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Introduction to Acoustics

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Optical Methods for <strong>Acoustics</strong> and Vibration Measurements 27.2 Measurement Principles and Some Applications 1105<br />

27.1.5 Some Pros and Cons<br />

of Optical Metrology<br />

In the following, measuring principles for holographic<br />

interferometry, speckle metrology, vibrometry, pulsed<br />

TV holography, Moiré methods and PIV are discussed<br />

<strong>to</strong>gether with some applications. The main advantages<br />

of these methods are:<br />

• There are no contact probes. They are nondisturbing.<br />

• Most of them are whole-field, all-electronic methods.<br />

They give pictures.<br />

• They give not only qualitative but also quantitative<br />

measures.<br />

• The (digital) processing is often very fast, sometimes<br />

as if in real time.<br />

27.2 Measurement Principles and Some Applications<br />

27.2.1 Holographic Interferometry<br />

for the Study of Vibrations<br />

With the introduction of holographic interferometry in<br />

1965, amplitude fields of vibrating, diffusely reflecting<br />

surfaces could be mapped. Earlier only mirror-like,<br />

polished objects were used in interferometry but now<br />

suddenly all kinds of objects could be studied. The interest<br />

in holographic methods increased dramatically.<br />

The most often used technique for vibration studies<br />

was time-average holographic interferometry [27.9,10].<br />

A hologram of the vibrating object was recorded while<br />

the object was vibrating. The exposure time of the pho<strong>to</strong>graphic<br />

plates was quite long, often about one second.<br />

This time was long compared <strong>to</strong> the period time of the<br />

object vibration so light fields from many cycles contributed<br />

<strong>to</strong> the <strong>to</strong>tal exposure of the pho<strong>to</strong>graphic plate.<br />

After development this plate is called a hologram. In<br />

the optical reconstruction of the hologram, these object<br />

fields were reconstructed simultaneously. Now, a sinusoidally<br />

vibrating object spends most of its time in each<br />

cycle at the turning points, where the velocity is momentarily<br />

zero. These parts (at a distance of twice the<br />

amplitude of vibration) therefore contribute the most<br />

(spend the longest time) <strong>to</strong> the <strong>to</strong>tal exposure and therefore<br />

these parts will also dominate the reconstructed<br />

fields. A time-average field is therefore reconstructed,<br />

and essentially light beams from the turning points interfere<br />

with each other. Iso-amplitude fringes that cover<br />

• Pulsed lasers give very short light pulses (exposure<br />

times ≈ 10 ns), that freezes propagating sound fields<br />

and vibrations as if stationary.<br />

Some disadvantages are:<br />

• Optical equipment and lasers are, in many cases, still<br />

quite expensive.<br />

• Trained personnel are needed <strong>to</strong> get full use of hightechnology<br />

equipment.<br />

• Speckle interferometry methods such as TV holography<br />

(DSPI, ESPI) most often need auxiliary<br />

equipment such as vibration-isolated optical tables<br />

placed in rooms that are not <strong>to</strong>o dusty or noisy. Others,<br />

such as pulsed TV holography and vibrometry<br />

instruments, work well in more hostile environments<br />

without vibration isolation.<br />

• Lasers are used and must be handled in a safe way.<br />

the object surface are mapped using this technique. The<br />

intensity of the reconstructed image of a sinusoidally<br />

vibrating surface can be described by<br />

I(x, y) = I0(x, y)J 2 0 (Ω) , (27.1)<br />

where I0(x, y) is the intensity of the object at rest and J0<br />

is the zero-order Bessel function of the first kind. The<br />

exposure does not have <strong>to</strong> span many cycles <strong>to</strong> get the J 2 0<br />

function in time-average techniques. It is also possible<br />

<strong>to</strong> record time-average interferograms of low-frequency<br />

vibrations.<br />

The argument<br />

Ω = K · L , (27.2)<br />

where K is a sensitivity vec<strong>to</strong>r defined as<br />

K = k1 − k2 , (27.3)<br />

and L(x, y) is the vibration amplitude field. k1 and k2 are<br />

the illumination and observation directions, respectively,<br />

measured relative <strong>to</strong> the normal of the object surface.<br />

With normal illumination and observation directions the<br />

maximum sensitivity becomes<br />

|K| = 4π/λ , (27.4)<br />

where λ is the laser wavelength used.<br />

A deformation field or a vibration field L(x, y) is<br />

however vec<strong>to</strong>rial, that is, it has three components.<br />

Part H 27.2

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