WO2019062030A1 - Star network-based bds/gps broadcast network rtk algorithm - Google Patents

Star network-based bds/gps broadcast network rtk algorithm Download PDF

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WO2019062030A1
WO2019062030A1 PCT/CN2018/078492 CN2018078492W WO2019062030A1 WO 2019062030 A1 WO2019062030 A1 WO 2019062030A1 CN 2018078492 W CN2018078492 W CN 2018078492W WO 2019062030 A1 WO2019062030 A1 WO 2019062030A1
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difference
satellite
double
indicates
station
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PCT/CN2018/078492
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Chinese (zh)
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潘树国
王彦恒
张瑞成
尚睿
汪登辉
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东南大学
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    • GPHYSICS
    • G01MEASURING; TESTING
    • G01SRADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
    • G01S19/00Satellite radio beacon positioning systems; Determining position, velocity or attitude using signals transmitted by such systems
    • G01S19/38Determining a navigation solution using signals transmitted by a satellite radio beacon positioning system
    • G01S19/39Determining a navigation solution using signals transmitted by a satellite radio beacon positioning system the satellite radio beacon positioning system transmitting time-stamped messages, e.g. GPS [Global Positioning System], GLONASS [Global Orbiting Navigation Satellite System] or GALILEO
    • G01S19/42Determining position
    • G01S19/43Determining position using carrier phase measurements, e.g. kinematic positioning; using long or short baseline interferometry

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  • the invention relates to a star network based BDS/GPS broadcast network RTK algorithm, in particular to a star network based BDS compatible GPS broadcast mode and compatible with two-way communication network RTK (Real Time Kinematic, real-time dynamic positioning technology Implementation technology, belongs to the field of GNSS real-time high-precision fast positioning.
  • RTK Real Time Kinematic, real-time dynamic positioning technology Implementation technology
  • Network RTK technology has become one of the most widely used GNSS precision positioning technologies, and can provide users with multi-scale positioning services such as meter, decimeter and centimeter in real time [1-3] .
  • the mainstream network RTK technology can be divided into VRS (Virtual Reference Station) technology, MAC (Master Auxiliary Concept) technology and FKP (Flachen Korrektur Parameter). Technology [4] .
  • the user first uploads its own probability coordinates, and the CORS (Continuously Operating Reference System) central solution software (hereinafter referred to as the central software) generates a virtual reference station in the vicinity of the user according to the user probability position, the user and the user
  • the virtual reference station forms an ultra-short baseline for solution.
  • the disadvantages of this technology are: 1 requires two-way communication, increases data delay 2 When the user position changes greatly (more than 5km), the virtual reference station will change, the user needs to re-initialize; 3 the center software needs to be based on the user's approximate location Generate virtual reference station information for each user, limiting user capacity; 4 because the virtual information is used, the differential correction information cannot be tracked; 5 although the VRS technology itself does not limit the number of reference stations in the network element, the current The software is basically based on triangulation, lacking redundant information; 6 atmospheric error processing is only determined by the central software, so that users can not use better algorithms [4] ; 7 need to upload user's general location information, exposing the user's location, especially In some special areas, this method is not even desirable, such as the military field.
  • MAC technology supports single two-way communication.
  • two-way communication the user uploads his own approximate location information.
  • the central software selects the reference station closest to the user as the primary reference station according to the user's location, and broadcasts the differential correction information to the user; in one-way communication, The user needs to know the predefined network element in which he is located, and then obtain the corresponding differential correction information.
  • this technology still has the same shortcomings as the VRS technology.
  • the one-way communication although the shortcomings of the VRS technology are overcome, the user himself needs to know the network element in which he is located, which is for the user. It is difficult to implement, especially when users enter unfamiliar areas.
  • software using MAC technology uses non-difference algorithms for network solution, with many parameters and complex models, which makes the solution efficiency of network elements. Low, network initialization time (from boot to network RTK service available) long.
  • the central software uses non-difference algorithm to realize network solution, extracts non-difference error, and performs regional modeling on spatial correlation error, parameterizes non-difference space correlation error of mobile station, broadcasts by broadcast mode, and rover Real-time positioning based on these parameters and their location.
  • the disadvantages of this technology are as follows: 1 The central software uses the non-difference algorithm for network solution, with many parameters and complex models, which makes the settlement efficiency low and the network initialization time long; 2 The establishment of the spatial correlation error model is completed by the central software, which limits the user's use. A more optimized algorithm.
  • the present invention provides a BDS/GPS broadcast network RTK algorithm based on a star network, and is compatible with two-way communication, and supports differential correction data by ground equipment, aviation aircraft or satellite broadcasting.
  • the server uses the UDP protocol to broadcast the differential correction data of all the star network elements in the whole network in real time, and the users in the broadcast mode receive the data, and then perform network element selection, atmospheric interpolation and baseline solution.
  • the user who uses the two-way communication uploads its own approximate location through the Ntrip protocol or the TCP/IP protocol, and the server broadcasts the user's network element differential correction data to the user, and the user obtains the data and performs atmospheric interpolation and baseline solution.
  • the server broadcasts the differential correction number to the two-way communication user, the data broadcasted according to the broadcast mode is still uninterrupted.
  • the invention provides a star network-based BDS/GPS broadcast network RTK algorithm, which comprises the following specific steps:
  • Step 1 Obtain the base station coordinates from the database, use the Delaunay triangulation algorithm to generate the Delaunay triangulation, and generate a star-shaped network composed of several star network elements and control the whole region on the basis of the triangulation network, wherein each A star network element consists of a primary station and a number of secondary stations corresponding thereto;
  • Step 2 Obtain the base station data in real time, form a double-difference observation with the baseline in the Delaunay triangulation, construct a first Kalman filter, estimate the baseline double-difference ambiguity and the zenith tropospheric wet delay ZTD in real time, and then generate each Baseline double difference atmospheric error of the baseline;
  • Step 3 Assign the baseline double-difference atmospheric error generated in step 2 to the corresponding star network element baseline, and use the star-shaped network element as a unit to unify the reference star, and generate a single-element atmosphere between each baseline satellite station of the star-shaped network element. error;
  • Step 4 Using a star-shaped network element as a unit, encoding a single-difference atmospheric error, all base station coordinates, and a master station observation value of each baseline satellite station of the star network element, and the encoded data is performed by using a UDP protocol. Broadcast or use two-way communication for broadcast, in which UDP protocol broadcasts all data and then proceeds to step 5; when using two-way communication, firstly, the user uploads the approximate location information, and then the central software broadcasts only to the user according to the user's location through Ntrip protocol or TCP/IP. The data of the star network element where the user is located, proceeds to step 6;
  • Step 5 the user receives the data in real time and judges the network element where it is located, according to the differential data of the network element in which the network element is interpolated to obtain the single-difference atmospheric error between the station and the primary station, and corrects the observation value to the primary station, and proceeds to step 7;
  • Step 6 the user receives the data in real time, according to the differential data of the network element, the inter-station single difference atmospheric error between the station and the main station is interpolated, and corrected to the observation value of the main station, and proceeds to step 7;
  • step 7 the user constructs a double-difference observation value by using the corrected observation value of the primary station and the user observation value corrected by step 5 or 6, and constructs a second Kalman filter including the user position parameter and the ambiguity parameter to perform baseline solution.
  • the step 1 includes the following steps:
  • Step 11 generating a triangulation network by using a Delaunay triangulation algorithm
  • Step 12 extracting a triangulation network boundary reference station and a non-boundary reference station, wherein if the sum of the angles of the inner angles of the vertices of the base station in all the triangles connected to a reference station is greater than a set threshold, the base station a non-boundary base station, otherwise a boundary reference station;
  • Step 13 initializing the star network element set: all the non-boundary base stations are used as the primary station, and all the base stations connected thereto are used as the corresponding auxiliary stations;
  • Step 14 Find a set of base stations that do not participate in the star network networking in the boundary reference station;
  • Step 15 selecting the base station with the largest number of base stations connected to it as the new primary station in the base station set not participating in the networking, and the base station connected thereto as the corresponding secondary station, updating the star network set and not a set of base stations participating in a star network network;
  • Step 16 Repeat step 15 until the number of base stations that are not participating in the star network networking is zero.
  • the step 2 includes the following steps:
  • Step 21 The base station k receives the pseudorange and carrier observation signals of the satellite s, and the carrier and pseudorange observation equations are expressed as:
  • Step 22 according to the carrier observation value obtained by step 21 and the pseudorange observation value constitute a double difference observation value, the double difference carrier observation equation and the double difference pseudo range observation equation of the reference station k and the reference station y are respectively:
  • a double-difference carrier observation indicating the j-th frequency point Indicates the star distance of the double-difference station, Indicates the double-difference full-circumference ambiguity at the jth frequency point, Indicates double-difference tropospheric delay, Indicates the doubled ionospheric delay at the first frequency point, Means the double-difference carrier multipath effect in meters on the jth frequency point, Indicates the double-difference carrier observation noise in meters on the jth frequency point, Indicates the double-difference pseudorange observation at the jth frequency point, Representing the double-difference pseudorange multipath effect at the jth frequency point, Representing the double difference pseudorange observation noise at the jth frequency point;
  • Step 23 Combine the double-difference observations formed in step 22 into a double-difference wide lane combined observation value, and calculate the wide lane combined ambiguity:
  • Step 24 using a combination of no ionosphere, constructing a narrow lane filter, and separating the base ambiguity by using a combination of no ionosphere and wide lane versus Includes the following steps:
  • step 241 a combined observation of the double-difference ionosphere is formed:
  • Step 242 constructing a first Kalman filter:
  • E(g) represents the mathematical expectation and Cov(g) represents the covariance.
  • the base station k and the reference station y have n GPS satellites and g BDS satellites, wherein the nth GPS satellite and the g-th BDS satellite are reference stars of each system.
  • the estimation parameters include double-difference ambiguity and baseline relative zenith tropospheric wet delay.
  • the filter model to be estimated parameter vector, observation vector and design matrix are expressed as:
  • Step 243 Perform filtering according to the first Kalman filter established in step 242, and solve a basic carrier ambiguity vector parameter.
  • Step 25 according to the result of step 24, generating a baseline double difference atmospheric error:
  • the step 3 includes the following steps:
  • Step 31 The primary station and the secondary station of the star network element form a baseline, and the baseline consisting of the same base station is searched in the baseline list of the entire network of the triangular network. If the two baseline directions are opposite, the baseline commutation is required, thereby obtaining Baseline double-difference atmospheric error for each type of star network element;
  • Step 32 Check whether the baseline reference stars of the star network elements are consistent. If they are inconsistent, the reference star is unified and the reference star transformation is performed on the atmospheric error;
  • Step 33 Generate a single-difference atmospheric error between the star-type network elements: the single-difference atmospheric error between the reference satellite stations is 0, and the single-difference atmospheric error value of the other satellites is equal to the double-difference atmospheric error;
  • Step 34 Extract satellites of each star-shaped network element that can be shared by the baseline, and generate a single-difference atmospheric error between the satellite stations of the star-shaped network element.
  • the method for determining the network element where the step 5 is located is: the user decodes the received data and calculates the linear distance of the user to each primary station, represented by the primary station with the smallest distance.
  • the NE is the NE of the user.
  • the step 5 or 6 interpolates the difference between the station and the primary station according to the differential data of the network element in which the network element is located, and corrects the observation to the primary station observation value, including the following steps:
  • Step 1 Using the linear interpolation algorithm to interpolate the user's atmospheric error, the single-difference atmospheric error between the user and the primary station is calculated as follows:
  • m denotes the primary station
  • u denotes the user
  • ⁇ 1 , ⁇ 2 , ⁇ 3 denote the tropospheric interpolation coefficient
  • ⁇ 1 , ⁇ 2 denote the ionospheric interpolation coefficient
  • w denote the number of secondary stations
  • tropospheric interpolation coefficients The tropospheric interpolation coefficients and ionospheric interpolation coefficients are calculated as follows:
  • step 2 the atmospheric error value obtained by the interpolation is corrected to the observation value of the primary station, and the pseudorange and the carrier observation value are respectively as follows:
  • the double difference observation in the step 7 is expressed as:
  • Representing GPS satellite double-difference pseudorange observations Indicates the satellite distance of the GPS satellite double-difference station, Representing GPS satellite double-difference pseudorange multipath effect, Representing GPS satellite double-difference pseudorange observation noise, Indicates the GPS satellite double-difference carrier observation, and ⁇ G represents the wavelength of the GPS observation corresponding to the frequency point.
  • Represents the GPS satellite double-difference ambiguity Represents the GPS satellite double-difference carrier multipath effect in weeks, Representing GPS satellite double-difference carrier observation noise in weeks, Indicates the double-difference pseudorange observation of the BDS satellite, Indicates the star distance of the BDS satellite double-difference station, Representing the double-signal pseudorange multipath effect of BDS satellites, Representing BDS satellite double-difference pseudorange observation noise, Indicates the BDS satellite double-difference carrier observation, and ⁇ C represents the wavelength of the BDS observation corresponding to the frequency point. Indicates the double-difference ambiguity of the BDS satellite, Representing the double-signal carrier multipath effect of the BDS satellite in weeks, Indicates the BDS satellite double-difference carrier observation noise in weeks.
  • the second Kalman filter in step 7 is constructed as follows:
  • the user and the star network have n GPS satellites and g BDS satellites, of which the nth GPS satellite and the gth BDS satellite are reference stars of each system, and all satellites are combined.
  • L1 carrier and P1 pseudorange observation data, filter model to be estimated parameter matrix Observation matrix Design matrix Expressed as:
  • Three-dimensional coordinate parameter vector and floating-point ambiguity parameter vector The coordinate parameter vector after fixing the ambiguity, To fix the ambiguity parameter vector, Corresponding to each parameter filtering solution covariance matrix.
  • the present invention has the following technical effects:
  • the present invention uses a star network for atmospheric interpolation to provide redundant observations
  • the present invention truly realizes the broadcast mode network RTK, and takes into consideration two-way communication, and the user capacity is not limited;
  • the differential data can be broadcasted by ground equipment or by air plane or satellite, and can be used for wide-area differential and satellite-based enhanced data broadcast.
  • FIG. 1 is a flow chart of a BDS/GPS broadcast network RTK algorithm based on a star network according to the present invention.
  • FIG. 2 is a flow chart of a star network element generation algorithm.
  • the invention designs a BDS/GPS broadcast network RTK algorithm based on a star network, as shown in FIG. 1 , comprising the following steps:
  • Step 1 Obtain the base station coordinates from the database, use the Delaunay triangulation algorithm to generate the Delaunay triangulation, and generate a star-shaped network composed of several star network elements and control the whole region on the basis of the triangulation network, wherein each A star network element consists of a primary station and a number of secondary stations corresponding to it.
  • the step 1 includes the following steps:
  • Step 11 using a Delaunay triangulation algorithm to generate a triangulation, wherein the maximum angle threshold of the triangle is 165° (the threshold is set according to personal experience);
  • Step 12 extracting a triangulation network boundary reference station and a non-boundary reference station, wherein if the sum of the angles of the inner angles of the vertices of the base station in all the triangles connected to a reference station is greater than a set threshold of 195°, then The base station is a non-boundary base station, otherwise it is a boundary base station;
  • Step 13 initializing the star network element set: all the non-boundary base stations are used as the primary station, and all the base stations connected thereto are used as the corresponding auxiliary stations;
  • Step 14 Find a set of base stations that are not participating in the star network networking in the border reference station (neither the primary station nor the primary station);
  • Step 15 selecting the base station with the largest number of base stations connected to it as the new primary station in the base station set not participating in the networking, and the base station connected thereto as the corresponding secondary station, updating the star network set and not a set of base stations participating in a star network network;
  • Step 16 Repeat step 15 until the number of base stations that are not participating in the star network networking is zero.
  • Step 2 Obtain the base station data in real time, form a double-difference observation with the baseline in the Delaunay triangulation, construct a first Kalman filter, estimate the baseline double-difference ambiguity and the zenith tropospheric wet delay ZTD in real time, and then generate each Baseline double difference atmospheric error for the baseline.
  • Step 2 includes the following steps:
  • Step 21 The base station k receives the pseudorange and carrier observation signals of the satellite s, and the carrier and pseudorange observation equations are expressed as:
  • Step 22 according to the carrier observation value obtained by step 21 and the pseudorange observation value to form a double difference observation value, the double difference carrier observation equation and the double difference pseudo range observation equation of the reference station k and the reference station y are respectively:
  • a double-difference carrier observation indicating the j-th frequency point Indicates the star distance of the double-difference station, Indicates the double-difference full-circumference ambiguity at the jth frequency point, Indicates double-difference tropospheric delay, Indicates the doubled ionospheric delay at the first frequency point, Means the double-difference carrier multipath effect in meters on the jth frequency point, Indicates the double-difference carrier observation noise in meters on the jth frequency point, Indicates the double-difference pseudorange observation at the jth frequency point, Representing the double-difference pseudorange multipath effect at the jth frequency point, Indicates the double-difference pseudorange observation noise at the jth frequency point.
  • step 23 the double-difference observations formed in step 22 are combined into a double-difference wide lane combined observation value to solve the wide lane combined ambiguity.
  • the MW combination is used to solve the wide lane ambiguity, it is only affected by the carrier and pseudorange observation noise (ignoring multipath), and the observation noise obeys the Gaussian white noise distribution. Therefore, the multi-epoch smoothing rounding can be adopted for the wide lane combination ambiguity.
  • the specific formula is as follows:
  • Step 24 using a combination of no ionosphere, constructing a narrow lane filter, and separating the base ambiguity by using a combination of no ionosphere and wide lane versus Includes the following steps:
  • step 241 a combined observation of the double-difference ionosphere is formed:
  • Step 242 constructing a first Kalman filter:
  • E(g) represents the mathematical expectation and Cov(g) represents the covariance.
  • the base station k and the reference station y have n GPS satellites and g BDS satellites, wherein the nth GPS satellite and the g-th BDS satellite are reference stars of each system.
  • the estimation parameters include double-difference ambiguity and baseline relative zenith tropospheric wet delay.
  • the filter model to be estimated parameter vector, observation vector and design matrix are expressed as:
  • Step 243 Filter according to the first Kalman filter established in step 242, and solve the basic carrier ambiguity vector parameter.
  • the ambiguity obtained here is the full-circumference ambiguity at the first frequency point).
  • satellites with different elevation angles adopt a weighting method based on satellite elevation angle.
  • the zenith tropospheric wet delay adopts random walk.
  • the receiver observation noise obeys Gaussian white noise distribution, and the ambiguity is determined as time-invariant parameter.
  • Step 25 according to the result of step 24, generating a baseline double difference atmospheric error:
  • step 3 the generated baseline atmospheric error is assigned to the corresponding star network baseline, and the baseline direction transformation is performed if necessary.
  • the star-shaped network is used as a unit to unify the reference star and carry out the reference star transformation to generate a single-difference atmospheric error between the star-shaped network elements and the satellite stations.
  • step 3 generating a single-difference atmospheric error between the star network stations includes the following steps:
  • a star network primary station and a secondary station form a baseline, and a baseline consisting of the same base station is searched in the entire network baseline list. If the two baseline directions are opposite, a baseline commutation is required. This results in a baseline atmospheric error for the star network.
  • Step 42 Check whether the baseline reference stars of the star network elements are consistent. If they are inconsistent, select a unified reference star and perform a reference star transformation on the atmospheric error.
  • step 43 a single difference atmospheric error between the star network elements is generated. If the single-difference atmospheric error between the reference satellite stations is 0, the inter-station single-difference atmospheric error value of other satellites is equal to the double-difference atmospheric error.
  • Step 44 Extract all the satellites of the star network element that are common to each baseline, and generate a single-difference atmospheric error between the satellite stations of the star-shaped network element.
  • Step 4 Using the star network element as a unit, encoding the single-difference atmospheric error, all base station coordinates, and the observation value of the primary station for each baseline satellite station of the star network element, and broadcasting by using the UDP protocol (broadcasting
  • the mode can be broadcasted by equipment such as ground equipment, aviation aircraft or satellite) or two-way communication (the user can upload the approximate location information, and only broadcast the data of the user's star network element to the user through Ntrip protocol or TCP/IP according to the user's location) .
  • GNSS Beidou/Global Satellite Navigation System
  • II Beidou/Global Satellite Navigation System
  • BDS MSM4 observations 1050 BDS ionospheric correction value single difference between stations 1051 BDS geometric correction value single difference between stations Tropospheric delay in the present invention 1074 GPS MSM4 observations 1015 GPS ionospheric correction value single difference between stations 1016 GPS geometric correction value single difference between stations Tropospheric delay in the present invention 1006 Master station ECEF coordinate information 1033 Master station receiver and antenna information 1014 Secondary station coordinate information Coordinate difference between the auxiliary station and the main station 1013 Status and frequency information of message broadcast
  • Step 5 The user receives the data in real time and judges the network element where it is located, and interpolates the difference between the station and the primary station according to the difference data of the network element in which the network element is located, and corrects the error to the observation value of the primary station, and proceeds to step 7. Wherein, when the user decodes the received data and calculates the linear distance of the rover to each primary station, the network element represented by the primary station with the smallest distance is used as the network element where the mobile station is located.
  • step 6 the user receives the data in real time, and interpolates the difference between the station and the main station according to the differential data of the network element in which the network element is located, and corrects the error to the observation value of the primary station, and proceeds to step 7.
  • step 5 or 6 according to the differential data of the network element in which the network element is interpolated, the single-difference atmospheric error between the station and the primary station is obtained, and corrected to the observation value of the primary station, including the following steps:
  • Step 1 Using the linear interpolation algorithm to interpolate the user's atmospheric error, the single-difference atmospheric error between the user and the primary station is calculated as follows:
  • m denotes the primary station
  • u denotes the user
  • ⁇ 1 , ⁇ 2 , ⁇ 3 denote the tropospheric interpolation coefficient
  • ⁇ 1 , ⁇ 2 denote the ionospheric interpolation coefficient
  • w denote the number of secondary stations
  • tropospheric interpolation coefficients The tropospheric interpolation coefficients and ionospheric interpolation coefficients are calculated as follows:
  • step 2 the atmospheric error value obtained by the interpolation is corrected to the observation value of the primary station, and the pseudorange and the carrier observation value are respectively as follows:
  • step 7 the user constructs a double-cavity observation using the observation of the primary station corrected by step 5 and the user observation (received by the user receiver itself) to construct a second Kalman filter including the user position parameter and the ambiguity parameter. , perform a baseline solution.
  • the baseline solution in step 7 includes the following steps:
  • step 71 a double difference observation equation is formed, and the pseudorange and carrier double difference observation equation can be expressed as:
  • Representing GPS satellite double-difference pseudorange observations Indicates the satellite distance of the GPS satellite double-difference station, Representing GPS satellite double-difference pseudorange multipath effect, Representing GPS satellite double-difference pseudorange observation noise, Indicates the GPS satellite double-difference carrier observation, and ⁇ G represents the wavelength of the GPS observation corresponding to the frequency point.
  • Represents the GPS satellite double-difference ambiguity Represents the GPS satellite double-difference carrier multipath effect in weeks, Representing GPS satellite double-difference carrier observation noise in weeks, Indicates the double-difference pseudorange observation of the BDS satellite, Indicates the star distance of the BDS satellite double-difference station, Representing the double-signal pseudorange multipath effect of BDS satellites, Representing BDS satellite double-difference pseudorange observation noise, Indicates the BDS satellite double-difference carrier observation, and ⁇ C represents the wavelength of the BDS observation corresponding to the frequency point.
  • Step 72 constructing a Kalman filter, comprising the following steps:
  • the user and the star network have n GPS satellites and g BDS satellites, of which the nth GPS satellite and the gth BDS satellite are reference stars of each system, and all satellites are combined.
  • L1 carrier and P1 pseudorange observation data, filter model to be estimated parameter matrix Observation matrix Design matrix Expressed as:
  • the satellites with different elevation angles adopt the weighting method based on the satellite elevation angle.
  • the three-dimensional coordinate parameters adopt random walk.
  • the receiver observation noise obeys the Gaussian white noise distribution, and the ambiguity is determined as the time-invariant parameter.
  • Step 72 after fixing the ambiguity, using the following formula to solve the fixed solution of the user's three-dimensional coordinates:
  • the filtering solution of the medium-long baseline can be realized by designing the wide lane and narrow lane filtering model, taking into account the tropospheric delay and the ionosphere.
  • Network RTK technology is one of the most widely used technologies in the field of high precision real-time positioning. Based on the star network, the method uses the double difference mode for network solution, and the model is simple and the parameters are few.
  • the broadcast mode RTK differential correction number is used in the broadcast mode, and the two-way communication is taken into consideration, and the network RTK of the broadcast mode is truly realized.
  • the role of the rover is fully utilized, so that the rover can use a more optimized algorithm.
  • baseline solution taking into account the network RTK and the traditional RTK mode, it can ensure that the central solution solver does not complete the network initialization, the rover uses the original observation of the primary station for single baseline solution.
  • the invention satisfies both the ordinary network RTK users and the special domain users, such as the military field in which the user coordinates cannot be exposed, and the user capacity is not limited.
  • broadcast mode differential data can be broadcast either by ground equipment or by air or satellite. There are no shortcomings of VRS technology, FKP technology, and MAC technology.

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Abstract

Disclosed is a star network-based BDS/GPS broadcast network RTK algorithm. All base stations form a triangulation network by using Delaunay triangulation algorithm; and a controllable full-region star network formed by a plurality of star network elements is generated on the basis of the triangulation network. Data of the base stations is obtained in real time and network element calculation is performed to generate a baseline atmospheric error. In addition, on the basis of on a UDP protocol, a server broadcasts a master station observation value, base station coordinates, and the baseline atmospheric error to a user by using the star network as a unit; the user selects, according to an approximate location thereof and the location of the master station, a network element where the user is located; and interpolation is performed on an inter-station single-difference atmospheric error of the baseline formed by the user and the master station, and the obtained atmospheric error is corrected to the master station observation value to perform baseline calculation. The user can also upload approximate coordinates by means of two-way communication and the server broadcasts differential data of the network element where the user is located. In addition, differential data broadcasting by equipment such as ground equipment, an airplane, or a satellite is also supported.

Description

基于星型网络的BDS/GPS广播式网络RTK算法BDS/GPS broadcast network RTK algorithm based on star network 技术领域Technical field
本发明涉及一种基于星型网络的BDS/GPS广播式网络RTK算法,特别涉及一种基于星型网络的BDS兼容GPS的广播模式并兼容双向通讯的网络RTK(Real Time Kinematic,实时动态定位技术)实现技术,属于GNSS实时高精度快速定位领域。The invention relates to a star network based BDS/GPS broadcast network RTK algorithm, in particular to a star network based BDS compatible GPS broadcast mode and compatible with two-way communication network RTK (Real Time Kinematic, real-time dynamic positioning technology Implementation technology, belongs to the field of GNSS real-time high-precision fast positioning.
背景技术Background technique
网络RTK技术已成为目前使用最为广泛的GNSS精密定位技术之一,可以实时为用户提供米级、分米级、厘米级等多尺度定位服务 [1-3]。根据差分数据播发方法,目前,主流的网络RTK技术可分为VRS(Virtual Reference Station,虚拟参考站)技术,MAC(Master Auxiliary Concept,主辅站)技术与FKP(Flachen Korrektur Parameter,区域改正参数)技术 [4]Network RTK technology has become one of the most widely used GNSS precision positioning technologies, and can provide users with multi-scale positioning services such as meter, decimeter and centimeter in real time [1-3] . According to the differential data distribution method, the mainstream network RTK technology can be divided into VRS (Virtual Reference Station) technology, MAC (Master Auxiliary Concept) technology and FKP (Flachen Korrektur Parameter). Technology [4] .
VRS技术中,用户首先上传自身概率坐标,CORS(Continuously Operating Reference System,连续运行参考站系统)中心解算软件(以下简称中心软件)根据用户概率位置在用户附近生成一个虚拟的参考站,用户与虚拟参考站形成超短基线进行解算。这种技术的缺点在于:①需要双向通讯,增加了数据时延②当用户位置变化较大时(超过5km),虚拟参考站会发生变化,用户需要重新初始化;③中心软件需要根据用户概略位置为每个用户生成虚拟参考站信息,限制了用户容量;④由于使用了虚拟的信息,差分改正信息无法追踪;⑤虽然VRS技术本身并未对网元中参考站的数量进行限制,但是目前的软件基本上基于三角网实现,缺少冗余信息;⑥大气误差处理方式仅由中心软件决定,使得用户无法使用更优的算法 [4];⑦需要上传用户概略位置信息,暴露了用户位置,尤其在一些特殊领域,此法甚至不可取,如军事领域。 In the VRS technology, the user first uploads its own probability coordinates, and the CORS (Continuously Operating Reference System) central solution software (hereinafter referred to as the central software) generates a virtual reference station in the vicinity of the user according to the user probability position, the user and the user The virtual reference station forms an ultra-short baseline for solution. The disadvantages of this technology are: 1 requires two-way communication, increases data delay 2 When the user position changes greatly (more than 5km), the virtual reference station will change, the user needs to re-initialize; 3 the center software needs to be based on the user's approximate location Generate virtual reference station information for each user, limiting user capacity; 4 because the virtual information is used, the differential correction information cannot be tracked; 5 although the VRS technology itself does not limit the number of reference stations in the network element, the current The software is basically based on triangulation, lacking redundant information; 6 atmospheric error processing is only determined by the central software, so that users can not use better algorithms [4] ; 7 need to upload user's general location information, exposing the user's location, especially In some special areas, this method is not even desirable, such as the military field.
MAC技术支持单双向通讯,在双向通讯中,用户上传自身概略位置信息,中心软件根据用户位置选择距用户最近的参考站作为主参考站,将差分改正信息播发给用户;在单向通讯中,用户需要事先知道自己所处的预定义网元,然后获取相应的差分改正信息。此技术在双向通讯中,仍存在与VRS技术中①②相同的缺点;在单向通讯中,虽然克服了VRS技术存在的缺点,但是用户本身需要事先知道自己所处的网元,这对于用户来说,实现比较困难,尤其当用户进入陌生的区域时,几乎不可能实现;目前使用MAC技术的软件在进行网络解算时使用了非差算法,参数多,模型复杂,使得网元解算效率低,网络初始化时间(从开机到可提供网络RTK服务)长。MAC technology supports single two-way communication. In two-way communication, the user uploads his own approximate location information. The central software selects the reference station closest to the user as the primary reference station according to the user's location, and broadcasts the differential correction information to the user; in one-way communication, The user needs to know the predefined network element in which he is located, and then obtain the corresponding differential correction information. In the two-way communication, this technology still has the same shortcomings as the VRS technology. In the one-way communication, although the shortcomings of the VRS technology are overcome, the user himself needs to know the network element in which he is located, which is for the user. It is difficult to implement, especially when users enter unfamiliar areas. Currently, software using MAC technology uses non-difference algorithms for network solution, with many parameters and complex models, which makes the solution efficiency of network elements. Low, network initialization time (from boot to network RTK service available) long.
FKP技术中,中心软件使用非差算法实现网络解算,提取非差误差,并对空间相关误差进行区域建模,将移动站的非差空间相关误差参数化,利用广播模式进行播发,流动站根据 这些参数及自身位置进行实时定位。此技术的缺点在于:①中心软件利用非差算法进行网络解算,参数多,模型复杂,使得结算效率低,网络初始化时间长;②空间相关误差模型的建立由中心软件完成,限制了用户使用更优化的算法。In FKP technology, the central software uses non-difference algorithm to realize network solution, extracts non-difference error, and performs regional modeling on spatial correlation error, parameterizes non-difference space correlation error of mobile station, broadcasts by broadcast mode, and rover Real-time positioning based on these parameters and their location. The disadvantages of this technology are as follows: 1 The central software uses the non-difference algorithm for network solution, with many parameters and complex models, which makes the settlement efficiency low and the network initialization time long; 2 The establishment of the spatial correlation error model is completed by the central software, which limits the user's use. A more optimized algorithm.
发明内容Summary of the invention
为克服现有网络RTK技术中存在的不足,本发明提供一种基于星型网络的BDS/GPS广播式网络RTK算法,并兼容双向通讯,并支持由地面设备、航空飞机或卫星广播差分改正数据。服务端实时不间断地使用UDP协议向外广播整网所有星型网元的差分改正数据,使用广播模式的用户接收到数据后进行网元选择、大气内插及基线解算。使用双向通讯的用户,通过Ntrip协议或TCP/IP协议上传自身概略位置,服务端向该用户播发用户所在网元差分改正数据,该用户获得数据后进行大气内插及基线解算。服务端在向双向通讯用户播发差分改正数时,其按照广播模式播发的数据仍然不间断播。In order to overcome the deficiencies in the existing network RTK technology, the present invention provides a BDS/GPS broadcast network RTK algorithm based on a star network, and is compatible with two-way communication, and supports differential correction data by ground equipment, aviation aircraft or satellite broadcasting. . The server uses the UDP protocol to broadcast the differential correction data of all the star network elements in the whole network in real time, and the users in the broadcast mode receive the data, and then perform network element selection, atmospheric interpolation and baseline solution. The user who uses the two-way communication uploads its own approximate location through the Ntrip protocol or the TCP/IP protocol, and the server broadcasts the user's network element differential correction data to the user, and the user obtains the data and performs atmospheric interpolation and baseline solution. When the server broadcasts the differential correction number to the two-way communication user, the data broadcasted according to the broadcast mode is still uninterrupted.
本发明为解决上述技术问题采用以下技术方案:The present invention adopts the following technical solutions to solve the above technical problems:
本发明提供一种基于星型网络的BDS/GPS广播式网络RTK算法,包括以下具体步骤:The invention provides a star network-based BDS/GPS broadcast network RTK algorithm, which comprises the following specific steps:
步骤1,从数据库获取基准站坐标,利用Delaunay三角剖分算法生成Delaunay三角网,在三角网的基础上生成由若干个星型网元组成的可控制全区域的星型网络,其中,每个星型网元由一个主站与若干与之对应的辅站组成;Step 1: Obtain the base station coordinates from the database, use the Delaunay triangulation algorithm to generate the Delaunay triangulation, and generate a star-shaped network composed of several star network elements and control the whole region on the basis of the triangulation network, wherein each A star network element consists of a primary station and a number of secondary stations corresponding thereto;
步骤2,实时获取基准站数据,以Delaunay三角网中的基线为单元形成双差观测值,构建第一卡尔曼滤波器,实时估计基线双差模糊度及天顶对流层湿延迟ZTD,然后生成每条基线的基线双差大气误差;Step 2: Obtain the base station data in real time, form a double-difference observation with the baseline in the Delaunay triangulation, construct a first Kalman filter, estimate the baseline double-difference ambiguity and the zenith tropospheric wet delay ZTD in real time, and then generate each Baseline double difference atmospheric error of the baseline;
步骤3,将步骤2生成的基线双差大气误差赋给相应的星型网元基线,以星型网元为单元统一参考星,生成星型网元每条基线共视卫星站间单差大气误差;Step 3: Assign the baseline double-difference atmospheric error generated in step 2 to the corresponding star network element baseline, and use the star-shaped network element as a unit to unify the reference star, and generate a single-element atmosphere between each baseline satellite station of the star-shaped network element. error;
步骤4,以星型网元为单元,对星型网元的每条基线共视卫星站间单差大气误差、所有基准站坐标及主站观测值进行编码,编码后的数据利用UDP协议进行广播或使用双向通讯进行播发,其中,UDP协议广播所有数据后进入步骤5;使用双向通讯时,首先由用户上传概略位置信息,然后中心软件根据用户位置通过Ntrip协议或TCP/IP仅向用户播发用户所在星型网元的数据,进入步骤6;Step 4: Using a star-shaped network element as a unit, encoding a single-difference atmospheric error, all base station coordinates, and a master station observation value of each baseline satellite station of the star network element, and the encoded data is performed by using a UDP protocol. Broadcast or use two-way communication for broadcast, in which UDP protocol broadcasts all data and then proceeds to step 5; when using two-way communication, firstly, the user uploads the approximate location information, and then the central software broadcasts only to the user according to the user's location through Ntrip protocol or TCP/IP. The data of the star network element where the user is located, proceeds to step 6;
步骤5,用户实时接收数据并判断其所在网元,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7;Step 5, the user receives the data in real time and judges the network element where it is located, according to the differential data of the network element in which the network element is interpolated to obtain the single-difference atmospheric error between the station and the primary station, and corrects the observation value to the primary station, and proceeds to step 7;
步骤6,用户实时接收数据,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7;Step 6, the user receives the data in real time, according to the differential data of the network element, the inter-station single difference atmospheric error between the station and the main station is interpolated, and corrected to the observation value of the main station, and proceeds to step 7;
步骤7,用户利用经步骤5或6修正后的主站观测值与用户观测值组成双差观测值,构建包含用户位置参数及模糊度参数的第二卡尔曼滤波器,进行基线解算。In step 7, the user constructs a double-difference observation value by using the corrected observation value of the primary station and the user observation value corrected by step 5 or 6, and constructs a second Kalman filter including the user position parameter and the ambiguity parameter to perform baseline solution.
作为本发明的进一步优化方案,所述步骤1包括以下步骤:As a further optimization of the present invention, the step 1 includes the following steps:
步骤11,利用Delaunay三角剖分算法生成三角网;Step 11, generating a triangulation network by using a Delaunay triangulation algorithm;
步骤12,提取三角网整网边界基准站与非边界基准站,其中,若与某基准站相连的所有三角形中以此基准站为顶点的内角的角度之和大于设定阈值,则该基准站为非边界基准站,否则为边界基准站;Step 12: extracting a triangulation network boundary reference station and a non-boundary reference station, wherein if the sum of the angles of the inner angles of the vertices of the base station in all the triangles connected to a reference station is greater than a set threshold, the base station a non-boundary base station, otherwise a boundary reference station;
步骤13,初始化星型网元集合:以所有非边界基准站作为主站,与之相连的所有基准站作为相应的辅站;Step 13, initializing the star network element set: all the non-boundary base stations are used as the primary station, and all the base stations connected thereto are used as the corresponding auxiliary stations;
步骤14,在边界基准站中寻找未参与星型网络组网的基准站集合;Step 14: Find a set of base stations that do not participate in the star network networking in the boundary reference station;
步骤15,在未参与组网的基准站集合中选取与之相连的基准站数最多的基准站作为新的主站,与之连接的基准站作为相应的辅站,更新星型网络集合及未参与星型网络组网的基准站集合;Step 15, selecting the base station with the largest number of base stations connected to it as the new primary station in the base station set not participating in the networking, and the base station connected thereto as the corresponding secondary station, updating the star network set and not a set of base stations participating in a star network network;
步骤16,重复步骤15,直至未参与星型网络组网的基准站数为0。Step 16. Repeat step 15 until the number of base stations that are not participating in the star network networking is zero.
作为本发明的进一步优化方案,所述步骤2中包括以下步骤:As a further optimization of the present invention, the step 2 includes the following steps:
步骤21,基准站k接收到卫星s的伪距与载波观测信号,则载波与伪距观测方程表示为:Step 21: The base station k receives the pseudorange and carrier observation signals of the satellite s, and the carrier and pseudorange observation equations are expressed as:
Figure PCTCN2018078492-appb-000001
Figure PCTCN2018078492-appb-000001
Figure PCTCN2018078492-appb-000002
Figure PCTCN2018078492-appb-000002
式中:
Figure PCTCN2018078492-appb-000003
表示基准站站k接收到的卫星s的第j个频点上以周为单位的载波观测值,j=1,2,
Figure PCTCN2018078492-appb-000004
表示基准站k到卫星s的站星距,
Figure PCTCN2018078492-appb-000005
表示基准站k接收到的卫星s的第j个频点上的整周模糊度,c表示光速,dT k表示基准站k的接收机钟差,dT s表示卫星s的卫星钟差,
Figure PCTCN2018078492-appb-000006
表示基准站k接收到的卫星s的对流层延迟,
Figure PCTCN2018078492-appb-000007
表示基准站k接收到的卫星s第1个频点上电离层延迟,
Figure PCTCN2018078492-appb-000008
f j表示卫星s对应的卫星系统第j个频点上的频率值,f 1表示卫星s对应的卫星系统第1个频点上的频率值,rel s表示卫星s的相对论效应,
Figure PCTCN2018078492-appb-000009
表示基准站k接收到的卫星s的第j个频点上以米为单位的载波多路径效应,
Figure PCTCN2018078492-appb-000010
表示基准站k第j个频点上以米为单位的接收机端载波偏差,
Figure PCTCN2018078492-appb-000011
表示卫星s上第j个频点上以米为单位的卫星端载波偏差,
Figure PCTCN2018078492-appb-000012
表示基准站k接收到的卫星s第j个频点上以米为单位的载波观测噪声,
Figure PCTCN2018078492-appb-000013
表 示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测值,
Figure PCTCN2018078492-appb-000014
表示基准站k接收到的卫星的第j个频点上以米为单位的伪距多路径效应,
Figure PCTCN2018078492-appb-000015
表示基准站k第j个频点接收到的以米为单位的接收机端伪距偏差,
Figure PCTCN2018078492-appb-000016
表示卫星s第j个频点上卫星端以米为单位的伪距偏差,
Figure PCTCN2018078492-appb-000017
表示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测噪声,λ j表示卫星s对应的卫星系统第j个频点的波长;
In the formula:
Figure PCTCN2018078492-appb-000003
Indicates the carrier observation value in weeks on the jth frequency point of the satellite s received by the base station k, j=1, 2,
Figure PCTCN2018078492-appb-000004
Indicates the station star distance from the base station k to the satellite s,
Figure PCTCN2018078492-appb-000005
Indicates the full-circumference ambiguity at the j-th frequency point of the satellite s received by the reference station k, c represents the speed of light, dT k represents the receiver clock difference of the reference station k, and dT s represents the satellite clock difference of the satellite s,
Figure PCTCN2018078492-appb-000006
Indicates the tropospheric delay of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000007
Indicates the ionospheric delay at the first frequency of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000008
f j represents the frequency value at the jth frequency point of the satellite system corresponding to the satellite s, f 1 represents the frequency value at the 1st frequency point of the satellite system corresponding to the satellite s , and rel s represents the relativistic effect of the satellite s,
Figure PCTCN2018078492-appb-000009
Means the carrier multipath effect in meters on the jth frequency of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000010
Indicates the receiver-side carrier deviation in meters of the j-th frequency point of the base station k,
Figure PCTCN2018078492-appb-000011
Indicates the satellite-side carrier deviation in meters on the j-th frequency point on the satellite s.
Figure PCTCN2018078492-appb-000012
Indicates the carrier observation noise in meters per unit j of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000013
Indicates the pseudo-range observation value in meters on the j-th frequency point of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000014
Represents the pseudorange multipath effect in meters at the jth frequency of the satellite received by the base station k,
Figure PCTCN2018078492-appb-000015
Indicates the receiver-side pseudorange deviation in meters per unit received by the jth frequency point of the reference station k,
Figure PCTCN2018078492-appb-000016
Indicates the pseudorange deviation of the satellite end in meters at the jth frequency point of the satellite s,
Figure PCTCN2018078492-appb-000017
Representing the pseudorange observation noise in meters at the jth frequency point of the satellite s received by the reference station k, and λ j indicating the wavelength of the jth frequency point of the satellite system corresponding to the satellite s;
步骤22,根据步骤21获得的载波观测值与伪距观测值组成双差观测值,则基准站k与基准站y所组的双差载波观测方程与双差伪距观测方程分别为:Step 22, according to the carrier observation value obtained by step 21 and the pseudorange observation value constitute a double difference observation value, the double difference carrier observation equation and the double difference pseudo range observation equation of the reference station k and the reference station y are respectively:
Figure PCTCN2018078492-appb-000018
Figure PCTCN2018078492-appb-000018
Figure PCTCN2018078492-appb-000019
Figure PCTCN2018078492-appb-000019
式中,上标r表示参考卫星,
Figure PCTCN2018078492-appb-000020
表示第j个频点的双差载波观测值,
Figure PCTCN2018078492-appb-000021
表示双差站星距,
Figure PCTCN2018078492-appb-000022
表示第j个频点上的双差整周模糊度,
Figure PCTCN2018078492-appb-000023
表示双差对流层延迟,
Figure PCTCN2018078492-appb-000024
表示第一个频点上双差电离层延迟,
Figure PCTCN2018078492-appb-000025
表示第j个频点上以米为单位的双差载波多路径效应,
Figure PCTCN2018078492-appb-000026
表示第j个频点上以米为单位的双差载波观测噪声,
Figure PCTCN2018078492-appb-000027
表示第j个频点上的双差伪距观测值,
Figure PCTCN2018078492-appb-000028
表示第j个频点上的双差伪距多路径效应,
Figure PCTCN2018078492-appb-000029
表示第j个频点上的双差伪距观测噪声;
Where the superscript r represents the reference satellite,
Figure PCTCN2018078492-appb-000020
a double-difference carrier observation indicating the j-th frequency point,
Figure PCTCN2018078492-appb-000021
Indicates the star distance of the double-difference station,
Figure PCTCN2018078492-appb-000022
Indicates the double-difference full-circumference ambiguity at the jth frequency point,
Figure PCTCN2018078492-appb-000023
Indicates double-difference tropospheric delay,
Figure PCTCN2018078492-appb-000024
Indicates the doubled ionospheric delay at the first frequency point,
Figure PCTCN2018078492-appb-000025
Means the double-difference carrier multipath effect in meters on the jth frequency point,
Figure PCTCN2018078492-appb-000026
Indicates the double-difference carrier observation noise in meters on the jth frequency point,
Figure PCTCN2018078492-appb-000027
Indicates the double-difference pseudorange observation at the jth frequency point,
Figure PCTCN2018078492-appb-000028
Representing the double-difference pseudorange multipath effect at the jth frequency point,
Figure PCTCN2018078492-appb-000029
Representing the double difference pseudorange observation noise at the jth frequency point;
步骤23,根据步骤22形成的双差观测值组合成双差宽巷组合观测值,解算宽巷组合模糊度:Step 23: Combine the double-difference observations formed in step 22 into a double-difference wide lane combined observation value, and calculate the wide lane combined ambiguity:
采用MW组合解算宽巷组合模糊度,则解算方程为:Using the MW combination to solve the wide-altitude combination ambiguity, the solution equation is:
Figure PCTCN2018078492-appb-000030
Figure PCTCN2018078492-appb-000030
式中:
Figure PCTCN2018078492-appb-000031
Figure PCTCN2018078492-appb-000032
表示双差宽巷组合观测值,
Figure PCTCN2018078492-appb-000033
表示宽巷组合模糊度,λ WL表示宽巷波长;
In the formula:
Figure PCTCN2018078492-appb-000031
Figure PCTCN2018078492-appb-000032
Indicates the combined observation of double-difference wide lanes,
Figure PCTCN2018078492-appb-000033
Indicates the wide lane combination ambiguity, λ WL represents the wide lane wavelength;
对宽巷组合模糊度采用多历元平滑四舍五入取整,具体公式如下:For the wide lane combination ambiguity, multi-epoch smoothing is rounded off, and the specific formula is as follows:
Figure PCTCN2018078492-appb-000034
Figure PCTCN2018078492-appb-000034
式中:
Figure PCTCN2018078492-appb-000035
表示第i个观测历元解算得到的宽巷组合模糊度浮点解,z表示观测 历元总数,round表示四舍五入取整算子;
In the formula:
Figure PCTCN2018078492-appb-000035
The wide-altitude combined ambiguity floating-point solution obtained by the i-th observation epoch is calculated, z represents the total number of observation epochs, and round represents a rounding-and-rounding operator;
步骤24,采用无电离层组合,构建窄巷滤波器,利用无电离层组合联合宽巷组合分离出基础模糊度
Figure PCTCN2018078492-appb-000036
Figure PCTCN2018078492-appb-000037
包括以下步骤:
Step 24, using a combination of no ionosphere, constructing a narrow lane filter, and separating the base ambiguity by using a combination of no ionosphere and wide lane
Figure PCTCN2018078492-appb-000036
versus
Figure PCTCN2018078492-appb-000037
Includes the following steps:
步骤241,形成双差无电离层组合观测值:In step 241, a combined observation of the double-difference ionosphere is formed:
Figure PCTCN2018078492-appb-000038
Figure PCTCN2018078492-appb-000038
Figure PCTCN2018078492-appb-000039
Figure PCTCN2018078492-appb-000039
Figure PCTCN2018078492-appb-000040
Figure PCTCN2018078492-appb-000040
式中:
Figure PCTCN2018078492-appb-000041
表示双差无电离层组合观测值,
Figure PCTCN2018078492-appb-000042
表示无电离层组合模糊度,λ NL=c/(f 1+f 2);
In the formula:
Figure PCTCN2018078492-appb-000041
Represents a double-difference ionospheric combined observation,
Figure PCTCN2018078492-appb-000042
Represents no ionospheric combined ambiguity, λ NL = c / (f 1 + f 2 );
步骤242,构建第一卡尔曼滤波器:Step 242, constructing a first Kalman filter:
Figure PCTCN2018078492-appb-000043
Figure PCTCN2018078492-appb-000043
Figure PCTCN2018078492-appb-000044
Figure PCTCN2018078492-appb-000044
式中,E(g)表示求数学期望,Cov(g)表示求协方差,
Figure PCTCN2018078492-appb-000045
分别表示第i历元和第i-1历元的状态向量;
Figure PCTCN2018078492-appb-000046
表示状态转移矩阵;
Figure PCTCN2018078492-appb-000047
表示动态噪声向量,
Figure PCTCN2018078492-appb-000048
表示动态噪声协方差矩阵;
Figure PCTCN2018078492-appb-000049
表示第i历元观测向量,
Figure PCTCN2018078492-appb-000050
表示设计矩阵,
Figure PCTCN2018078492-appb-000051
表示第i历元观测噪声向量;
Figure PCTCN2018078492-appb-000052
表示为第i历元观测噪声协方差阵,
Figure PCTCN2018078492-appb-000053
表示第i历元状态向量协方差阵,
Figure PCTCN2018078492-appb-000054
表示状态向量预测协方差阵,
Figure PCTCN2018078492-appb-000055
表示第i历元状态向量方差-协方差阵,
Figure PCTCN2018078492-appb-000056
表示增益矩阵,
Figure PCTCN2018078492-appb-000057
表示单位矩阵;
Where E(g) represents the mathematical expectation and Cov(g) represents the covariance.
Figure PCTCN2018078492-appb-000045
State vectors representing the i-th epoch and the i-th epoch, respectively;
Figure PCTCN2018078492-appb-000046
Representing a state transition matrix;
Figure PCTCN2018078492-appb-000047
Represents a dynamic noise vector,
Figure PCTCN2018078492-appb-000048
Representing a dynamic noise covariance matrix;
Figure PCTCN2018078492-appb-000049
Represents the i-th eigen observation vector,
Figure PCTCN2018078492-appb-000050
Representing the design matrix,
Figure PCTCN2018078492-appb-000051
Representing the i-th eigen observation noise vector;
Figure PCTCN2018078492-appb-000052
Expressed as the i-th epoch observed noise covariance matrix,
Figure PCTCN2018078492-appb-000053
Representing the i-th epoch state vector covariance matrix,
Figure PCTCN2018078492-appb-000054
Representing a state vector prediction covariance matrix,
Figure PCTCN2018078492-appb-000055
Representing the i-th epoch state vector variance-covariance matrix,
Figure PCTCN2018078492-appb-000056
Representing the gain matrix,
Figure PCTCN2018078492-appb-000057
Express the unit matrix;
设在第i历元,基准站k与基准站y有n颗GPS共视卫星与g颗BDS共视卫星,其中,第n颗GPS卫星与第g颗BDS卫星为各系统的参考星,待估参数包括双差整周模糊度与基线相对天顶对流层湿延迟,其滤波模型待估参数向量、观测值向量及设计矩阵表示为:Based on the i-th epoch, the base station k and the reference station y have n GPS satellites and g BDS satellites, wherein the nth GPS satellite and the g-th BDS satellite are reference stars of each system. The estimation parameters include double-difference ambiguity and baseline relative zenith tropospheric wet delay. The filter model to be estimated parameter vector, observation vector and design matrix are expressed as:
Figure PCTCN2018078492-appb-000058
其中:
Figure PCTCN2018078492-appb-000058
among them:
Figure PCTCN2018078492-appb-000059
Figure PCTCN2018078492-appb-000059
Figure PCTCN2018078492-appb-000060
Figure PCTCN2018078492-appb-000060
Figure PCTCN2018078492-appb-000061
Figure PCTCN2018078492-appb-000061
式中:
Figure PCTCN2018078492-appb-000062
表示n+g-1维的状态向量(待估参数向量),包含1个相对天顶对流层湿延迟参数RZTD与n+g-2维双差整周模糊度参数向量
Figure PCTCN2018078492-appb-000063
Figure PCTCN2018078492-appb-000064
表示n+g-2维的双差载波观测值向量,
Figure PCTCN2018078492-appb-000065
表示GPS双差载波观测值,o=1,2,L,n-1,
Figure PCTCN2018078492-appb-000066
表示GPS窄巷波长,
Figure PCTCN2018078492-appb-000067
表示GPS第1个频点的波长,
Figure PCTCN2018078492-appb-000068
表示GPS双差无电离层组合载波观测值,
Figure PCTCN2018078492-appb-000069
表示GPS双差站星距,
Figure PCTCN2018078492-appb-000070
表示GPS卫星双差对流层干延迟,
Figure PCTCN2018078492-appb-000071
表示GPS双差宽巷整周模糊度,
Figure PCTCN2018078492-appb-000072
表示GPS第1个频点的频率值,
Figure PCTCN2018078492-appb-000073
表示GPS第2个频点的频率值,
Figure PCTCN2018078492-appb-000074
表示BDS双差载波观测值,s=1,2,L,g-1,
Figure PCTCN2018078492-appb-000075
表示BDS窄巷波长,
Figure PCTCN2018078492-appb-000076
表示BDS第一个频点的波长,
Figure PCTCN2018078492-appb-000077
表示BDS双差无电离层组合载波观测值,
Figure PCTCN2018078492-appb-000078
表示BDS双差站星距,
Figure PCTCN2018078492-appb-000079
表示BDS卫星双差对流层干延迟,
Figure PCTCN2018078492-appb-000080
表示BDS双差宽巷整周模糊度,
Figure PCTCN2018078492-appb-000081
表示BDS第1个频点的频率值,
Figure PCTCN2018078492-appb-000082
表示BDS第2个频点的频率值,
Figure PCTCN2018078492-appb-000083
表示基准站k上GPS 系统卫星o的对流层映射函数,
Figure PCTCN2018078492-appb-000084
表示基准站y上GPS系统参考卫星n的对流层映射函数,
Figure PCTCN2018078492-appb-000085
表示基准站k上BDS系统卫星s的对流层映射函数,
Figure PCTCN2018078492-appb-000086
表示基准站y上BDS系统参考卫星g的对流层映射函数,
Figure PCTCN2018078492-appb-000087
表示(n+g-2)×(n+g-1)维的设计矩阵;
In the formula:
Figure PCTCN2018078492-appb-000062
A state vector representing the n+g-1 dimension (the parameter vector to be estimated), including a relative zenith tropospheric wet delay parameter RZTD and n+g-2 dimensional double difference whole-circumference ambiguity parameter vector
Figure PCTCN2018078492-appb-000063
Figure PCTCN2018078492-appb-000064
a vector of double-difference carrier observations representing n+g-2 dimensions,
Figure PCTCN2018078492-appb-000065
Indicates GPS double-difference carrier observations, o=1, 2, L, n-1,
Figure PCTCN2018078492-appb-000066
Indicates the GPS narrow lane wavelength,
Figure PCTCN2018078492-appb-000067
Indicates the wavelength of the first frequency point of GPS,
Figure PCTCN2018078492-appb-000068
Indicates the GPS double-difference ionosphere-free combined carrier observation,
Figure PCTCN2018078492-appb-000069
Indicates the GPS star distance,
Figure PCTCN2018078492-appb-000070
Represents the GPS satellite double-difference tropospheric dry delay,
Figure PCTCN2018078492-appb-000071
Indicates the full-circumference ambiguity of the GPS double-difference wide lane
Figure PCTCN2018078492-appb-000072
Indicates the frequency value of the first frequency point of GPS.
Figure PCTCN2018078492-appb-000073
Indicates the frequency value of the second frequency point of GPS.
Figure PCTCN2018078492-appb-000074
Indicates the BDS double-difference carrier observation, s = 1, 2, L, g-1,
Figure PCTCN2018078492-appb-000075
Indicates the BDS narrow lane wavelength,
Figure PCTCN2018078492-appb-000076
Indicates the wavelength of the first frequency of the BDS,
Figure PCTCN2018078492-appb-000077
Indicates the BDS double-difference ionosphere-free combined carrier observation,
Figure PCTCN2018078492-appb-000078
Indicates the star distance of the BDS double-difference station,
Figure PCTCN2018078492-appb-000079
Indicates the double-difference tropospheric dry delay of the BDS satellite,
Figure PCTCN2018078492-appb-000080
Indicates the full-circumference ambiguity of the BDS double-difference wide lane,
Figure PCTCN2018078492-appb-000081
Indicates the frequency value of the first frequency point of the BDS.
Figure PCTCN2018078492-appb-000082
Indicates the frequency value of the 2nd frequency point of the BDS.
Figure PCTCN2018078492-appb-000083
Indicates the tropospheric mapping function of the GPS system satellite o on the base station k,
Figure PCTCN2018078492-appb-000084
Indicates the tropospheric mapping function of the GPS system reference satellite n on the base station y,
Figure PCTCN2018078492-appb-000085
Indicates the tropospheric mapping function of the BDS system satellite s on the base station k,
Figure PCTCN2018078492-appb-000086
Indicates the tropospheric mapping function of the reference satellite g of the BDS system on the base station y,
Figure PCTCN2018078492-appb-000087
a design matrix representing (n+g-2)×(n+g-1) dimensions;
步骤243,根据步骤242建立的第一卡尔曼滤波器进行滤波,并解算基础载波模糊度向量参数;Step 243: Perform filtering according to the first Kalman filter established in step 242, and solve a basic carrier ambiguity vector parameter.
从滤波器中提取出模糊度参数向量浮点解
Figure PCTCN2018078492-appb-000088
与方差-协方差阵利用lambda算法进行搜索,获得第1个频点双差整周模糊度
Figure PCTCN2018078492-appb-000089
(BDS)与
Figure PCTCN2018078492-appb-000090
(GPS),进一步得到第2个频点的双差整周模糊度
Figure PCTCN2018078492-appb-000091
Figure PCTCN2018078492-appb-000092
Figure PCTCN2018078492-appb-000093
Figure PCTCN2018078492-appb-000094
Extracting the ambiguity parameter vector floating point solution from the filter
Figure PCTCN2018078492-appb-000088
And the variance-covariance matrix is searched by the lambda algorithm to obtain the first frequency double-difference full-circumference ambiguity
Figure PCTCN2018078492-appb-000089
(BDS) and
Figure PCTCN2018078492-appb-000090
(GPS), further obtain the double difference whole-circumference ambiguity of the second frequency point
Figure PCTCN2018078492-appb-000091
versus
Figure PCTCN2018078492-appb-000092
Figure PCTCN2018078492-appb-000093
Figure PCTCN2018078492-appb-000094
步骤25,根据步骤24的结果,生成基线双差大气误差:Step 25, according to the result of step 24, generating a baseline double difference atmospheric error:
Figure PCTCN2018078492-appb-000095
Figure PCTCN2018078492-appb-000095
Figure PCTCN2018078492-appb-000096
Figure PCTCN2018078492-appb-000096
Figure PCTCN2018078492-appb-000097
Figure PCTCN2018078492-appb-000097
Figure PCTCN2018078492-appb-000098
Figure PCTCN2018078492-appb-000098
式中,
Figure PCTCN2018078492-appb-000099
Figure PCTCN2018078492-appb-000100
分别表示GPS与BDS双差对流层延迟,
Figure PCTCN2018078492-appb-000101
Figure PCTCN2018078492-appb-000102
分别表示GPS与BDS第一个频点双差载波观测值,
Figure PCTCN2018078492-appb-000103
Figure PCTCN2018078492-appb-000104
分别表示GPS与BDS第二个频点双差载波观测值,
Figure PCTCN2018078492-appb-000105
Figure PCTCN2018078492-appb-000106
分别表示GPS与BDS第1个频点双差电离层延迟。
In the formula,
Figure PCTCN2018078492-appb-000099
versus
Figure PCTCN2018078492-appb-000100
Representing the double-difference tropospheric delay between GPS and BDS,
Figure PCTCN2018078492-appb-000101
versus
Figure PCTCN2018078492-appb-000102
Representing the GPS and BDS first frequency double-difference carrier observations,
Figure PCTCN2018078492-appb-000103
versus
Figure PCTCN2018078492-appb-000104
Representing the second frequency difference observation of GPS and BDS respectively,
Figure PCTCN2018078492-appb-000105
versus
Figure PCTCN2018078492-appb-000106
It indicates the 1st frequency doubled ionospheric delay of GPS and BDS respectively.
作为本发明的进一步优化方案,所述步骤3中包括以下步骤:As a further optimization of the present invention, the step 3 includes the following steps:
步骤31,星型网元的主站与辅站组成基线,在三角网整网基线列表中寻找由相同基准站组成的基线,若两条基线方向相反,则需进行基线换向,由此获得星型网元各条基线双差大气误差;Step 31: The primary station and the secondary station of the star network element form a baseline, and the baseline consisting of the same base station is searched in the baseline list of the entire network of the triangular network. If the two baseline directions are opposite, the baseline commutation is required, thereby obtaining Baseline double-difference atmospheric error for each type of star network element;
步骤32,检查星型网元各条基线参考星是否一致,若不一致,则统一参考星并对大气误 差进行参考星变换;Step 32: Check whether the baseline reference stars of the star network elements are consistent. If they are inconsistent, the reference star is unified and the reference star transformation is performed on the atmospheric error;
步骤33,生成星型网元站间单差大气误差:视参考星站间单差大气误差为0,则其他卫星的站间单差大气误差值等于双差大气误差;Step 33: Generate a single-difference atmospheric error between the star-type network elements: the single-difference atmospheric error between the reference satellite stations is 0, and the single-difference atmospheric error value of the other satellites is equal to the double-difference atmospheric error;
步骤34,提取星型网元各条基线均能共视的卫星,生成星型网元共视卫星站间单差大气误差。Step 34: Extract satellites of each star-shaped network element that can be shared by the baseline, and generate a single-difference atmospheric error between the satellite stations of the star-shaped network element.
作为本发明的进一步优化方案,所述步骤5判断其所在网元的方法为:用户对接收到的数据进行解码并计算用户到每个主站的直线距离,以距离最小的主站所代表的网元作为用户所在网元。As a further optimization scheme of the present invention, the method for determining the network element where the step 5 is located is: the user decodes the received data and calculates the linear distance of the user to each primary station, represented by the primary station with the smallest distance. The NE is the NE of the user.
作为本发明的进一步优化方案,所述步骤5或6中根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,包括以下步骤:As a further optimization scheme of the present invention, the step 5 or 6 interpolates the difference between the station and the primary station according to the differential data of the network element in which the network element is located, and corrects the observation to the primary station observation value, including the following steps:
步骤①,利用线性内插算法进行用户大气误差内插,则用户与主站站间单差大气误差计算如下:Step 1. Using the linear interpolation algorithm to interpolate the user's atmospheric error, the single-difference atmospheric error between the user and the primary station is calculated as follows:
Figure PCTCN2018078492-appb-000107
Figure PCTCN2018078492-appb-000107
Figure PCTCN2018078492-appb-000108
Figure PCTCN2018078492-appb-000108
式中,下标m表示主站,u表示用户,α 123表示对流层内插系数,β 12表示电离层内插系数,w表示辅站数目,
Figure PCTCN2018078492-appb-000109
表示卫星s的站间单差对流层延迟,Δx m,u,Δy m,u,Δh m,u分别表示主站与用户的坐标差,
Figure PCTCN2018078492-appb-000110
表示站间单差电离层延迟;
Where subscript m denotes the primary station, u denotes the user, α 1 , α 2 , α 3 denote the tropospheric interpolation coefficient, β 1 , β 2 denote the ionospheric interpolation coefficient, and w denote the number of secondary stations,
Figure PCTCN2018078492-appb-000109
Indicates the inter-station single-difference tropospheric delay of the satellite s, Δx m, u , Δy m, u , Δh m, u represent the coordinate difference between the primary station and the user , respectively.
Figure PCTCN2018078492-appb-000110
Indicates the single-difference ionospheric delay between stations;
对流层内插系数与电离层内插系数计算方法如下:The tropospheric interpolation coefficients and ionospheric interpolation coefficients are calculated as follows:
Figure PCTCN2018078492-appb-000111
Figure PCTCN2018078492-appb-000111
Figure PCTCN2018078492-appb-000112
Figure PCTCN2018078492-appb-000112
Figure PCTCN2018078492-appb-000113
Figure PCTCN2018078492-appb-000113
Figure PCTCN2018078492-appb-000114
Figure PCTCN2018078492-appb-000114
Figure PCTCN2018078492-appb-000115
Figure PCTCN2018078492-appb-000115
式中:Δx m,t,Δy m,t,Δh m,t表示主站与辅站坐标差,t=1,2,L,w; Where: Δx m,t , Δy m,t , Δh m,t represents the coordinate difference between the primary station and the secondary station, t=1, 2, L, w;
步骤②,将内插得到的大气误差值修正至主站观测值,伪距与载波观测值分别如下:In step 2, the atmospheric error value obtained by the interpolation is corrected to the observation value of the primary station, and the pseudorange and the carrier observation value are respectively as follows:
Figure PCTCN2018078492-appb-000116
Figure PCTCN2018078492-appb-000116
Figure PCTCN2018078492-appb-000117
Figure PCTCN2018078492-appb-000117
式中:
Figure PCTCN2018078492-appb-000118
分别表示修正了大气误差后的卫星s第j个频点在主站上的伪距与载波观测值,
Figure PCTCN2018078492-appb-000119
分别表示卫星s第j个频点在主站上的原始伪距与载波观测值,
Figure PCTCN2018078492-appb-000120
表示通过内插得到的卫星s的站间对流层延迟,
Figure PCTCN2018078492-appb-000121
表示通过内插得到的卫星s的站间电离层延迟。
In the formula:
Figure PCTCN2018078492-appb-000118
It shows the pseudorange and carrier observation values of the jth frequency point of the satellite s after the correction of the atmospheric error on the primary station.
Figure PCTCN2018078492-appb-000119
Representing the original pseudorange and carrier observations of the jth frequency point of the satellite s on the primary station,
Figure PCTCN2018078492-appb-000120
Indicates the inter-station tropospheric delay of the satellite s obtained by interpolation,
Figure PCTCN2018078492-appb-000121
Indicates the inter-site ionospheric delay of the satellite s obtained by interpolation.
作为本发明的进一步优化方案,所述步骤7中双差观测值表示为:As a further optimization of the present invention, the double difference observation in the step 7 is expressed as:
Figure PCTCN2018078492-appb-000122
Figure PCTCN2018078492-appb-000122
Figure PCTCN2018078492-appb-000123
Figure PCTCN2018078492-appb-000123
Figure PCTCN2018078492-appb-000124
Figure PCTCN2018078492-appb-000124
Figure PCTCN2018078492-appb-000125
Figure PCTCN2018078492-appb-000125
式中,
Figure PCTCN2018078492-appb-000126
表示GPS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000127
表示GPS卫星双差站星距,
Figure PCTCN2018078492-appb-000128
表示GPS卫星双差伪距多路径效应,
Figure PCTCN2018078492-appb-000129
表示GPS卫星双差伪距观测噪声,
Figure PCTCN2018078492-appb-000130
表示GPS卫星双差载波观测值,λ G表示GPS观测值对应频点的波长,
Figure PCTCN2018078492-appb-000131
表示GPS卫星双差整周模糊度,
Figure PCTCN2018078492-appb-000132
表示以周为单位的GPS卫星双差载波多路径效应,
Figure PCTCN2018078492-appb-000133
表示以周为单位的GPS卫星双差载波观测噪声,
Figure PCTCN2018078492-appb-000134
表示BDS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000135
表示BDS卫星双差站星距,
Figure PCTCN2018078492-appb-000136
表示BDS卫星双差伪距多路径效应,
Figure PCTCN2018078492-appb-000137
表示BDS卫星双差伪距观测噪声,
Figure PCTCN2018078492-appb-000138
表示BDS卫星双差载波观测值,λ C表示BDS观测值对应频点的波长,
Figure PCTCN2018078492-appb-000139
表示BDS卫星双差整周模糊度,
Figure PCTCN2018078492-appb-000140
表示以周为单位的BDS卫星双差载波多路径效应,
Figure PCTCN2018078492-appb-000141
表示以周为单位的BDS卫星双差载波观测噪声。
In the formula,
Figure PCTCN2018078492-appb-000126
Representing GPS satellite double-difference pseudorange observations,
Figure PCTCN2018078492-appb-000127
Indicates the satellite distance of the GPS satellite double-difference station,
Figure PCTCN2018078492-appb-000128
Representing GPS satellite double-difference pseudorange multipath effect,
Figure PCTCN2018078492-appb-000129
Representing GPS satellite double-difference pseudorange observation noise,
Figure PCTCN2018078492-appb-000130
Indicates the GPS satellite double-difference carrier observation, and λ G represents the wavelength of the GPS observation corresponding to the frequency point.
Figure PCTCN2018078492-appb-000131
Represents the GPS satellite double-difference ambiguity,
Figure PCTCN2018078492-appb-000132
Represents the GPS satellite double-difference carrier multipath effect in weeks,
Figure PCTCN2018078492-appb-000133
Representing GPS satellite double-difference carrier observation noise in weeks,
Figure PCTCN2018078492-appb-000134
Indicates the double-difference pseudorange observation of the BDS satellite,
Figure PCTCN2018078492-appb-000135
Indicates the star distance of the BDS satellite double-difference station,
Figure PCTCN2018078492-appb-000136
Representing the double-signal pseudorange multipath effect of BDS satellites,
Figure PCTCN2018078492-appb-000137
Representing BDS satellite double-difference pseudorange observation noise,
Figure PCTCN2018078492-appb-000138
Indicates the BDS satellite double-difference carrier observation, and λ C represents the wavelength of the BDS observation corresponding to the frequency point.
Figure PCTCN2018078492-appb-000139
Indicates the double-difference ambiguity of the BDS satellite,
Figure PCTCN2018078492-appb-000140
Representing the double-signal carrier multipath effect of the BDS satellite in weeks,
Figure PCTCN2018078492-appb-000141
Indicates the BDS satellite double-difference carrier observation noise in weeks.
作为本发明的进一步优化方案,步骤7中第二卡尔曼滤波器构建如下:As a further optimization of the invention, the second Kalman filter in step 7 is constructed as follows:
设在第i历元,用户与星型网有n颗GPS共视卫星和g颗BDS共视卫星,其中第n颗GPS卫星与第g颗BDS卫星分别为各系统的参考星,联合所有卫星L1载波和P1伪距观测数据,其滤波模型待估参数矩阵
Figure PCTCN2018078492-appb-000142
观测值矩阵
Figure PCTCN2018078492-appb-000143
及设计矩阵
Figure PCTCN2018078492-appb-000144
表示为:
Based on the i-th epoch, the user and the star network have n GPS satellites and g BDS satellites, of which the nth GPS satellite and the gth BDS satellite are reference stars of each system, and all satellites are combined. L1 carrier and P1 pseudorange observation data, filter model to be estimated parameter matrix
Figure PCTCN2018078492-appb-000142
Observation matrix
Figure PCTCN2018078492-appb-000143
Design matrix
Figure PCTCN2018078492-appb-000144
Expressed as:
Figure PCTCN2018078492-appb-000145
Figure PCTCN2018078492-appb-000145
Figure PCTCN2018078492-appb-000146
Figure PCTCN2018078492-appb-000146
式中,
Figure PCTCN2018078492-appb-000147
表示n+g+1维的待估参数向量,包含3维位置参数向量
Figure PCTCN2018078492-appb-000148
与n+g-2维双差整周模糊度参数向量
Figure PCTCN2018078492-appb-000149
Figure PCTCN2018078492-appb-000150
表示2(n+g-2)维双差观测值向量,包括伪距与载波观测值;
Figure PCTCN2018078492-appb-000151
表示2(n+g-2)×(n+g+1)维设计矩阵,其中l o,n,G,p o,n,G,q o,n,G表示GPS卫星方向余弦(上标o=1,2L,n-1),l s,g,C,p s,g,C,q s,g,C(上标s=1,2L,t-1)表示BDS卫星方向余弦,
Figure PCTCN2018078492-appb-000152
表示以米为单位的GPS卫星双差载波观测值,
Figure PCTCN2018078492-appb-000153
表示GPS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000154
表示GPS卫星双差站星距,
Figure PCTCN2018078492-appb-000155
表示BDS卫星双差站星距,
Figure PCTCN2018078492-appb-000156
表示以米为单位的BDS卫星双差载波观测值,
Figure PCTCN2018078492-appb-000157
表示BDS卫星双差伪距观测值;
In the formula,
Figure PCTCN2018078492-appb-000147
An estimated parameter vector representing n+g+1 dimensions, including a 3-dimensional positional parameter vector
Figure PCTCN2018078492-appb-000148
Double-difference whole-circumference ambiguity parameter vector with n+g-2
Figure PCTCN2018078492-appb-000149
Figure PCTCN2018078492-appb-000150
Representing a 2(n+g-2) dimensional double difference observation vector, including pseudorange and carrier observations;
Figure PCTCN2018078492-appb-000151
Represents a 2(n+g-2)×(n+g+1) dimensional design matrix, where l o,n,G ,p o,n,G ,q o,n,G represent the cosine of the GPS satellite direction (superscript o=1,2L,n-1),l s,g,C ,p s,g,C ,q s,g,C (superscript s=1,2L,t-1) represent the cosine of the BDS satellite direction,
Figure PCTCN2018078492-appb-000152
Means the GPS satellite double-difference carrier observation in meters,
Figure PCTCN2018078492-appb-000153
Representing GPS satellite double-difference pseudorange observations,
Figure PCTCN2018078492-appb-000154
Indicates the satellite distance of the GPS satellite double-difference station,
Figure PCTCN2018078492-appb-000155
Indicates the star distance of the BDS satellite double-difference station,
Figure PCTCN2018078492-appb-000156
Indicates the BDS satellite double-difference carrier observations in meters,
Figure PCTCN2018078492-appb-000157
Indicates the double-difference pseudorange observation of the BDS satellite;
将上述参数赋值并带入第二卡尔曼滤波器中逐历元解算,然后提取浮点模糊度向量与其方差-协方差阵,利用lambda算法搜索即可获得模糊度固定解;The above parameters are assigned and brought into the second Kalman filter to solve the epoch epoch, then the floating ambiguity vector and its variance-covariance matrix are extracted, and the ambiguity fixed solution can be obtained by searching with the lambda algorithm;
固定模糊度后,利用下式解得用户三维坐标固定解:After fixing the ambiguity, the fixed solution of the user's three-dimensional coordinates is solved by the following formula:
Figure PCTCN2018078492-appb-000158
Figure PCTCN2018078492-appb-000158
其中,
Figure PCTCN2018078492-appb-000159
分别为三维坐标参数向量及浮点模糊度参数向量,
Figure PCTCN2018078492-appb-000160
为固定模糊度后的坐标参数向量,
Figure PCTCN2018078492-appb-000161
为固定模糊度参数向量,
Figure PCTCN2018078492-appb-000162
分别对应各参数滤波解协方差阵。
among them,
Figure PCTCN2018078492-appb-000159
Three-dimensional coordinate parameter vector and floating-point ambiguity parameter vector,
Figure PCTCN2018078492-appb-000160
The coordinate parameter vector after fixing the ambiguity,
Figure PCTCN2018078492-appb-000161
To fix the ambiguity parameter vector,
Figure PCTCN2018078492-appb-000162
Corresponding to each parameter filtering solution covariance matrix.
本发明采用以上技术方案与现有技术相比,具有以下技术效果:Compared with the prior art, the present invention has the following technical effects:
(1)本发明采用了星型网络进行大气内插,可以提供冗余观测值;(1) The present invention uses a star network for atmospheric interpolation to provide redundant observations;
(2)本发明真正实现了广播模式网络RTK,并兼顾双向通讯,用户容量不受限制;(2) The present invention truly realizes the broadcast mode network RTK, and takes into consideration two-way communication, and the user capacity is not limited;
(3)本发明所采用的广播模式,差分数据既可以通过地面设备播发,也可通过航空飞机或卫星播发,可用于广域差分和星基增强数据播发。(3) The broadcast mode adopted by the present invention, the differential data can be broadcasted by ground equipment or by air plane or satellite, and can be used for wide-area differential and satellite-based enhanced data broadcast.
附图说明DRAWINGS
图1是本发明一种基于星型网络的BDS/GPS广播式网络RTK算法流程图。1 is a flow chart of a BDS/GPS broadcast network RTK algorithm based on a star network according to the present invention.
图2是星型网元生成算法流程图。2 is a flow chart of a star network element generation algorithm.
具体实施方式Detailed ways
下面结合附图对本发明的技术方案做进一步的详细说明:The technical solution of the present invention will be further described in detail below with reference to the accompanying drawings:
本发明设计一种基于星型网络的BDS/GPS广播式网络RTK算法,如图1所示,包括以下步骤:The invention designs a BDS/GPS broadcast network RTK algorithm based on a star network, as shown in FIG. 1 , comprising the following steps:
步骤1,从数据库获取基准站坐标,利用Delaunay三角剖分算法生成Delaunay三角网,在三角网的基础上生成由若干个星型网元组成的可控制全区域的星型网络,其中,每个星型网元由一个主站与若干与之对应的辅站组成。Step 1: Obtain the base station coordinates from the database, use the Delaunay triangulation algorithm to generate the Delaunay triangulation, and generate a star-shaped network composed of several star network elements and control the whole region on the basis of the triangulation network, wherein each A star network element consists of a primary station and a number of secondary stations corresponding to it.
如图2所示,所述步骤1包括以下步骤:As shown in FIG. 2, the step 1 includes the following steps:
步骤11,利用Delaunay三角剖分算法生成三角网,其中,三角形最大角度阈值为165°(该阈值根据个人经验进行设定);Step 11, using a Delaunay triangulation algorithm to generate a triangulation, wherein the maximum angle threshold of the triangle is 165° (the threshold is set according to personal experience);
步骤12,提取三角网整网边界基准站与非边界基准站,其中,若与某基准站相连的所有三角形中以此基准站为顶点的内角的角度之和大于设定阈值195°,则该基准站为非边界基准站,否则为边界基准站;Step 12: extracting a triangulation network boundary reference station and a non-boundary reference station, wherein if the sum of the angles of the inner angles of the vertices of the base station in all the triangles connected to a reference station is greater than a set threshold of 195°, then The base station is a non-boundary base station, otherwise it is a boundary base station;
步骤13,初始化星型网元集合:以所有非边界基准站作为主站,与之相连的所有基准站作为相应的辅站;Step 13, initializing the star network element set: all the non-boundary base stations are used as the primary station, and all the base stations connected thereto are used as the corresponding auxiliary stations;
步骤14,在边界基准站中寻找未参与星型网络组网的基准站集合(既不是主站,又未与任何主站相连);Step 14. Find a set of base stations that are not participating in the star network networking in the border reference station (neither the primary station nor the primary station);
步骤15,在未参与组网的基准站集合中选取与之相连的基准站数最多的基准站作为新的 主站,与之连接的基准站作为相应的辅站,更新星型网络集合及未参与星型网络组网的基准站集合;Step 15, selecting the base station with the largest number of base stations connected to it as the new primary station in the base station set not participating in the networking, and the base station connected thereto as the corresponding secondary station, updating the star network set and not a set of base stations participating in a star network network;
步骤16,重复步骤15,直至未参与星型网络组网的基准站数为0。Step 16. Repeat step 15 until the number of base stations that are not participating in the star network networking is zero.
步骤2,实时获取基准站数据,以Delaunay三角网中的基线为单元形成双差观测值,构建第一卡尔曼滤波器,实时估计基线双差模糊度及天顶对流层湿延迟ZTD,然后生成每条基线的基线双差大气误差。Step 2: Obtain the base station data in real time, form a double-difference observation with the baseline in the Delaunay triangulation, construct a first Kalman filter, estimate the baseline double-difference ambiguity and the zenith tropospheric wet delay ZTD in real time, and then generate each Baseline double difference atmospheric error for the baseline.
步骤2中包括以下步骤:Step 2 includes the following steps:
步骤21,基准站k接收到卫星s的伪距与载波观测信号,则载波与伪距观测方程表示为:Step 21: The base station k receives the pseudorange and carrier observation signals of the satellite s, and the carrier and pseudorange observation equations are expressed as:
Figure PCTCN2018078492-appb-000163
Figure PCTCN2018078492-appb-000163
Figure PCTCN2018078492-appb-000164
Figure PCTCN2018078492-appb-000164
式中:
Figure PCTCN2018078492-appb-000165
表示基准站站k接收到的卫星s的第j个频点上以周为单位的载波观测值,j=1,2,
Figure PCTCN2018078492-appb-000166
表示基准站k到卫星s的站星距,
Figure PCTCN2018078492-appb-000167
表示基准站k接收到的卫星s的第j个频点上的整周模糊度,c表示光速,dT k表示基准站k的接收机钟差,dT s表示卫星s的卫星钟差,
Figure PCTCN2018078492-appb-000168
表示基准站k接收到的卫星s的对流层延迟,
Figure PCTCN2018078492-appb-000169
表示基准站k接收到的卫星s第1个频点上电离层延迟,
Figure PCTCN2018078492-appb-000170
f j表示卫星s对应的卫星系统第j个频点上的频率值,f 1表示卫星s对应的卫星系统第1个频点上的频率值,rel s表示卫星s的相对论效应,
Figure PCTCN2018078492-appb-000171
表示基准站k接收到的卫星s的第j个频点上以米为单位的载波多路径效应,
Figure PCTCN2018078492-appb-000172
表示基准站k第j个频点上以米为单位的接收机端载波偏差,
Figure PCTCN2018078492-appb-000173
表示卫星s上第j个频点上以米为单位的卫星端载波偏差,
Figure PCTCN2018078492-appb-000174
表示基准站k接收到的卫星s第j个频点上以米为单位的载波观测噪声,
Figure PCTCN2018078492-appb-000175
表示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测值,
Figure PCTCN2018078492-appb-000176
表示基准站k接收到的卫星的第j个频点上以米为单位的伪距多路径效应,
Figure PCTCN2018078492-appb-000177
表示基准站k第j个频点接收到的以米为单位的接收机端伪距偏差,
Figure PCTCN2018078492-appb-000178
表示卫星s第j个频点上卫星端以米为单位的伪距偏差,
Figure PCTCN2018078492-appb-000179
表示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测噪声,λ j表示卫星s对应的卫星系统第j个频点的波长。
In the formula:
Figure PCTCN2018078492-appb-000165
Indicates the carrier observation value in weeks on the jth frequency point of the satellite s received by the base station k, j=1, 2,
Figure PCTCN2018078492-appb-000166
Indicates the station star distance from the base station k to the satellite s,
Figure PCTCN2018078492-appb-000167
Indicates the full-circumference ambiguity at the j-th frequency point of the satellite s received by the reference station k, c represents the speed of light, dT k represents the receiver clock difference of the reference station k, and dT s represents the satellite clock difference of the satellite s,
Figure PCTCN2018078492-appb-000168
Indicates the tropospheric delay of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000169
Indicates the ionospheric delay at the first frequency of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000170
f j represents the frequency value at the jth frequency point of the satellite system corresponding to the satellite s, f 1 represents the frequency value at the 1st frequency point of the satellite system corresponding to the satellite s , and rel s represents the relativistic effect of the satellite s,
Figure PCTCN2018078492-appb-000171
Means the carrier multipath effect in meters on the jth frequency of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000172
Indicates the receiver-side carrier deviation in meters of the j-th frequency point of the base station k,
Figure PCTCN2018078492-appb-000173
Indicates the satellite-side carrier deviation in meters on the j-th frequency point on the satellite s.
Figure PCTCN2018078492-appb-000174
Indicates the carrier observation noise in meters per unit j of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000175
Indicates the pseudo-range observation value in meters on the j-th frequency point of the satellite s received by the base station k,
Figure PCTCN2018078492-appb-000176
Represents the pseudorange multipath effect in meters at the jth frequency of the satellite received by the base station k,
Figure PCTCN2018078492-appb-000177
Indicates the receiver-side pseudorange deviation in meters per unit received by the jth frequency point of the reference station k,
Figure PCTCN2018078492-appb-000178
Indicates the pseudorange deviation of the satellite end in meters at the jth frequency point of the satellite s,
Figure PCTCN2018078492-appb-000179
It represents the pseudorange observation noise in meters at the jth frequency point of the satellite s received by the reference station k, and λ j represents the wavelength of the jth frequency point of the satellite system corresponding to the satellite s.
步骤22,根据步骤21获得的载波观测值与伪距观测值组成双差观测值,则基准站k与基 准站y所组的双差载波观测方程与双差伪距观测方程分别为:Step 22, according to the carrier observation value obtained by step 21 and the pseudorange observation value to form a double difference observation value, the double difference carrier observation equation and the double difference pseudo range observation equation of the reference station k and the reference station y are respectively:
Figure PCTCN2018078492-appb-000180
Figure PCTCN2018078492-appb-000180
Figure PCTCN2018078492-appb-000181
Figure PCTCN2018078492-appb-000181
式中,上标r表示参考卫星,
Figure PCTCN2018078492-appb-000182
表示第j个频点的双差载波观测值,
Figure PCTCN2018078492-appb-000183
表示双差站星距,
Figure PCTCN2018078492-appb-000184
表示第j个频点上的双差整周模糊度,
Figure PCTCN2018078492-appb-000185
表示双差对流层延迟,
Figure PCTCN2018078492-appb-000186
表示第一个频点上双差电离层延迟,
Figure PCTCN2018078492-appb-000187
表示第j个频点上以米为单位的双差载波多路径效应,
Figure PCTCN2018078492-appb-000188
表示第j个频点上以米为单位的双差载波观测噪声,
Figure PCTCN2018078492-appb-000189
表示第j个频点上的双差伪距观测值,
Figure PCTCN2018078492-appb-000190
表示第j个频点上的双差伪距多路径效应,
Figure PCTCN2018078492-appb-000191
表示第j个频点上的双差伪距观测噪声。
Where the superscript r represents the reference satellite,
Figure PCTCN2018078492-appb-000182
a double-difference carrier observation indicating the j-th frequency point,
Figure PCTCN2018078492-appb-000183
Indicates the star distance of the double-difference station,
Figure PCTCN2018078492-appb-000184
Indicates the double-difference full-circumference ambiguity at the jth frequency point,
Figure PCTCN2018078492-appb-000185
Indicates double-difference tropospheric delay,
Figure PCTCN2018078492-appb-000186
Indicates the doubled ionospheric delay at the first frequency point,
Figure PCTCN2018078492-appb-000187
Means the double-difference carrier multipath effect in meters on the jth frequency point,
Figure PCTCN2018078492-appb-000188
Indicates the double-difference carrier observation noise in meters on the jth frequency point,
Figure PCTCN2018078492-appb-000189
Indicates the double-difference pseudorange observation at the jth frequency point,
Figure PCTCN2018078492-appb-000190
Representing the double-difference pseudorange multipath effect at the jth frequency point,
Figure PCTCN2018078492-appb-000191
Indicates the double-difference pseudorange observation noise at the jth frequency point.
步骤23,根据步骤22形成的双差观测值组合成双差宽巷组合观测值,解算宽巷组合模糊度。In step 23, the double-difference observations formed in step 22 are combined into a double-difference wide lane combined observation value to solve the wide lane combined ambiguity.
采用MW组合解算宽巷组合模糊度,则解算方程为:Using the MW combination to solve the wide-altitude combination ambiguity, the solution equation is:
Figure PCTCN2018078492-appb-000192
Figure PCTCN2018078492-appb-000192
式中:
Figure PCTCN2018078492-appb-000193
Figure PCTCN2018078492-appb-000194
表示双差宽巷组合观测值,
Figure PCTCN2018078492-appb-000195
表示宽巷组合模糊度,λ WL表示宽巷波长。
In the formula:
Figure PCTCN2018078492-appb-000193
Figure PCTCN2018078492-appb-000194
Indicates the combined observation of double-difference wide lanes,
Figure PCTCN2018078492-appb-000195
Indicates the wide lane combination ambiguity, and λ WL represents the wide lane wavelength.
因使用MW组合解算宽巷模糊度,仅受载波与伪距观测噪声影响(忽略多路径),而观测噪声服从高斯白噪声分布,因此可对宽巷组合模糊度采用多历元平滑四舍五入取整,具体公式如下:Because the MW combination is used to solve the wide lane ambiguity, it is only affected by the carrier and pseudorange observation noise (ignoring multipath), and the observation noise obeys the Gaussian white noise distribution. Therefore, the multi-epoch smoothing rounding can be adopted for the wide lane combination ambiguity. The specific formula is as follows:
Figure PCTCN2018078492-appb-000196
Figure PCTCN2018078492-appb-000196
式中:
Figure PCTCN2018078492-appb-000197
表示第i个观测历元解算得到的宽巷组合模糊度浮点解,z表示观测历元总数,round表示四舍五入取整算子。
In the formula:
Figure PCTCN2018078492-appb-000197
It represents the wide-altitude combined ambiguity floating-point solution obtained by the i-th observation epoch, z represents the total number of observation epochs, and round represents the rounding-and-rounding operator.
步骤24,采用无电离层组合,构建窄巷滤波器,利用无电离层组合联合宽巷组合分离出基础模糊度
Figure PCTCN2018078492-appb-000198
Figure PCTCN2018078492-appb-000199
包括以下步骤:
Step 24, using a combination of no ionosphere, constructing a narrow lane filter, and separating the base ambiguity by using a combination of no ionosphere and wide lane
Figure PCTCN2018078492-appb-000198
versus
Figure PCTCN2018078492-appb-000199
Includes the following steps:
步骤241,形成双差无电离层组合观测值:In step 241, a combined observation of the double-difference ionosphere is formed:
Figure PCTCN2018078492-appb-000200
Figure PCTCN2018078492-appb-000200
Figure PCTCN2018078492-appb-000201
Figure PCTCN2018078492-appb-000201
Figure PCTCN2018078492-appb-000202
Figure PCTCN2018078492-appb-000202
式中:
Figure PCTCN2018078492-appb-000203
表示双差无电离层组合观测值,
Figure PCTCN2018078492-appb-000204
表示无电离层组合模糊度,此模糊度不具有整数特性,此组合消除了电离层延迟一阶项的影响,λ NL=c/(f 1+f 2)。
In the formula:
Figure PCTCN2018078492-appb-000203
Represents a double-difference ionospheric combined observation,
Figure PCTCN2018078492-appb-000204
Indicates that there is no ionospheric combined ambiguity, which does not have an integer characteristic. This combination eliminates the influence of the first-order term of the ionospheric delay, λ NL = c / (f 1 + f 2 ).
步骤242,构建第一卡尔曼滤波器:Step 242, constructing a first Kalman filter:
Figure PCTCN2018078492-appb-000205
Figure PCTCN2018078492-appb-000205
Figure PCTCN2018078492-appb-000206
Figure PCTCN2018078492-appb-000206
式中,E(g)表示求数学期望,Cov(g)表示求协方差,
Figure PCTCN2018078492-appb-000207
Figure PCTCN2018078492-appb-000208
分别表示第i历元和第i-1历元的状态向量;
Figure PCTCN2018078492-appb-000209
表示状态转移矩阵;
Figure PCTCN2018078492-appb-000210
表示动态噪声向量,
Figure PCTCN2018078492-appb-000211
表示动态噪声协方差矩阵;
Figure PCTCN2018078492-appb-000212
表示第i历元观测向量,
Figure PCTCN2018078492-appb-000213
表示设计矩阵,
Figure PCTCN2018078492-appb-000214
表示第i历元观测噪声向量;
Figure PCTCN2018078492-appb-000215
表示为第i历元观测噪声协方差阵,
Figure PCTCN2018078492-appb-000216
表示第i历元状态向量协方差阵,
Figure PCTCN2018078492-appb-000217
表示状态向量预测协方差阵,
Figure PCTCN2018078492-appb-000218
表示第i历元状态向量方差-协方差阵,
Figure PCTCN2018078492-appb-000219
表示增益矩阵,
Figure PCTCN2018078492-appb-000220
表示单位矩阵。
Where E(g) represents the mathematical expectation and Cov(g) represents the covariance.
Figure PCTCN2018078492-appb-000207
Figure PCTCN2018078492-appb-000208
State vectors representing the i-th epoch and the i-th epoch, respectively;
Figure PCTCN2018078492-appb-000209
Representing a state transition matrix;
Figure PCTCN2018078492-appb-000210
Represents a dynamic noise vector,
Figure PCTCN2018078492-appb-000211
Representing a dynamic noise covariance matrix;
Figure PCTCN2018078492-appb-000212
Represents the i-th eigen observation vector,
Figure PCTCN2018078492-appb-000213
Representing the design matrix,
Figure PCTCN2018078492-appb-000214
Representing the i-th eigen observation noise vector;
Figure PCTCN2018078492-appb-000215
Expressed as the i-th epoch observed noise covariance matrix,
Figure PCTCN2018078492-appb-000216
Representing the i-th epoch state vector covariance matrix,
Figure PCTCN2018078492-appb-000217
Representing a state vector prediction covariance matrix,
Figure PCTCN2018078492-appb-000218
Representing the i-th epoch state vector variance-covariance matrix,
Figure PCTCN2018078492-appb-000219
Representing the gain matrix,
Figure PCTCN2018078492-appb-000220
Represents the identity matrix.
设在第i历元,基准站k与基准站y有n颗GPS共视卫星与g颗BDS共视卫星,其中,第n颗GPS卫星与第g颗BDS卫星为各系统的参考星,待估参数包括双差整周模糊度与基线相对天顶对流层湿延迟,其滤波模型待估参数向量、观测值向量及设计矩阵表示为:Based on the i-th epoch, the base station k and the reference station y have n GPS satellites and g BDS satellites, wherein the nth GPS satellite and the g-th BDS satellite are reference stars of each system. The estimation parameters include double-difference ambiguity and baseline relative zenith tropospheric wet delay. The filter model to be estimated parameter vector, observation vector and design matrix are expressed as:
Figure PCTCN2018078492-appb-000221
Figure PCTCN2018078492-appb-000221
其中:among them:
Figure PCTCN2018078492-appb-000222
Figure PCTCN2018078492-appb-000222
Figure PCTCN2018078492-appb-000223
Figure PCTCN2018078492-appb-000223
Figure PCTCN2018078492-appb-000224
Figure PCTCN2018078492-appb-000224
式中:
Figure PCTCN2018078492-appb-000225
表示n+g-1维的状态向量(待估参数向量),包含1个相对天顶对流层湿延迟参数RZTD与n+g-2维双差整周模糊度参数向量
Figure PCTCN2018078492-appb-000226
Figure PCTCN2018078492-appb-000227
表示n+g-2维的双差载波观测值向量,
Figure PCTCN2018078492-appb-000228
表示GPS双差载波观测值,o=1,2,L,n-1,
Figure PCTCN2018078492-appb-000229
表示GPS窄巷波长,
Figure PCTCN2018078492-appb-000230
表示GPS第1个频点的波长,
Figure PCTCN2018078492-appb-000231
表示GPS双差无电离层组合载波观测值,
Figure PCTCN2018078492-appb-000232
表示GPS双差站星距,
Figure PCTCN2018078492-appb-000233
表示GPS卫星双差对流层干延迟,
Figure PCTCN2018078492-appb-000234
表示GPS双差宽巷整周模糊度,
Figure PCTCN2018078492-appb-000235
表示GPS第1个频点的频率值,
Figure PCTCN2018078492-appb-000236
表示GPS第2个频点的频率值,
Figure PCTCN2018078492-appb-000237
表示BDS双差载波观测值,s=1,2,L,g-1,
Figure PCTCN2018078492-appb-000238
表示BDS窄巷波长,
Figure PCTCN2018078492-appb-000239
表示BDS第一个频点的波长,
Figure PCTCN2018078492-appb-000240
表示BDS双差无电离层组合载波观测值,
Figure PCTCN2018078492-appb-000241
表示BDS双差站星距,
Figure PCTCN2018078492-appb-000242
表示BDS卫星双差对流层干延迟,
Figure PCTCN2018078492-appb-000243
表示BDS双差宽巷整周模糊度,
Figure PCTCN2018078492-appb-000244
表示BDS第1个频点的频率值,
Figure PCTCN2018078492-appb-000245
表示BDS第2个频点的频率值,
Figure PCTCN2018078492-appb-000246
表示基准站k上GPS 系统卫星o的对流层映射函数,
Figure PCTCN2018078492-appb-000247
表示基准站y上GPS系统参考卫星n的对流层映射函数,
Figure PCTCN2018078492-appb-000248
表示基准站k上BDS系统卫星s的对流层映射函数,
Figure PCTCN2018078492-appb-000249
表示基准站y上BDS系统参考卫星g的对流层映射函数,
Figure PCTCN2018078492-appb-000250
表示(n+g-2)×(n+g-1)维的设计矩阵。
In the formula:
Figure PCTCN2018078492-appb-000225
A state vector representing the n+g-1 dimension (the parameter vector to be estimated), including a relative zenith tropospheric wet delay parameter RZTD and n+g-2 dimensional double difference whole-circumference ambiguity parameter vector
Figure PCTCN2018078492-appb-000226
Figure PCTCN2018078492-appb-000227
a vector of double-difference carrier observations representing n+g-2 dimensions,
Figure PCTCN2018078492-appb-000228
Indicates GPS double-difference carrier observations, o=1, 2, L, n-1,
Figure PCTCN2018078492-appb-000229
Indicates the GPS narrow lane wavelength,
Figure PCTCN2018078492-appb-000230
Indicates the wavelength of the first frequency point of GPS,
Figure PCTCN2018078492-appb-000231
Indicates the GPS double-difference ionosphere-free combined carrier observation,
Figure PCTCN2018078492-appb-000232
Indicates the GPS star distance,
Figure PCTCN2018078492-appb-000233
Represents the GPS satellite double-difference tropospheric dry delay,
Figure PCTCN2018078492-appb-000234
Indicates the full-circumference ambiguity of the GPS double-difference wide lane
Figure PCTCN2018078492-appb-000235
Indicates the frequency value of the first frequency point of GPS.
Figure PCTCN2018078492-appb-000236
Indicates the frequency value of the second frequency point of GPS.
Figure PCTCN2018078492-appb-000237
Indicates the BDS double-difference carrier observation, s = 1, 2, L, g-1,
Figure PCTCN2018078492-appb-000238
Indicates the BDS narrow lane wavelength,
Figure PCTCN2018078492-appb-000239
Indicates the wavelength of the first frequency of the BDS,
Figure PCTCN2018078492-appb-000240
Indicates the BDS double-difference ionosphere-free combined carrier observation,
Figure PCTCN2018078492-appb-000241
Indicates the star distance of the BDS double-difference station,
Figure PCTCN2018078492-appb-000242
Indicates the double-difference tropospheric dry delay of the BDS satellite,
Figure PCTCN2018078492-appb-000243
Indicates the full-circumference ambiguity of the BDS double-difference wide lane,
Figure PCTCN2018078492-appb-000244
Indicates the frequency value of the first frequency point of the BDS.
Figure PCTCN2018078492-appb-000245
Indicates the frequency value of the 2nd frequency point of the BDS.
Figure PCTCN2018078492-appb-000246
Indicates the tropospheric mapping function of the GPS system satellite o on the base station k,
Figure PCTCN2018078492-appb-000247
Indicates the tropospheric mapping function of the GPS system reference satellite n on the base station y,
Figure PCTCN2018078492-appb-000248
Indicates the tropospheric mapping function of the BDS system satellite s on the base station k,
Figure PCTCN2018078492-appb-000249
Indicates the tropospheric mapping function of the reference satellite g of the BDS system on the base station y,
Figure PCTCN2018078492-appb-000250
A design matrix representing (n + g - 2) × (n + g - 1) dimensions.
步骤243,根据步骤242建立的第一卡尔曼滤波器进行滤波,并解算基础载波模糊度向量参数。Step 243: Filter according to the first Kalman filter established in step 242, and solve the basic carrier ambiguity vector parameter.
从滤波器中提取出模糊度参数向量浮点解
Figure PCTCN2018078492-appb-000251
与方差-协方差阵利用lambda算法进行搜索,可获得模糊度参数向量固定解
Figure PCTCN2018078492-appb-000252
(此处获得的模糊度是第一个频点上的整周模糊度)。
Extracting the ambiguity parameter vector floating point solution from the filter
Figure PCTCN2018078492-appb-000251
And the variance-covariance matrix is searched by the lambda algorithm, and the ambiguity parameter vector fixed solution can be obtained.
Figure PCTCN2018078492-appb-000252
(The ambiguity obtained here is the full-circumference ambiguity at the first frequency point).
对于观测噪声,不同高度角卫星采用基于卫星高度角的定权方式,天顶对流层湿延迟采用随机游走,接收机观测噪声服从高斯白噪声分布,模糊度确定为时不变参数。For observation noise, satellites with different elevation angles adopt a weighting method based on satellite elevation angle. The zenith tropospheric wet delay adopts random walk. The receiver observation noise obeys Gaussian white noise distribution, and the ambiguity is determined as time-invariant parameter.
获得第1个频点双差整周模糊度
Figure PCTCN2018078492-appb-000253
(BDS)与
Figure PCTCN2018078492-appb-000254
(GPS)后,可得到第2个频点的双差整周模糊度
Figure PCTCN2018078492-appb-000255
Figure PCTCN2018078492-appb-000256
Figure PCTCN2018078492-appb-000257
Figure PCTCN2018078492-appb-000258
Obtain the first frequency double-difference full-circumference ambiguity
Figure PCTCN2018078492-appb-000253
(BDS) and
Figure PCTCN2018078492-appb-000254
After (GPS), the double-difference ambiguity of the second frequency point can be obtained.
Figure PCTCN2018078492-appb-000255
versus
Figure PCTCN2018078492-appb-000256
Figure PCTCN2018078492-appb-000257
Figure PCTCN2018078492-appb-000258
步骤25,根据步骤24的结果,生成基线双差大气误差:Step 25, according to the result of step 24, generating a baseline double difference atmospheric error:
Figure PCTCN2018078492-appb-000259
Figure PCTCN2018078492-appb-000259
Figure PCTCN2018078492-appb-000260
Figure PCTCN2018078492-appb-000260
Figure PCTCN2018078492-appb-000261
Figure PCTCN2018078492-appb-000261
Figure PCTCN2018078492-appb-000262
Figure PCTCN2018078492-appb-000262
式中,
Figure PCTCN2018078492-appb-000263
Figure PCTCN2018078492-appb-000264
分别表示GPS与BDS双差对流层延迟,
Figure PCTCN2018078492-appb-000265
Figure PCTCN2018078492-appb-000266
分别表示GPS与BDS第一个频点双差载波观测值,
Figure PCTCN2018078492-appb-000267
Figure PCTCN2018078492-appb-000268
分别表示GPS与BDS第二个频点双差载波观测值,
Figure PCTCN2018078492-appb-000269
Figure PCTCN2018078492-appb-000270
分别表示GPS与BDS第1个频点双差电离层延迟。
In the formula,
Figure PCTCN2018078492-appb-000263
versus
Figure PCTCN2018078492-appb-000264
Representing the double-difference tropospheric delay between GPS and BDS,
Figure PCTCN2018078492-appb-000265
versus
Figure PCTCN2018078492-appb-000266
Representing the GPS and BDS first frequency double-difference carrier observations,
Figure PCTCN2018078492-appb-000267
versus
Figure PCTCN2018078492-appb-000268
Representing the second frequency difference observation of GPS and BDS respectively,
Figure PCTCN2018078492-appb-000269
versus
Figure PCTCN2018078492-appb-000270
It indicates the 1st frequency doubled ionospheric delay of GPS and BDS respectively.
步骤3,将生成的基线大气误差赋给相应的星型网络基线,必要时进行基线方向变换。以星型网络为单元统一参考星并进行参考星变换,生成星型网元共视卫星站间单差大气误差。In step 3, the generated baseline atmospheric error is assigned to the corresponding star network baseline, and the baseline direction transformation is performed if necessary. The star-shaped network is used as a unit to unify the reference star and carry out the reference star transformation to generate a single-difference atmospheric error between the star-shaped network elements and the satellite stations.
所述步骤3中,生成星型网络站间单差大气误差包括以下步骤:In the step 3, generating a single-difference atmospheric error between the star network stations includes the following steps:
步骤41,以星型网络主站与辅站组成基线,在整网基线列表中寻找由相同基准站组成的基线,若两条基线方向相反,则需进行基线换向。由此获得星型网络各条基线大气误差。In step 41, a star network primary station and a secondary station form a baseline, and a baseline consisting of the same base station is searched in the entire network baseline list. If the two baseline directions are opposite, a baseline commutation is required. This results in a baseline atmospheric error for the star network.
步骤42,检查星型网元各条基线参考星是否一致,若不一致,则选择统一参考星并对大气误差进行参考星变换。Step 42: Check whether the baseline reference stars of the star network elements are consistent. If they are inconsistent, select a unified reference star and perform a reference star transformation on the atmospheric error.
步骤43,生成星型网元站间单差大气误差。视参考星站间单差大气误差为0,则其他卫星的站间单差大气误差值等于双差大气误差。In step 43, a single difference atmospheric error between the star network elements is generated. If the single-difference atmospheric error between the reference satellite stations is 0, the inter-station single-difference atmospheric error value of other satellites is equal to the double-difference atmospheric error.
步骤44,提取星型网元所有基线均共视的卫星,生成星型网元共视卫星站间单差大气误差。Step 44: Extract all the satellites of the star network element that are common to each baseline, and generate a single-difference atmospheric error between the satellite stations of the star-shaped network element.
步骤4,以星型网元为单元,对星型网元的每条基线共视卫星站间单差大气误差、所有基准站坐标及主站观测值进行编码,并利用UDP协议进行广播(广播模式可通过地面设备、航空飞机或卫星等设备进行播发)或使用双向通讯(由用户上传概略位置信息,根据用户位置通过Ntrip协议或TCP/IP仅向用户播发用户所在星型网元的数据)。Step 4: Using the star network element as a unit, encoding the single-difference atmospheric error, all base station coordinates, and the observation value of the primary station for each baseline satellite station of the star network element, and broadcasting by using the UDP protocol (broadcasting The mode can be broadcasted by equipment such as ground equipment, aviation aircraft or satellite) or two-way communication (the user can upload the approximate location information, and only broadcast the data of the user's star network element to the user through Ntrip protocol or TCP/IP according to the user's location) .
当用户使用双向通讯时,仅向该用户播发其所在网元的差分数据,以广播模式播发的数据仍然不间断地向外播发。When the user uses two-way communication, only the differential data of the network element in which the user is located is broadcast to the user, and the data broadcasted in the broadcast mode is still advertised without interruption.
以2015年10月19日发布,2015年11月1日开始实施的《北斗/全球卫星导航系统(GNSS)接收机差分数据格式(二)》为标准进行数据编码,包括以下电文:The Beidou/Global Satellite Navigation System (GNSS) Receiver Differential Data Format (II), which was released on October 19, 2015 and implemented on November 1, 2015, is encoded as a standard, including the following messages:
电文号Message number 电文作用描述Description of the role of the message 备注Remarks
11241124 BDS MSM4观测值BDS MSM4 observations  
10501050 BDS电离层改正值站间单差BDS ionospheric correction value single difference between stations  
10511051 BDS几何改正值站间单差BDS geometric correction value single difference between stations 本发明中所述对流层延迟Tropospheric delay in the present invention
10741074 GPS MSM4观测值GPS MSM4 observations  
10151015 GPS电离层改正值站间单差GPS ionospheric correction value single difference between stations  
10161016 GPS几何改正值站间单差GPS geometric correction value single difference between stations 本发明中所述对流层延迟Tropospheric delay in the present invention
10061006 主站ECEF坐标信息Master station ECEF coordinate information  
10331033 主站接收机与天线信息说明Master station receiver and antenna information  
10141014 辅站坐标信息Secondary station coordinate information 辅站与主站大地坐标差Coordinate difference between the auxiliary station and the main station
10131013 电文播发的状态和频度信息Status and frequency information of message broadcast  
步骤5,用户实时接收数据并判断其所在网元,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7。其中,当用户对接收到 的数据解码并计算流动站到每个主站的直线距离,以距离最小的主站所代表的网元作为流动站所在网元。Step 5: The user receives the data in real time and judges the network element where it is located, and interpolates the difference between the station and the primary station according to the difference data of the network element in which the network element is located, and corrects the error to the observation value of the primary station, and proceeds to step 7. Wherein, when the user decodes the received data and calculates the linear distance of the rover to each primary station, the network element represented by the primary station with the smallest distance is used as the network element where the mobile station is located.
步骤6,用户实时接收数据,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7。In step 6, the user receives the data in real time, and interpolates the difference between the station and the main station according to the differential data of the network element in which the network element is located, and corrects the error to the observation value of the primary station, and proceeds to step 7.
步骤5或6中,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,包括以下步骤:In step 5 or 6, according to the differential data of the network element in which the network element is interpolated, the single-difference atmospheric error between the station and the primary station is obtained, and corrected to the observation value of the primary station, including the following steps:
步骤①,利用线性内插算法进行用户大气误差内插,则用户与主站站间单差大气误差计算如下:Step 1. Using the linear interpolation algorithm to interpolate the user's atmospheric error, the single-difference atmospheric error between the user and the primary station is calculated as follows:
Figure PCTCN2018078492-appb-000271
Figure PCTCN2018078492-appb-000271
Figure PCTCN2018078492-appb-000272
Figure PCTCN2018078492-appb-000272
式中,下标m表示主站,u表示用户,α 123表示对流层内插系数,β 12表示电离层内插系数,w表示辅站数目,
Figure PCTCN2018078492-appb-000273
表示卫星s的站间单差对流层延迟,Δx m,u,Δy m,u,Δh m,u分别表示主站与用户的坐标差,
Figure PCTCN2018078492-appb-000274
表示站间单差电离层延迟;
Where subscript m denotes the primary station, u denotes the user, α 1 , α 2 , α 3 denote the tropospheric interpolation coefficient, β 1 , β 2 denote the ionospheric interpolation coefficient, and w denote the number of secondary stations,
Figure PCTCN2018078492-appb-000273
Indicates the inter-station single-difference tropospheric delay of the satellite s, Δx m, u , Δy m, u , Δh m, u represent the coordinate difference between the primary station and the user , respectively.
Figure PCTCN2018078492-appb-000274
Indicates the single-difference ionospheric delay between stations;
对流层内插系数与电离层内插系数计算方法如下:The tropospheric interpolation coefficients and ionospheric interpolation coefficients are calculated as follows:
Figure PCTCN2018078492-appb-000275
Figure PCTCN2018078492-appb-000275
Figure PCTCN2018078492-appb-000276
Figure PCTCN2018078492-appb-000276
Figure PCTCN2018078492-appb-000277
Figure PCTCN2018078492-appb-000277
Figure PCTCN2018078492-appb-000278
Figure PCTCN2018078492-appb-000278
Figure PCTCN2018078492-appb-000279
Figure PCTCN2018078492-appb-000279
式中:Δx m,t,Δy m,t,Δh m,t表示主站与辅站坐标差,t=1,2,L,w; Where: Δx m,t , Δy m,t , Δh m,t represents the coordinate difference between the primary station and the secondary station, t=1, 2, L, w;
步骤②,将内插得到的大气误差值修正至主站观测值,伪距与载波观测值分别如下:In step 2, the atmospheric error value obtained by the interpolation is corrected to the observation value of the primary station, and the pseudorange and the carrier observation value are respectively as follows:
Figure PCTCN2018078492-appb-000280
Figure PCTCN2018078492-appb-000280
Figure PCTCN2018078492-appb-000281
Figure PCTCN2018078492-appb-000281
式中:
Figure PCTCN2018078492-appb-000282
分别表示修正了大气误差后的卫星s第j个频点在主站上的伪距与载波观测值,
Figure PCTCN2018078492-appb-000283
分别表示卫星s第j个频点在主站上的原始伪距与载波观测值,
Figure PCTCN2018078492-appb-000284
表示通过内插得到的卫星s的站间对流层延迟,
Figure PCTCN2018078492-appb-000285
表示通过内插得到的卫星s的站间电离层延迟。
In the formula:
Figure PCTCN2018078492-appb-000282
It shows the pseudorange and carrier observation values of the jth frequency point of the satellite s after the correction of the atmospheric error on the primary station.
Figure PCTCN2018078492-appb-000283
Representing the original pseudorange and carrier observations of the jth frequency point of the satellite s on the primary station,
Figure PCTCN2018078492-appb-000284
Indicates the inter-station tropospheric delay of the satellite s obtained by interpolation,
Figure PCTCN2018078492-appb-000285
Indicates the inter-site ionospheric delay of the satellite s obtained by interpolation.
步骤7,用户利用经步骤5修正后的主站观测值与用户观测值(由用户接收机自身接收到)组成双差观测值,构建包含用户位置参数及模糊度参数的第二卡尔曼滤波器,进行基线解算。In step 7, the user constructs a double-cavity observation using the observation of the primary station corrected by step 5 and the user observation (received by the user receiver itself) to construct a second Kalman filter including the user position parameter and the ambiguity parameter. , perform a baseline solution.
步骤7中基线解算包括以下步骤:The baseline solution in step 7 includes the following steps:
步骤71,形成双差观测方程,伪距和载波双差观测方程可表示为:In step 71, a double difference observation equation is formed, and the pseudorange and carrier double difference observation equation can be expressed as:
Figure PCTCN2018078492-appb-000286
Figure PCTCN2018078492-appb-000286
Figure PCTCN2018078492-appb-000287
Figure PCTCN2018078492-appb-000287
Figure PCTCN2018078492-appb-000288
Figure PCTCN2018078492-appb-000288
Figure PCTCN2018078492-appb-000289
Figure PCTCN2018078492-appb-000289
式中,
Figure PCTCN2018078492-appb-000290
表示GPS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000291
表示GPS卫星双差站星距,
Figure PCTCN2018078492-appb-000292
表示GPS卫星双差伪距多路径效应,
Figure PCTCN2018078492-appb-000293
表示GPS卫星双差伪距观测噪声,
Figure PCTCN2018078492-appb-000294
表示GPS卫星双差载波观测值,λ G表示GPS观测值对应频点的波长,
Figure PCTCN2018078492-appb-000295
表示GPS卫星双差整周模糊度,
Figure PCTCN2018078492-appb-000296
表示以周为单位的GPS卫星双差载波多路径效应,
Figure PCTCN2018078492-appb-000297
表示以周为单位的GPS卫星双差载波观测噪声,
Figure PCTCN2018078492-appb-000298
表示BDS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000299
表示BDS卫星双差站星距,
Figure PCTCN2018078492-appb-000300
表示BDS卫星双差伪距多路径效应,
Figure PCTCN2018078492-appb-000301
表示BDS卫星双差伪距观测噪声,
Figure PCTCN2018078492-appb-000302
表示BDS卫星双差载波观测值,λ C表示BDS观测值对应频点的波长,
Figure PCTCN2018078492-appb-000303
表示BDS卫星双差整周模糊度,
Figure PCTCN2018078492-appb-000304
表示以周为单位的BDS卫星双差载波多路径效应,
Figure PCTCN2018078492-appb-000305
表示以周为单位的BDS卫星双差载波观测噪声。由于已经在主站观测值上大气误差做了改正,因此上述双差观测方程中忽略了大气误差。
In the formula,
Figure PCTCN2018078492-appb-000290
Representing GPS satellite double-difference pseudorange observations,
Figure PCTCN2018078492-appb-000291
Indicates the satellite distance of the GPS satellite double-difference station,
Figure PCTCN2018078492-appb-000292
Representing GPS satellite double-difference pseudorange multipath effect,
Figure PCTCN2018078492-appb-000293
Representing GPS satellite double-difference pseudorange observation noise,
Figure PCTCN2018078492-appb-000294
Indicates the GPS satellite double-difference carrier observation, and λ G represents the wavelength of the GPS observation corresponding to the frequency point.
Figure PCTCN2018078492-appb-000295
Represents the GPS satellite double-difference ambiguity,
Figure PCTCN2018078492-appb-000296
Represents the GPS satellite double-difference carrier multipath effect in weeks,
Figure PCTCN2018078492-appb-000297
Representing GPS satellite double-difference carrier observation noise in weeks,
Figure PCTCN2018078492-appb-000298
Indicates the double-difference pseudorange observation of the BDS satellite,
Figure PCTCN2018078492-appb-000299
Indicates the star distance of the BDS satellite double-difference station,
Figure PCTCN2018078492-appb-000300
Representing the double-signal pseudorange multipath effect of BDS satellites,
Figure PCTCN2018078492-appb-000301
Representing BDS satellite double-difference pseudorange observation noise,
Figure PCTCN2018078492-appb-000302
Indicates the BDS satellite double-difference carrier observation, and λ C represents the wavelength of the BDS observation corresponding to the frequency point.
Figure PCTCN2018078492-appb-000303
Indicates the double-difference ambiguity of the BDS satellite,
Figure PCTCN2018078492-appb-000304
Representing the double-signal carrier multipath effect of the BDS satellite in weeks,
Figure PCTCN2018078492-appb-000305
Indicates the BDS satellite double-difference carrier observation noise in weeks. Since the atmospheric error has been corrected at the observations of the primary station, the atmospheric error is ignored in the above-mentioned double-difference observation equation.
步骤72,构建卡尔曼滤波器,包括以下步骤:Step 72, constructing a Kalman filter, comprising the following steps:
设在第i历元,用户与星型网有n颗GPS共视卫星和g颗BDS共视卫星,其中第n颗GPS卫星与第g颗BDS卫星分别为各系统的参考星,联合所有卫星L1载波和P1伪距观测数据,其滤波模型待估参数矩阵
Figure PCTCN2018078492-appb-000306
观测值矩阵
Figure PCTCN2018078492-appb-000307
及设计矩阵
Figure PCTCN2018078492-appb-000308
表示为:
Based on the i-th epoch, the user and the star network have n GPS satellites and g BDS satellites, of which the nth GPS satellite and the gth BDS satellite are reference stars of each system, and all satellites are combined. L1 carrier and P1 pseudorange observation data, filter model to be estimated parameter matrix
Figure PCTCN2018078492-appb-000306
Observation matrix
Figure PCTCN2018078492-appb-000307
Design matrix
Figure PCTCN2018078492-appb-000308
Expressed as:
Figure PCTCN2018078492-appb-000309
Figure PCTCN2018078492-appb-000309
Figure PCTCN2018078492-appb-000310
Figure PCTCN2018078492-appb-000310
式中,
Figure PCTCN2018078492-appb-000311
表示n+g+1维的待估参数向量,包含3维位置参数向量
Figure PCTCN2018078492-appb-000312
与n+g-2维双差整周模糊度参数向量
Figure PCTCN2018078492-appb-000313
表示2(n+g-2)维双差观测值向量,包括伪距与载波观测值;
Figure PCTCN2018078492-appb-000314
表示2(n+g-2)×(n+g+1)维设计矩阵,其中l o,n,G,p o,n,G,q o,n,G表示GPS卫星方向余弦(上标o=1,2L,n-1),l s,g,C,p s,g,C,q s,g,C(上标s=1,2L,t-1)表示BDS卫星方向余弦,
Figure PCTCN2018078492-appb-000315
表示以米为单位的GPS卫星双差载波观测值,
Figure PCTCN2018078492-appb-000316
表示GPS卫星双差伪距观测值,
Figure PCTCN2018078492-appb-000317
表示GPS卫星双差站星距,
Figure PCTCN2018078492-appb-000318
表示BDS卫星双差站星距,
Figure PCTCN2018078492-appb-000319
表示以米为单位的BDS卫星双差载波观测值,
Figure PCTCN2018078492-appb-000320
表示BDS卫星双差伪距观测值。将上述参数赋值并带入卡尔曼滤波器中逐历元计算,然后提取浮点模糊度向量与其方差-协方差阵,利用lambda算法搜索即可获得模糊度固定解。
In the formula,
Figure PCTCN2018078492-appb-000311
An estimated parameter vector representing n+g+1 dimensions, including a 3-dimensional positional parameter vector
Figure PCTCN2018078492-appb-000312
Double-difference whole-circumference ambiguity parameter vector with n+g-2
Figure PCTCN2018078492-appb-000313
Representing a 2(n+g-2) dimensional double difference observation vector, including pseudorange and carrier observations;
Figure PCTCN2018078492-appb-000314
Represents a 2(n+g-2)×(n+g+1) dimensional design matrix, where l o,n,G ,p o,n,G ,q o,n,G represent the cosine of the GPS satellite direction (superscript o=1,2L,n-1),l s,g,C ,p s,g,C ,q s,g,C (superscript s=1,2L,t-1) represent the cosine of the BDS satellite direction,
Figure PCTCN2018078492-appb-000315
Means the GPS satellite double-difference carrier observation in meters,
Figure PCTCN2018078492-appb-000316
Representing GPS satellite double-difference pseudorange observations,
Figure PCTCN2018078492-appb-000317
Indicates the satellite distance of the GPS satellite double-difference station,
Figure PCTCN2018078492-appb-000318
Indicates the star distance of the BDS satellite double-difference station,
Figure PCTCN2018078492-appb-000319
Indicates the BDS satellite double-difference carrier observations in meters,
Figure PCTCN2018078492-appb-000320
Indicates the double-difference pseudorange observation of the BDS satellite. The above parameters are assigned and brought into the Kalman filter to calculate by epoch, then the floating-point ambiguity vector and its variance-covariance matrix are extracted, and the ambiguity fixed solution can be obtained by searching with the lambda algorithm.
对于观测噪声,不同高度角卫星采用基于卫星高度角的定权方式,三维坐标参数采用随机游走,接收机观测噪声服从高斯白噪声分布,模糊度确定为时不变参数。For observation noise, the satellites with different elevation angles adopt the weighting method based on the satellite elevation angle. The three-dimensional coordinate parameters adopt random walk. The receiver observation noise obeys the Gaussian white noise distribution, and the ambiguity is determined as the time-invariant parameter.
步骤72,固定模糊度后,利用下式解得用户三维坐标固定解:Step 72, after fixing the ambiguity, using the following formula to solve the fixed solution of the user's three-dimensional coordinates:
Figure PCTCN2018078492-appb-000321
Figure PCTCN2018078492-appb-000321
其中,
Figure PCTCN2018078492-appb-000322
分别为三维坐标参数向量及浮点模糊度参数向量,
Figure PCTCN2018078492-appb-000323
为固定模糊度后的坐标参数向量,
Figure PCTCN2018078492-appb-000324
为固定模糊度参数向量,
Figure PCTCN2018078492-appb-000325
分别对应各参数滤波解协方差阵。在卡尔曼滤波模型的建立中,在辅站数目少于2的中长基线情况下,可通过设计宽巷、窄巷滤波模型,顾及对流层延迟及电离层,实现中长基线的滤波解算。
among them,
Figure PCTCN2018078492-appb-000322
Three-dimensional coordinate parameter vector and floating-point ambiguity parameter vector,
Figure PCTCN2018078492-appb-000323
The coordinate parameter vector after fixing the ambiguity,
Figure PCTCN2018078492-appb-000324
To fix the ambiguity parameter vector,
Figure PCTCN2018078492-appb-000325
Corresponding to each parameter filtering solution covariance matrix. In the establishment of the Kalman filter model, in the case of a medium-long baseline with a number of secondary stations less than 2, the filtering solution of the medium-long baseline can be realized by designing the wide lane and narrow lane filtering model, taking into account the tropospheric delay and the ionosphere.
网络RTK技术是高精度实时定位领域中使用最为广泛的技术之一。本方法在星型网络基础上,采用双差模式进行网络解算,模型简单,参数少。采用广播模式播发网络RTK差分改正数,同时兼顾双向通讯,真正实现了广播模式的网络RTK。支持从地面设备、航空飞机、卫星等设备进行差分数据广播。在大气误差处理方面,充分发挥了流动站作用,使得流动站可以使用更优化的算法。在基线解算方面,兼顾网络RTK与传统RTK模式,可以保证中心解算软件在未完成网络初始化的情况下,流动站使用主站原始观测值进行单基线解算。本发明既满足普通网络RTK用户,又兼顾特殊领域用户,如不能暴露用户坐标的军事领域,并且用户容量不受限制。广播模式下,差分数据既可通过地面设备播发,也可通过航空飞机或卫星进行播发。不存在VRS技术、FKP技术、MAC技术所存在的缺点。Network RTK technology is one of the most widely used technologies in the field of high precision real-time positioning. Based on the star network, the method uses the double difference mode for network solution, and the model is simple and the parameters are few. The broadcast mode RTK differential correction number is used in the broadcast mode, and the two-way communication is taken into consideration, and the network RTK of the broadcast mode is truly realized. Support differential data broadcasting from ground equipment, aviation aircraft, satellite and other equipment. In the aspect of atmospheric error processing, the role of the rover is fully utilized, so that the rover can use a more optimized algorithm. In terms of baseline solution, taking into account the network RTK and the traditional RTK mode, it can ensure that the central solution solver does not complete the network initialization, the rover uses the original observation of the primary station for single baseline solution. The invention satisfies both the ordinary network RTK users and the special domain users, such as the military field in which the user coordinates cannot be exposed, and the user capacity is not limited. In broadcast mode, differential data can be broadcast either by ground equipment or by air or satellite. There are no shortcomings of VRS technology, FKP technology, and MAC technology.
以上所述,仅为本发明中的具体实施方式,但本发明的保护范围并不局限于此,任何熟悉该技术的人在本发明所揭露的技术范围内,可理解想到的变换或替换,都应涵盖在本发明的包含范围之内,因此,本发明的保护范围应该以权利要求书的保护范围为准。The above is only the specific embodiment of the present invention, but the scope of the present invention is not limited thereto, and any person skilled in the art can understand the alteration or replacement within the scope of the technical scope of the present invention. The scope of the invention should be construed as being included in the scope of the invention.

Claims (8)

  1. 基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,包括以下具体步骤:The star network-based BDS/GPS broadcast network RTK algorithm is characterized by the following specific steps:
    步骤1,从数据库获取基准站坐标,利用Delaunay三角剖分算法生成Delaunay三角网,在三角网的基础上生成由若干个星型网元组成的可控制全区域的星型网络,其中,每个星型网元由一个主站与若干与之对应的辅站组成;Step 1: Obtain the base station coordinates from the database, use the Delaunay triangulation algorithm to generate the Delaunay triangulation, and generate a star-shaped network composed of several star network elements and control the whole region on the basis of the triangulation network, wherein each A star network element consists of a primary station and a number of secondary stations corresponding thereto;
    步骤2,实时获取基准站数据,以Delaunay三角网中的基线为单元形成双差观测值,构建第一卡尔曼滤波器,实时估计基线双差模糊度及天顶对流层湿延迟ZTD,然后生成每条基线的基线双差大气误差;Step 2: Obtain the base station data in real time, form a double-difference observation with the baseline in the Delaunay triangulation, construct a first Kalman filter, estimate the baseline double-difference ambiguity and the zenith tropospheric wet delay ZTD in real time, and then generate each Baseline double difference atmospheric error of the baseline;
    步骤3,将步骤2生成的基线双差大气误差赋给相应的星型网元基线,以星型网元为单元统一参考星,生成星型网元每条基线共视卫星站间单差大气误差;Step 3: Assign the baseline double-difference atmospheric error generated in step 2 to the corresponding star network element baseline, and use the star-shaped network element as a unit to unify the reference star, and generate a single-element atmosphere between each baseline satellite station of the star-shaped network element. error;
    步骤4,以星型网元为单元,对星型网元的每条基线共视卫星站间单差大气误差、所有基准站坐标及主站观测值进行编码,编码后的数据利用UDP协议进行广播或使用双向通讯进行播发,其中,UDP协议广播所有数据后进入步骤5;使用双向通讯时,首先由用户上传概略位置信息,然后中心软件根据用户位置通过Ntrip协议或TCP/IP仅向用户播发用户所在星型网元的数据,进入步骤6;Step 4: Using a star-shaped network element as a unit, encoding a single-difference atmospheric error, all base station coordinates, and a master station observation value of each baseline satellite station of the star network element, and the encoded data is performed by using a UDP protocol. Broadcast or use two-way communication for broadcast, in which UDP protocol broadcasts all data and then proceeds to step 5; when using two-way communication, firstly, the user uploads the approximate location information, and then the central software broadcasts only to the user according to the user's location through Ntrip protocol or TCP/IP. The data of the star network element where the user is located, proceeds to step 6;
    步骤5,用户实时接收数据并判断其所在网元,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7;Step 5, the user receives the data in real time and judges the network element where it is located, according to the differential data of the network element in which the network element is interpolated to obtain the single-difference atmospheric error between the station and the primary station, and corrects the observation value to the primary station, and proceeds to step 7;
    步骤6,用户实时接收数据,根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,进入步骤7;Step 6, the user receives the data in real time, according to the differential data of the network element, the inter-station single difference atmospheric error between the station and the main station is interpolated, and corrected to the observation value of the main station, and proceeds to step 7;
    步骤7,用户利用经步骤5或6修正后的主站观测值与用户观测值组成双差观测值,构建包含用户位置参数及模糊度参数的第二卡尔曼滤波器,进行基线解算。In step 7, the user constructs a double-difference observation value by using the corrected observation value of the primary station and the user observation value corrected by step 5 or 6, and constructs a second Kalman filter including the user position parameter and the ambiguity parameter to perform baseline solution.
  2. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤1包括以下步骤:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the step 1 comprises the following steps:
    步骤11,利用Delaunay三角剖分算法生成三角网;Step 11, generating a triangulation network by using a Delaunay triangulation algorithm;
    步骤12,提取三角网整网边界基准站与非边界基准站,其中,若与某基准站相连的所有三角形中以此基准站为顶点的内角的角度之和大于设定阈值,则该基准站为非边界基准站,否则为边界基准站;Step 12: extracting a triangulation network boundary reference station and a non-boundary reference station, wherein if the sum of the angles of the inner angles of the vertices of the base station in all the triangles connected to a reference station is greater than a set threshold, the base station a non-boundary base station, otherwise a boundary reference station;
    步骤13,初始化星型网元集合:以所有非边界基准站作为主站,与之相连的所有基准站作为相应的辅站;Step 13, initializing the star network element set: all the non-boundary base stations are used as the primary station, and all the base stations connected thereto are used as the corresponding auxiliary stations;
    步骤14,在边界基准站中寻找未参与星型网络组网的基准站集合;Step 14: Find a set of base stations that do not participate in the star network networking in the boundary reference station;
    步骤15,在未参与组网的基准站集合中选取与之相连的基准站数最多的基准站作为新的主站,与之连接的基准站作为相应的辅站,更新星型网络集合及未参与星型网络组网的基准 站集合;Step 15, selecting the base station with the largest number of base stations connected to it as the new primary station in the base station set not participating in the networking, and the base station connected thereto as the corresponding secondary station, updating the star network set and not a set of base stations participating in a star network network;
    步骤16,重复步骤15,直至未参与星型网络组网的基准站数为0。Step 16. Repeat step 15 until the number of base stations that are not participating in the star network networking is zero.
  3. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤2中包括以下步骤:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the step 2 includes the following steps:
    步骤21,基准站k接收到卫星s的伪距与载波观测信号,则载波与伪距观测方程表示为:Step 21: The base station k receives the pseudorange and carrier observation signals of the satellite s, and the carrier and pseudorange observation equations are expressed as:
    Figure PCTCN2018078492-appb-100001
    Figure PCTCN2018078492-appb-100001
    Figure PCTCN2018078492-appb-100002
    Figure PCTCN2018078492-appb-100002
    式中:
    Figure PCTCN2018078492-appb-100003
    表示基准站站k接收到的卫星s的第j个频点上以周为单位的载波观测值,j=1,2,
    Figure PCTCN2018078492-appb-100004
    表示基准站k到卫星s的站星距,
    Figure PCTCN2018078492-appb-100005
    表示基准站k接收到的卫星s的第j个频点上的整周模糊度,c表示光速,dT k表示基准站k的接收机钟差,dT s表示卫星s的卫星钟差,
    Figure PCTCN2018078492-appb-100006
    表示基准站k接收到的卫星s的对流层延迟,
    Figure PCTCN2018078492-appb-100007
    表示基准站k接收到的卫星s第1个频点上电离层延迟,
    Figure PCTCN2018078492-appb-100008
    f j表示卫星s对应的卫星系统第j个频点上的频率值,f 1表示卫星s对应的卫星系统第1个频点上的频率值,rel s表示卫星s的相对论效应,
    Figure PCTCN2018078492-appb-100009
    表示基准站k接收到的卫星s的第j个频点上以米为单位的载波多路径效应,
    Figure PCTCN2018078492-appb-100010
    表示基准站k第j个频点上以米为单位的接收机端载波偏差,
    Figure PCTCN2018078492-appb-100011
    表示卫星s上第j个频点上以米为单位的卫星端载波偏差,
    Figure PCTCN2018078492-appb-100012
    表示基准站k接收到的卫星s第j个频点上以米为单位的载波观测噪声,
    Figure PCTCN2018078492-appb-100013
    表示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测值,
    Figure PCTCN2018078492-appb-100014
    表示基准站k接收到的卫星的第j个频点上以米为单位的伪距多路径效应,
    Figure PCTCN2018078492-appb-100015
    表示基准站k第j个频点接收到的以米为单位的接收机端伪距偏差,
    Figure PCTCN2018078492-appb-100016
    表示卫星s第j个频点上卫星端以米为单位的伪距偏差,
    Figure PCTCN2018078492-appb-100017
    表示基准站k接收到的卫星s的第j个频点上以米为单位的伪距观测噪声,λ j表示卫星s对应的卫星系统第j个频点的波长;
    In the formula:
    Figure PCTCN2018078492-appb-100003
    Indicates the carrier observation value in weeks on the jth frequency point of the satellite s received by the base station k, j=1, 2,
    Figure PCTCN2018078492-appb-100004
    Indicates the station star distance from the base station k to the satellite s,
    Figure PCTCN2018078492-appb-100005
    Indicates the full-circumference ambiguity at the j-th frequency point of the satellite s received by the reference station k, c represents the speed of light, dT k represents the receiver clock difference of the reference station k, and dT s represents the satellite clock difference of the satellite s,
    Figure PCTCN2018078492-appb-100006
    Indicates the tropospheric delay of the satellite s received by the base station k,
    Figure PCTCN2018078492-appb-100007
    Indicates the ionospheric delay at the first frequency of the satellite s received by the base station k,
    Figure PCTCN2018078492-appb-100008
    f j represents the frequency value at the jth frequency point of the satellite system corresponding to the satellite s, f 1 represents the frequency value at the 1st frequency point of the satellite system corresponding to the satellite s , and rel s represents the relativistic effect of the satellite s,
    Figure PCTCN2018078492-appb-100009
    Means the carrier multipath effect in meters on the jth frequency of the satellite s received by the base station k,
    Figure PCTCN2018078492-appb-100010
    Indicates the receiver-side carrier deviation in meters of the j-th frequency point of the base station k,
    Figure PCTCN2018078492-appb-100011
    Indicates the satellite-side carrier deviation in meters on the j-th frequency point on the satellite s.
    Figure PCTCN2018078492-appb-100012
    Indicates the carrier observation noise in meters per unit j of the satellite s received by the base station k,
    Figure PCTCN2018078492-appb-100013
    Indicates the pseudo-range observation value in meters on the j-th frequency point of the satellite s received by the base station k,
    Figure PCTCN2018078492-appb-100014
    Represents the pseudorange multipath effect in meters at the jth frequency of the satellite received by the base station k,
    Figure PCTCN2018078492-appb-100015
    Indicates the receiver-side pseudorange deviation in meters per unit received by the jth frequency point of the reference station k,
    Figure PCTCN2018078492-appb-100016
    Indicates the pseudorange deviation of the satellite end in meters at the jth frequency point of the satellite s,
    Figure PCTCN2018078492-appb-100017
    Representing the pseudorange observation noise in meters at the jth frequency point of the satellite s received by the reference station k, and λ j indicating the wavelength of the jth frequency point of the satellite system corresponding to the satellite s;
    步骤22,根据步骤21获得的载波观测值与伪距观测值组成双差观测值,则基准站k与基准站y所组的双差载波观测方程与双差伪距观测方程分别为:Step 22, according to the carrier observation value obtained by step 21 and the pseudorange observation value constitute a double difference observation value, the double difference carrier observation equation and the double difference pseudo range observation equation of the reference station k and the reference station y are respectively:
    Figure PCTCN2018078492-appb-100018
    Figure PCTCN2018078492-appb-100018
    Figure PCTCN2018078492-appb-100019
    Figure PCTCN2018078492-appb-100019
    式中,上标r表示参考卫星,
    Figure PCTCN2018078492-appb-100020
    表示第j个频点的双差载波观测值,
    Figure PCTCN2018078492-appb-100021
    表示双差站星距,
    Figure PCTCN2018078492-appb-100022
    表示第j个频点上的双差整周模糊度,
    Figure PCTCN2018078492-appb-100023
    表示双差对流层延迟,
    Figure PCTCN2018078492-appb-100024
    表示第一个频点上双差电离层延迟,
    Figure PCTCN2018078492-appb-100025
    表示第j个频点上以米为单位的双差载波多路径效应,
    Figure PCTCN2018078492-appb-100026
    表示第j个频点上以米为单位的双差载波观测噪声,
    Figure PCTCN2018078492-appb-100027
    表示第j个频点上的双差伪距观测值,
    Figure PCTCN2018078492-appb-100028
    表示第j个频点上的双差伪距多路径效应,
    Figure PCTCN2018078492-appb-100029
    表示第j个频点上的双差伪距观测噪声;
    Where the superscript r represents the reference satellite,
    Figure PCTCN2018078492-appb-100020
    a double-difference carrier observation indicating the j-th frequency point,
    Figure PCTCN2018078492-appb-100021
    Indicates the star distance of the double-difference station,
    Figure PCTCN2018078492-appb-100022
    Indicates the double-difference full-circumference ambiguity at the jth frequency point,
    Figure PCTCN2018078492-appb-100023
    Indicates double-difference tropospheric delay,
    Figure PCTCN2018078492-appb-100024
    Indicates the doubled ionospheric delay at the first frequency point,
    Figure PCTCN2018078492-appb-100025
    Means the double-difference carrier multipath effect in meters on the jth frequency point,
    Figure PCTCN2018078492-appb-100026
    Indicates the double-difference carrier observation noise in meters on the jth frequency point,
    Figure PCTCN2018078492-appb-100027
    Indicates the double-difference pseudorange observation at the jth frequency point,
    Figure PCTCN2018078492-appb-100028
    Representing the double-difference pseudorange multipath effect at the jth frequency point,
    Figure PCTCN2018078492-appb-100029
    Representing the double difference pseudorange observation noise at the jth frequency point;
    步骤23,根据步骤22形成的双差观测值组合成双差宽巷组合观测值,解算宽巷组合模糊度:Step 23: Combine the double-difference observations formed in step 22 into a double-difference wide lane combined observation value, and calculate the wide lane combined ambiguity:
    采用MW组合解算宽巷组合模糊度,则解算方程为:Using the MW combination to solve the wide-altitude combination ambiguity, the solution equation is:
    Figure PCTCN2018078492-appb-100030
    Figure PCTCN2018078492-appb-100030
    式中:
    Figure PCTCN2018078492-appb-100031
    λ WL=c/(f 1-f 2),
    Figure PCTCN2018078492-appb-100032
    表示双差宽巷组合观测值,
    Figure PCTCN2018078492-appb-100033
    表示宽巷组合模糊度,λ WL表示宽巷波长;
    In the formula:
    Figure PCTCN2018078492-appb-100031
    λ WL =c/(f 1 -f 2 ),
    Figure PCTCN2018078492-appb-100032
    Indicates the combined observation of double-difference wide lanes,
    Figure PCTCN2018078492-appb-100033
    Indicates the wide lane combination ambiguity, λ WL represents the wide lane wavelength;
    对宽巷组合模糊度采用多历元平滑四舍五入取整,具体公式如下:For the wide lane combination ambiguity, multi-epoch smoothing is rounded off, and the specific formula is as follows:
    Figure PCTCN2018078492-appb-100034
    Figure PCTCN2018078492-appb-100034
    式中:
    Figure PCTCN2018078492-appb-100035
    表示第i个观测历元解算得到的宽巷组合模糊度浮点解,z表示观测历元总数,round表示四舍五入取整算子;
    In the formula:
    Figure PCTCN2018078492-appb-100035
    The wide-altitude combined ambiguity floating-point solution obtained by the i-th observation epoch is calculated, z represents the total number of observation epochs, and round represents a rounding-and-rounding operator;
    步骤24,采用无电离层组合,构建窄巷滤波器,利用无电离层组合联合宽巷组合分离出基础模糊度
    Figure PCTCN2018078492-appb-100036
    Figure PCTCN2018078492-appb-100037
    包括以下步骤:
    Step 24, using a combination of no ionosphere, constructing a narrow lane filter, and separating the base ambiguity by using a combination of no ionosphere and wide lane
    Figure PCTCN2018078492-appb-100036
    versus
    Figure PCTCN2018078492-appb-100037
    Includes the following steps:
    步骤241,形成双差无电离层组合观测值:In step 241, a combined observation of the double-difference ionosphere is formed:
    Figure PCTCN2018078492-appb-100038
    Figure PCTCN2018078492-appb-100038
    Figure PCTCN2018078492-appb-100039
    Figure PCTCN2018078492-appb-100039
    Figure PCTCN2018078492-appb-100040
    Figure PCTCN2018078492-appb-100040
    式中:
    Figure PCTCN2018078492-appb-100041
    表示双差无电离层组合观测值,
    Figure PCTCN2018078492-appb-100042
    表示无电离层组合模糊度,λ NL=c/(f 1+f 2);
    In the formula:
    Figure PCTCN2018078492-appb-100041
    Represents a double-difference ionospheric combined observation,
    Figure PCTCN2018078492-appb-100042
    Represents no ionospheric combined ambiguity, λ NL = c / (f 1 + f 2 );
    步骤242,构建第一卡尔曼滤波器:Step 242, constructing a first Kalman filter:
    Figure PCTCN2018078492-appb-100043
    Figure PCTCN2018078492-appb-100043
    Figure PCTCN2018078492-appb-100044
    Figure PCTCN2018078492-appb-100044
    式中,E(g)表示求数学期望,Cov(g)表示求协方差,
    Figure PCTCN2018078492-appb-100045
    分别表示第i历元和第i-1历元的状态向量;
    Figure PCTCN2018078492-appb-100046
    表示状态转移矩阵;
    Figure PCTCN2018078492-appb-100047
    表示动态噪声向量,
    Figure PCTCN2018078492-appb-100048
    表示动态噪声协方差矩阵;
    Figure PCTCN2018078492-appb-100049
    表示第i历元观测向量,
    Figure PCTCN2018078492-appb-100050
    表示设计矩阵,
    Figure PCTCN2018078492-appb-100051
    表示第i历元观测噪声向量;
    Figure PCTCN2018078492-appb-100052
    表示为第i历元观测噪声协方差阵,
    Figure PCTCN2018078492-appb-100053
    表示第i历元状态向量协方差阵,
    Figure PCTCN2018078492-appb-100054
    表示状态向量预测协方差阵,
    Figure PCTCN2018078492-appb-100055
    表示第i历元状态向量方差-协方差阵,
    Figure PCTCN2018078492-appb-100056
    表示增益矩阵,
    Figure PCTCN2018078492-appb-100057
    表示单位矩阵;
    Where E(g) represents the mathematical expectation and Cov(g) represents the covariance.
    Figure PCTCN2018078492-appb-100045
    State vectors representing the i-th epoch and the i-th epoch, respectively;
    Figure PCTCN2018078492-appb-100046
    Representing a state transition matrix;
    Figure PCTCN2018078492-appb-100047
    Represents a dynamic noise vector,
    Figure PCTCN2018078492-appb-100048
    Representing a dynamic noise covariance matrix;
    Figure PCTCN2018078492-appb-100049
    Represents the i-th eigen observation vector,
    Figure PCTCN2018078492-appb-100050
    Representing the design matrix,
    Figure PCTCN2018078492-appb-100051
    Representing the i-th eigen observation noise vector;
    Figure PCTCN2018078492-appb-100052
    Expressed as the i-th epoch observed noise covariance matrix,
    Figure PCTCN2018078492-appb-100053
    Representing the i-th epoch state vector covariance matrix,
    Figure PCTCN2018078492-appb-100054
    Representing a state vector prediction covariance matrix,
    Figure PCTCN2018078492-appb-100055
    Representing the i-th epoch state vector variance-covariance matrix,
    Figure PCTCN2018078492-appb-100056
    Representing the gain matrix,
    Figure PCTCN2018078492-appb-100057
    Express the unit matrix;
    设在第i历元,基准站k与基准站y有n颗GPS共视卫星与g颗BDS共视卫星,其中,第n颗GPS卫星与第g颗BDS卫星为各系统的参考星,待估参数包括双差整周模糊度与基线相对天顶对流层湿延迟,其滤波模型待估参数向量、观测值向量及设计矩阵表示为:Based on the i-th epoch, the base station k and the reference station y have n GPS satellites and g BDS satellites, wherein the nth GPS satellite and the g-th BDS satellite are reference stars of each system. The estimation parameters include double-difference ambiguity and baseline relative zenith tropospheric wet delay. The filter model to be estimated parameter vector, observation vector and design matrix are expressed as:
    Figure PCTCN2018078492-appb-100058
    其中:
    Figure PCTCN2018078492-appb-100058
    among them:
    Figure PCTCN2018078492-appb-100059
    Figure PCTCN2018078492-appb-100059
    Figure PCTCN2018078492-appb-100060
    Figure PCTCN2018078492-appb-100060
    Figure PCTCN2018078492-appb-100061
    Figure PCTCN2018078492-appb-100061
    式中:
    Figure PCTCN2018078492-appb-100062
    表示n+g-1维的状态向量(待估参数向量),包含1个相对天顶对流层湿延迟参数RZTD与n+g-2维双差整周模糊度参数向量
    Figure PCTCN2018078492-appb-100063
    表示n+g-2维的双差载波观测值向量,
    Figure PCTCN2018078492-appb-100064
    表示GPS双差载波观测值,o=1,2,L,n-1,
    Figure PCTCN2018078492-appb-100065
    表示GPS窄巷波长,λ 1 G表示GPS第1个频点的波长,
    Figure PCTCN2018078492-appb-100066
    表示GPS双差无电离层组合载波观测值,
    Figure PCTCN2018078492-appb-100067
    表示GPS双差站星距,
    Figure PCTCN2018078492-appb-100068
    表示GPS卫星双差对流层干延迟,
    Figure PCTCN2018078492-appb-100069
    表示GPS双差宽巷整周模糊度,f 1 G表示GPS第1个频点的频率值,
    Figure PCTCN2018078492-appb-100070
    表示GPS第2个频点的频率值,
    Figure PCTCN2018078492-appb-100071
    表示BDS双差载波观测值,s=1,2,L,g-1,
    Figure PCTCN2018078492-appb-100072
    表示BDS窄巷波长,
    Figure PCTCN2018078492-appb-100073
    表示BDS第一个频点的波长,
    Figure PCTCN2018078492-appb-100074
    表示BDS双差无电离层组合载波观测值,
    Figure PCTCN2018078492-appb-100075
    表示BDS双差站星距,
    Figure PCTCN2018078492-appb-100076
    表示BDS卫星双差对流层干延迟,
    Figure PCTCN2018078492-appb-100077
    表示BDS双差宽巷整周模糊度,f 1 C表示BDS第1个频点的频率值,
    Figure PCTCN2018078492-appb-100078
    表示BDS第2个频点的频率值,
    Figure PCTCN2018078492-appb-100079
    表示基准站k上GPS系统卫星o的对流层映射函数,
    Figure PCTCN2018078492-appb-100080
    表示基准站y上GPS系统参考卫星n的对流层映射函数,
    Figure PCTCN2018078492-appb-100081
    表示基准站k上BDS系统卫星s的对流层映射函数,
    Figure PCTCN2018078492-appb-100082
    表示基准站y上BDS系统参考卫星g的对流层映射函数,
    Figure PCTCN2018078492-appb-100083
    表示(n+g-2)×(n+g-1)维的设计矩阵;
    In the formula:
    Figure PCTCN2018078492-appb-100062
    A state vector representing the n+g-1 dimension (the parameter vector to be estimated), including a relative zenith tropospheric wet delay parameter RZTD and n+g-2 dimensional double difference whole-circumference ambiguity parameter vector
    Figure PCTCN2018078492-appb-100063
    a vector of double-difference carrier observations representing n+g-2 dimensions,
    Figure PCTCN2018078492-appb-100064
    Indicates GPS double-difference carrier observations, o=1, 2, L, n-1,
    Figure PCTCN2018078492-appb-100065
    Indicates the GPS narrow lane wavelength, λ 1 G represents the wavelength of the GPS first frequency point,
    Figure PCTCN2018078492-appb-100066
    Indicates the GPS double-difference ionosphere-free combined carrier observation,
    Figure PCTCN2018078492-appb-100067
    Indicates the GPS star distance,
    Figure PCTCN2018078492-appb-100068
    Represents the GPS satellite double-difference tropospheric dry delay,
    Figure PCTCN2018078492-appb-100069
    Indicates the full-circumference ambiguity of the GPS double-difference wide lane, and f 1 G represents the frequency value of the first frequency point of the GPS.
    Figure PCTCN2018078492-appb-100070
    Indicates the frequency value of the second frequency point of GPS.
    Figure PCTCN2018078492-appb-100071
    Indicates the BDS double-difference carrier observation, s = 1, 2, L, g-1,
    Figure PCTCN2018078492-appb-100072
    Indicates the BDS narrow lane wavelength,
    Figure PCTCN2018078492-appb-100073
    Indicates the wavelength of the first frequency of the BDS,
    Figure PCTCN2018078492-appb-100074
    Indicates the BDS double-difference ionosphere-free combined carrier observation,
    Figure PCTCN2018078492-appb-100075
    Indicates the star distance of the BDS double-difference station,
    Figure PCTCN2018078492-appb-100076
    Indicates the double-difference tropospheric dry delay of the BDS satellite,
    Figure PCTCN2018078492-appb-100077
    Indicates the full-circumference ambiguity of the BDS double-difference wide lane, and f 1 C represents the frequency value of the first frequency point of the BDS.
    Figure PCTCN2018078492-appb-100078
    Indicates the frequency value of the 2nd frequency point of the BDS.
    Figure PCTCN2018078492-appb-100079
    a tropospheric mapping function representing the GPS system satellite o on the base station k,
    Figure PCTCN2018078492-appb-100080
    Indicates the tropospheric mapping function of the GPS system reference satellite n on the base station y,
    Figure PCTCN2018078492-appb-100081
    Indicates the tropospheric mapping function of the BDS system satellite s on the base station k,
    Figure PCTCN2018078492-appb-100082
    Indicates the tropospheric mapping function of the reference satellite g of the BDS system on the base station y,
    Figure PCTCN2018078492-appb-100083
    a design matrix representing (n+g-2)×(n+g-1) dimensions;
    步骤243,根据步骤242建立的第一卡尔曼滤波器进行滤波,并解算基础载波模糊度向量参数;Step 243: Perform filtering according to the first Kalman filter established in step 242, and solve a basic carrier ambiguity vector parameter.
    从滤波器中提取出模糊度参数向量浮点解
    Figure PCTCN2018078492-appb-100084
    与方差-协方差阵利用lambda算法进行搜索,获得第1个频点双差整周模糊度
    Figure PCTCN2018078492-appb-100085
    Figure PCTCN2018078492-appb-100086
    进一步得到第2 个频点的双差整周模糊度
    Figure PCTCN2018078492-appb-100087
    Figure PCTCN2018078492-appb-100088
    Figure PCTCN2018078492-appb-100089
    Extracting the ambiguity parameter vector floating point solution from the filter
    Figure PCTCN2018078492-appb-100084
    And the variance-covariance matrix is searched by the lambda algorithm to obtain the first frequency double-difference full-circumference ambiguity
    Figure PCTCN2018078492-appb-100085
    versus
    Figure PCTCN2018078492-appb-100086
    Further obtaining the double-difference full-circumference ambiguity of the second frequency point
    Figure PCTCN2018078492-appb-100087
    versus
    Figure PCTCN2018078492-appb-100088
    Figure PCTCN2018078492-appb-100089
    步骤25,根据步骤24的结果,生成基线双差大气误差:Step 25, according to the result of step 24, generating a baseline double difference atmospheric error:
    Figure PCTCN2018078492-appb-100090
    Figure PCTCN2018078492-appb-100090
    Figure PCTCN2018078492-appb-100091
    Figure PCTCN2018078492-appb-100091
    Figure PCTCN2018078492-appb-100092
    Figure PCTCN2018078492-appb-100092
    Figure PCTCN2018078492-appb-100093
    Figure PCTCN2018078492-appb-100093
    式中,
    Figure PCTCN2018078492-appb-100094
    Figure PCTCN2018078492-appb-100095
    分别表示GPS与BDS双差对流层延迟,
    Figure PCTCN2018078492-appb-100096
    Figure PCTCN2018078492-appb-100097
    分别表示GPS与BDS第一个频点双差载波观测值,
    Figure PCTCN2018078492-appb-100098
    Figure PCTCN2018078492-appb-100099
    分别表示GPS与BDS第二个频点双差载波观测值,
    Figure PCTCN2018078492-appb-100100
    Figure PCTCN2018078492-appb-100101
    分别表示GPS与BDS第1个频点双差电离层延迟。
    In the formula,
    Figure PCTCN2018078492-appb-100094
    versus
    Figure PCTCN2018078492-appb-100095
    Representing the double-difference tropospheric delay between GPS and BDS,
    Figure PCTCN2018078492-appb-100096
    versus
    Figure PCTCN2018078492-appb-100097
    Representing the GPS and BDS first frequency double-difference carrier observations,
    Figure PCTCN2018078492-appb-100098
    versus
    Figure PCTCN2018078492-appb-100099
    Representing the second frequency difference observation of GPS and BDS respectively,
    Figure PCTCN2018078492-appb-100100
    versus
    Figure PCTCN2018078492-appb-100101
    It indicates the 1st frequency doubled ionospheric delay of GPS and BDS respectively.
  4. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤3中包括以下步骤:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the step 3 includes the following steps:
    步骤31,星型网元的主站与辅站组成基线,在三角网整网基线列表中寻找由相同基准站组成的基线,若两条基线方向相反,则需进行基线换向,由此获得星型网元各条基线双差大气误差;Step 31: The primary station and the secondary station of the star network element form a baseline, and the baseline consisting of the same base station is searched in the baseline list of the entire network of the triangular network. If the two baseline directions are opposite, the baseline commutation is required, thereby obtaining Baseline double-difference atmospheric error for each type of star network element;
    步骤32,检查星型网元各条基线参考星是否一致,若不一致,则统一参考星并对大气误差进行参考星变换;Step 32: Check whether the baseline reference stars of the star network element are consistent. If they are inconsistent, the reference star is unified and the reference star transformation is performed on the atmospheric error;
    步骤33,生成星型网元站间单差大气误差:视参考星站间单差大气误差为0,则其他卫星的站间单差大气误差值等于双差大气误差;Step 33: Generate a single-difference atmospheric error between the star-type network elements: the single-difference atmospheric error between the reference satellite stations is 0, and the single-difference atmospheric error value of the other satellites is equal to the double-difference atmospheric error;
    步骤34,提取星型网元各条基线均能共视的卫星,生成星型网元共视卫星站间单差大气误差。Step 34: Extract satellites of each star-shaped network element that can be shared by the baseline, and generate a single-difference atmospheric error between the satellite stations of the star-shaped network element.
  5. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤5判断其所在网元的方法为:用户对接收到的数据进行解码并计算用户到每个主站的直线距离,以距离最小的主站所代表的网元作为用户所在网元。The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the step 5 determines that the network element is located by the user: the user decodes the received data and calculates the user to The linear distance of each primary station is the network element represented by the primary station with the smallest distance as the user's network element.
  6. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤5或6中根据所在网元的差分数据内插得到自身与主站间的站间单差大气误差,并修正至主站观测值,包括以下步骤:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the step 5 or 6 interpolates between the station and the master station according to the differential data of the network element in which the network element is located. Single difference atmospheric error, and corrected to the observation of the primary station, including the following steps:
    步骤①,利用线性内插算法进行用户大气误差内插,则用户与主站站间单差大气误差计算如下:Step 1. Using the linear interpolation algorithm to interpolate the user's atmospheric error, the single-difference atmospheric error between the user and the primary station is calculated as follows:
    Figure PCTCN2018078492-appb-100102
    Figure PCTCN2018078492-appb-100102
    Figure PCTCN2018078492-appb-100103
    Figure PCTCN2018078492-appb-100103
    式中,下标m表示主站,u表示用户,α 123表示对流层内插系数,β 12表示电离层内插系数,w表示辅站数目,
    Figure PCTCN2018078492-appb-100104
    表示卫星s的站间单差对流层延迟,△x m,u,△y m,u,△h m,u分别表示主站与用户的坐标差,
    Figure PCTCN2018078492-appb-100105
    表示站间单差电离层延迟;
    Where subscript m denotes the primary station, u denotes the user, α 1 , α 2 , α 3 denote the tropospheric interpolation coefficient, β 1 , β 2 denote the ionospheric interpolation coefficient, and w denote the number of secondary stations,
    Figure PCTCN2018078492-appb-100104
    Indicates the inter-station single-difference tropospheric delay of the satellite s, Δx m, u , Δy m, u , Δh m, u represent the coordinate difference between the primary station and the user , respectively.
    Figure PCTCN2018078492-appb-100105
    Indicates the single-difference ionospheric delay between stations;
    对流层内插系数与电离层内插系数计算方法如下:The tropospheric interpolation coefficients and ionospheric interpolation coefficients are calculated as follows:
    Figure PCTCN2018078492-appb-100106
    Figure PCTCN2018078492-appb-100106
    Figure PCTCN2018078492-appb-100107
    Figure PCTCN2018078492-appb-100107
    Figure PCTCN2018078492-appb-100108
    Figure PCTCN2018078492-appb-100108
    Figure PCTCN2018078492-appb-100109
    Figure PCTCN2018078492-appb-100109
    Figure PCTCN2018078492-appb-100110
    Figure PCTCN2018078492-appb-100110
    式中:△x m,t,△y m,t,△h m,t表示主站与辅站坐标差,t=1,2,L,w; Where: Δx m,t , Δy m,t , Δh m,t represents the coordinate difference between the primary station and the secondary station, t=1, 2, L, w;
    步骤②,将内插得到的大气误差值修正至主站观测值,伪距与载波观测值分别如下:In step 2, the atmospheric error value obtained by the interpolation is corrected to the observation value of the primary station, and the pseudorange and the carrier observation value are respectively as follows:
    Figure PCTCN2018078492-appb-100111
    Figure PCTCN2018078492-appb-100111
    Figure PCTCN2018078492-appb-100112
    Figure PCTCN2018078492-appb-100112
    式中:
    Figure PCTCN2018078492-appb-100113
    分别表示修正了大气误差后的卫星s第j个频点在主站上的伪距与载波观测值,
    Figure PCTCN2018078492-appb-100114
    分别表示卫星s第j个频点在主站上的原始伪距与载波观测值,
    Figure PCTCN2018078492-appb-100115
    表示通过内插得到的卫星s的站间对流层延迟,
    Figure PCTCN2018078492-appb-100116
    表示通过内插得到的卫星s的站间电离层延迟。
    In the formula:
    Figure PCTCN2018078492-appb-100113
    It shows the pseudorange and carrier observation values of the jth frequency point of the satellite s after the correction of the atmospheric error on the primary station.
    Figure PCTCN2018078492-appb-100114
    Representing the original pseudorange and carrier observations of the jth frequency point of the satellite s on the primary station,
    Figure PCTCN2018078492-appb-100115
    Indicates the inter-station tropospheric delay of the satellite s obtained by interpolation,
    Figure PCTCN2018078492-appb-100116
    Indicates the inter-site ionospheric delay of the satellite s obtained by interpolation.
  7. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,所述步骤7中双差观测值表示为:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the double difference observation value in the step 7 is expressed as:
    Figure PCTCN2018078492-appb-100117
    Figure PCTCN2018078492-appb-100117
    Figure PCTCN2018078492-appb-100118
    Figure PCTCN2018078492-appb-100118
    Figure PCTCN2018078492-appb-100119
    Figure PCTCN2018078492-appb-100119
    Figure PCTCN2018078492-appb-100120
    Figure PCTCN2018078492-appb-100120
    式中,
    Figure PCTCN2018078492-appb-100121
    表示GPS卫星双差伪距观测值,
    Figure PCTCN2018078492-appb-100122
    表示GPS卫星双差站星距,
    Figure PCTCN2018078492-appb-100123
    表示GPS卫星双差伪距多路径效应,
    Figure PCTCN2018078492-appb-100124
    表示GPS卫星双差伪距观测噪声,
    Figure PCTCN2018078492-appb-100125
    表示GPS卫星双差载波观测值,λ G表示GPS观测值对应频点的波长,
    Figure PCTCN2018078492-appb-100126
    表示GPS卫星双差整周模糊度,
    Figure PCTCN2018078492-appb-100127
    表示以周为单位的GPS卫星双差载波多路径效应,
    Figure PCTCN2018078492-appb-100128
    表示以周为单位的GPS卫星双差载波观测噪声,
    Figure PCTCN2018078492-appb-100129
    表示BDS卫星双差伪距观测值,
    Figure PCTCN2018078492-appb-100130
    表示BDS卫星双差站星距,
    Figure PCTCN2018078492-appb-100131
    表示BDS卫星双差伪距多路径效应,
    Figure PCTCN2018078492-appb-100132
    表示BDS卫星双差伪距观测噪声,
    Figure PCTCN2018078492-appb-100133
    表示BDS卫星双差载波观测值,λ C表示BDS观测值对应频点的波长,
    Figure PCTCN2018078492-appb-100134
    表示BDS卫星双差整周模糊度,
    Figure PCTCN2018078492-appb-100135
    表示以周为单位的BDS卫星双差载波多路径效应,
    Figure PCTCN2018078492-appb-100136
    表示以周为单位的BDS卫星双差载波观测噪声。
    In the formula,
    Figure PCTCN2018078492-appb-100121
    Representing GPS satellite double-difference pseudorange observations,
    Figure PCTCN2018078492-appb-100122
    Indicates the satellite distance of the GPS satellite double-difference station,
    Figure PCTCN2018078492-appb-100123
    Representing GPS satellite double-difference pseudorange multipath effect,
    Figure PCTCN2018078492-appb-100124
    Representing GPS satellite double-difference pseudorange observation noise,
    Figure PCTCN2018078492-appb-100125
    Indicates the GPS satellite double-difference carrier observation, and λ G represents the wavelength of the GPS observation corresponding to the frequency point.
    Figure PCTCN2018078492-appb-100126
    Represents the GPS satellite double-difference ambiguity,
    Figure PCTCN2018078492-appb-100127
    Represents the GPS satellite double-difference carrier multipath effect in weeks,
    Figure PCTCN2018078492-appb-100128
    Representing GPS satellite double-difference carrier observation noise in weeks,
    Figure PCTCN2018078492-appb-100129
    Indicates the double-difference pseudorange observation of the BDS satellite,
    Figure PCTCN2018078492-appb-100130
    Indicates the star distance of the BDS satellite double-difference station,
    Figure PCTCN2018078492-appb-100131
    Representing the double-signal pseudorange multipath effect of BDS satellites,
    Figure PCTCN2018078492-appb-100132
    Representing BDS satellite double-difference pseudorange observation noise,
    Figure PCTCN2018078492-appb-100133
    Indicates the BDS satellite double-difference carrier observation, and λ C represents the wavelength of the BDS observation corresponding to the frequency point.
    Figure PCTCN2018078492-appb-100134
    Indicates the double-difference ambiguity of the BDS satellite,
    Figure PCTCN2018078492-appb-100135
    Representing the double-signal carrier multipath effect of the BDS satellite in weeks,
    Figure PCTCN2018078492-appb-100136
    Indicates the BDS satellite double-difference carrier observation noise in weeks.
  8. 根据权利要求1所述的基于星型网络的BDS/GPS广播式网络RTK算法,其特征在于,步骤7中第二卡尔曼滤波器构建如下:The star network-based BDS/GPS broadcast network RTK algorithm according to claim 1, wherein the second Kalman filter in step 7 is constructed as follows:
    设在第i历元,用户与星型网有n颗GPS共视卫星和g颗BDS共视卫星,其中第n颗GPS卫星与第g颗BDS卫星分别为各系统的参考星,联合所有卫星L1载波和P1伪距观测数据,其滤波模型待估参数矩阵
    Figure PCTCN2018078492-appb-100137
    观测值矩阵
    Figure PCTCN2018078492-appb-100138
    及设计矩阵
    Figure PCTCN2018078492-appb-100139
    表示为:
    Based on the i-th epoch, the user and the star network have n GPS satellites and g BDS satellites, of which the nth GPS satellite and the gth BDS satellite are reference stars of each system, and all satellites are combined. L1 carrier and P1 pseudorange observation data, filter model to be estimated parameter matrix
    Figure PCTCN2018078492-appb-100137
    Observation matrix
    Figure PCTCN2018078492-appb-100138
    Design matrix
    Figure PCTCN2018078492-appb-100139
    Expressed as:
    Figure PCTCN2018078492-appb-100140
    其中,
    Figure PCTCN2018078492-appb-100141
    Figure PCTCN2018078492-appb-100140
    among them,
    Figure PCTCN2018078492-appb-100141
    Figure PCTCN2018078492-appb-100142
    Figure PCTCN2018078492-appb-100142
    式中,
    Figure PCTCN2018078492-appb-100143
    表示n+g+1维的待估参数向量,包含3维位置参数向量
    Figure PCTCN2018078492-appb-100144
    与n+g-2维双差 整周模糊度参数向量
    Figure PCTCN2018078492-appb-100145
    表示2(n+g-2)维双差观测值向量,包括伪距与载波观测值;
    Figure PCTCN2018078492-appb-100146
    表示2(n+g-2)×(n+g+1)维设计矩阵,其中l o,n,G,p o,n,G,q o,n,G表示GPS卫星方向余弦(上标o=1,2L,n-1),l s,g,C,p s,g,C,q s,g,C表示BDS卫星方向余弦,s=1,2L,t-1,
    Figure PCTCN2018078492-appb-100147
    表示以米为单位的GPS卫星双差载波观测值,
    Figure PCTCN2018078492-appb-100148
    表示GPS卫星双差伪距观测值,
    Figure PCTCN2018078492-appb-100149
    表示GPS卫星双差站星距,
    Figure PCTCN2018078492-appb-100150
    表示BDS卫星双差站星距,
    Figure PCTCN2018078492-appb-100151
    表示以米为单位的BDS卫星双差载波观测值,
    Figure PCTCN2018078492-appb-100152
    表示BDS卫星双差伪距观测值;
    In the formula,
    Figure PCTCN2018078492-appb-100143
    An estimated parameter vector representing n+g+1 dimensions, including a 3-dimensional positional parameter vector
    Figure PCTCN2018078492-appb-100144
    Double-difference whole-circumference ambiguity parameter vector with n+g-2
    Figure PCTCN2018078492-appb-100145
    Representing a 2(n+g-2) dimensional double difference observation vector, including pseudorange and carrier observations;
    Figure PCTCN2018078492-appb-100146
    Represents a 2(n+g-2)×(n+g+1) dimensional design matrix, where l o,n,G ,p o,n,G ,q o,n,G represent the cosine of the GPS satellite direction (superscript o=1,2L,n-1),l s,g,C ,p s,g,C ,q s,g,C denotes the cosine of the BDS satellite direction, s=1, 2L, t-1,
    Figure PCTCN2018078492-appb-100147
    Means the GPS satellite double-difference carrier observation in meters,
    Figure PCTCN2018078492-appb-100148
    Representing GPS satellite double-difference pseudorange observations,
    Figure PCTCN2018078492-appb-100149
    Indicates the satellite distance of the GPS satellite double-difference station,
    Figure PCTCN2018078492-appb-100150
    Indicates the star distance of the BDS satellite double-difference station,
    Figure PCTCN2018078492-appb-100151
    Indicates the BDS satellite double-difference carrier observations in meters,
    Figure PCTCN2018078492-appb-100152
    Indicates the double-difference pseudorange observation of the BDS satellite;
    将上述参数赋值并带入第二卡尔曼滤波器中逐历元解算,然后提取浮点模糊度向量与其方差-协方差阵,利用lambda算法搜索即可获得模糊度固定解;The above parameters are assigned and brought into the second Kalman filter to solve the epoch epoch, then the floating ambiguity vector and its variance-covariance matrix are extracted, and the ambiguity fixed solution can be obtained by searching with the lambda algorithm;
    固定模糊度后,利用下式解得用户三维坐标固定解:After fixing the ambiguity, the fixed solution of the user's three-dimensional coordinates is solved by the following formula:
    Figure PCTCN2018078492-appb-100153
    Figure PCTCN2018078492-appb-100153
    其中,
    Figure PCTCN2018078492-appb-100154
    分别为三维坐标参数向量及浮点模糊度参数向量,
    Figure PCTCN2018078492-appb-100155
    为固定模糊度后的坐标参数向量,
    Figure PCTCN2018078492-appb-100156
    为固定模糊度参数向量,
    Figure PCTCN2018078492-appb-100157
    分别对应各参数滤波解协方差阵。
    among them,
    Figure PCTCN2018078492-appb-100154
    Three-dimensional coordinate parameter vector and floating-point ambiguity parameter vector,
    Figure PCTCN2018078492-appb-100155
    The coordinate parameter vector after fixing the ambiguity,
    Figure PCTCN2018078492-appb-100156
    To fix the ambiguity parameter vector,
    Figure PCTCN2018078492-appb-100157
    Corresponding to each parameter filtering solution covariance matrix.
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