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Rotating Horn Doppler Shift

\begin{figure}\centering
\input fig/fhorn100.pstex_t
\\ {\LARGE Relevant geometry for a rotating horn}
\end{figure}

Source velocity projected onto source-listener path:

$\displaystyle \underline{v}_{sl}= {\cal P}_{\underline{x}_{sl}}(\underline{v}_s...
...line{x}_s\,\right\Vert^2}\left(\underline{x}_l-\underline{x}_s\right).
\protect$

Choosing $ \underline{x}_l=(r_l,0)$ yields

$\displaystyle \underline{v}_{sl}= \frac{-r_l r_s\omega_m\sin(\omega_m t)}{r_l^2...
...l-r_s\cos(\omega_m t) \\ [2pt] -r_s\sin(\omega_m)t \end{array}\right].
\protect$

Far field approximation:

$\displaystyle \underline{v}_{sl}\approx -r_s\omega_m\sin(\omega_m t) \left[\begin{array}{c} 1 \\ [2pt] 0 \end{array}\right].
\protect$


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Download DelayVar.pdf
Download DelayVar_2up.pdf
Download DelayVar_4up.pdf

``Time Varying Delay Effects'', by Julius O. Smith III, (From Lecture Overheads, Music 420).
Copyright © 2008-02-08 by Julius O. Smith III
Center for Computer Research in Music and Acoustics (CCRMA),   Stanford University
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