CN112666513A - Improved MUSIC direction of arrival estimation method - Google Patents
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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
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 theta1,θ2,…,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
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=[θ1,θ2,…,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=ARSAH+σ2I (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:
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λK>λK+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 asThe range of variation isWherein M is the number of antenna elements of the array antenna;
in setting the number of signal sourcesOn the basis of (1), a noise subspace is obtained, the expression of which is
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,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
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 toThus, the settings are differentDifferent arrival angle estimation results are obtained according to the formula (8) in the step S5;sequentially taking values from 1 to M-1 to obtain M-1 kinds of arrival angle estimation results, which are expressed as 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 onThe number of the judged signal sources isAngle of arrival of signal of
S7, mixingForm 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 sourcesThe number appearing in the vectorThe serial number positions are marked, and the serial numbers areThe number of occurrences is given as num; to obtainThen, will correspond to the numberThe arrival angles of the signals form a row vector represented asVector formed by num group signal arrival anglesAveraging to obtain the final signal arrival angle estimation value expressed as
Obtaining the number of the signal sources estimated finallyAnd the final estimated angle of arrival
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 matrixWhereinIs 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 Forming a column vector, counting the most appeared numbers from the column vector as the number of the signal sources to be finally estimated
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 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 asT1Is a signalThe noise is complex Gaussian white noise, and the input signal-to-noise ratio (SNR) is defined asWhereinAndrepresenting 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 theta1,θ2,θ3Incident on an array of 8 sensors, and the observed signal of the array at time t is X (t) and is expressed as
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=[θ1,θ2,θ3]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=ARSAH+σ2I (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:
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥λ3>λ4≈…≈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
in setting the number of signal sourcesOn the basis of (1), a noise subspace is obtained, the expression of which is
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,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
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
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 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 sourcesIt is obvious thatThe 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
Vector formed by the arrival angles of the 6 groups of signalsAveraging to obtain the final signal arrival angle estimation value expressed as
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
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=ARSAH+σ2I (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:
in the equation (5), the characteristic values satisfy the following relationship:
λ1>λ2≈…≈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
in setting the number of signal sourcesOn the basis of (1), a noise subspace is obtained, the expression of which is
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,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
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
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 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 sourcesIt is obvious thatThe 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
Vector formed by the angle of arrival of the 3 groups of signalsAveraging to obtain the final signal arrival angle estimation value expressed as
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 theta1,θ2,θ3,θ4Incident on an array of 8 sensors, and the observed signal of the array at time t is X (t) and is expressed as
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=[θ1,θ2,θ3,θ4]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=ARSAH+σ2I (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:
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λ4>λ5≈…≈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
in setting the number of signal sourcesOn the basis of (1), a noise subspace is obtained, the expression of which is
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,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
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
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 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 sourcesIt is obvious thatThe 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
Vector formed by the angle of arrival of the 3 groups of signalsAveraging to obtain the final signal arrival angle estimation value expressed as
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 theta1,θ2,…,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
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=[θ1,θ2,…,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 asThe range of variation isWherein M is the number of antenna elements of the array antenna;
in setting the number of signal sourcesOn the basis of (1), a noise subspace is obtained, the expression of which is
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,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
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 differentDifferent arrival angle estimation results are obtained according to the formula (8) in the step S5;sequentially taking values from 1 to M-1 to obtain M-1 kinds of arrival angle estimation results, which are expressed as 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 onThe number of the judged signal sources isAngle of arrival of signal of
S7, mixingForm 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 sourcesThe number appearing in the vectorThe serial number positions are marked, and the serial numbers areThe number of occurrences is given as num; to obtainThen, will correspond to the numberThe arrival angles of the signals form a row vector represented asVector formed by num group signal arrival anglesAveraging to obtain the final signal arrival angle estimation value expressed as
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 matrixWhereinIs 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=ARSAH+σ2I (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:
in the equation (5), the characteristic values satisfy the following relationship:
λ1≥λ2≥…≥λK>λK+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。
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Cited By (4)
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 |
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Citations (21)
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 |
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 |
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 |
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 |
-
2020
- 2020-12-11 CN CN202011450983.0A patent/CN112666513B/en active Active
Patent Citations (21)
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)
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)
Publication number | Priority date | Publication date | Assignee | Title |
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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 |
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