing the fault-tolerance capacity of the autonomous navigation information processing. The autonomous navigation system is also be adequate for the high degree of accuracy autonomous navigation of the near earth orbit, the deep space, the interplanetary flight space vehicle, the a celestial body lander without thickset atmosphere and the surface peripatetic machine.
Owner:BEIJING INST OF SPACECRAFT SYST ENG

Constellation orientated simulating system and method based on X-ray pulsar

The invention discloses a constellation orientated simulating system and method based on an X-ray pulsar. The constellation orientated simulating method is characterized by comprising the steps of measuring a relative distance between stars by using an equation of light spread by an inter-star link or X-ray pulsar signal between satellites, obtaining an included angle between satellite base lines in a constellation, meanwhile, extracting a pulsar radiation direction vector by a satellite borne X-ray detector and a collimator which are matched, calculating an included angle between the vector and the satellite base lines, further calculating an included angle between the vector and the plane of the constellation, measuring integral rotation and drift of earth orbiting satellites or constellation and correcting. The constellation orientated simulating system based on the X-ray pulsar comprises a signal simulating unit, a time maintaining unit, a modulation unit, a controllable light time delay unit, an optical sending unit, an optical receiving unit, a photon detecting unit and an oriented simulating unit. The constellation orientated simulating system is capable of performing analogue simulation on realization of signal generation, transmission, acquisition, processing and oriented algorithm in the process of orienting the X-ray pulsar.
Owner:XIDIAN UNIV

Mars ultimate approach segment autonomous navigation method based on multi-source information fusion

The invention discloses a mars ultimate approach segment autonomous navigation method based on multi-source information fusion, relates to a mars ultimate approach segment autonomous navigation method and belongs to the technical field of deep space exploration. The method is characterized in that optical measurement, radio measurement based on a mars orbiter and X-ray pulsar measurement information are combined based on a mars ultimate approach segment dynamical model, are effectively fused in the application range based on a federated filtering structure and are standby for one another, and the advantages of various navigation systems are fully exerted; on the basis of establishing a mars ultimate approach segment state model and a mars ultimate approach segment autonomous navigation model, detector real-time navigation status information is resolved by the utilization of an integrated navigation filtering algorithm of a federation structure to realize the mars ultimate approach segment autonomous navigation. According to the mars ultimate approach segment autonomous navigation method, the precision and the real time of the mars ultimate approach segment autonomous navigation can be improved, and the reliability and the fault tolerance of a navigation system can be improved. The method can provide a technical support for the design of a future mars exploration task autonomous navigation solution.
Owner:BEIJING INSTITUTE OF TECHNOLOGYGY

X-ray pulsar navigation positioning method and system based on nonlinear prediction strong tracking traceless Kalman filtering

The invention discloses an X-ray pulsar navigation positioning method and system based on nonlinear prediction strong tracking traceless Kalman filtering. The navigation positioning method comprises the following steps of taking a spacecraft position vector and a velocity vector as a navigation state variable, establishing a navigation system state model and obtaining a spacecraft state predictionvalue; determining a pulsar signal observation value and establishing a navigation system observation model; using a non-linear prediction strong tracking traceless Kalman filtering method to processa pulsar signal observation value and a spacecraft state prediction value, in the spacecraft state prediction stage, acquiring a minimum navigation system state model error according to a constraintfunction, and correcting a navigation system state model error in a quasi real-time mode; and in a spacecraft state updating stage, introducing a fading factor to suppress a noise interference, predicting and updating the state of a spacecraft. A spacecraft state model error is estimated and corrected, and simultaneously, the problems of filter divergence and the low precision of X-ray pulsar navigation caused by the noise interference are solved.
Owner:XIDIAN UNIV

Doppler differential velocity model and method for combined navigation by using doppler differential velocity model and X-ray pulsar

The invention discloses a doppler differential velocity model and a method for combined navigation by using a doppler differential velocity model and an X-ray pulsar. The doppler differential velocity model is Y<s>(t)=h<s>(X, t)+omegav, wherein omegav is doppler measurement noise; Y<s> and h<s> respectively represent a measurement value and a measurement equation; Y<s>=vD2-vD1; the equation is as shown in the specification. The method for combined navigation by using the doppler differential velocity model and the X-ray pulsar comprises the following steps: 1, building an orbital dynamics model of a deep space probe; 2, building an X-ray pulsar navigation ranging model; 3, building the doppler differential velocity model; 4, filtering by using an extended kalman filter. Compared with the prior art, the doppler differential velocity model has the advantages that (1) compared with the existing pulsar/doppler combined navigation methods, the doppler differential velocity model still can normally and stably work under an unstable solar spectrum; (2) compared with the pulsar navigation method and the doppler navigation method, a plurality of navigation messages are fully utilized by the method, the method has complete observability, and the locating information with higher precision can be provided.
Owner:WUHAN UNIV OF SCI & TECH

Large-area X-ray pulse detection device based on microchannel plate split joint

The invention relates to a large-area X-ray pulse detection device based on microchannel plate split joint. The large-area X-ray pulse detection device comprises an X-ray photoelectric cathode, a first insulating layer, a microchannel plate (MCP) input electrode press ring, a second insulating layer, an MCP input electrode, a first MCP layer, an intermediate electrode, a second MCP layer, a third insulating layer, an MCP output electrode, a fourth insulating layer, and an anode which are sequentially stacked up, wherein the first MCP layer and the second MCP layer are both large-area MCP detectors, and each MCP detector comprises a detector body, a split-joint framework and a processing circuit. The large-area X-ray pulse detection device resolves the technical problems that an existing MCP detector is adopted to detect the X-ray pulse, extremely long observation time is needed, and detection efficiency of the whole system is low, a detection method and a device which are high in detection efficiency are provided for an X-ray pulsar navigation system, photon measurement information with high time resolution and high time accuracy is provided for X-ray pulsar navigation, and guarantee is provided for high precision of navigation positioning.
Owner:XI'AN INST OF OPTICS & FINE MECHANICS - CHINESE ACAD OF SCI

Deep space explorer acquisition phase celestial navigation method based on target object ephemeris correction

The invention relates to a deep space explorer acquisition phase celestial navigation method based on target object ephemeris correction. According to the method, firstly, a Martian explorer state model, a startlight angle navigation sub system measuring model and an X-ray pulsar navigation sub system measuring model are built; then, the startlight angle and the X-ray pulsar quantity measurements are respectively obtained; filtering estimation is performed to obtain the position and the speed of a detector in a heliocentric inertia coordinate system and a target object center inertia coordinate system; on the basis, a state model and a measuring model of target object ephemeris error are built; the quantity measurement about the target object ephemeris error is obtained through estimation state vectors of the startlight angle navigation sub system and the X-ray pulsar navigation sub system; a Kalman filtering method is used for estimating the target object ephemeris error; the target object ephemeris error is fed back into a navigation system model; the position of a target object in the navigation model is corrected. The deep space explorer acquisition phase celestial navigation method belongs to the technical field of aerospace navigation, can be used for estimating the object ephemeris error and correcting the model error of the navigation system on line, and is applicable to the explorer acquisition phase.
Owner:BEIHANG UNIV

Mars final approaching section autonomous navigation method based on relative measurement information

The invention discloses a Mars final approaching section autonomous navigation method based on relative measurement information, and belongs to the technical field of deep space exploration. For achieving Mars final approaching section autonomous navigation, a final approaching and surrounding dynamic model is established. According to differential information of X-ray pulsar arrival time and Doppler velocity measurement information of a Mars orbiter, based on nonlinear filtering algorithm, the states of an approaching detector and the Mars orbiter undergo joint estimation, absolute navigation is achieved through utilization of two kinds of relative measurement information including the differential information of X-ray pulsar arrival time and the Doppler velocity measurement information of the Mars orbiter, and the accuracy of Mars final approaching section autonomous navigation and the accuracy of entry point state estimation are improved. The method has the following advantages: introduction of a planet ephemeris error is avoided, the adverse effect on navigation performance due to nondeterminacy of pulsar parameters is limited, the problem of state divergence resulting from long observation time of pulsars is overcome, the navigation performance of two detectors is improved at the same time, and the navigation filter accuracy and the convergence speed are increased.
Owner:BEIJING INSTITUTE OF TECHNOLOGYGY

Interplanetary autonomous navigation ground test verification system based on information fusion

The invention discloses an interplanetary autonomous navigation ground test verification system based on information fusion. The interplanetary autonomous navigation ground test verification system comprises a navigation sensor, a dynamic celestial body simulator, an X-ray pulsar signal simulator, a navigation calculation module, a shading cover, a simulation main control module and a mechanical turntable, wherein the navigation sensor is arranged on the mechanical turntable; the simulation main control module sends an instruction to the navigation calculation module; the navigation calculation module receives the instruction, controls the navigation sensor to image a celestial body image generated by the dynamic celestial body simulator and sends a celestial body imaging result to the navigation calculation module; the navigation calculation module receives the imaging result and then calculates position information of a spacecraft; and furthermore, the navigation calculation module also calculates the position information of the spacecraft according to a received pulse signal of the X-ray pulsar signal simulator and calculates the position information of the spacecraft by an information fusion algorithm. By the interplanetary autonomous navigation ground test verification system, the authenticity and the reliability of ground simulation verification of an autonomous interplanetary navigation technology are improved.
Owner:BEIJING INST OF CONTROL ENG

X-ray pulsar photon signal ground simulation system with high time-frequency stability

The invention discloses an X-ray pulsar photon signal ground simulation system with high time-frequency stability, comprising a program control computer, a high time-frequency stability signal source, an electric control visible light source, an adjustable optical attenuator, an optical shielding cavity, a photomultiplier and an electronic reading circuit. The high time-frequency stability signal source is used for obtaining a pulsar cycle and outline data output by the program control computer, generating a trigger signal to synchronize the electronic reading circuit, generating a high time-frequency stability voltage, inputting the voltage to the electric control visible light source and controlling the electric control visible light source to generate the visible light with light power which is in direct proportion with the input voltage, wherein the visible light is attenuated into photon stream by the adjustable optical attenuator; the photomultiplier detects out that the photo stream generates electric pulse, calibrates the electric pulse by the electronic reading circuit and then outputs to the program control computer. The system has the advantages of high simulation reliability, high outline precision and high time precision and can be used as an experimental device for timing observation, weak signal treatment and navigation design.
Owner:XIDIAN UNIV

Precise and synchronous positioning and time-keeping method and system of Mars orbiting detector

The invention discloses a precise and synchronous positioning and time-keeping method and system of a Mars orbiting detector. The precise and synchronous positioning and time-keeping method comprises the following steps: firstly inputting initial data including a simulated nominal orbit and relative parameters for filtering initialization; simulating observation data, and simulating the observed quantity of a pulsar according to a measurement equation of the pulsar, wherein measurement noises relative to the observed quantity comprise clock errors, and the clock errors are simulated by a clock error model; and performing adaptive Kalman filtering according to a filtering state equation and an observation equation of self-positioning and time keeping of the Mars orbiting detector to obtain orbits and the clock errors of the detector. According to the precise and synchronous positioning and time-keeping method and system disclosed by the invention, on the basis of establishing an observation model of an X-ray pulsar, the observation model, a detector kinetic model and the clock error model of a satellite-borne atomic clock are organically combined, and the position, speed and clock error parameters of the detector are also estimated so as to ensure that the clock error correction can be achieved, influences of the clock errors to the positioning accuracy can also be weakened, and the self-positioning accuracy can also be improved.
Owner:WUHAN UNIV

Chaotic frequency measuring system and method in similar micro-photon source navigation system

InactiveCN101982782AEliminate the influence of calculation step size factorFrequency measurement arrangementSatellite radio beaconingIntegratorState parameter
The invention discloses a chaotic frequency measuring system and a method in a similar micro-photon source navigation system, mainly solving the problems that low SNR micro-photon signal frequency in a similar photon source advanced navigation positioning and time synchronization system is hard to measure or has low measurement precision. The system is mainly composed of a photon detector, a sampling integrator, a chaos detector, a phase path analyzer, an evaluation unit, a parameter setting unit and other modules. The frequency measuring method of the invention comprises the following steps: inputting micro-photon pulse profile information obtained by sampling integration to a chaos detection model; analyzing the plane of the phase path to determine a critical chaos state parameter; obtaining a frequency parameter by a chaotic frequency measuring principle and a realization method; and carrying out evaluation. The invention has the characteristics that the low SNR micro-photon signal frequency can be accurately detected and recognized under the environment of strong noise. The invention can be used for measuring, calibrating and recognizing the signal resource frequency of advanced navigation systems, such as X-ray pulsar, quantum and the like, and can expand to application fields, such as radar multi-base signal reception, other SNR signal detection and the like.
Owner:XIDIAN UNIV

X-ray pulsar navigation TOA estimation method based on Bayes estimation

The invention belongs to the technical field of X-ray pulsar autonomous navigation and discloses an X-ray pulsar navigation TOA estimation method based on Bayes estimation. Under the condition that the overall trend of a photon counting rate accords with the Poisson distribution, an X-ray photon arrival time sequence can be modeled into a non-homogeneous Poisson process; the flow characteristics of PSR B0531 + 21 pulsars accord with the Poisson distribution, and a Poisson distribution signal model is established and divided into a time-frequency model and a frequency-stabilizing model; the frequency-stabilizing model of the photon sequence is selected to perform Fourier transform and then the frequency-stabilizing model is converted into a frequency domain to obtain a photon flow probability function expression with time delay estimation parameters; the photon flow probability function expression is converted into a likelihood function capable of calculating a time delay parameter by using a Bayes theorem for solving; and a Tool multi-mode nested sampling algorithm is calculated by Bayes estimation, iteration is carried out, and the parameter estimation value of the likelihood function is further calculated. The invention effectively improves the TOA estimation precision within the observation time and meets the future engineering development requirement of pulsar navigation.
Owner:XIDIAN UNIV

Frequency domain weighting phase comparison method for X-ray pulsar photon sequences

The invention discloses a frequency domain weighting phase comparison method for X-ray pulsar photon sequences and solves the problems that in the prior art, detailed information of a useful signal is lost, calculation complexity is high, and the signal to noise ratio is low. The method comprises the following steps: 1, conducting evenly-spaced sampling on two photon arrival time sequences received by two spacecrafts, and obtaining corresponding photon intensity sequences; 2, converting the two photon intensity sequences in a time domain into a frequency domain through an FFT; 3, extracting phase information of the two photon intensity sequences, conducting subtraction arithmetic, and obtaining phase differences between the two photon intensity sequences; 4, accumulating the phase differences which are sectionalized, and extracting ratios of the phase differences to corresponding frequency points; 5, conducting energy weighting and proportional multiplication on the ratios of the phase differences to frequency in the frequency domain, and obtaining a normalized delay phase within the time domain. By means of the frequency domain weighting phase comparison method, phase estimation accuracy can be effectively improved, calculation complexity can be lowered, and the method can be applied to estimation of the relative movement state of an X-ray pulsar relative to a navigational positioning system.
Owner:XIDIAN UNIV

Precision temperature control device for X-ray pulsar navigation sensor

The invention discloses a precision temperature control device for an X-ray pulsar navigation sensor; the precision temperature control device comprises a heat isolation pad, an outboard temperature control loop, a front wheel disc, a first heat isolation assembly, a second heat isolation assembly, a temperature sensor, a detector, a heat isolation gasket, a detector mount, a cabin temperature control loop, a heat conductive copper block and a heat conductive copper belt; the heat isolation pad, the outboard temperature control loop and the front wheel disc are connected in sequence; the first heat isolation assembly is arranged on an optics lens; the temperature sensor is wrapped on an optical bench by the second heat isolation assembly; a preamplifier assembly is provided with the detector mount and the heat isolation gasket; the detector, the cabin temperature control loop, the heat conductive copper block and the heat conductive copper belt are connected in order; the precision temperature control device can fully consider light, machine, electric, heat and space track environment conditions, and can respectively use different temperature control means for different assemblies, thus adapting to different heat environments, effectively ensuring normal works of each assembly, realizing integral temperature control optimization of the device, and solving the problems that a conventional satellite platform temperature homogeneity is poor.
Owner:BEIJING INST OF CONTROL ENG
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