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| Josh's Notes: 最优阵列处理(Part 2.1 —— 谱加权) | true | true | true |
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61f0754c | 2023-06-19 16:25:26 |
谱加权(Spectral Weighting)技术主要研究对如何每个传感器输出进行加权,以获得具有理想性质的频率-波数响应和波束方向图。加权的过程在一些文献中也称为锐化 (tapering) 或赋形 (shading) 。许多阵列加权技术等价于时间序列谱分析中的加窗或锐化 (Taper) 技术。
对于一个阵元间距小于或等于 \lambda/2 的线阵,由于不需要考虑栅瓣和空域混迭,可以直接应用连续函数的傅里叶变换理论对权重和频率-波数响应之间存在的傅里叶变换关系进行分析。本文关注线性阵列,讨论如何在降低旁瓣的同时使主瓣宽度的增长最小(最小化方向性损失),将尝试不同的权值矢量,并分析它们的性能。
考虑傅里叶变换对
$$\begin{equation} \varUpsilon(\omega,k) = \int_{-\infty}^\infty w_a^\ast (z) e^{-jkz}, \mathrm{d}z \end{equation}$$
$$\begin{equation} w_a^\ast (z) = \frac{1}{2\pi} \int_{-\infty}^\infty \varUpsilon(\omega,k) e^{jkz}, \mathrm{d}k \end{equation}$$
其中省略了 k_z 的下标 $z$。
1. 均匀加权
均匀权值为
$$\begin{equation} w_n = \frac{1}{N}, \quad n = 0,\cdots,N-1 \end{equation}$$
在 u 空间的波束方向图为
$$\begin{equation} \begin{aligned} B_u(u) &= \frac{1}{N} \frac{\sin\left( \displaystyle\frac{\pi Nd}{\lambda} u \right)}{\sin\left( \displaystyle\frac{\pi d}{\lambda} u \right)} \ &= \boldsymbol{w}^\mathrm{H}\boldsymbol{v}u(u) = e^{-j\left(\frac{N-1}{2} \right) \frac{2\pi d}{\lambda} u} \sum{n=0}^{N-1} w_n^\ast e^{j n \frac{2\pi d}{\lambda} u} \end{aligned} \end{equation}$$
对于标准线阵,有
$$\begin{equation} B_u(u) = \frac{1}{N} \frac{\sin\left( \displaystyle\frac{\pi Nu}{2} \right)}{\sin\left( \displaystyle\frac{\pi u}{2} \right)} \end{equation}$$
方向性
$$\begin{equation} D = N \end{equation}$$
由于下面经考虑实对称的权值,因此将阵元的位置也对称地进行表示,第 n 个阵元的位置表示为
$$\begin{equation} \tilde{n} = n - \frac{N-1}{2}, \quad n = 0,\cdots,N-1,\quad \tilde{n} = -\frac{N-1}{2}, \cdots, \frac{N-1}{2} \end{equation}$$
2. Cosine 加权
当 N 为奇数时,Cosine 权值为
$$\begin{equation} w(\tilde{n}) = \sin\left( \frac{\pi}{2N} \right)\cos\left( \pi\frac{\tilde{n}}{N} \right), \quad -\frac{N-1}{2} \leqslant \tilde{n} \leqslant \frac{N-1}{2} \end{equation}$$
其中归一化因子 \sin\left( \displaystyle\frac{\pi}{2N} \right) 是一个常数,使得 $B_u (0) = 1$。把 Cosine 写成指数形式,有
$$\begin{equation} w(\tilde{n}) = \sin\left( \frac{\pi}{2N} \right)\left[ \frac{e^{j\frac{\pi\tilde{n}}{N}} + e^{-j\frac{\pi\tilde{n}}{N}}}{2} \right], \quad -\frac{N-1}{2} \leqslant \tilde{n} \leqslant \frac{N-1}{2} \end{equation}$$
利用指数形式的阵列流形矢量,可得波束方向图
$$\begin{equation} B_u(u) = \frac{1}{2} \sin\left( \frac{\pi}{2N} \right) \left{ \sum_{\tilde{n} = -\frac{N-1}{2}}^{\frac{N-1}{2}} e^{j\frac{\pi \tilde{n}}{N}} e^{-j \tilde{n} \pi u} + \sum_{\tilde{n} = -\frac{N-1}{2}}^{\frac{N-1}{2}} e^{-j\frac{\pi \tilde{n}}{N}} e^{-j \tilde{n} \pi u} \right} \end{equation}$$
其中第一项和第二项分别对应指向 u_s = 1/N 和 u_s = -1/N 的常规波束方向图,因此
$$\begin{equation} B_u(u) = \frac{1}{2} \sin\left( \frac{\pi}{2N} \right) \left{ \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u - \frac{1}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u - \frac{1}{N} \right) \right)} + \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u + \frac{1}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u + \frac{1}{N} \right) \right)} \right} \end{equation}$$
下面将要介绍的很多方向图都是常规波束的叠加。图 2-1-1 给出了一个 11 阵元阵列使用 Cosine 加权得到的波束方向图,同时还给出了常规波束方向图作为参考。可以看到,旁瓣得到了降低,但是主波束变得更宽。两个波束方向图的参数为
| 加权方式 | HPBW | BW_{NN} |
第一旁瓣高度 | $D_N$1 |
|---|---|---|---|---|
| Uniform | 0.89 \displaystyle\frac{2}{N} |
2.0 \displaystyle\frac{2}{N} |
-13.0 \text{dB} |
1 |
| Cosine | 1.18 \displaystyle\frac{2}{N} |
3.0 \displaystyle\frac{2}{N} |
-23.5 \text{dB} |
0.816 |
{% note primary MATLAB Code %}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Figure 3.1
% Cosine weighting: Array beam patterns
% Kristine Bell
% Modified by Xin Zhang 3/17/99
% Lillian 04/16/2001, K. Bell 7/20/01, K. Bell 9/30/01
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
clear all
close all
M=11;
d=0.5; % sensor spacing wrt wavelength
D = (-(M-1)/2:1:(M-1)/2)*d; % sensor positions in wavelengths
% weights, normalized so that w(0)=1
W_unf = ones(1,M);
W_cos = cos(pi*D*2/M);
% Beampatterns
u = 0:0.001:1;
A = exp(-1i*2*pi*D.'*u);
G_unf = W_unf*A;
G_unf = G_unf/(max(abs(G_unf)));
G_cos = W_cos*A;
G_cos = G_cos/(max(abs(G_cos)));
figure
% array only
clf
plot(u,20*log10(abs(G_unf)),'--')
hold on
plot(u,20*log10(abs(G_cos)),'-')
hold off
axis([0 1 -80 0])
%title([int2str(M) ' element array'])
h=legend('Uniform','Cosine');
xlabel('$u$','Interpreter','latex')
ylabel('Beam pattern (dB)')
{% endnote %}
3. 升 Cosine 加权
可以把矩形均匀加权和 Cosine 加权组合起来,获得两种加权方法一些理想性质的组合。对应的阵列加权为
$$\begin{equation} w(\tilde{n}) = c(p) \left( p + (1-p) \cos \left( \pi \frac{\tilde{n}}{N} \right)\right), \quad \tilde{n} = -\frac{N-1}{2}, \cdots, \frac{N-1}{2} \end{equation}$$
其中归一化常数
$$\begin{equation} c(p) = \frac{p}{N} + \frac{1-p}{2} \sin\left( \frac{\pi}{2N} \right) \end{equation}$$
使得 $B_u(0) = 1$。
在图 2.1.2 中给出了 p = 0.31, 0.17, 0 时的升 Cosine 加权的波束方向图。当 p 减小时,第一旁瓣的高度减小,主波束宽度增加。波束方向图参数如下:
p |
HPBW | BW_{NN} |
第一旁瓣高度 | D_N |
|---|---|---|---|---|
| 0.31 | 1.03 \displaystyle\frac{2}{N} |
2.50 \displaystyle\frac{2}{N} |
-20.0 \text{dB} |
0.928 |
| 0.17 | 1.09 \displaystyle\frac{2}{N} |
3.70 \displaystyle\frac{2}{N} |
-22.0 \text{dB} |
0.886 |
| 0 | 1.18 \displaystyle\frac{2}{N} |
3.00 \displaystyle\frac{2}{N} |
-23.5 \text{dB} |
0.816 |
{% note primary MATLAB Code %}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Figure 3.2
% Raised cosine weighting function
% Kristine Bell
% Modified by Xin Zhang 3/17/99
% Lillian Xu 04/16/2001, K. Bell 7/20/01, 9/30/01
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
clear all
close all
M=11;
d=0.5; % sensor spacing wrt wavelength
D = (-(M-1)/2:1:(M-1)/2)*d; % sensor positions in wavelengths
% weights, normalized so that w(0)=1
p=[0;0.17;0.31;1];
W_rcos = p*ones(1,M)+(ones(4,1)-p)*cos(pi*D*2/M);
% Beampatterns
u = 0:0.001:1;
c=p+(ones(4,1)-p)*2/pi;
A = exp(-1i*2*pi*D.'*u);
G_rcos = W_rcos*A;
for m=1:4
G_rcos(m,:) = G_rcos(m,:)/(max(abs(G_rcos(m,:))));
end
figure
clf
plot(u,20*log10(abs(G_rcos(3,:))),'-.')
hold on
plot(u,20*log10(abs(G_rcos(2,:))),'--')
plot(u,20*log10(abs(G_rcos(1,:))),'-')
hold off
axis([0 1 -80 0])
h=legend({'$p=0.31$','$p=0.17$','$p=0$'},'Interpreter','latex');
xlabel('$u$','Interpreter','latex')
ylabel('Beam pattern (dB)')
{% endnote %}
至此,我们已经可以使 HPBW 变窄,并使得第一旁瓣比均匀分布的情况要低得多。
4. Cosine$^m$ 加权
下面考虑一系列 Cosine 加权,形式为 $\cos^m(\pi \tilde{n} / N)$。阵列的权值为
$$\begin{equation} w_m(\tilde{n}) = \begin{cases} c_2 \cos^2 \left( \displaystyle \frac{\pi \tilde{n}}{N} \right),\quad m = 2 \ c_3 \cos^3 \left( \displaystyle \frac{\pi \tilde{n}}{N} \right),\quad m = 3 \ c_4 \cos^4 \left( \displaystyle \frac{\pi \tilde{n}}{N} \right),\quad m = 4 \ \end{cases} \end{equation}$$
其中 c_2, c_3, c_4 是归一化常数。
$m=2$ 时的加权有时称为是 Hann 加权2 。同样,波束方向图可以利用 Cosine 函数的指数形式来计算。波束方向图在图 2.1.3 中给出。当 m 增加时,旁瓣减小,但是主波束变宽。波束方向图的参数为:
m |
HPBW | BW_{NN} |
第一旁瓣高度 | D_N |
|---|---|---|---|---|
| 2 | 1.44 \displaystyle\frac{2}{N} |
4 \displaystyle\frac{2}{N} |
-31.4 \text{dB} |
0.667 |
| 3 | 1.66 \displaystyle\frac{2}{N} |
5 \displaystyle\frac{2}{N} |
-39.4 \text{dB} |
0.576 |
| 4 | 1.85 \displaystyle\frac{2}{N} |
6 \displaystyle\frac{2}{N} |
-46.7 \text{dB} |
0.514 |
{% note primary MATLAB Code %}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Figure 3.3
% Cosine^m weighting: m = 2,3,and 4
% Kristine Bell
% Modified by Xin Zhang 3/17/99
% Lillian Xu 04/16/2001, K. Bell 7/20/01, 9/30/01
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
clear all
close all
M=11;
d=0.5; % sensor spacing wrt wavelength
D = (-(M-1)/2:1:(M-1)/2)*d; % sensor positions in wavelengths
% weights, normalized so that w(0)=1
W_cos2 = cos(pi*D*2/M).^2;
W_cos3 = cos(pi*D*2/M).^3;
W_cos4 = cos(pi*D*2/M).^4;
% Beampatterns
u = 0:0.001:1;
A = exp(-1i*2*pi*D.'*u);
G_cos2 = W_cos2*A;
G_cos2 = G_cos2/(max(abs(G_cos2)));
G_cos3 = W_cos3*A;
G_cos3 = G_cos3/(max(abs(G_cos3)));
G_cos4 = W_cos4*A;
G_cos4 = G_cos4/(max(abs(G_cos4)));
figure
clf
plot(u,20*log10(abs(G_cos2)),'--')
hold on
plot(u,20*log10(abs(G_cos3)),'-')
plot(u,20*log10(abs(G_cos4)),'-.')
hold off
axis([0 1 -80 0])
h=legend({'$m=2$','$m=3$','$m=4$'},'Interpreter','latex');
set(h,'Fontsize',12)
xlabel('$u$','Interpreter','latex')
ylabel('Beam pattern (dB)')
{% endnote %}
5. 升 Cosine 平方加权
升 Cosine 平方系列的加权为
$$\begin{equation} \begin{aligned} w(\tilde{n}) &= c_2 (p) \left{ p + (1-p) \cos^2 \left( \frac{\pi \tilde{n}}{N} \right) \right} \ &= \frac{c_2(p)}{2} \left{ (1+p) + (1-p) \cos \left( \frac{2 \pi \tilde{n}}{N} \right) \right}, \quad \tilde{n} = -\frac{N-1}{2}, \cdots, \frac{N-1}{2} \end{aligned} \end{equation}$$
其中 c_2 (p) 是归一化常数。下面考虑一个特别的加权,称为 Hamming 加权。
6. Hamming 加权
Hamming 加权利用了矩形方向图和 Cosine 平方方向图的特点,在第一旁瓣的峰值上放置了一个零点。加权函数为
$$\begin{equation} w(\tilde{n}) = g_0 + g_1 \cos \left( \frac{2 \pi \tilde{n}}{N} \right), \quad \tilde{n} = -\frac{N-1}{2}, \cdots, \frac{N-1}{2} \end{equation}$$
选择系数 g_0 和 g_1 的使 u = 3/N 的位置上有一个零点,并将正侧向的响应归一化,有
$$\begin{equation} w(\tilde{n}) = 0.54 + 0.46 \cos \left( \frac{2 \pi \tilde{n}}{N} \right), \quad -\frac{N-1}{2} \leqslant \tilde{n} \leqslant \frac{N-1}{2} \end{equation}$$
对应升 Cosine 平方加权中 p = 0.08 的情况,得到的波束方向图是三个常规波束方向图的和
$$\begin{equation} B_u(u) = 0.54 \frac{\sin\left(\displaystyle\frac{N\pi u}{2}\right)}{\sin\left(\displaystyle\frac{\pi u}{2}\right)} + 0.23 \left[ \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u - \frac{2}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u - \frac{2}{N} \right) \right)} + \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u + \frac{2}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u + \frac{2}{N} \right) \right)} \right] \end{equation}$$
图 2.1.4 给出了 Hamming 加权、Hann 加权和 Blackman-Harris 加权的波束方向图。第一个零点的位置在 $u = 4/N$,第一个非零旁瓣的高度为 $-39.5\text{dB}$。由于加权具有步进不连续性(step discontinuity),旁瓣的衰减渐近为 $O(1/n)$。但是,第一个旁瓣被完全对消掉了,尽管剩余的旁瓣衰减得比较慢,它们的幅度都不是很高。而且注意到 Hamming 窗的波束宽度小于 Hann 加权的波束宽度,且第一旁瓣更低。
{% note primary MATLAB Code %}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Figure 3.4
% Beam patterns for Hann, Hamming, and Blackman-Harris
% Kristine Bell
% Modified by Xin Zhang 3/17/99
% Lillian Xu 04/16/2001, K. Bell 7/20/01, 9/30/01
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Hann, Hamming, Blackman-Harris
% M-element array, d=lambda/2
clear all
close all
M=11;
d=0.5; % sensor spacing wrt wavelength
D = (-(M-1)/2:1:(M-1)/2)*d; % sensor positions in wavelengths
% weights, normalized so that w(0)=1
W_Hann = 0.5*(ones(1,M)+cos(2*pi*D*2/M));
W_Hamm = 0.54*ones(1,M)+0.46*cos(2*pi*D*2/M);
W_BH = 0.42*ones(1,M)+0.5*cos(2*pi*D*2/M)+0.08*cos(4*pi*D*2/M);
% Beampatterns
u = 0:0.001:1;
A = exp(-1i*2*pi*D.'*u);
G_Hann = W_Hann*A;
G_Hann = G_Hann/(max(abs(G_Hann)));
G_Hamm = W_Hamm*A;
G_Hamm = G_Hamm/(max(abs(G_Hamm)));
G_BH = W_BH*A;
G_BH = G_BH/(max(abs(G_BH)));
figure
clf
plot(u,20*log10(abs(G_Hann)),'--')
hold on
plot(u,20*log10(abs(G_Hamm)),'-')
plot(u,20*log10(abs(G_BH)),'-.')
hold off
axis([0 1 -80 0])
h=legend('Hann','Hamming','Blackman-Harris');
xlabel('$u$','Interpreter','latex')
ylabel('Beam pattern (dB)')
{% endnote %}
7. Blackman-Harris 加权
Blackman-Harris 加权把加权过程扩展到了更高阶谐波的情况,并在前两个旁瓣的峰值位置上放置了零点。加权函数为
$$\begin{equation} w(\tilde{n}) = 0.42 + 0.5 \cos\left( \frac{2\pi \tilde{n}}{N} \right) + 0.08 \cos\left( \frac{4\pi \tilde{n}}{N} \right), \quad \tilde{n} = -\frac{N-1}{2}, \cdots, \frac{N-1}{2} \end{equation}$$
对应的波束方向图是多个常规波束方向图的和,已在图 2.1.4 中给出
$$\begin{equation} \begin{aligned} B_u(u) =& 0.42 \frac{\sin\left( \displaystyle\frac{N\pi u}{2} \right)}{\sin\left( \displaystyle\frac{\pi u}{2} \right)} + 0.25 \left[ \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u - \frac{2}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u - \frac{2}{N} \right) \right)} + \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u + \frac{2}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u + \frac{2}{N} \right) \right)} \right] \ &+ 0.04 \left[ \frac{\sin\left( \displaystyle\frac{N\pi}{2} \left( u - \frac{2}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{2} \left( u - \frac{2}{N} \right) \right)} + \frac{\sin\left( \displaystyle\frac{N\pi}{4} \left( u + \frac{4}{N} \right) \right)}{\sin\left( \displaystyle\frac{\pi}{4} \left( u + \frac{4}{N} \right) \right)} \right] \end{aligned} \end{equation}$$
波束方向图的参数为
| 加权方式 | HPBW | BW_{NN} |
第一旁瓣高度 | D_N |
|---|---|---|---|---|
| Hann | 1.44 \displaystyle\frac{2}{N} |
4.0 \displaystyle\frac{2}{N} |
-31.4 \text{dB} |
0.667 |
| Hamming | 1.31 \displaystyle\frac{2}{N} |
4.0 \displaystyle\frac{2}{N} |
-39.5 \text{dB} |
0.730 |
| Blackman-Harris | 1.65 \displaystyle\frac{2}{N} |
6.0 \displaystyle\frac{2}{N} |
-56.6 \text{dB} |
0.577 |
至此,所有的加权方法都是基于各种正弦函数进行的。现在看看其他类型的阵列加权技术,试试能否更好在波束宽度和旁瓣之间的获得折中。
8. 长球函数 (Prolate Spheroidal Functions)
在设计加权方案时,我们的目标是使得一个给定角度范围内的能量占总能量的比例最大,也即最大化如下比值
$$\begin{equation} \alpha = \frac{\displaystyle\iint_{\varOmega_1}\left| B(\theta,\varphi) \right|^2 \sin\theta,\mathrm{d}\theta,\mathrm{d}\varphi}{\displaystyle\int_0^\pi \int_0^{2\pi}\left| B(\theta,\varphi) \right|^2 \sin\theta,\mathrm{d}\varphi,\mathrm{d}\theta} \end{equation}$$
其中 \varOmega_1 是主波束周围的一个区域。对于标准线性阵列,可以写成
$$\begin{equation} \alpha = \frac{\displaystyle\int_{-\psi_0}^{\psi_0}\left| B(\psi) \right|^2,\mathrm{d}\psi}{\displaystyle\int_{-\pi}^{\pi}\left| B(\psi) \right|^2,\mathrm{d}\psi} \end{equation}$$
其分子和分母部分可分别写为
$$\begin{equation} \begin{aligned} &\alpha_N &&\xlongequal{B(\psi) = \boldsymbol{w}^\mathrm{H}\boldsymbol{v}\psi(\psi)} \int{-\psi_0}^{\psi_0}\boldsymbol{w}^\mathrm{H}\boldsymbol{v}\psi(\psi) \boldsymbol{v}\psi^\mathrm{H}(\psi)\boldsymbol{w},\mathrm{d}\psi \ & &&= \boldsymbol{w}^\mathrm{H} \left[ \int_{-\psi_0}^{\psi_0} \boldsymbol{v}\psi(\psi) \boldsymbol{v}\psi^\mathrm{H}(\psi) ,\mathrm{d}\psi \right]\boldsymbol{w} \ & &&= \boldsymbol{w}^\mathrm{H}\boldsymbol{A}\boldsymbol{w} \
&\alpha_D &&\xlongequal{B(\psi) = \boldsymbol{w}^\mathrm{H}\boldsymbol{v}_\psi(\psi)} \int_{-\pi}^{\pi}\boldsymbol{w}^\mathrm{H}\boldsymbol{v}_\psi(\psi) \boldsymbol{v} \\
& &&= \boldsymbol{w}^\mathrm{H}\boldsymbol{A}\boldsymbol{w}
\end{aligned} \end{equation}$$
$$\begin{equation} \end{equation}$$
其中
$$\begin{equation} \begin{aligned} \boldsymbol{A} &\triangleq \int_{-\psi_0}^{\psi_0} \boldsymbol{v}\psi(\psi) \boldsymbol{v}\psi^\mathrm{H}(\psi) ,\mathrm{d}\psi \ \boldsymbol{B} &\triangleq \int_{-\pi}^{\pi} \boldsymbol{v}\psi(\psi) \boldsymbol{v}\psi^\mathrm{H}(\psi) ,\mathrm{d}\psi = 2\pi \boldsymbol{I} \end{aligned} \end{equation}$$
$$\begin{equation} [\boldsymbol{A}]{mn} = \int{-\psi_0}^{\psi_0} e^{jm\psi} e^{-jn\psi} ,\mathrm{d}\psi = \frac{2\sin ((m-n)\psi_0)}{m-n} = 2\psi_0 ,\mathrm{sinc}((m-n)\psi_0) \end{equation}$$
因此
$$\begin{equation} \alpha = \frac{\boldsymbol{w}^\mathrm{H}\boldsymbol{A}\boldsymbol{w}}{2\pi \boldsymbol{w}^\mathrm{H}\boldsymbol{w}} \end{equation}$$