CN112666513A - Improved MUSIC direction of arrival estimation method - Google Patents

Improved MUSIC direction of arrival estimation method Download PDF

Info

Publication number
CN112666513A
CN112666513A CN202011450983.0A CN202011450983A CN112666513A CN 112666513 A CN112666513 A CN 112666513A CN 202011450983 A CN202011450983 A CN 202011450983A CN 112666513 A CN112666513 A CN 112666513A
Authority
CN
China
Prior art keywords
signal
noise
vector
arrival
signals
Prior art date
Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
Granted
Application number
CN202011450983.0A
Other languages
Chinese (zh)
Other versions
CN112666513B (en
Inventor
王川川
董晓博
曾勇虎
汪连栋
李志鹏
朱宁
陆科宇
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
UNIT 63892 OF PLA
Original Assignee
UNIT 63892 OF PLA
Priority date (The priority date is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the date listed.)
Filing date
Publication date
Application filed by UNIT 63892 OF PLA filed Critical UNIT 63892 OF PLA
Priority to CN202011450983.0A priority Critical patent/CN112666513B/en
Publication of CN112666513A publication Critical patent/CN112666513A/en
Application granted granted Critical
Publication of CN112666513B publication Critical patent/CN112666513B/en
Active legal-status Critical Current
Anticipated expiration legal-status Critical

Links

Images

Abstract

The invention discloses an improved MUSIC direction of arrival estimation method, which comprises the following steps: constructing a DOA estimation model of the far-field signal; calculating a covariance matrix of the array observation signals, and performing characteristic decomposition on the covariance matrix; presetting the number of signal sources, and solving a noise subspace; performing spatial spectrum estimation by applying an MUSIC algorithm, and estimating an arrival angle by searching a peak; for a group of observed signals, the arrival angle of the signals is estimated for multiple times, and then the DOA finally estimated is obtained through an averaging processing mode. The method can estimate the number of the signal sources, can avoid the adverse effect of inaccurate estimation of the number of the signal sources on DOA estimation by adopting other technologies to estimate the number of the signal sources, and improves the estimation precision of the incoming wave direction of the signal.

Description

Improved MUSIC direction of arrival estimation method
Technical Field
The invention belongs to the technical field of signal processing, relates to the technical field of radar and communication countermeasure reconnaissance, and particularly relates to an improved MUSIC direction of arrival estimation method, which is used for estimating the direction of incoming waves of narrow-band signal sources such as radar signals and communication signals in a complex electromagnetic environment.
Background
In electronic warfare, a passive detection system aiming at signal reconnaissance performs reconnaissance by intercepting electromagnetic signals radiated by electronic equipment of an enemy, has the advantages of long acting distance, good concealment, strong anti-electronic interference capability and the like, and plays an important role in modern electronic warfare. The estimation of the Direction of radiation source signals, also called Direction of Arrival (DOA), is an important link in the activities of implementing Direction-finding positioning and performing comprehensive reconnaissance. The direction of arrival estimation of the passive detection system is to obtain the information of the incident angle of the target by receiving the target radiation electromagnetic wave, and the detection system does not radiate the electromagnetic wave, so the passive detection system has good concealment, difficult exposure and strong anti-interference capability, and is widely applied to electronic warfare.
DOA estimation develops rapidly in almost thirty years, beam forming, maximum likelihood estimation, subspace class and the like are the most common methods in DOA estimation, and abundant research results are obtained in the aspects of Gaussian/non-Gaussian noise, color noise, non-uniform noise, broadband signals, coherent signals, array element coupling, operation complexity and the like. Compared with beam forming and maximum likelihood estimation, the subspace method has higher resolution and moderate computational complexity, and becomes a mainstream method in related fields such as DOA estimation. Among them, the Multiple Signal Classification (MUSIC) method has a milestone meaning in the development history of high-resolution direction finding technology, realizes array super-resolution direction finding in the true sense, and is one of the methods used by researchers most, on the basis of which, the researchers have made various beneficial improvements.
Generally, before estimating the incoming wave direction of a signal, the number of signal sources needs to be known first. In an electronic reconnaissance environment, due to the non-cooperative countermeasure characteristic of the two parties, the number of signal sources needs to be estimated by adopting another technology, and then the direction-finding algorithm is applied to estimate the DOA. If the number of the estimated signals is not consistent with the actual number, the number of the spectral peaks obtained by a plurality of super-resolution algorithms is inconsistent with the actual number of the spectral peaks, so that the DOA estimation is wrong, and the estimation of the number of the signal sources has important influence on the direction finding effect; however, the estimation of the number of signal sources is also a technical difficulty in the field of array signal processing, and it is very difficult to achieve accurate estimation of the number of signal sources under complicated electromagnetic environment conditions such as low signal-to-noise ratio.
Disclosure of Invention
Aiming at the problem that the MUSIC method needs to estimate the number of signal sources in advance through other technologies in DOA estimation, the invention aims to provide an improved MUSIC direction-of-arrival estimation method.
In order to achieve the purpose, the invention adopts the following technical scheme:
an improved MUSIC direction of arrival estimation method comprises the following steps:
s1, constructing a far-field signal DOA estimation model
Set with K far-field signals from the direction theta12,…,θKIncident on an array consisting of M sensors, and observing signals of the array at the time t are X (t) and are expressed as
Figure BDA0002831874120000021
Wherein X (t) ═ X1(t),X2(t),…,XM(t)]TFor array observation signal vectors, T represents transposition;
a(θk) Is an array direction vector;
A(θ)=[a(θ1),a(θ2),…,a(θK)]a steering vector matrix formed by the direction vectors;
θ=[θ12,…,θK]Tis the parameter vector of the incoming wave angle of the signal;
S(t)=[s1(t),s2(t),…,sK(t)]Tis an incident signal vector;
k is the number of signals;
N(t)=[n1(t),n2(t),…,nM(t)]Tfor additive noise vectors, sample point T is 1,2, …, T1,T1Counting the number of signal sampling points;
s2, calculating the covariance matrix R of the array observation signals X (t) in the step S1, and performing feature decomposition on the covariance matrix
A covariance matrix of the array observation signal x (t) is calculated, expressed as:
R=E[XXH]=AE[SSH]AH+E[NNH]=ARSAH+RN (2)
wherein R isSAnd RNRespectively a signal covariance matrix and a noise covariance matrix, wherein H represents conjugate transposition; since the signal and the noise are independent of each other, the data covariance matrix is decomposed into two parts, AR, related to the signal and the noiseSAHIs a signal portion; for spatially perfect white noise, and the noise power is σ2Then, there are:
R=ARSAH+RN=ARSAH2I (3)
and (3) performing characteristic decomposition on the covariance matrix R, namely:
R=ARSAH+RN=Q∑QH (4)
wherein, matrix Q is the eigenvector matrix, diagonal matrix sigma is formed by the eigenvalue, namely:
Figure BDA0002831874120000031
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λKK+1≈…≈λM≈σ2
the steering vector matrix A is a Van der Monte matrix, provided that the target signal direction θi≠θp(i ≠ p), wherein i and p respectively represent the serial numbers of the signals, and K characteristic values corresponding to different target signals are total;
corresponding to the characteristic value lambdaiI is 1,2, …, M, and its feature vector is ei,i=1,2,…,M;
S3, presetting the number of signal sources, and obtaining the noise subspace
Setting the number of signal sources as
Figure BDA0002831874120000032
The range of variation is
Figure BDA0002831874120000033
Wherein M is the number of antenna elements of the array antenna;
in setting the number of signal sources
Figure BDA0002831874120000034
On the basis of (1), a noise subspace is obtained, the expression of which is
Figure BDA0002831874120000035
Wherein λ ispAnd epRespectively carrying out characteristic value decomposition on the covariance matrix R to obtain a pth characteristic value and a characteristic vector;
s4, theoretically, under the condition that the signal sources are independent and have no noise, the signal subspace ESAnd noise subspace EN′Orthogonal, it is known that the steering vector in the signal subspace is also orthogonal to the noise subspace, i.e.
aH(θ)EN′=0 (7)
Wherein the steering vector matrix
aH(θ)=[exp(-j2πfτ1k),exp(-j2πfτ2k),…,exp(-j2πfτMk)]H
Figure BDA0002831874120000041
The time delay of the kth signal reaching the mth array element relative to the 1 st array element, M is 1,2, …, M, K is 1,2, …, K;
c is the speed of light;
d is the interval between adjacent array elements;
s5, in practice, the vector a is guided by the presence of noiseH(theta) and noise subspace EN′And cannot be completely orthogonal, so DOA is realized by taking the maximum value of the spatial spectrum, and the calculation formula of the spatial spectrum estimation by applying the MUSIC algorithm is
Figure BDA0002831874120000042
Changing theta from-90 degrees to 90 degrees according to a certain step length by the above formula, and estimating an arrival angle by searching a peak;
s6, due to
Figure BDA0002831874120000043
Thus, the settings are different
Figure BDA0002831874120000044
Different arrival angle estimation results are obtained according to the formula (8) in the step S5;
Figure BDA0002831874120000045
sequentially taking values from 1 to M-1 to obtain M-1 kinds of arrival angle estimation results, which are expressed as
Figure BDA0002831874120000046
Figure BDA0002831874120000047
Figure BDA0002831874120000048
The number of angles of (a) represents the number of estimated signal sources, the angle value represents the incoming wave direction of the signal source, and the setting is based on
Figure BDA0002831874120000049
The number of the judged signal sources is
Figure BDA00028318741200000410
Angle of arrival of signal of
Figure BDA00028318741200000411
S7, mixing
Figure BDA00028318741200000412
Form a row vector, denoted ne=[n1,n2,…,nM-1]Counting the number of the signal sources which appear most from the vector as the final estimated number of the signal sources
Figure BDA00028318741200000413
The number appearing in the vector
Figure BDA00028318741200000414
The serial number positions are marked, and the serial numbers are
Figure BDA00028318741200000415
The number of occurrences is given as num; to obtain
Figure BDA00028318741200000416
Then, will correspond to the number
Figure BDA00028318741200000417
The arrival angles of the signals form a row vector represented as
Figure BDA0002831874120000051
Vector formed by num group signal arrival angles
Figure BDA0002831874120000052
Averaging to obtain the final signal arrival angle estimation value expressed as
Figure BDA0002831874120000053
Obtaining the number of the signal sources estimated finally
Figure BDA0002831874120000054
And the final estimated angle of arrival
Figure BDA0002831874120000055
Further, in step S1, the far-field signals are mutually independent narrow-band stationary signals, and satisfy the mean value E { S (t) ═ 0} and the covariance matrix
Figure BDA0002831874120000056
Wherein
Figure BDA0002831874120000057
Is the power of the kth signal; the superimposed noise in the array observation signal vector is additive white Gaussian noise and is independent from the signal; the number of far-field signals is less than the number of array elements and the number of sampling points, i.e. K<min(M,T1) (ii) a The signals are propagated in an ideal space, and the array sensor has omnidirectional consistency.
Further, in the above step S7, the above step may be performed
Figure BDA0002831874120000058
Figure BDA0002831874120000059
Forming a column vector, counting the most appeared numbers from the column vector as the number of the signal sources to be finally estimated
Figure BDA00028318741200000510
Furthermore, the number K of the signal sources is at most half of the number of the antenna elements, i.e. the number K of the signal sources is equal to the number of the antenna elements
Figure BDA00028318741200000511
Figure BDA00028318741200000512
Figure BDA00028318741200000513
Indicating a rounding down.
Due to the adoption of the technical scheme, the invention has the following advantages:
according to the improved MUSIC direction-of-arrival estimation method, the number of signal sources is estimated without additionally adopting other technologies, the number of the signal sources can be automatically estimated, and the function of the MUSIC direction-finding method is expanded; for a group of observation signals, the arrival angle of the signal is estimated for multiple times, and then the finally estimated DOA is obtained through a mean value solving processing mode, so that the problem that the information source number is difficult to estimate in the incoming wave direction estimation by applying the MUSIC algorithm can be solved, the adverse effect on the DOA estimation caused by inaccurate information source number estimation is avoided, the estimation precision of the incoming wave direction of the signal is improved, and the method has good popularization and application values.
Drawings
Fig. 1 shows the spatial spectrum estimation result when the SNR is-5 dB and the number of signal sources is 3;
fig. 2 shows the spatial spectrum estimation result when the SNR is 10dB and the number of signal sources is 1;
fig. 3 shows the spatial spectrum estimation result when the SNR is 10dB and the number of signal sources is 4.
Detailed Description
The technical solution of the present invention will be further described in detail with reference to the accompanying drawings and examples.
The experimental verification of the improved MUSIC direction of arrival estimation method is carried out under the simulation conditions of DELL9020MT type personal computer, Intel (R) core (TM) i7-4770 CPU @3.40GHz and 64-bit Windows operating system, and MATLAB R2010a is adopted as simulation software.
The radiation source signal is taken as
Figure BDA0002831874120000061
T1Is a signalThe noise is complex Gaussian white noise, and the input signal-to-noise ratio (SNR) is defined as
Figure BDA0002831874120000062
Wherein
Figure BDA0002831874120000063
And
Figure BDA0002831874120000064
representing the variance of the signal and noise, respectively.
Example one
The input signal-to-noise ratio SNR is-5 dB, and the number of signal sampling points is T1The number of signals is 3, the arrival angles of the signals are-45 degrees, 30 degrees and 60 degrees respectively, and the number of array elements is M-8.
An improved MUSIC direction of arrival estimation method comprises the following specific steps:
s1, constructing a far-field signal DOA estimation model
Set with 3 far-field signals from the direction theta123Incident on an array of 8 sensors, and the observed signal of the array at time t is X (t) and is expressed as
Figure BDA0002831874120000065
Wherein X (t) ═ X1(t),X2(t),…,XM(t)]TFor array observation signal vectors, T represents transposition;
a(θk) Is an array direction vector;
A(θ)=[a(θ1),a(θ2),a(θ3)]a steering vector matrix formed by the direction vectors;
θ=[θ123]Tis the parameter vector of the incoming wave angle of the signal;
S(t)=[s1(t),s2(t),s3(t)]Tis an incident signal vector;
k is the number of signals, and K is 3;
N(t)=[n1(t),n2(t),…,nM(t)]Tfor additive noise vectors, sample point T is 1,2, …, T1,T1Number of signal samples, T1=1024;
S2, calculating the covariance matrix R of the array observation signals X (t) in the step S1, and performing feature decomposition on the covariance matrix
A covariance matrix of the array observation signal x (t) is calculated, expressed as:
R=E[XXH]=AE[SSH]AH+E[NNH]=ARSAH+RN (2)
wherein R isSAnd RNRespectively a signal covariance matrix and a noise covariance matrix, wherein H represents conjugate transposition; since the signal and the noise are independent of each other, the data covariance matrix is decomposed into two parts, AR, related to the signal and the noiseSAHIs a signal portion; for spatially perfect white noise, and the noise power is σ2Then, there are:
R=ARSAH+RN=ARSAH2I (3)
and (3) performing characteristic decomposition on the covariance matrix R, namely:
R=ARSAH+RN=Q∑QH (4)
wherein, matrix Q is the eigenvector matrix, diagonal matrix sigma is formed by the eigenvalue, namely:
Figure BDA0002831874120000071
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥λ34≈…≈λM≈σ2
the steering vector matrix A is a Van der Monte matrix, and K is 3 eigenvalues corresponding to different target signals;
corresponds to specialEigenvalue λiI is 1,2, …, M, and its feature vector is ei,i=1,2,…,M;
S3, presetting the number of signal sources, and obtaining the noise subspace
Setting the number of signal sources as
Figure BDA0002831874120000072
Figure BDA0002831874120000073
Respectively taking the values of 1,2 and … 7;
in setting the number of signal sources
Figure BDA0002831874120000074
On the basis of (1), a noise subspace is obtained, the expression of which is
Figure BDA0002831874120000075
Wherein λ ispAnd epRespectively carrying out characteristic value decomposition on the covariance matrix R to obtain a pth characteristic value and a characteristic vector;
s4, theoretically, under the condition that the signal sources are independent and have no noise, the signal subspace ESAnd noise subspace EN′Orthogonal, it is known that the steering vector in the signal subspace is also orthogonal to the noise subspace, i.e.
aH(θ)EN′=0 (7)
Wherein the steering vector matrix
aH(θ)=[exp(-j2πfτ1k),exp(-j2πfτ2k),…,exp(-j2πfτMk)]H
Figure BDA0002831874120000081
The time delay of the kth signal reaching the mth array element relative to the 1 st array element, M is 1,2, …, M, K is 1,2, …, K;
c is the speed of light;
d is the interval between adjacent array elements;
s5 factIn the interim, the steering vector a is present due to the presence of noiseH(theta) and noise subspace EN′And cannot be completely orthogonal, so DOA is realized by taking the maximum value of the spatial spectrum, and the calculation formula of the spatial spectrum estimation by applying the MUSIC algorithm is
Figure BDA0002831874120000082
Changing theta from-90 degrees to 90 degrees according to a certain step length by the above formula, and estimating an arrival angle by searching a peak to obtain MUSIC spectral functions shown as (a) to (g) in figure 1 respectively;
s6, with the array element number M being 8, 7 arrival angle estimation results are obtained, which are expressed as
Figure BDA0002831874120000083
Figure BDA0002831874120000084
DOA1=[-48.9°,31.3°,61.5°]That is, the arrival angles are-48.9 deg., 31.3 deg., 61.5 deg., respectively, and the estimated number of signal sources is n1=3;
DOA2=[-45.5°,29.8°,61.2°]That is, the arrival angles are-45.5 deg., 29.8 deg., 61.2 deg., respectively, and the estimated number of signal sources is n2=3;
DOA3=[-45.2°,30.0°,60.2°]That is, the arrival angles are-48.9 deg., 31.3 deg., 61.5 deg., respectively, and the estimated number of signal sources is n3=3;
DOA4=[-45.0°,29.8°,59.6°]That is, the arrival angles are-45.0 degrees, 29.8 degrees and 59.6 degrees, respectively, and the estimated number of signal sources is n4=3;
DOA5=[-45.2°,30.0°,60.0°]That is, the arrival angles are-45.5 deg., 29.8 deg., 61.2 deg., respectively, and the estimated number of signal sources is n5=3;
DOA6=[-45.6°,30.1°,60.1°]That is, the arrival angles are-45.6 degrees, 30.1 degrees and 60.1 degrees, respectively, and the estimated number of signal sources is n6=3;
DOA7=[-45.5°,9.7°,29.6°,60.9°]That is, the arrival angles are-45.5 °,9.7 °,29.6 °, and 60.9 °, respectively, and the estimated number of signal sources is n7=4;
S7, mixing
Figure BDA0002831874120000091
Figure BDA0002831874120000092
Form a row vector, denoted ne=[3,3,3,3,3,3,4]Counting the number of the signal sources which appear most from the vector as the final estimated number of the signal sources
Figure BDA0002831874120000093
It is obvious that
Figure BDA0002831874120000094
The number of times num of occurrence is 6; the DOA estimation results with the number of signal sources of 3 (namely 3 spectral peaks) are respectively the 1 st, 2 nd, 3 rd, 4 th, 5 th and 6 th groups
Figure BDA0002831874120000095
Vector formed by the arrival angles of the 6 groups of signals
Figure BDA0002831874120000096
Averaging to obtain the final signal arrival angle estimation value expressed as
Figure BDA0002831874120000097
Example two
As shown in fig. 2, the input signal-to-noise ratio SNR is 10dB, and the number of signal samples is T11024, the number of signals is 1, the arrival angle of the signals is-60 degrees, and the number of array elements is M-8.
An improved MUSIC direction of arrival estimation method comprises the following specific steps:
s1, constructing a far-field signal DOA estimation model
Set with 1 far-field signal from direction theta1Incident on an array of 8 sensors, and the observed signal of the array at time t is X (t) and is expressed as
Figure BDA0002831874120000098
Wherein X (t) ═ X1(t),X2(t),…,XM(t)]TFor array observation signal vectors, T represents transposition;
a(θk) Is an array direction vector;
A(θ)=[a(θ1)]a steering vector matrix formed by the direction vectors;
θ=[θ1]Tis the parameter vector of the incoming wave angle of the signal;
S(t)=[s1(t)]Tis an incident signal vector;
k is the number of signals, and K is 1;
N(t)=[n1(t),n2(t),…,nM(t)]Tfor additive noise vectors, sample point T is 1,2, …, T1,T1Number of signal samples, T1=1024;
S2, calculating the covariance matrix R of the array observation signals X (t) in the step S1, and performing feature decomposition on the covariance matrix
A covariance matrix of the array observation signal x (t) is calculated, expressed as:
R=E[XXH]=AE[SSH]AH+E[NNH]=ARSAH+RN (2)
wherein R isSAnd RNRespectively a signal covariance matrix and a noise covariance matrix, wherein H represents conjugate transposition; since the signal and the noise are independent of each other, the data covariance matrix is decomposed into two parts, AR, related to the signal and the noiseSAHIs a signal portion; for spatially perfect white noise, and the noise power is σ2Then, there are:
R=ARSAH+RN=ARSAH2I (3)
and (3) performing characteristic decomposition on the covariance matrix R, namely:
R=ARSAH+RN=Q∑QH (4)
wherein, matrix Q is the eigenvector matrix, diagonal matrix sigma is formed by the eigenvalue, namely:
Figure BDA0002831874120000101
in the equation (5), the characteristic values satisfy the following relationship:
λ12≈…≈λM≈σ2
the steering vector matrix A is a Van der Monte matrix, and K is 1 in total and corresponds to different characteristic values of the target signals;
corresponding to the characteristic value lambdaiI is 1,2, …, M, and its feature vector is ei,i=1,2,…,M;
S3, presetting the number of signal sources, and obtaining the noise subspace
Setting the number of signal sources as
Figure BDA0002831874120000102
Figure BDA0002831874120000103
Respectively taking the values of 1,2 and … 7;
in setting the number of signal sources
Figure BDA0002831874120000104
On the basis of (1), a noise subspace is obtained, the expression of which is
Figure BDA0002831874120000105
Wherein λ ispAnd epThe p-th one after characteristic value decomposition is respectively carried out on the covariance matrix REigenvalues and eigenvectors;
s4, theoretically, under the condition that the signal sources are independent and have no noise, the signal subspace ESAnd noise subspace EN′Orthogonal, it is known that the steering vector in the signal subspace is also orthogonal to the noise subspace, i.e.
aH(θ)EN′=0 (7)
Wherein the steering vector matrix
aH(θ)=[exp(-j2πfτ1k),exp(-j2πfτ2k),…,exp(-j2πfτMk)]H
Figure BDA0002831874120000111
The time delay of the kth signal reaching the mth array element relative to the 1 st array element, wherein M is 1,2, …, and M, k is 1;
c is the speed of light;
d is the interval between adjacent array elements;
s5, in practice, the vector a is guided by the presence of noiseH(theta) and noise subspace EN′And cannot be completely orthogonal, so DOA is realized by taking the maximum value of the spatial spectrum, and the calculation formula of the spatial spectrum estimation by applying the MUSIC algorithm is
Figure BDA0002831874120000112
From the above formula, changing theta from-90 degrees to 90 degrees according to a certain step length, estimating an arrival angle by searching a peak, and respectively obtaining MUSIC spectral functions as shown in (a) to (g) of FIG. 2;
s6, with the array element number M being 8, 7 arrival angle estimation results are obtained, which are expressed as
Figure BDA0002831874120000113
Figure BDA0002831874120000114
DOA1=[-59.9°]I.e. the angle of arrival is-59.9 deg., the estimated signal sourceThe number is n1=1;
DOA2=[-60.0°,-27.5°,-3.8°]I.e. angles of arrival of-60.0 deg. -27.5 deg. -3.8 deg., respectively, the estimated number of signal sources is n2=3;
DOA3=[-60.0°,44.5°]That is, the arrival angles are-60.0 DEG and 44.5 DEG, respectively, and the estimated number of signal sources is n3=2;
DOA4=[-59.9°]I.e. the angle of arrival is-59.9 deg., the estimated number of signal sources is n4=1;
DOA5=[-60.0°]I.e. the angle of arrival is-60.0 deg., the estimated number of signal sources is n5=1;
DOA6=[-60.1°,-31.1°,-11.4°,20.2°,53.9°]I.e. angles of arrival of-60.1 deg. -31.1 deg. -11.4 deg., 20.2 deg., 53.9 deg., respectively, the estimated number of signal sources being n6=5;
DOA7=[-59.8°,-7.1°,17.2°,35.7°,56.8°]I.e. the angles of arrival are-59.8 deg. -7.1 deg., 17.2 deg., 35.7 deg., 56.8 deg., respectively, and the estimated number of signal sources is n7=5;
S7, mixing
Figure BDA0002831874120000121
Figure BDA0002831874120000122
Form a row vector, denoted ne=[1,3,2,1,1,5,5]Counting the number of the signal sources which appear most from the vector as the final estimated number of the signal sources
Figure BDA0002831874120000123
It is obvious that
Figure BDA0002831874120000124
The number of times num of occurrence is 3; the DOA estimation results with the number of signal sources of 1 (namely 1 spectral peak) are respectively the 1 st, 4 th and 5 th groups
Figure BDA0002831874120000125
Vector formed by the angle of arrival of the 3 groups of signals
Figure BDA0002831874120000126
Averaging to obtain the final signal arrival angle estimation value expressed as
Figure BDA0002831874120000127
Since the actual number of signal sources is 1 and the incoming wave angle is-60 °, comparing the estimation result with the actual result, it can be found that the arrival direction estimation method of the present invention can realize accurate estimation of the number of signal sources and realize estimation of the arrival angle of the signal with very small error.
EXAMPLE III
The input signal-to-noise ratio SNR is 10dB, and the number of signal sampling points is T1The number of signals is 4, the arrival angles of the signals are respectively-60 degrees, 15 degrees, 30 degrees and 45 degrees, and the number of array elements is 8.
An improved MUSIC direction of arrival estimation method comprises the following specific steps:
s1, constructing a far-field signal DOA estimation model
4 far-field signals are set from the direction theta1234Incident on an array of 8 sensors, and the observed signal of the array at time t is X (t) and is expressed as
Figure BDA0002831874120000128
Wherein X (t) ═ X1(t),X2(t),…,XM(t)]TFor array observation signal vectors, T represents transposition;
a(θk) Is an array direction vector;
A(θ)=[a(θ1),a(θ2),a(θ3),a(θ4)]a steering vector matrix formed by the direction vectors;
θ=[θ1234]Tis the parameter vector of the incoming wave angle of the signal;
S(t)=[s1(t),s2(t),s3(t),s4(t)]Tis an incident signal vector;
k is the number of signals, and K is 4;
N(t)=[n1(t),n2(t),…,nM(t)]Tfor additive noise vectors, sample point T is 1,2, …, T1,T1Number of signal samples, T1=1024;
S2, calculating the covariance matrix R of the array observation signals X (t) in the step S1, and performing feature decomposition on the covariance matrix
A covariance matrix of the array observation signal x (t) is calculated, expressed as:
R=E[XXH]=AE[SSH]AH+E[NNH]=ARSAH+RN (2)
wherein R isSAnd RNRespectively a signal covariance matrix and a noise covariance matrix, wherein H represents conjugate transposition; since the signal and the noise are independent of each other, the data covariance matrix is decomposed into two parts, AR, related to the signal and the noiseSAHIs a signal portion; for spatially perfect white noise, and the noise power is σ2Then, there are:
R=ARSAH+RN=ARSAH2I (3)
and (3) performing characteristic decomposition on the covariance matrix R, namely:
R=ARSAH+RN=Q∑QH (4)
wherein, matrix Q is the eigenvector matrix, diagonal matrix sigma is formed by the eigenvalue, namely:
Figure BDA0002831874120000131
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λ45≈…≈λM≈σ2
the steering vector matrix A is a Van der Monte matrix, and K is 4 eigenvalues corresponding to different target signals;
corresponding to the characteristic value lambdaiI is 1,2, …, M, and its feature vector is ei,i=1,2,…,M;
S3, presetting the number of signal sources, and obtaining the noise subspace
Setting the number of signal sources as
Figure BDA0002831874120000132
Figure BDA0002831874120000133
Respectively taking the values of 1,2 and … 7;
in setting the number of signal sources
Figure BDA0002831874120000141
On the basis of (1), a noise subspace is obtained, the expression of which is
Figure BDA0002831874120000142
Wherein λ ispAnd epRespectively carrying out characteristic value decomposition on the covariance matrix R to obtain a pth characteristic value and a characteristic vector;
s4, theoretically, under the condition that the signal sources are independent and have no noise, the signal subspace ESAnd noise subspace EN′Orthogonal, it is known that the steering vector in the signal subspace is also orthogonal to the noise subspace, i.e.
aH(θ)EN′=0 (7)
Wherein the steering vector matrix
aH(θ)=[exp(-j2πfτ1k),exp(-j2πfτ2k),…,exp(-j2πfτMk)]H
Figure BDA0002831874120000143
The time delay of the kth signal reaching the mth array element relative to the 1 st array element, M is 1,2, …, M, K is 1,2, …, K;
c is the speed of light;
d is the interval between adjacent array elements;
s5, in practice, the vector a is guided by the presence of noiseH(theta) and noise subspace EN′And cannot be completely orthogonal, so DOA is realized by taking the maximum value of the spatial spectrum, and the calculation formula of the spatial spectrum estimation by applying the MUSIC algorithm is
Figure BDA0002831874120000144
From the above formula, changing theta from-90 degrees to 90 degrees according to a certain step length, estimating an arrival angle by searching a peak, and obtaining MUSIC spectral functions shown as (a) to (g) in FIG. 3 respectively;
s6, since the number of array elements is M ═ 8, 7 arrival angle estimation results are obtained, and are expressed as
Figure BDA0002831874120000145
Figure BDA0002831874120000146
DOA1=[38.3°]I.e. the angle of arrival is 38.3 deg., the estimated number of signal sources is n1=1;
DOA2=[-60.9°,38.4°]That is, the arrival angles are-60.9 DEG and 38.4 DEG, respectively, and the estimated number of signal sources is n2=2;
DOA3=[-61.4°,17.4°,37.2°]That is, the arrival angles are-61.4 deg., 17.4 deg., 37.2 deg., respectively, and the estimated number of signal sources is n3=3;
DOA4=[-60.0°,15.0°,29.9°,45.0°]That is, the arrival angles are-60.0 degrees, 15.0 degrees, 29.9 degrees and 45.0 degrees, respectively, and the estimated number of signal sources is n4=4;
DOA5=[-60.0°,15.0°,30.0°,45.0°]That is, the arrival angles are-60.0 degrees, 15.0 degrees, 30.0 degrees and 45.0 degrees, respectively, and the estimated number of signal sources is n5=4;
DOA6=[-60.0°,15.0°,29.9°,44.9°]That is, the arrival angles are-60.0 °,15.0 °,29.9 °, and 44.9 °, respectively, and the estimated number of signal sources is n6=4;
DOA7=[-60.0°,-14.4°,14.9°,29.8°,44.8°]I.e. the angles of arrival are-60.0 deg. -14.4 deg., 14.9 deg., 29.8 deg., 44.8 deg., respectively, and the estimated number of signal sources is n7=5;
S7, mixing
Figure BDA0002831874120000151
Figure BDA0002831874120000152
Form a row vector, denoted ne=[1,2,3,4,4,4,5]Counting the number of the signal sources which appear most from the vector as the final estimated number of the signal sources
Figure BDA0002831874120000153
It is obvious that
Figure BDA0002831874120000154
The number of times num of occurrence is 3; the DOA estimation results with 4 signal sources (namely 4 spectrum peaks) are respectively set as 4 th, 5 th and 6 th
Figure BDA0002831874120000155
Vector formed by the angle of arrival of the 3 groups of signals
Figure BDA0002831874120000156
Averaging to obtain the final signal arrival angle estimation value expressed as
Figure BDA0002831874120000157
The actual number of the signal sources is determined to be 4, the incoming wave angles of the signal sources are-60 degrees, 15 degrees, 30 degrees and 45 degrees respectively, and the estimation result and the actual result are compared, so that the arrival direction estimation method can realize accurate estimation of the number of the signal sources and realize estimation of the arrival angle of the signal with small error.
In the above embodiments, step S4 provides a steering vector matrix of uniform linear arrays; the technical scheme of the invention is also suitable for uniform circular arrays.
The above description is only a preferred embodiment of the present invention, and not intended to limit the present invention, and all equivalent changes and modifications made within the scope of the claims of the present invention should fall within the protection scope of the present invention.

Claims (4)

1. An improved MUSIC direction of arrival estimation method is characterized in that: which comprises the following steps:
s1, constructing a far-field signal DOA estimation model
Set with K far-field signals from the direction theta12,…,θKIncident on an array consisting of M sensors, and observing signals of the array at the time t are X (t) and are expressed as
Figure FDA0002831874110000011
Wherein X (t) ═ X1(t),X2(t),…,XM(t)]TFor array observation signal vectors, T represents transposition;
a(θk) Is an array direction vector;
A(θ)=[a(θ1),a(θ2),…,a(θK)]a steering vector matrix formed by the direction vectors;
θ=[θ12,…,θK]Tis the parameter vector of the incoming wave angle of the signal;
S(t)=[s1(t),s2(t),…,sK(t)]Tis an incident signal vector;
k is the number of signals;
N(t)=[n1(t),n2(t),…,nM(t)]Tfor additive noise vectors, sample point T is 1,2, …, T1,T1Counting the number of signal sampling points;
s2, calculating a covariance matrix R of the array observation signals X (t) in the step S1, and performing feature decomposition on the covariance matrix;
s3, presetting the number of signal sources, and obtaining the noise subspace
Setting the number of signal sources as
Figure FDA0002831874110000012
The range of variation is
Figure FDA0002831874110000013
Wherein M is the number of antenna elements of the array antenna;
in setting the number of signal sources
Figure FDA0002831874110000014
On the basis of (1), a noise subspace is obtained, the expression of which is
Figure FDA0002831874110000015
Wherein λ ispAnd epRespectively carrying out characteristic value decomposition on the covariance matrix R to obtain a pth characteristic value and a characteristic vector;
s4, theoretically, under the condition that the signal sources are independent and have no noise, the signal subspace ESAnd noise subspace EN′Orthogonal, it is known that the steering vector in the signal subspace is also orthogonal to the noise subspace, i.e.
aH(θ)EN′=0 (7)
Wherein the steering vector matrix
aH(θ)=[exp(-j2πfτ1k),exp(-j2πfτ2k),…,exp(-j2πfτMk)]H
Figure FDA0002831874110000021
The time delay of the kth signal reaching the mth array element relative to the 1 st array element, M is 1,2, …, M, K is 1,2, …, K;
c is the speed of light;
d is the interval between adjacent array elements;
s5, in practice, the vector a is guided by the presence of noiseH(theta) and noise subspace EN′And cannot be completely orthogonal, so DOA is realized by taking the maximum value of the spatial spectrum, and the calculation formula of the spatial spectrum estimation by applying the MUSIC algorithm is
Figure FDA0002831874110000022
Changing theta from-90 degrees to 90 degrees according to a certain step length by the above formula, and estimating an arrival angle by searching a peak;
s6, setting different
Figure FDA0002831874110000023
Different arrival angle estimation results are obtained according to the formula (8) in the step S5;
Figure FDA0002831874110000024
sequentially taking values from 1 to M-1 to obtain M-1 kinds of arrival angle estimation results, which are expressed as
Figure FDA0002831874110000025
Figure FDA0002831874110000026
Figure FDA0002831874110000027
The number of angles of (a) represents the number of estimated signal sources, the angle value represents the incoming wave direction of the signal source, and the setting is based on
Figure FDA0002831874110000028
The number of the judged signal sources is
Figure FDA0002831874110000029
Angle of arrival of signal of
Figure FDA00028318741100000210
S7, mixing
Figure FDA00028318741100000211
Form a row vector, denoted ne=[n1,n2,…,nM-1]Counting the number of the signal sources which appear most from the vector as the final estimated number of the signal sources
Figure FDA00028318741100000212
The number appearing in the vector
Figure FDA00028318741100000213
The serial number positions are marked, and the serial numbers are
Figure FDA00028318741100000214
The number of occurrences is given as num; to obtain
Figure FDA00028318741100000215
Then, will correspond to the number
Figure FDA00028318741100000216
The arrival angles of the signals form a row vector represented as
Figure FDA00028318741100000217
Vector formed by num group signal arrival angles
Figure FDA0002831874110000031
Averaging to obtain the final signal arrival angle estimation value expressed as
Figure FDA0002831874110000032
Obtaining the number of the signal sources estimated finally
Figure FDA0002831874110000033
And the final estimated angle of arrival
Figure FDA0002831874110000034
2. The improved MUSIC direction of arrival estimation method of claim 1, wherein: in step S1, the far-field signals are mutually independent narrow-band stationary signals, and satisfy the mean value E { S (t) ═ 0} and the covariance matrix
Figure FDA0002831874110000035
Wherein
Figure FDA0002831874110000036
Is the power of the kth signal; the superimposed noise in the array observation signal vector is additive white Gaussian noise and is independent from the signal; the number of far-field signals is less than the number of array elements and the number of sampling points, i.e. K<min(M,T1) (ii) a The signals are propagated in an ideal space, and the array sensor has omnidirectional consistency.
3. The improved MUSIC direction of arrival estimation method of claim 1, wherein: in step S2, a covariance matrix of the array observation signal x (t) is calculated, which is expressed as:
R=E[XXH]=AE[SSH]AH+E[NNH]=ARSAH+RN (2)
wherein R isSAnd RNAre respectively a signalCovariance matrix and noise covariance matrix, H represents conjugate transpose; since the signal and the noise are independent of each other, the data covariance matrix is decomposed into two parts, AR, related to the signal and the noiseSAHIs a signal portion; for spatially perfect white noise, and the noise power is σ2Then, there are:
R=ARSAH+RN=ARSAH2I (3)
and (3) performing characteristic decomposition on the covariance matrix R, namely:
R=ARSAH+RN=Q∑QH (4)
wherein, matrix Q is the eigenvector matrix, diagonal matrix sigma is formed by the eigenvalue, namely:
Figure FDA0002831874110000037
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λKK+1≈…≈λM≈σ2
the steering vector matrix A is a Van der Monte matrix, provided that the target signal direction θi≠θp(i ≠ p), wherein i and p respectively represent the serial numbers of the signals, and K characteristic values corresponding to different target signals are total;
corresponding to the characteristic value lambdaiI is 1,2, …, M, and its feature vector is ei,i=1,2,…,M。
4. The improved MUSIC direction of arrival estimation method of claim 1, wherein: the number K of signal sources is at most half of the number of antenna elements, i.e.
Figure FDA0002831874110000041
Indicating a rounding down.
CN202011450983.0A 2020-12-11 2020-12-11 Improved MUSIC (multiple input multiple output) direction-of-arrival estimation method Active CN112666513B (en)

Priority Applications (1)

Application Number Priority Date Filing Date Title
CN202011450983.0A CN112666513B (en) 2020-12-11 2020-12-11 Improved MUSIC (multiple input multiple output) direction-of-arrival estimation method

Applications Claiming Priority (1)

Application Number Priority Date Filing Date Title
CN202011450983.0A CN112666513B (en) 2020-12-11 2020-12-11 Improved MUSIC (multiple input multiple output) direction-of-arrival estimation method

Publications (2)

Publication Number Publication Date
CN112666513A true CN112666513A (en) 2021-04-16
CN112666513B CN112666513B (en) 2024-05-07

Family

ID=75402323

Family Applications (1)

Application Number Title Priority Date Filing Date
CN202011450983.0A Active CN112666513B (en) 2020-12-11 2020-12-11 Improved MUSIC (multiple input multiple output) direction-of-arrival estimation method

Country Status (1)

Country Link
CN (1) CN112666513B (en)

Cited By (4)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN113286363A (en) * 2021-07-23 2021-08-20 网络通信与安全紫金山实验室 Wireless positioning parameter estimation method and device, computer equipment and storage medium
CN114578282A (en) * 2022-03-01 2022-06-03 中国海洋大学 DOA estimation method applied to non-fixed phase center antenna array
CN114745240A (en) * 2022-04-08 2022-07-12 展讯通信(上海)有限公司 Method and device for determining frequency offset value of signal
CN116047404A (en) * 2023-03-29 2023-05-02 南京邮电大学 Arrival angle measurement method based on Pmatic spectrum peak diagram

Citations (21)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US20030012262A1 (en) * 2001-04-27 2003-01-16 Mitsubishi Denki Kabushiki Kaisha Method for estimating a direction of arrival
JP2006078331A (en) * 2004-09-09 2006-03-23 Oki Electric Ind Co Ltd Signal source direction estimation method and its device
WO2006067869A1 (en) * 2004-12-24 2006-06-29 Fujitsu Limited Arriving correction deducing device and program
EP1821445A1 (en) * 2006-02-16 2007-08-22 Siemens S.p.A. Method to improve the channel estimate in broadband simo/mimo cellular radio networks during abrupt interference variations
US20150362580A1 (en) * 2014-06-11 2015-12-17 Agency For Defense Development Method for estimating angle of arrival of multi-target moving at high speed
CN106443568A (en) * 2016-09-09 2017-02-22 上海电机学院 Missile-borne array passive direction finding method
CN106802402A (en) * 2017-03-09 2017-06-06 西安电子科技大学 DOA estimation method based on dual-layer Parallel circular array antenna
CN106970349A (en) * 2017-03-23 2017-07-21 南京航空航天大学 A kind of ADS B signal Wave arrival direction estimating methods based on improved MUSIC algorithms
CN107092007A (en) * 2017-05-25 2017-08-25 电子科技大学 A kind of Wave arrival direction estimating method of virtual second order array extension
CN107290709A (en) * 2017-05-05 2017-10-24 浙江大学 The relatively prime array Wave arrival direction estimating method decomposed based on vandermonde
CN109188344A (en) * 2018-08-23 2019-01-11 北京邮电大学 Based on mutually circulation correlation MUSIC algorithm information source number and arrival bearing's angular estimation method under impulse noise environment
CN109633558A (en) * 2018-10-25 2019-04-16 上海无线电设备研究所 A kind of DOA estimation algorithm based on polarization time-frequency distributions
CN109633522A (en) * 2018-12-26 2019-04-16 西安烽火电子科技有限责任公司 Wave arrival direction estimating method based on improved MUSIC algorithm
CN109709510A (en) * 2018-12-24 2019-05-03 贵州航天计量测试技术研究所 A kind of estimation method and system of coherent 2-d direction finding
CN110007266A (en) * 2019-04-22 2019-07-12 哈尔滨工程大学 A kind of General Cell coherent source direction-finding method under impact noise
CN110031794A (en) * 2019-04-16 2019-07-19 中国人民解放军国防科技大学 Coherent information source DOA estimation method based on difference common matrix reconstruction
CN110895325A (en) * 2019-11-28 2020-03-20 宁波大学 Arrival angle estimation method based on enhanced quaternion multiple signal classification
CN111007488A (en) * 2019-11-21 2020-04-14 中国人民解放军63892部队 Information source number estimation method based on Gerr circle transformation and modified Rao score test
CN111046591A (en) * 2019-12-31 2020-04-21 哈尔滨工程大学 Joint estimation method for sensor amplitude-phase error and target arrival angle
CN111596285A (en) * 2019-11-21 2020-08-28 中国人民解放军63892部队 Information source number estimation method based on characteristic value to angular loading and construction of second-order statistics
CN111693937A (en) * 2020-05-25 2020-09-22 西安交通大学 Near-field signal source positioning method based on sparse reconstruction and without gridding

Patent Citations (21)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US20030012262A1 (en) * 2001-04-27 2003-01-16 Mitsubishi Denki Kabushiki Kaisha Method for estimating a direction of arrival
JP2006078331A (en) * 2004-09-09 2006-03-23 Oki Electric Ind Co Ltd Signal source direction estimation method and its device
WO2006067869A1 (en) * 2004-12-24 2006-06-29 Fujitsu Limited Arriving correction deducing device and program
EP1821445A1 (en) * 2006-02-16 2007-08-22 Siemens S.p.A. Method to improve the channel estimate in broadband simo/mimo cellular radio networks during abrupt interference variations
US20150362580A1 (en) * 2014-06-11 2015-12-17 Agency For Defense Development Method for estimating angle of arrival of multi-target moving at high speed
CN106443568A (en) * 2016-09-09 2017-02-22 上海电机学院 Missile-borne array passive direction finding method
CN106802402A (en) * 2017-03-09 2017-06-06 西安电子科技大学 DOA estimation method based on dual-layer Parallel circular array antenna
CN106970349A (en) * 2017-03-23 2017-07-21 南京航空航天大学 A kind of ADS B signal Wave arrival direction estimating methods based on improved MUSIC algorithms
CN107290709A (en) * 2017-05-05 2017-10-24 浙江大学 The relatively prime array Wave arrival direction estimating method decomposed based on vandermonde
CN107092007A (en) * 2017-05-25 2017-08-25 电子科技大学 A kind of Wave arrival direction estimating method of virtual second order array extension
CN109188344A (en) * 2018-08-23 2019-01-11 北京邮电大学 Based on mutually circulation correlation MUSIC algorithm information source number and arrival bearing's angular estimation method under impulse noise environment
CN109633558A (en) * 2018-10-25 2019-04-16 上海无线电设备研究所 A kind of DOA estimation algorithm based on polarization time-frequency distributions
CN109709510A (en) * 2018-12-24 2019-05-03 贵州航天计量测试技术研究所 A kind of estimation method and system of coherent 2-d direction finding
CN109633522A (en) * 2018-12-26 2019-04-16 西安烽火电子科技有限责任公司 Wave arrival direction estimating method based on improved MUSIC algorithm
CN110031794A (en) * 2019-04-16 2019-07-19 中国人民解放军国防科技大学 Coherent information source DOA estimation method based on difference common matrix reconstruction
CN110007266A (en) * 2019-04-22 2019-07-12 哈尔滨工程大学 A kind of General Cell coherent source direction-finding method under impact noise
CN111007488A (en) * 2019-11-21 2020-04-14 中国人民解放军63892部队 Information source number estimation method based on Gerr circle transformation and modified Rao score test
CN111596285A (en) * 2019-11-21 2020-08-28 中国人民解放军63892部队 Information source number estimation method based on characteristic value to angular loading and construction of second-order statistics
CN110895325A (en) * 2019-11-28 2020-03-20 宁波大学 Arrival angle estimation method based on enhanced quaternion multiple signal classification
CN111046591A (en) * 2019-12-31 2020-04-21 哈尔滨工程大学 Joint estimation method for sensor amplitude-phase error and target arrival angle
CN111693937A (en) * 2020-05-25 2020-09-22 西安交通大学 Near-field signal source positioning method based on sparse reconstruction and without gridding

Non-Patent Citations (9)

* Cited by examiner, † Cited by third party
Title
YA LING CHEN: "Estimating direction of arrival for coherent signals by using projection subspace without source number information", 《2016 INTERNATIONAL CONFERENCE ON ADVANCED MATERIALS FOR SCIENCE AND ENGINEERING (ICAMSE)》, 6 February 2017 (2017-02-06), pages 9 - 12 *
冯伟: "高分辨阵列测向技术研究", 《中国优秀硕士学位论文全文数据库 信息科技辑》, 15 February 2016 (2016-02-15), pages 136 - 915 *
尹广旭: "基于多重信号分类算法的宽带相干源空间谱估计", 《中国优秀硕士学位论文全文数据库 信息科技辑》, 15 August 2013 (2013-08-15), pages 136 - 122 *
曾勇虎: "基于双极化融合的外辐射源雷达实验分析", 《现代雷达》, 15 October 2017 (2017-10-15), pages 11 - 15 *
李晗静: "基于极化敏感阵列的测向技术研究", 《中国优秀硕士学位论文全文数据库 信息科技辑》, 15 January 2020 (2020-01-15), pages 136 - 90 *
潘捷: "非线性阵列Khatri-Rao子空间宽带DOA估计", 《应用科学学报》, 30 March 2013 (2013-03-30), pages 159 - 164 *
王炎: "极化敏感阵列的二维DOA与极化参数估计算法研究", 《中国博士学位论文全文数据库 信息科技辑》, 25 May 2020 (2020-05-25), pages 136 - 14 *
陈明建: "基于空间差分平滑的非相关与相干信源数估计", 《火力与指挥控制》, 15 January 2019 (2019-01-15), pages 51 - 56 *
韩强强: "多信号识别与压制式干扰测向技术研究", 《中国优秀硕士学位论文全文数据库 信息科技辑》, 15 April 2014 (2014-04-15), pages 136 - 73 *

Cited By (4)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN113286363A (en) * 2021-07-23 2021-08-20 网络通信与安全紫金山实验室 Wireless positioning parameter estimation method and device, computer equipment and storage medium
CN114578282A (en) * 2022-03-01 2022-06-03 中国海洋大学 DOA estimation method applied to non-fixed phase center antenna array
CN114745240A (en) * 2022-04-08 2022-07-12 展讯通信(上海)有限公司 Method and device for determining frequency offset value of signal
CN116047404A (en) * 2023-03-29 2023-05-02 南京邮电大学 Arrival angle measurement method based on Pmatic spectrum peak diagram

Also Published As

Publication number Publication date
CN112666513B (en) 2024-05-07

Similar Documents

Publication Publication Date Title
CN112666513B (en) Improved MUSIC (multiple input multiple output) direction-of-arrival estimation method
CN110045323B (en) Matrix filling-based co-prime matrix robust adaptive beamforming algorithm
CN109116293A (en) A kind of Wave arrival direction estimating method based on sparse Bayesian out of place
CN109946643B (en) Non-circular signal direction-of-arrival angle estimation method based on MUSIC solution
CN112379327A (en) Two-dimensional DOA estimation and cross coupling correction method based on rank loss estimation
CN107037398B (en) Parallel computing method for estimating direction of arrival by two-dimensional MUSIC algorithm
Li et al. Combining sum-difference and auxiliary beams for adaptive monopulse in jamming
CN113253194A (en) Broadband arrival angle and polarization combined measurement method based on sparse representation
CN113835063B (en) Unmanned aerial vehicle array amplitude and phase error and signal DOA joint estimation method
Zhao et al. Two-dimensional DOA estimation with reduced-dimension MUSIC algorithm
CN111366893A (en) Non-circular signal azimuth angle estimation method under unknown mutual coupling condition of uniform circular array
CN113625220A (en) New method for quickly estimating direction of arrival and diffusion angle of multipath signal
Abdullah et al. Comparative Study of Super-Performance DOA Algorithms based for RF Source Direction Finding and Tracking
CN112763972B (en) Sparse representation-based double parallel line array two-dimensional DOA estimation method and computing equipment
Chen et al. Capon-like method for direction of arrival estimation Using acoustics vector sensor
Chen et al. Joint design of transmit sequence and receive filter based on Riemannian manifold of Gaussian mixture distribution for MIMO radar
CN112363108A (en) Signal subspace weighted super-resolution direction-of-arrival detection method and system
CN114460531A (en) Uniform linear array MUSIC spatial spectrum estimation method
CN113702898B (en) Method for estimating direction of arrival of known waveform source based on distributed array
CN113311383B (en) Antenna direction finding and polarization parameter joint estimation method based on rectangular array
CN115656918A (en) Far-field target azimuth estimation method suitable for small samples
CN115085827B (en) Underwater sound target array amplitude phase error calibration method based on rank-one decomposition theorem
CN113359086B (en) Weighted subspace data fusion direct positioning method based on augmented mutual mass array
Zhao et al. Fast DOA Estimation Algorithm Based on Phase Coded MIMO Radar
CN114184999B (en) Method for processing generated model of cross-coupling small-aperture array

Legal Events

Date Code Title Description
PB01 Publication
PB01 Publication
SE01 Entry into force of request for substantive examination
SE01 Entry into force of request for substantive examination
GR01 Patent grant