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Blackman Window Family

When $ L=3$ in (3.3), we obtain the Blackman family:

$\displaystyle w_{B}(n)= w_R(n)\left[\alpha_0
+ \alpha_1 \cos(\Omega_M n)
+ \alpha_2 \cos(2\Omega_M n)\right]
$

Relative to the generalized Hamming family (§3.2), we have added one more cosine weighted by $ \alpha_2$. We now therefore have three degrees of freedom to work with instead of two. In the Hamming family, we used one degree of freedom to normalize the window amplitude and the second was used either to maximize roll-off rate (Hann) or side-lobe rejection (Hamming). Now we can use two remaining degrees of freedom (after normalization) to optimize these objectives, or we can use one for each, resulting in three subtypes within the Blackman window family.


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written by Julius Orion Smith III
Julius Smith's background is in electrical engineering (BS Rice 1975, PhD Stanford 1983). He is presently Professor of Music and Associate Professor (by courtesy) of Electrical Engineering at Stanford's Center for Computer Research in Music and Acoustics (CCRMA), teaching courses and pursuing research related to signal processing applied to music and audio systems. See http://ccrma.stanford.edu/~jos/ for details.


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