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Introduction to Acoustics

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ural waves is much smaller than the overall curvature,<br />

the vibrational modes will be closely related <strong>to</strong> the flexural<br />

waves of a circular disc, with frequencies satisfying<br />

Chladni’s generalised empirical law, fmn ∼ c(m + 2n) p ,<br />

as confirmed by Perrin et al. [15.218].<br />

The flexural modes involve radial displacements<br />

proportional <strong>to</strong> cos(mφ). Continuity requires that there<br />

must also be a tangential displacement, such that u +<br />

∂v/∂φ = 0, where u and v are the radial and tangential<br />

velocities respectively. Coupling <strong>to</strong> the tangential<br />

motion explains why it is possible <strong>to</strong> feed energy in<strong>to</strong><br />

a vibrating wine glass or the individual glass resona<strong>to</strong>rs<br />

of a glass harmonica (Rossing [15.201] Chap. 14), by<br />

rubbing a wetted finger around the rim. The excitation is<br />

very similar <strong>to</strong> the slip–stick mechanism used <strong>to</strong> excite<br />

the bowed string (Sect. 15.2.4).<br />

Figure 15.136 illustrates a set of holographic measurements<br />

by Rossing ([15.201], Fig. 12.4), which is<br />

typical of most bell shapes. The (m, 1) and (m, 2)<br />

modes can immediatly be related <strong>to</strong> the (m, n) modes<br />

of a cupped disc. However, there is a distinct change<br />

in character for n > 0, with an additional node appearing<br />

close <strong>to</strong> the rim – referred <strong>to</strong> as a (m, 1#)<br />

mode. Some insight is provided by the finite element<br />

solutions for a typical large English church bell<br />

illustrated in Fig. 15.137 [15.221]. The three modes<br />

illustrated are very similar <strong>to</strong> the (3, 0), (3, 1) and<br />

(3, 2) modes expected from the simple cupped disc<br />

model, except for the lowest frequency (3, 0) mode,<br />

2,0 3,0 4,1# 5,1# 6,1#<br />

2,1 3,1 4,1 5,1 6,1<br />

2,2 3,2 4,2 5,2 6,2<br />

Fig. 15.136 Holographic interferograms and nomenclature<br />

for vibrational modes of a hand bell (after Rossing [15.201])<br />

Musical <strong>Acoustics</strong> 15.4 Percussion Instruments 659<br />

(3,1) (3,1#) (3,2)<br />

Fig. 15.137 Finite-element solutions for the lowest-order m<br />

= 3 modes of an English church bell (after Perrin et al.<br />

[15.219]) illustrating the (3,1), (3,1#) and (3,2) modes<br />

in which the <strong>to</strong>p surfaces of the bell move in antiphase<br />

with the rim, <strong>to</strong> give a nodal line about<br />

half-way along the length. Similarly, the anticipated<br />

(4, 0), (5, 0) and (6, 0) modes of the handbell investigated<br />

by Rossing [15.201] acquire an additional<br />

nodal line close <strong>to</strong> the end rim denoted as (4, 1#),<br />

(5, 1#) and (6, #) modes. Such features can generally<br />

only be accounted for by detailed computational<br />

analysis.<br />

Bell Tuning<br />

Figure 15.138 shows the frequencies and associated<br />

modes of a well-tuned traditional church bell (Rossing<br />

and Perrin [15.220]), ordered in<strong>to</strong> groups based on mode<br />

Group 0<br />

Group I<br />

Group II<br />

Group III<br />

End view<br />

(2,0) 0.5<br />

0.30<br />

Prime<br />

1.0<br />

0.54<br />

0.19<br />

(2,2) 2.7<br />

0.54<br />

Tierce Nominal (Twelfth) (Upper octave)<br />

(3,1) 1.2 (4,1) 2.0 (5,1) 3.0 (6,1) 4.2<br />

Quint (Major third)<br />

0.19<br />

(3,1#) 1.5 (4,1#) 2.5 (5,1#) 3.7 (6,1#) 5.0<br />

(3,2) 2.6 (4,2) 3.3 (5,2) 4.5 (6,2) 5.9<br />

Fig. 15.138 Measured frequencies for a typical D5 church bell,<br />

indicating the relative frequencies of the observed mode, with the traditional<br />

names associated with such modes indicated (after Rossing<br />

and Perrin [15.220])<br />

Part E 15.4

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