CN1773307A - Aperture Expansion and Spatial Signal Processing Method of Small Antenna Array - Google Patents

Aperture Expansion and Spatial Signal Processing Method of Small Antenna Array Download PDF

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CN1773307A
CN1773307A CN 200510019633 CN200510019633A CN1773307A CN 1773307 A CN1773307 A CN 1773307A CN 200510019633 CN200510019633 CN 200510019633 CN 200510019633 A CN200510019633 A CN 200510019633A CN 1773307 A CN1773307 A CN 1773307A
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CN100380134C (en
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高火涛
张小林
陈丽
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Wuhan University WHU
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Abstract

The present invention relates to a small type antenna array aperture expanding and space signal processing method. Said method includes the following steps: making antenna array into any array form: dividing scanning area of whole antenna into several subregions, finely-dividing any one subregion of said several subregions; in the finely-divided subregion constructing actual array flow form of antenna array and array flow form of expanded array so as to further obtain the array expansion conversion matrix; utilizing the obtained array expansion conversion matrix to reconstitute the signal of expanded antenna array; then making said signal undergo the process of digital beam formation or adaptive beam formation or utilizing space high resolution algorithm to obtain space arrival angle of signal.

Description

小型天线阵口径扩展与空间信号处理方法Aperture Expansion and Spatial Signal Processing Method of Small Antenna Array

技术领域technical field

本发明涉及一种小型天线阵口径扩展与空问信号处理方法。The invention relates to a small antenna array aperture expansion and space signal processing method.

背景技术Background technique

根据经典的天线理论,雷达的角分辨率与天线波束宽度有关,雷达天线波束宽度与天线电长度近似成反比,即According to the classical antenna theory, the angular resolution of the radar is related to the antenna beam width, and the radar antenna beam width is approximately inversely proportional to the electrical length of the antenna, that is

θ 3 dB ∝ λ L (弧度) θ 3 dB ∝ λ L (radian)

其中,θ3dB为天线波束半功率宽度,λ为雷达工作波长,L为天线阵列长度。当天线单元之间的间距为雷达工作波长的一半左右时,要获得高的角分辨率,就需采用大型相控阵天线和大量的接收通道。但在雷达天线阵地受限的场合,例如,对于高频地波或高频天波超视距雷达,为了获得高分辨的海洋表面流和海面目标方位信息,一般采用(多重信号分类算法)MUSIC等高分辨算法,为了获得高分辨的海面风浪信息,一般采用DBF技术。例如,如果高频雷达工作为频率为5MHz,要想获得1°的角分辨率,雷达天线阵长将达3000米。而且,为了能有效地激起沿海面传播的表面波,雷达天线阵应尽可能地靠近海水设置,这一距离通常要求1~2个雷达波长,这在实际海岸条件下,不仅难以找到能与大型天线阵相配套的天线场地,而且极大地增加了雷达建站费用和日常的维护费。同时由于雷达天线阵过大,其远场范围达数千米,对雷达系统的校准也极为困难。所有这些都将限制了包括高频表面波雷达在内的许多雷达的推广应用。Among them, θ 3dB is the half-power width of the antenna beam, λ is the working wavelength of the radar, and L is the length of the antenna array. When the spacing between antenna elements is about half of the operating wavelength of the radar, a large phased array antenna and a large number of receiving channels are required to obtain high angular resolution. However, in the case where the radar antenna position is limited, for example, for high-frequency ground wave or high-frequency sky-wave over-the-horizon radar, in order to obtain high-resolution ocean surface current and sea surface target orientation information, (Multiple Signal Classification Algorithm) MUSIC etc. are generally used High-resolution algorithm, in order to obtain high-resolution sea surface wind and wave information, DBF technology is generally used. For example, if a high-frequency radar operates at a frequency of 5MHz, to obtain an angular resolution of 1°, the radar antenna array length will reach 3000 meters. Moreover, in order to effectively excite the surface waves propagating along the sea surface, the radar antenna array should be set as close to the sea water as possible. This distance usually requires 1 to 2 radar wavelengths. Under actual coastal conditions, it is not only difficult to find Antenna sites that are matched with large antenna arrays also greatly increase the cost of radar station construction and daily maintenance costs. At the same time, because the radar antenna array is too large, its far-field range reaches several kilometers, and it is extremely difficult to calibrate the radar system. All of these will limit the popularization and application of many radars including high frequency surface wave radar.

发明内容Contents of the invention

针对现有多通道大型相控阵雷达的局限性,本发明的目的是提供一种小型天线阵口径扩展与空间信号处理方法,该方法利用阵列扩展技术来实现只有大型相控阵雷达才能实现的功能。Aiming at the limitations of the existing multi-channel large-scale phased array radar, the purpose of the present invention is to provide a small-scale antenna array aperture expansion and space signal processing method, which uses the array expansion technology to realize what only large-scale phased-array radars can achieve. Function.

为了实现上述目的,本发明提供一种小型天线阵口径扩展与空间信号处理方法,将天线阵列设置为任意阵列形式;将整个天线扫描区域划分为若干区域,再将其中任一个子区域细分:在细分的子区域内构建天线阵列的实际阵流形A=[a(θ1),a(θ1+Δθ),a(θ2+2Δθ),…,a(θr)]和扩展阵列的阵流形 A=[a(θ1), a(θ1+Δθ), a(θ2+2Δθ),…, a(θr)],进而得到阵列扩展变换矩阵B= AA-1,其中,θ1,θr分别为子区域的左右边界,Δθ为子区域细分的步长;利用已获得的阵列扩展变换矩阵重构出扩展阵列天线的信号Z=BX,其中,X为原始天线阵接收的信号;将重构的扩展阵列天线的信号Z进行数字波束形成或自适应波束形成或利用空间高分辨算法求出信号的空间到达角。In order to achieve the above object, the present invention provides a small antenna array aperture expansion and space signal processing method, the antenna array is set to any array form; the entire antenna scanning area is divided into several areas, and any sub-area is subdivided: Construct the actual array manifold A=[a(θ 1 ), a(θ 1 +Δθ), a(θ 2 +2Δθ),…, a(θ r )] and extended Array manifold A=[a(θ 1 ), a(θ 1 +Δθ), a(θ 2 +2Δθ),…, a(θ r )], and then the array expansion transformation matrix B= AA -1 , where θ 1 and θ r are the left and right boundaries of the sub-region respectively, and Δθ is the subdivision step size of the sub-region; the signal Z=BX of the extended array antenna is reconstructed by using the obtained array expansion transformation matrix, where X is The signal received by the original antenna array; the signal Z of the reconstructed extended array antenna is subjected to digital beamforming or adaptive beamforming, or the spatial angle of arrival of the signal is obtained by using a spatial high-resolution algorithm.

按照本发明,当实际阵流形A是非方阵时,将矩阵A进行对角加载。According to the present invention, when the actual matrix manifold A is a non-square matrix, the matrix A is loaded diagonally.

另外,本发明可利用‖ A-BA‖的范数最小值,确定扩展阵列的单元数。In addition, the present invention can utilize ‖ The minimum value of the norm of A-BA‖, which determines the number of elements of the extended array.

本发明的优势在于其出色的实用性能:(1)通过上述方法大大扩展了天线阵的口径和天线阵元数;(2)利用软件独特的优势,重构扩展天线单元的信号,使之能够灵活地运用现代数字信号处理技术,进行数字波束形成、波束形状的改变、空间超分辨测向和天线自适应抗干扰;(3)由于天线口径扩展是建立在软件的基础上,可以大大减少天线单元数和接收通道,极大地降低了研发成本和建站费用;(4)通过对小型任意天线阵实施扩展变换,与原始阵相比,它不仅增加了可检测的信源数,提高了天线阵的过载能力,而且可克服阵列可能出现的信号模糊问题,提高了阵列的解相干能力。The advantage of the present invention lies in its excellent practical performance: (1) the caliber of the antenna array and the number of elements of the antenna array are greatly expanded by the above method; Flexible use of modern digital signal processing technology for digital beamforming, beam shape change, spatial super-resolution direction finding and antenna adaptive anti-interference; (3) Since the antenna aperture expansion is based on software, it can greatly reduce the number of antennas The number of units and receiving channels greatly reduces the cost of research and development and site construction; (4) By implementing extended transformations on small arbitrary antenna arrays, compared with the original array, it not only increases the number of detectable sources, but also improves the quality of antenna arrays. The overload capability of the array can be overcome, and the signal ambiguity problem that may occur in the array can be overcome, and the decoherence ability of the array is improved.

本发明针对雷达天线布阵受限制的特殊场合,打破一般相控阵雷达设计的老程式,提出了一种通过对小型密集相控阵天线实施扩展变换以增加天线阵孔径的方法,为相控阵雷达减少天线单元和接收通道,降低成本、简单易建提供了新途径。本发明不仅适于均匀阵列,还适于任意非均匀阵列,扩展后的天线口径相当于三倍以上的原天线口径所达到的性能。将之应用于高频地波超视距雷达,通过扩展后的天线阵列,不仅可以获得高分辨的海洋表面流和海面目标的方位信息,还可以形成相对窄的波束,获得满足海洋工程要求的风浪信息。本发明为雷达天线阵小型化提供了理论和工程依据。Aiming at the special occasions where the radar antenna array is limited, the present invention breaks the old formula of general phased array radar design, and proposes a method of increasing the aperture of the antenna array by performing extended transformation on the small dense phased array antenna. Array radar reduces antenna units and receiving channels, reduces cost, and provides a new way to be simple and easy to build. The invention is not only suitable for uniform arrays, but also suitable for any non-uniform arrays, and the expanded antenna aperture is equivalent to the performance achieved by more than three times the original antenna aperture. Applying it to high-frequency ground-wave over-the-horizon radar, through the extended antenna array, not only can obtain high-resolution ocean surface currents and azimuth information of sea surface targets, but also form relatively narrow beams to obtain ocean engineering requirements. Storm information. The invention provides theoretical and engineering basis for the miniaturization of radar antenna array.

本发明应用于工程实际,不仅研发和设备维护费用相对低廉,在软件的灵活配合下,还具有目前传统大型相控阵雷达没有的功能。本发明对在天线阵地和电磁兼容受限的场合使用相控阵,对航空、航天、空防、海防等国防建设和经济建设,以及使相控阵雷达小型化和降低成本,具有重要的理论价值和工程意义。The invention is applied to engineering practice, and not only the research and development and equipment maintenance costs are relatively low, but also has functions that the current traditional large-scale phased array radar does not have under the flexible cooperation of software. The present invention has an important theory for the use of phased arrays in the occasions where antenna positions and electromagnetic compatibility are limited, for national defense construction and economic construction such as aviation, aerospace, air defense, and coastal defense, as well as for miniaturization and cost reduction of phased array radars. value and engineering significance.

大量的理论分析和雷达试验表明,通过本发明提出的阵列扩展,实现了天线阵元数的有效扩展,即通过阵列扩展变换使扩展阵列具有更多的阵元数,其优势是明显的,它不仅增加了可检测的信号源数即提高了阵列的过载能力,而且可克服阵列可能出现的信号模糊问题,提高了阵列的解相干能力,大大减少实际天线的口径和接收通道数,降低了雷达研制成本,满足了本发明提出的利用阵列扩展技术实现空间超分辨的要求。A large number of theoretical analysis and radar experiments show that the array expansion proposed by the present invention realizes the effective expansion of the number of antenna array elements, that is, the extended array has more array elements through the array expansion transformation, and its advantages are obvious. It not only increases the number of detectable signal sources, which improves the overload capability of the array, but also overcomes the possible signal ambiguity problem of the array, improves the decoherence capability of the array, greatly reduces the actual antenna aperture and the number of receiving channels, and reduces the radar The development cost satisfies the requirement of the present invention to realize spatial super-resolution by using the array extension technology.

附图说明Description of drawings

图1、图2和图3分别为扫描角为40°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 1, Figure 2 and Figure 3 are the Doppler spectra of the original array, extended array and traditional large array when the scanning angle is 40°;

图4、图5和图6分别为扫描角为60°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 4, Figure 5 and Figure 6 are the Doppler spectra of the original array, extended array and traditional large array when the scanning angle is 60°;

图7、图8和图9分别为扫描角为80°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 7, Figure 8 and Figure 9 are the Doppler spectra of the original array, extended array and traditional large array when the scan angle is 80°;

图10、图11和图12分别为扫描角为100°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 10, Figure 11 and Figure 12 are the Doppler spectra of the original array, extended array and traditional large array when the scanning angle is 100°;

图13、图14和图15分别为扫描角为120°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 13, Figure 14 and Figure 15 are the Doppler spectra of the original array, extended array and traditional large array when the scanning angle is 120°;

图16、图17和图18分别为扫描角为140°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 16, Figure 17 and Figure 18 are the Doppler spectra of the original array, extended array and traditional large array when the scan angle is 140°;

图19、图20和图21分别为信噪比为25dB、扫描角为40°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 19, Figure 20 and Figure 21 are the Doppler spectra of the original array, extended array and traditional large array when the signal-to-noise ratio is 25dB and the scan angle is 40°;

图22、图23和图24分别为信噪比为25dB、扫描角为60°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 22, Figure 23 and Figure 24 are the Doppler spectra of the original array, extended array and traditional large array when the signal-to-noise ratio is 25dB and the scan angle is 60°;

图25、图26和图27分别为信噪比为25dB、扫描角为80°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 25, Figure 26 and Figure 27 are the Doppler spectra of the original array, extended array and traditional large array when the signal-to-noise ratio is 25dB and the scan angle is 80°;

图28、图29和图30分别为信噪比为25dB、扫描角为100°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 28, Figure 29 and Figure 30 are the Doppler spectra of the original array, extended array and traditional large array when the signal-to-noise ratio is 25dB and the scan angle is 100°;

图31、图32和图33分别为信噪比为25dB、扫描角为120°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 31, Figure 32 and Figure 33 are the Doppler spectra of the original array, extended array and traditional large array when the signal-to-noise ratio is 25dB and the scanning angle is 120°;

图34、图35和图36分别为信噪比为25dB、扫描角为140°时的原阵、扩展阵和传统大型阵的Doppler谱;Figure 34, Figure 35 and Figure 36 are the Doppler spectra of the original array, the extended array and the traditional large array when the signal-to-noise ratio is 25dB and the scanning angle is 140°;

图37为原阵波束指向60°的Doppler谱;Figure 37 is the Doppler spectrum of the original array beam pointing at 60°;

图38为阵列扩展后波束指向60°的回波谱;Figure 38 is the echo spectrum of the beam pointing to 60° after the array is expanded;

图39为原阵波束指向120°的Doppler谱;Figure 39 is the Doppler spectrum of the original array beam pointing at 120°;

图40为阵列扩展后波束指向120°的回波谱;Figure 40 is the echo spectrum of the beam pointing to 120° after array expansion;

图41为阵列扩展前的MUSIC谱;Figure 41 is the MUSIC spectrum before array expansion;

图42为阵列扩展后的MUSIC谱。Figure 42 is the MUSIC spectrum after array expansion.

具体实施方式Detailed ways

下面结合附图和实施例,对本发明作更加详细的说明。The present invention will be described in more detail below in conjunction with the accompanying drawings and embodiments.

为了实现上述目的,本发明采用一种任意天线阵列口径扩展与空间超分辨方法,将天线阵列设置为任意阵列形式;将整个天线扫描区域划分为若干区域,再将某个子区域细分;通过实际阵列流形A和扩展阵流形 A之间的关系,获得阵列扩展变换矩阵B= AA-1;利用已获得的阵列扩展矩阵重构出扩展阵列天线的信号Z=BX(其中,X为原始天线阵接收的信号);将重构扩展阵列接收的数据Z进行波束形成,或利用空间高分辨算法求出信号的空间超分辨到达角。In order to achieve the above object, the present invention adopts an arbitrary antenna array aperture expansion and space super-resolution method, and the antenna array is set in an arbitrary array form; the entire antenna scanning area is divided into several areas, and then a certain sub-area is subdivided; through actual The relationship between the array manifold A and the extended array manifold A is obtained by obtaining the array extended transformation matrix B=AA -1 ; using the obtained array extended matrix to reconstruct the signal Z=BX of the extended array antenna (wherein, X is the original The signal received by the antenna array); beamforming the data Z received by the reconstructed extended array, or using a spatial high-resolution algorithm to obtain the spatial super-resolution angle of arrival of the signal.

1、原始阵列信号模型1. Original array signal model

不失一般性,假设空间阵由m个阵元组成,有d个信号源,信号以平面波形式入射到阵列上。则第i个阵元接收的数据为:Without loss of generality, it is assumed that the space array is composed of m array elements, and there are d signal sources, and the signals are incident on the array in the form of plane waves. Then the data received by the i-th array element is:

xx ii == ΣΣ kk == 11 dd ee -- jj ww 00 ττ ikik sthe s kk (( tt )) ++ nno ii (( tt )) ,, ii == 1,21,2 ,, ·&Center Dot; ·&Center Dot; ·· ,, mm -- -- -- (( 11 ))

则m个阵元在t时刻的输出快拍数据构成的矢量如下:Then the vector formed by the output snapshot data of m array elements at time t is as follows:

      X(t)=[x1(t),x2(t),...,xm(t)]T         (2)X(t)=[x 1 (t), x 2 (t), . . . , x m (t)] T (2)

A为阵列流形A is the array manifold

      A=[a(θ1),a(θ2),...,a(θd)]          (3)A=[a(θ 1 ), a(θ 2 ), . . . , a(θ d )] (3)

其中θk第k个入射信号的方向角,a(θi)如下式表示:Where θ k is the direction angle of the kth incident signal, a(θ i ) is expressed as follows:

aa (( θθ ii )) == [[ ee -- jj ww 00 ττ 11 ii ,, ee -- jj ww 00 ττ 22 ii ,, .. .. .. ,, ee -- jj ww 00 ττ mimi ]] TT -- -- -- (( 44 ))

τki=(xkcos(θi)+yksin(θi))/c为第i个信号在第k个阵元上的延迟,(xk,yk)为此阵元的位置坐标,c为光速。τ ki =(x k cos(θ i )+y k sin(θ i ))/c is the delay of the i-th signal on the k-th array element, and (x k , y k ) is the position of this array element coordinates, c is the speed of light.

即阵列接收的数据矩阵:That is, the array receives the data matrix:

             X=AS             (5)X=AS (5)

2.扩展阵列的设计2. Design of extended array

2.1阵列扩展变换方法2.1 Array expansion transformation method

对于不规则的密集阵或非均匀阵列,现通过数字变换的方法将原阵列数据变换为一个扩展的均匀线阵的输出。For irregular dense arrays or non-uniform arrays, the original array data is transformed into an output of an extended uniform linear array by means of digital transformation.

设扩展后的均匀线阵的信号方向矢量为Let the signal direction vector of the expanded uniform linear array be

        a(θ)=[1,exp(-jkd cosθ),...,exp(-jk(N-1)dcosθ)]     (6)其中d为扩展后天线阵的阵元间距。设有一个N×N阶非奇异矩阵T(Θ)满足如下关系`` a(θ)=[1, exp(-jkd cosθ),..., exp(-jk(N-1)dcosθ)] (6) where d is the element spacing of the extended antenna array. Suppose there is a non-singular matrix T(Θ) of order N×N that satisfies the following relationship

B(Θ)A(Θ)=[ a(θ1), a(θ2),..., a(θP)]= A(Θ)       (7)通过上式变换作用,矩阵B(Θ)就将原阵列的方向矩阵变换成了一个新均匀阵的方向矩阵,把像这样获得的新的均匀阵列我们称之为扩展阵列,而且一旦获得B(Θ)矩阵,即可得到扩展均匀线阵的输出矢量B(Θ)A(Θ)=[ a(θ 1 ), a(θ 2 ),..., a(θ P )]= A(Θ) (7) Through the transformation of the above formula, the matrix B(Θ ) transforms the direction matrix of the original array into a direction matrix of a new uniform array, we call the new uniform array obtained in this way an extended array, and once the B(Θ) matrix is obtained, the extended uniform line can be obtained output vector of array

                z(t)=B(Θ)x(t)                        (8)z(t)=B(Θ)x(t) (8)

2.2阵列变换矩阵的获得2.2 Obtaining the array transformation matrix

阵列扩展的处理思想是将整个天线扫描区域划分为若干个子区域,再将某个子区域细分。假设信号位于区域Θ内,将区域Θ均分为The processing idea of array extension is to divide the entire antenna scanning area into several sub-areas, and then subdivide a certain sub-area. Assuming that the signal is located in the area Θ, the area Θ is equally divided into

          Θ=[θ1,θ1+Δθ,θ1+2Δθ,...,θr]     (9)Θ=[θ 1 , θ 1 +Δθ, θ 1 +2Δθ,...,θ r ] (9)

θ1,θr为Θ为左右边界,Δθ为步长.则实际阵列的阵列流形矩阵为θ 1 , θ r is Θ is the left and right boundaries, Δθ is the step size. Then the array manifold matrix of the actual array is

          A=[a(θ1),a(θ1+Δθ),a(θ2+2Δθ),...,a(θr)]   (10)A=[a(θ 1 ), a(θ 1 +Δθ), a(θ 2 +2Δθ),..., a(θ r )] (10)

而在同一区域Θ内的扩展均匀线阵的阵列流形矩阵A为And the array manifold matrix A of the extended uniform linear array in the same area Θ is

           A=[ a(θ1), a(θ1+Δθ), a(θ2+2Δθ),…, a(θr)]   (11)A=[ a(θ 1 ), a(θ 1 +Δθ), a(θ 2 +2Δθ),…, a(θ r )] (11)

a(θi)如下式表示:a(θ i ) is represented by the following formula:

aa ‾‾ (( θθ ii )) == [[ ee -- jj ww 00 ΔΔ 11 ii ,, ee -- jj ww 00 ΔΔ 22 ii ,, .. .. .. ,, ee -- jj ww 00 ΔΔ nini ]] TT -- -- -- (( 1212 ))

其中,n为扩展阵列的阵元个数,Δki=(xxk cos(θi)+yyk sin(θi))/c为第i个信号在扩展阵列的第k个阵元上的延迟,(xxk,yyk)为此扩展阵元的位置坐标,c为光速。Among them, n is the number of array elements in the extended array, Δk i =(xx k cos(θ i )+yy k sin(θ i ))/c is the i-th signal on the k-th array element of the extended array Delay, (xx k , yy k ) is the position coordinate of the extended array element, and c is the speed of light.

则扩展的阵列与真实的阵列之间存在一个固定的变换关系B(T),使得BA= A_B= AA-1    (13)Then there is a fixed transformation relationship B(T) between the extended array and the real array, so that BA= A_B= AA -1 (13)

在上式中,涉及到对A的求逆。一般情况下,矩阵A不是方阵,不能直接求逆,因此我们采用对角加载技术,a为加载系数。In the above formula, it involves the inversion of A. In general, the matrix A is not a square matrix and cannot be directly inverted, so we use the diagonal loading technique, and a is the loading coefficient.

          C=A′*AC=A′*A

          A-1≈(C+a*eye(size(C,1)))-1*A′    (14)A -1 ≈(C+a*eye(size(C,1))) -1 *A′ (14)

假设某一矩阵Z满足Z=BX,Suppose a certain matrix Z satisfies Z=BX,

                 Z=BX= AA-1X= AA-1AS= AS     (15)Z=BX=AA -1 X=AA -1 AS= AS (15)

则Z可看作为由扩展阵列接收的数据。Then Z can be regarded as the data received by the expansion array.

2.3初始角和阵列扩展单元的确定2.3 Determination of initial angle and array expansion unit

从以上分析可知,扩展阵列的变换方法面临的首要问题就是初始角和天线单元数的确定,而信号源的方位角是待估计的参量,因此,在构造变换矩阵之前需要对方位角进行预估,而预估质量的好坏直接影响变换矩阵的优劣并最终影响估计结果。在实际应用中,一种简单的方法是,在对每个距离元空间信号进行处理时,可将整个天线扫描区按扩展阵列波束宽度划分为若干个雷达元,假设信号位于数字天线阵所在的数字波束区域内,然后计算 | | A ‾ ( Θ ^ ) - B ( Θ ^ ) A ( Θ ^ ) | | F 的范数,如果该值不是足够小,可以调整扩展天线的单元数、选择合适的波瓣宽度和信号初始角,然后再重新计算扩展变换矩阵

Figure A20051001963300072
以使 | | A ‾ ( Θ ^ ) - B ( Θ ^ ) A ( Θ ^ ) | | F 范数达到最小。From the above analysis, it can be seen that the primary problem faced by the transformation method of the extended array is the determination of the initial angle and the number of antenna elements, and the azimuth angle of the signal source is a parameter to be estimated. Therefore, the azimuth angle needs to be estimated before constructing the transformation matrix , and the quality of the prediction directly affects the quality of the transformation matrix and ultimately affects the estimation results. In practical applications, a simple method is to divide the entire antenna scanning area into several radar elements according to the beam width of the extended array when processing the spatial signal of each range element, assuming that the signal is located in the within the digital beam area, and then calculate | | A ‾ ( Θ ^ ) - B ( Θ ^ ) A ( Θ ^ ) | | f If the value is not small enough, you can adjust the number of elements of the extended antenna, select the appropriate lobe width and signal initial angle, and then recalculate the extended transformation matrix
Figure A20051001963300072
so that | | A ‾ ( Θ ^ ) - B ( Θ ^ ) A ( Θ ^ ) | | f Norm reaches the minimum.

2.4天线单元间距的确定2.4 Determination of antenna element spacing

进行阵列扩展首先要知道信号的初始方向,而初始角度估计

Figure A20051001963300074
总有误差,因此,设计扩展均匀线阵时,应该尽量选择对初始角度估计的误差最不敏感、形成的变换误差也最小的的阵列为扩展阵列。实际应用中,我们关心的是矩阵
Figure A20051001963300075
Figure A20051001963300076
的列空间是否一致。在列空间的意义上,矢量 与 a(θ)之间的距离可用两者之间的夹角
Figure A20051001963300078
表示:To perform array expansion, the initial direction of the signal must first be known, and the initial angle estimation
Figure A20051001963300074
There are always errors. Therefore, when designing an extended uniform linear array, one should try to select the array that is least sensitive to the error of the initial angle estimation and has the smallest transformation error as the extended array. In practice, we are concerned with the matrix
Figure A20051001963300075
and
Figure A20051001963300076
Is the column space consistent. In the column space sense, the vector The distance between a(θ) and the angle between the two can be used
Figure A20051001963300078
express:

γ ( θ ; θ ^ ) = arccos | a ‾ H ( θ ) B ( θ ^ ) a ( θ ) | | | a ‾ ( θ ) | | 2 · | | B ( θ ^ ) a ( θ ) | | 2 - - - ( 16 ) ‖·‖2和|·|分别表示谱范数和绝对值。最佳阵元间矩d,应使 γ ( θ ; θ ^ ) = arccos | a ‾ h ( θ ) B ( θ ^ ) a ( θ ) | | | a ‾ ( θ ) | | 2 &Center Dot; | | B ( θ ^ ) a ( θ ) | | 2 - - - ( 16 ) ‖·‖ 2 and |·| represent the spectral norm and absolute value, respectively. The optimal inter-element moment d should be

Figure A200510019633000710
最小,即
Figure A200510019633000710
minimum, ie

dd optopt == argarg minmin dd γγ (( θθ ;; θθ ^^ )) -- -- -- (( 1717 ))

一般dopt对θ和 不很敏感,因此为简单起见,θ可以选择为波束形成器最大输出方向。尽管如此,dopt的计算仍不方便。根据前面的讨论,为减小变换误差原阵列和扩展均匀线阵的主波束之幅相特性应尽量接近一致。故若原阵列的3dB主波束宽度为W,则均匀线阵阵元间距的一种简单的选择是[7] In general d opt for θ and is not very sensitive, so for simplicity, θ can be chosen to be the maximum output direction of the beamformer. Nevertheless, the calculation of d opt is still inconvenient. According to the previous discussion, in order to reduce the transformation error, the amplitude and phase characteristics of the main beam of the original array and the extended uniform linear array should be as close to the same as possible. Therefore, if the 3dB main beam width of the original array is W, a simple choice of uniform line array element spacing is [7]

dd == 0.8860.886 λλ NN ·· WW -- -- -- (( 1818 ))

其中,λ为波长。这样可使原阵列和扩展均匀线阵的3dB主波束宽度相等。计算机模拟表明,d一般接近于doptwhere λ is the wavelength. In this way, the 3dB main beam widths of the original array and the extended uniform linear array are equal. Computer simulations show that d is generally close to d opt .

2.5扩展变换误差分析2.5 Extended transformation error analysis

为考察酉变换矩阵的误差,在此以 Θ ^ = { θ ^ 1 , θ ^ 2 } 的一种简单情况为例。当阵元为全向阵元时,不难证明In order to examine the error of the unitary transformation matrix, here Θ ^ = { θ ^ 1 , θ ^ 2 } A simple case of . When the array element is omnidirectional, it is not difficult to prove that

|| || AA ‾‾ (( θθ ^^ 11 ,, θθ ^^ 22 )) -- BB (( θθ ^^ 11 ,, θθ ^^ 22 )) AA (( θθ ^^ 11 ,, θθ ^^ 22 )) || || Ff

Figure A20051001963300085
Figure A20051001963300085

其中, in,

研究(18)式可知,当_a→_b或当_a→0且_b→0时,(19)式左边趋近于零。这即是说,当

Figure A20051001963300087
Figure A20051001963300088
在一个波束宽度内时,要使变换矩阵误差最小,原阵列和扩展阵列的主波束之幅度特性和相位特性应尽量接近;而当
Figure A20051001963300089
Figure A200510019633000810
的间隔超过一个波束宽度时,两阵列旁瓣越低,则变换矩阵误差越小。当选择酉变换矩阵(15)式时,该结论不仅指出了阵列数据变换法对原阵列的要求,而且对扩展均匀线阵的设计也指明了方向。Study (18) shows that when _ a → _ b or when _ a → 0 and _ b → 0, the left side of (19) tends to zero. That is to say, when
Figure A20051001963300087
and
Figure A20051001963300088
Within one beam width, to minimize the transformation matrix error, the amplitude characteristics and phase characteristics of the main beam of the original array and the extended array should be as close as possible; and when
Figure A20051001963300089
and
Figure A200510019633000810
When the interval of is more than one beamwidth, the lower the sidelobes of the two arrays are, the smaller the error of the transformation matrix is. When the unitary transformation matrix (15) is selected, this conclusion not only points out the requirements of the array data transformation method for the original array, but also points out the direction for the design of the extended uniform linear array.

2.6扩展变换对噪声的影响2.6 Effect of extended transformation on noise

假设实际阵的数据协方差矩阵为R,噪声协方差矩阵为RN,则扩展阵列的数据协方差矩阵为Assuming that the data covariance matrix of the actual array is R and the noise covariance matrix is R N , then the data covariance matrix of the extended array is

RT=NRBH=B(ARsAH+RN)TH R T =NRB H =B(AR s A H +R N )T H

  =BARsAHTH+BRNTH                          (21)=BAR s A H T H +BR N T H (21)

当环境噪声为白噪声时,则When the ambient noise is white noise, then

BRNBH=σ2BBH                               (22)BR N B H = σ 2 BB H (22)

从上式可以看出,通过阵列扩展变换后,原阵列接收的白噪声变成了色噪声。It can be seen from the above formula that after the array expansion transformation, the white noise received by the original array becomes colored noise.

3、扩展阵的超分辨算法3. Super-resolution algorithm of extended array

从以上分析可知,由于对阵列通过扩展阵列变换后,原阵列接收的白噪声变成了色噪声,因此当各阵元接收的噪声相互独立时,可由下述方法估计协方差矩阵:From the above analysis, it can be seen that after the array is transformed by the extended array, the white noise received by the original array becomes colored noise, so when the noises received by each array element are independent of each other, the covariance matrix can be estimated by the following method:

RR TT == 11 Mm ΣΣ ii == 11 Mm xx (( ii :: LL -- Mm ++ ii -- 11 )) xx Hh (( ii ++ 11 :: LL -- Mm ++ ii )) -- -- -- (( 23twenty three ))

式中M为时域平滑次数,L为快拍数,其中x(i:j)表示第i次快拍到第j次快拍数据。显然,当各阵元噪声相互独立时,估计出的协方差矩阵的噪声项应为0。对RT进行特征分解,然后利用MUSIC空间谱估计器,即可得到信号DOA的超分辨估计。In the formula, M is the number of time-domain smoothing, L is the number of snapshots, where x(i:j) represents the i-th snapshot to the j-th snapshot data. Obviously, when the noise of each array element is independent of each other, the noise item of the estimated covariance matrix should be 0. By decomposing the eigenvalues of RT and using the MUSIC spatial spectrum estimator, the super-resolution estimation of signal DOA can be obtained.

4、算法性能仿真4. Algorithm performance simulation

模拟试验1:均匀线阵口径扩展Simulation Test 1: Uniform Linear Array Aperture Expansion

设有N=8的全向阵元均匀分布在长度为λ的直线上。现有6个信号背离雷达方向运动,其径向速度和运动方向分别为{4、8、12、16、20、24}m/s和{40°、60°、80°、100°、120°、140°}。数据采样点256。如图1、4、7、10、13和16分别表示阵列扩展前(原阵)波束指向40°、60°、80°、100°、120°和140°的回波Doppler谱。现将原阵扩展成天线间距为d=0.5λ的阵列。如图2、5、8、11、14和17分别表示阵列扩展后阵波束指向40°、60°、80°、100°、120°和140°的回波Doppler谱。如图3、6、9、12、15和18表示阵元间距为半波长的8元均匀直线阵。从此结果可以清楚看出,阵列扩展前,原阵无法分辨一个波束内存在的几个信号方向,但利用本文提出的方案对阵列进行扩展后,能非常清楚地分辨出各信号的方向和Doppler,而且扩展后的阵列与相等口径的实际阵的分辨效果几乎一样。进一步分析其原因可知,阵列扩展前,原阵的波束宽度约60°,而阵列扩展后阵列的波束宽度降为约15°,即该密集阵分辨率相当于原阵三倍的孔径。It is assumed that N=8 omnidirectional array elements are evenly distributed on a straight line with a length of λ. There are currently 6 signals moving away from the radar direction, and their radial speed and direction are {4, 8, 12, 16, 20, 24} m/s and {40°, 60°, 80°, 100°, 120 °, 140°}. Data sampling points 256. Figures 1, 4, 7, 10, 13, and 16 show the echo Doppler spectra of the array expansion front (original array) beam pointing at 40°, 60°, 80°, 100°, 120°, and 140°, respectively. Now expand the original array into an array whose antenna spacing is d=0.5λ. Figures 2, 5, 8, 11, 14, and 17 show the echo Doppler spectra of array beams pointing at 40°, 60°, 80°, 100°, 120°, and 140°, respectively, after array expansion. Figures 3, 6, 9, 12, 15 and 18 show an 8-element uniform linear array with an array element spacing of half a wavelength. From the results, it can be clearly seen that before the array expansion, the original array could not distinguish several signal directions in a beam, but after expanding the array with the scheme proposed in this paper, the direction of each signal and Doppler can be clearly distinguished. Moreover, the resolution effect of the expanded array is almost the same as that of the actual array with the same caliber. Further analysis of the reasons shows that before the array expansion, the beamwidth of the original array is about 60°, but after the array expansion, the beamwidth of the array is reduced to about 15°, that is, the resolution of the dense array is equivalent to three times the aperture of the original array.

模拟试验2:信噪比对均匀线阵口径扩展的影响Simulation Experiment 2: Effect of SNR on Aperture Expansion of Uniform Linear Array

设有N=8全向阵元均匀分布在长度为λ的直线上,入射波信号同模拟试验1,不同的是,各信号信噪比均为25dB。如图19、22、25、28、31和34分别表示阵列扩展前(原阵)波束指向40°、60°、80°、100°、120°和140°的回波Doppler谱。现将原阵扩展成天线间距为d=0.5λ的阵列。如图20、23、26、29、32和35分别表示阵列扩展后阵波束指向40°、60°、80°、100°、120°和140°的回波Doppler谱。如图21、24、27、30、33和36表示阵元间距为半波长的大型均匀直线阵。与模拟试验1所得的结论一样,阵列扩展前,原阵无法分辨一个波束内存在的几个信号方向,但利用本文提出方案对阵列进行扩展后,能非常清楚地分辨出各信号的方向和Doppler,进一步分析可知,随着信噪比的提高或原阵单元天线间距的增大,其分辨效果还会大大改善。Assuming that N=8 omnidirectional array elements are evenly distributed on a straight line with a length of λ, the incident wave signal is the same as the simulation test 1, the difference is that the signal-to-noise ratio of each signal is 25dB. Figures 19, 22, 25, 28, 31 and 34 show the echo Doppler spectra of the array expansion front (original array) beam pointing at 40°, 60°, 80°, 100°, 120° and 140° respectively. Now expand the original array into an array whose antenna spacing is d=0.5λ. Figures 20, 23, 26, 29, 32 and 35 show the echo Doppler spectra of the array beams pointing at 40°, 60°, 80°, 100°, 120° and 140° respectively after the array expansion. Figures 21, 24, 27, 30, 33 and 36 show a large uniform linear array with an element spacing of half a wavelength. Similar to the conclusion obtained in simulation experiment 1, before the array expansion, the original array cannot distinguish several signal directions in a beam, but after expanding the array with the scheme proposed in this paper, the direction of each signal and the direction of Doppler can be clearly distinguished. , further analysis shows that with the increase of the signal-to-noise ratio or the increase of the antenna spacing of the original array elements, the resolution effect will be greatly improved.

模拟试验3:大间距均匀线阵口径扩展Simulation Test 3: Large-Space Uniform Linear Array Aperture Expansion

设有N=8全向阵元均匀分布在长度为10λ的直线上(显然天线间距远大于半波长,原阵方向图将会出现栅瓣)。信噪比25dB。入射波信号同模拟试验1。典型模拟结果为:如图37表示阵列扩展前波束指向60°的回波Doppler谱。现将原阵扩展成天线间距为d=0.5λ的阵列。如图38表示阵列扩展后波束指向60°的回波谱。从此结果可以明显看出,阵列扩展前,在一个波束内出现了多个到达角,这显然是由于原天线阵间距过大,天线方向图出现栅瓣而产生的测向模糊。但利用本文提出方案对阵列进行扩展后,天线间距大大减少,消除了天线方向图出现的栅瓣,因此能非常清楚地分辨出波束内信号的方向和Doppler。It is assumed that N=8 omnidirectional array elements are evenly distributed on a straight line with a length of 10λ (obviously, the distance between the antennas is much larger than half a wavelength, and grating lobes will appear in the pattern of the original array). The signal-to-noise ratio is 25dB. The incident wave signal is the same as the simulation experiment 1. Typical simulation results are as follows: Figure 37 shows the echo Doppler spectrum with the beam pointing to 60° before array expansion. Now expand the original array into an array whose antenna spacing is d=0.5λ. Figure 38 shows the echo spectrum of the beam pointing to 60° after array expansion. From the results, it can be clearly seen that before the array expansion, multiple arrival angles appeared in one beam, which is obviously due to the direction-finding ambiguity caused by the grating lobes in the antenna pattern due to the excessive spacing of the original antenna array. However, after the array is extended by using the scheme proposed in this paper, the antenna spacing is greatly reduced, and the grating lobes appearing in the antenna pattern are eliminated, so the direction of the signal in the beam and the Doppler can be clearly distinguished.

模拟试验4:扩展阵元数多余实际阵元数Simulation test 4: The number of extended array elements exceeds the actual number of array elements

设有N=8全向阵元均匀分布在长度为λ的直线上,入射波信号同模拟试验1,不同的是,各信号信噪比均为20dB。典型模拟结果为:如图39表示阵列扩展前波束指向120°的回波Doppler谱。现将原阵扩展成天线间距为d=0.5λ的12元阵线阵。如图40表示阵列扩展后波束指向120°的回波谱。大量的随机模式实验表明,阵列扩展前,原阵无法分辨一个波束内存在的几个信号方向,但利用本文提出方案对阵列进行扩展后,能非常清楚地分辨出各信号的方向和Doppler。进一步分析还可知,此时天线阵的波束宽度比8均匀线阵的波束更窄,但结果更受信噪比的影响,信噪比越高,效果越好。Assume that N=8 omnidirectional array elements are evenly distributed on a straight line with a length of λ, and the incident wave signal is the same as that of the simulation experiment 1, except that the signal-to-noise ratio of each signal is 20dB. Typical simulation results are as follows: Figure 39 shows the echo Doppler spectrum with the beam pointing at 120° before array expansion. Now expand the original array into a 12-element array with an antenna spacing of d=0.5λ. Figure 40 shows the echo spectrum after the array expands and the beam points to 120°. A large number of random mode experiments show that before the array expansion, the original array cannot distinguish several signal directions in a beam, but after expanding the array with the scheme proposed in this paper, the direction of each signal and Doppler can be clearly distinguished. Further analysis shows that the beam width of the antenna array is narrower than that of the 8 uniform linear array at this time, but the result is more affected by the signal-to-noise ratio, and the higher the signal-to-noise ratio, the better the effect.

模拟试验5:非均匀阵口径扩展Simulation experiment 5: non-uniform array aperture expansion

设有N=8全向阵元随机分布在长度为λ的直线上(或均匀分布在半径为r=0.5λ的半圆上)。入射波信号同模拟试验1。现将原阵扩展成天线间距为d=0.5λ的阵列。大量随机模拟实验表明,阵列扩展前,原阵无法分辨一个波束内存在的几个信号方向,但利用本发明技术方案对阵列进行扩展后,能非常清楚地分辨出各信号的方向和Doppler。It is assumed that N=8 omnidirectional array elements are randomly distributed on a straight line with a length of λ (or uniformly distributed on a semicircle with a radius of r=0.5λ). The incident wave signal is the same as the simulation experiment 1. Now expand the original array into an array whose antenna spacing is d=0.5λ. A large number of random simulation experiments show that before the array is expanded, the original array cannot distinguish several signal directions in a beam, but after the array is expanded by using the technical solution of the present invention, the direction of each signal and Doppler can be clearly distinguished.

模拟试验6:扩展阵的高分辨算法Simulation Experiment 6: High Resolution Algorithm of Extended Array

设有N=8全向阵元均匀分布在长度为5λ的直线上。入射波信号同模拟试验1,信噪比为25dB。现将原阵扩展成天线间距为d=0.5λ的阵列。图41表示阵列扩展前利用MUSIC算法获得的超分辨空间谱。图42表示阵列扩展后利用MUSIC算法获得的超分辨空间谱。由此结果可知,天线阵扩展前,天线阵出现测向模糊,但利用本文提出的方法对原阵进行扩展,天线的分辨率不仅高,而且还消除了测向模糊。It is assumed that N=8 omnidirectional array elements are uniformly distributed on a straight line with a length of 5λ. The incident wave signal is the same as the simulation test 1, and the signal-to-noise ratio is 25dB. Now expand the original array into an array whose antenna spacing is d=0.5λ. Figure 41 shows the super-resolution spatial spectrum obtained using the MUSIC algorithm before array expansion. Figure 42 shows the super-resolution spatial spectrum obtained by using the MUSIC algorithm after array expansion. From the results, it can be seen that before the expansion of the antenna array, the direction finding ambiguity of the antenna array appears, but the method proposed in this paper is used to expand the original array, the resolution of the antenna is not only high, but also the direction finding ambiguity is eliminated.

5、讨论5. Discussion

本发明出的基于小型天线阵的口径扩展方法,具有如下特点:The aperture expansion method based on the small antenna array of the present invention has the following characteristics:

(a)变换过程不必知道信号的准确方向,只需假设信号的初始入射角,即可得到原阵列与扩展阵列的阵列流形矩阵,进而实现阵列的变换阵。在实际应用中,可预先存贮变换阵T,并实现阵列的扩展。(a) The transformation process does not need to know the exact direction of the signal, only the initial incident angle of the signal is assumed, and the array manifold matrix of the original array and the extended array can be obtained, and then the transformation matrix of the array can be realized. In practical applications, the transformation matrix T can be stored in advance, and the expansion of the array can be realized.

(b)一般阵列天线间距要求小于半波长,如果超过半波长,就会出现测向模糊,而通过阵列扩展变换,可将非等间距天线阵变成阵元间距小于半波长的天线阵,这样可以解决了阵列的信号模糊。(b) The general array antenna spacing is required to be less than half a wavelength. If it exceeds half a wavelength, direction finding ambiguity will appear. However, through array expansion transformation, the non-equidistant antenna array can be transformed into an antenna array whose element spacing is less than half a wavelength. In this way The signal ambiguity of the array can be resolved.

(c)增加了阵列的灵活性,由于扩展阵列增加了阵元数(自由度),这样在进行DOA估计时可根据实际环境灵活选择扩展阵列的数字阵元数,如信号数比较少时,可选择孔径小的扩展阵列,对于精度要求高的场合可适当增加阵元数来增加天线阵口径。(c) The flexibility of the array is increased. Since the number of array elements (degrees of freedom) is increased by the expansion array, the number of digital array elements of the expansion array can be flexibly selected according to the actual environment when performing DOA estimation. For example, when the number of signals is relatively small, it can be Choose an extended array with a small aperture, and increase the number of array elements to increase the aperture of the antenna array for occasions that require high precision.

(d)由于扩展的阵列比实际阵列可以具有更多的阵元数,因此,经过扩展后的阵列可以估计更多的信号源数。(d) Since the expanded array can have more array elements than the actual array, the expanded array can estimate more signal sources.

(e)扩展阵列单元数不可能无穷大,阵元数的选择只能在一定范围内有效。这是因为:从能量上讲,天线接收的能量和信息量是守恒的,任何数学意义上的变换只能对传统算法进行一定程度的改善,不会增加能量和有用信息量;从数学上讲,阵元数增加,扩展变换矩阵的条件数变大,重构扩展阵列天线单元幅相的误差变大,最后会给结果带来更大的误差。而且随着扩展阵元数的增加,为了获得工程可用的结果,其对信噪比的要求会大大增加。在实际应用中,扩展阵元的个数,应在信噪比、实际信号个数、扩展变换矩阵的条件数等因素之间进行折中。(e) The number of extended array elements cannot be infinite, and the selection of the number of array elements can only be valid within a certain range. This is because: in terms of energy, the energy and information received by the antenna are conserved, any transformation in the mathematical sense can only improve the traditional algorithm to a certain extent, and will not increase the energy and useful information; , the number of array elements increases, the condition number of the extended transformation matrix becomes larger, and the error of reconstructing the amplitude and phase of the extended array antenna elements becomes larger, which will eventually bring greater errors to the results. Moreover, as the number of extended array elements increases, in order to obtain engineering-usable results, the requirements for the signal-to-noise ratio will increase greatly. In practical applications, the number of extended array elements should be compromised among factors such as the signal-to-noise ratio, the number of actual signals, and the condition number of the extended transformation matrix.

(f)由于小型阵天线列孔径较小,这有利于减少天线阵的校准距离。(f) Due to the smaller aperture of the small array array, it is beneficial to reduce the calibration distance of the antenna array.

(g)将发明与现代高分辨算法相结合,可实现阵列空间超分辨测向。(g) Combining the invention with modern high-resolution algorithms, array space super-resolution direction finding can be realized.

Claims (3)

1. A method for aperture expansion and spatial signal processing of a small antenna array is characterized in that: setting the antenna array into any array form; dividing the whole antenna scanning area into a plurality of areas, and then subdividing any one of the sub-areas; constructing the actual array manifold a ═ a (θ) of the antenna array in subdivided sub-regions1),a(θ1+Δθ),a(θ2+2Δθ),...,a(θr)]And an array manifold a ═ a (θ) of the extended array1), a(θ1+Δθ), a(θ2+2Δθ),..., a(θr)]And further obtaining an array expansion transformation matrix B ═ AA-1Wherein, theta1,θrThe left and right boundaries of the sub-region are respectively, and delta theta is the step length of sub-region subdivision; reconstructing a signal Z ═ BX of an extended array antenna by using the obtained array extended transformation matrix, wherein X is a signal received by the original antenna array; and performing digital beam forming or adaptive beam forming on the reconstructed signal Z of the extended array antenna or solving the spatial arrival angle of the signal by using a spatial high-resolution algorithm.
2. The method of claim 1, wherein: and when the actual matrix manifold A is a non-square matrix, carrying out diagonal loading on the matrix A.
3. The method according to claim 1 or 2, characterized in that: the number of cells of the extended array is determined using a norm minimum of | a-BA |.
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Cited By (4)

* Cited by examiner, † Cited by third party
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CN101520507B (en) * 2007-07-20 2012-03-21 通用汽车环球科技运作公司 Ow cost short range radar
CN101272168B (en) * 2007-03-23 2012-08-15 中国科学院声学研究所 Signal sources estimation method and its DOA estimation method
CN104134354A (en) * 2013-04-30 2014-11-05 业纳遥控设备有限公司 Traffic monitoring system for speed measurement and assignment of moving vehicles in a multi-target recording module
CN108089147A (en) * 2017-12-07 2018-05-29 西南电子技术研究所(中国电子科技集团公司第十研究所) Improved shortwave unit localization method

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* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN101272168B (en) * 2007-03-23 2012-08-15 中国科学院声学研究所 Signal sources estimation method and its DOA estimation method
CN101520507B (en) * 2007-07-20 2012-03-21 通用汽车环球科技运作公司 Ow cost short range radar
CN104134354A (en) * 2013-04-30 2014-11-05 业纳遥控设备有限公司 Traffic monitoring system for speed measurement and assignment of moving vehicles in a multi-target recording module
CN108089147A (en) * 2017-12-07 2018-05-29 西南电子技术研究所(中国电子科技集团公司第十研究所) Improved shortwave unit localization method

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