Directivity Factor (Q(θ, ϕ))

In general, a directivity factor Qθ,ϕ may be defined as the ratio of the radial intensity 〈Iθϕt (at angles θ and ϕ and distance r from the source) to the radial intensity 〈Ist at the same distance r radiated from an omnidirectional source of the same total sound power (Figure 3.12). Thus

(3.53)equation

Schematic illustration of geometry used in derivation of directivity factor.
Figure 3.12 Geometry used in derivation of directivity factor.

For a directional source, the mean square sound pressure measured at distance r and angles θ and ϕ is p2rms (θ,ϕ).

In the far field of this source (r ≫ λ), then

(3.54)equation

But if the source were omnidirectional of the same power W, then

(3.55)equation

where p2rms is a constant, independent of angles θ and ϕ.

We may therefore write:

(3.56)equation

and

(3.57)equation

where images is the space‐averaged mean‐square sound pressure.

We define the directivity factor Q as

(3.58)equation

the ratio of the mean‐square sound pressure at distance r to the space‐averaged mean‐square pressure at r, or equivalently the directivity Q may be defined as the ratio of the mean‐square sound pressure at r divided by the mean‐square sound pressure at r for an omnidirectional sound source of the same sound power W, watts.


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