Main-Lobe Bandwidth

We saw in the previous section that our ability to resolve two closely spaced sinusoids is determined by the main-lobe width of the window transform we are using. We will now study this relationship in more detail.

For starters, let's define main-lobe width very simply (and somewhat crudely) as the distance between the first zero-crossings on either side of the main lobe, as shown in Fig.1.16 for a rectangular-window transform. Let $B_w$ denote this width in Hz. In normalized radian frequency units, as used in the frequency axis of Fig.1.16, $B_w$ Hz translates to $2\pi B_w / f_s$ radians per sample, where $f_s$ denotes the sampling rate in Hz.

Figure 1.16: Window transform with main lobe width marked.

For the length-$M$ unit-amplitude rectangular window defined in §1.5, the DTFT is given analytically by

$$W_R(\omega) = M\cdot\hbox{asinc}_M(\omega) \isdef \frac{ \sin \le... ...in(\omega T/2)} = \frac{ \sin \left( M\pi f T \right)}{\sin(\pi f T)}, \protect$$ (2.7)

where $f$ is frequency in Hz, and $T$ is the sampling interval in seconds ($T=1/f_s$). The main lobe of the rectangular-window transform is thus ``two sidelobes wide,'' or

$$\zbox {B_w = 2\frac{f_s}{M}}\quad \hbox{(\hbox{Hz})}$$

as can be seen in Fig.1.16.

Recall from §1.5.1 that the side-lobe width in a rectangular-window transform ($f_s/M$ Hz) is given in radians per sample by

$$\zbox {\Omega_M \isdef \frac{2\pi}{M}.}$$

As Fig.1.16 illustrates, the rectangular-window transform main-lobe width is $2\Omega_M$ radians per sample (two side-lobe widths). Table 1.1 lists the main-lobe widths for a variety of window types (which are defined and discussed further in Chapter 3).

Table 1.1: Main-lobe bandwidth for various windows.

Window Type	Main-Lobe Width $K\Omega_M$ (rad/sample)
Rectangular	$2\Omega_M$
Hamming	$4\Omega_M$
Hann	$4\Omega_M$
Generalized Hamming	$4\Omega_M$
Blackman	$6\Omega_M$
$L$-term Blackman-Harris	$2L\Omega_M$
Kaiser	depends on $\beta$
Chebyshev	depends on ripple spec