UNIVERSITY OF WISCONSIN.

Any one who has stood near a large naval gun during its discharge,

will, I think, be prepared to admit that the sound of the explosion

affects not only the ears, but the whole body as well, which

experiences something not unlike a sudden blow. This blow, or

concussion, as it is generally termed, is merely the impact of the wave

of compressed air, spreading out in all directions around the gun. In

the case of ordinary sounds, the compression of the air in the wave is

so slight that only the delicate auditory nerves respond to the impact,

hence we naturally conclude that sounds are perceived only by the ear.

When dealing with sounds of very great intensity, this notion must be

somewhat modified, for they certainly can be felt as well as heard. In

some extreme cases, in fact, the sensation of feeling may be stronger

than that of hearing, as in the case of which I shall speak presently.

Is it also possible that we can perceive sound through the medium of

any other sense organ, say the eye? ‘To see a noise’ certainly sounds

like an absurdity; yet under certain conditions, sound waves in air

can be made as distinctly visible as the ripples on a pond surrounding

the splash of a stone. That they are not seen under ordinary

conditions does not justify us in assuming them to be invisible. We

all know that the currents of hot air rising from a stove, while not

usually conspicuous, can be made visible by properly regulating the

illumination, as by looking along the surface of the stove towards a

window. The hot air is visible because in its optical properties it is

different from the cold air surrounding it. The rays of light, passing

through the unequally heated portions of the air, are bent in different

directions, causing a distortion of objects seen through the heated

currents. What we see, strictly speaking, is not the hot air itself,

but a wavering and swimming of the objects seen through it. Yet I think

we are justified in saying that the eye perceives the hot air.

Now sound waves in air, which are merely regions where the air is

somewhat compressed, differ in their optical properties from the

uncompressed portions, just as the hot air differs from the cold.

As the pictures illustrating this article testify, they may be seen

and photographed under proper conditions of illumination as readily

as solid objects. We must remember, in the first place, that a sound

wave travels with a velocity something greater than a thousand feet a

second, rather less than the speed of a modern rifle ball, yet ten

times faster than the fastest express train. The wave, even if it were

stationary, could be seen only by adjusting the illumination with far

greater care than was necessary in the case of the hot air, and we

consequently can easily understand why we never see the waves under

ordinary conditions.

While it is true that laboratory appliances are generally required to

render them visible, I should like at the outset to cite an example to

show that in the case of very loud sounds occurring in the open air

the wave can be perceived by the eye, without the aid of any apparatus

whatever. I will quote from an article by Prof. C. V. Boys, which

appeared in ‘Nature,’ June 24, 1897. Mr. Boys first cites the following

letter from Mr. E. J. Ryves: “On Tuesday, April 6th, I had occasion,

while carrying out some experiments with explosives, to detonate one

hundred pounds of a nitro-compound. The explosive was placed on the

ground in the center of a slight depression, and in order to view the

effect, I stationed myself, at a distance of about three hundred yards,

on the side of a neighboring-hill. The detonation was complete, and a

hole was made in the ground five feet deep and seven feet in diameter.

A most interesting observation was made during the experiment. The sun

was shining brightly, and at the moment of detonation the shadow of the

sound wave was most distinctly seen leaving the area of disturbance.

I heard the explosion as the shadow passed me, and I could follow it

distinctly in its course down the valley for at least half a mile; it

was so plainly visible that I believe it would photograph well with a

suitable shutter.”

Professor Boys at once made preparations for photographing the

phenomenon at the first opportunity. On May 19th the experiment was

made. One hundred and twenty pounds of a nitro-compound were exploded,

and an attempt made to photograph the sound shadow, both with the

camera and the kinematograph, the latter instrument designed and

operated by Mr. Paul. Writing of the experiment, Professor Boys says:

“On the day on which I was present, about one hundred and twenty pounds

of a nitro-compound were detonated, and ten pounds of black powder

were added to make sufficient smoke to show on the plate. As the

growth of the smoke cloud is far less rapid than the expansion of the

sound shadow, no confusion could result from this. At the time of the

explosion my whole attention was concentrated upon the camera, and for

the moment I had forgotten to look for the ‘Ryves ring,’ as I think

it might be called; but it was so conspicuous that it forced itself

upon my attention. I _felt_, rather than _heard_, the explosion at

the moment that it passed. We stationed ourselves as near as prudence

would allow, at a distance of one hundred and twenty yards, so that

only about one third of a second elapsed between the detonation and the

passage of the shadow. The actual appearance of the ring was that of

a strong, black, circular line, opening out with terrific speed from

the point of explosion as a center. It was impossible to judge of the

thickness of the shadow; it may have been three feet, or it may have

been more at first, and have gradually become less in thickness, or

possibly in depth of shade.”

Unfortunately, Professor Boys’s apparatus did not work satisfactorily,

but a most interesting series of pictures was secured by the

kinematograph. This instrument had been constructed especially for

taking pictures at a very high rate of speed, viz., eighty exposures

a second, or four times the usual number. The sound wave appears in

the first dozen pictures as a hazy ring of light, opening out from

the center of explosion. The ring, though not very conspicuous when

the pictures are viewed singly, becomes a striking object when they

are projected in rapid succession on the screen. We see the rush of

smoke along the ground to the box in which the explosion is confined

(the smoke of the quick fuse); then comes the burst of the explosion

with such startling reality that we involuntarily jump. The image of

the sound wave flies out in the form of a white ring, and is gone in

a moment; and there remain only the rolling clouds of smoke. It is

interesting to observe the development of the explosion by running the

machine quite slowly, and by thus magnifying time to follow the changes

which ordinarily occur in such rapid succession that the eye is unable

to perceive them.

Of this series of pictures, Professor Boys says: “The kinematograph

fails to show any _black_ ring; and this is not surprising, as with the

exposure of about one one hundredth of a second the shadow would have

to be at least eleven feet thick in order that some part should remain

obscured during the whole exposure. As a fact, there is clearly seen a

circular light shading, which does--so far as one can judge from the

supposed rate of working and the known distances--expand at about the

same rate as the observed shadow, but it is lighter than the ground and

shaded, instead of being dark and sharp, as seen by the eye.”

[Illustration: KINETOSCOPE FILM OF EXPLOSION.]

So much for the visibility of sound under ordinary conditions. In

the laboratory, by means of an optical contrivance due to the German

physicist Toepler, we can secure a means of illumination so sensitive

that the warm air rising from a person’s hand appears like dense

black smoke. Moreover, since we are working on a small scale, we can

use the electric spark as the source of light, and dispense with the

photographic shutter. This is a great advantage, for the time of the

exposure is, under these conditions, only about one fifty-thousandth of

a second, during which time the sound wave will move scarcely a quarter

of an inch. During the past year I have made a very complete series

of photographs of sound waves, which illustrate in a most beautiful

manner the fundamental principles of wave motion. It is not practicable

to give here a full description of the apparatus used, but a brief

outline may make the method intelligible. The sound photographed in

each case is the crack of an electric spark, which is illuminated and

photographed by the light of a second spark, occurring a brief instant

later. In front of a large lens (a telescope objective, for example)

two brass balls are mounted, between which the ‘sound spark,’ as I

shall call it, passes. The instant the spark jumps across the gap, a

spherical wave of condensed air starts out, which, when it reaches

our ear, gives the sensation of a snap. The object is to photograph

this wave before it gets beyond the limits of the lens. The camera is

mounted in front of the lens and focussed on the brass balls, which

appear in line in the picture, so that the sound spark is always hidden

by the front one. The spark, on jumping between the balls, charges a

Leyden jar, which instantly discharges itself between two wires placed

behind the lens, producing the illuminating spark. This second spark

can be made to lag behind the first just long enough to catch the sound

wave when it is but a few inches in diameter, notwithstanding the fact

that the spherical wave is expanding at the rate of eleven hundred feet

a second. The photographs show in every case the circle of the lens

filled up with the light of the illuminating spark, the brass balls

(in line) and the rods that support them, and the sound wave, which

appears in the simplest case as a circle of light and shade surrounding

the balls. By placing an obstacle in the way of the wave we get the

reflected wave or echo, and we shall see that the form of this echo may

be very complicated.

[Illustration: FIG. 1. SOUND WAVE REFLECTED FROM A PLANE SURFACE.]

It will be well at the outset to remind the reader of the close analogy

between sound and light. A burning candle gives out spherical light

waves, just as the snapping sparks give out sound waves. The form of

the reflected light wave will be identical with that of a sound wave

reflected under similar conditions. As we can not see the light waves

themselves, we can only determine their form by calculation, and

it is interesting to see that the forms photographed are identical

in every case with the calculated ones. The object in view was to

secure acoustical illustrations of as many of the phenomena connected

with light as possible. We will begin with the very simplest case of

all: the reflection of a spherical sound wave from a flat surface,

corresponding to the reflection of light from a plane mirror. It can be

shown by geometry that the reflected wave or echo will be a portion of

a sphere, the center of which lies as far below the reflecting surface

as the point at which the sound originates is above it. In the case of

light, this point constitutes the image in the mirror. Referring to the

photograph, we see the reflected wave in three successive positions,

the interval between the sound spark and the illuminating spark having

been progressively increased. The brass balls are shown at A, and

beneath them the flat plate B, which acts as a reflector. In the first

picture the sound wave C appears as a circle of light and shade, and

has just intersected the plate. The echo appears at D. In the next

two pictures the original wave has passed out of the field, and there

remains only the echo.

It may, perhaps, be not out of place to remind the reader of the

relation between rays of light and the wave surface. What we term light

rays have no real existence, the ray being merely the path traversed by

a small portion of consecutive wave surfaces. Since the wave surface

always moves in a direction perpendicular to itself, the rays are

always normal to it. For instance, in the above case of a spherical

wave diverging from a point, the rays radiate in all directions

from the point; the same is true in the case of the echo, the rays

radiating from the image point below the reflecting surface. In all

subsequent cases the reader can, if interested in tracing the analogy

between sound and light, draw lines perpendicular to the reflected wave

surfaces representing the system of reflected waves.

We will now consider a second case of reflection. We know that if a

lamp is placed in the focus of a concave mirror, the rays, instead of

diverging in all directions, issue from the mirror in a narrow beam.

The headlight of a locomotive and the naval searchlight are examples of

the practical use made of this property. If the curvature of the mirror

is parabolical, the rays leaving it are parallel; consequently mirrors

of this form are employed rather than spherical ones. But what has

the mirror done to the wave surface which is obviously spherical when

it leaves the lamp, and what is its form after reflection? The wave

surface, I have said, is always perpendicular to the rays; consequently

in cases where we have parallel rays we should expect the wave to be

flat or plane.

[Illustration: FIG. 2. SPHERICAL SOUND WAVE.]

Examine the second photograph, which shows a spherical, sound wave

starting at the focus of a parabolic mirror. The echo appears as a

_straight line_, instead of a circle as in the previous case, which

shows us that the wave surface is flat.

If now our mirror is a portion of a sphere instead of a paraboloid,

our reflected wave is not flat, and the reflected rays are not all

parallel, the departure from parallelism increasing as we consider

rays reflected from points farther and farther away from the center

of the mirror. A photograph illustrating the reflection of sound

under these conditions is next shown, the echo wave being shaped like

a flat-bottomed saucer. As the saucer moves upward the curved sides

converge to a focus at the edge of the flat bottom, disappearing for

the moment (as is shown in the fourth picture of the series), and then

reappearing on the under side after passing through the focus, the

saucer turning inside out.

If, instead of having a hemisphere, as in the last case, we have a

complete spherical mirror, shutting the wave up inside a hollow ball,

we get exceedingly curious forms; for the wave can not get out, and

is bounced back and forth, becoming more and more complicated at each

reflection. This is illustrated in our next photograph, the mirror

being a broad strip of metal bent into a circle.[D] Intricate as

these wave surfaces are, they have all been verified by geometrical

constructions, as I shall presently show.

[D] Cylindrical mirrors have been used instead of spherical,

for obvious reasons. A sectional view of the reflected wave

is the same in this case as when produced by a spherical

surface.

Another very interesting case of reflection is that occurring inside

an elliptical mirror. When light diverges from one of the two foci of

such a mirror, all the rays are brought accurately to the other focus.

If rays of light come to a focus from all directions, it is evident

that the wave surface must be a sphere, which, instead of expanding,

is collapsing. This is very beautifully shown in the photographs. The

sound wave starts in one focus and the reflected wave, of spherical

form also, shrinks to a point at the other focus. (See fig. 5.)

[Illustration: FIG. 3. A WAVE REFLECTED FROM A PORTION OF A SPHERE.]

[Illustration: FIG. 4. A WAVE FROM A CYLINDRICAL MIRROR.]

In the next series the wave starts outside of the field of the lens,

and enters a hemispherical mirror. We know that a concave mirror has

the power of bringing light to a focus at a point situated half-way

between the surface of the mirror and its center of curvature. If the

light comes from a very distant point, and the mirror is parabolic in

form, the rays are brought _accurately_ to a focus; which means that

the reflected wave is a converging sphere,--a condition the opposite of

that in which spherical waves start in the focus of such a mirror. If,

however, the mirror is spherical, only a portion of the light comes to

a focus. On examining the pictures we see that the reflected wave has

a form resembling a volcanic cone with a bowl-shaped crater. See the

third and fourth pictures of the series. The bowl of the crater shrinks

to a point half-way between the surface of the mirror and its center

of curvature, and represents that portion of the light which comes to

a focus, while the sides of the cone run in under the collapsing bowl,

and eventually cross. (No. 6 of the series.) From now on the portion

which has come to a focus diverges, uniting with the sides of the cone,

the whole passing out of the mirror in the form of a horseshoe.

[Illustration: FIG. 5. A WAVE FROM AN ELLIPTICAL MIRROR.]

[Illustration: FIG. 6. A WAVE STARTING OUTSIDE THE FIELD OF THE LENS.]

[Illustration: FIG. 7. A CASE OF REFRACTION.]

We will now consider a case of refraction, and show the slower velocity

of the sound wave in carbonic acid. A narrow glass tank, covered with

an exceedingly thin film of collodion, was filled with the heavy gas

and placed under the brass balls. When the sound wave strikes the

collodion surface, it breaks up into two components, one reflected

back into the air, the other transmitted down through the carbonic

acid. An examination of the series shows that the reflected wave in air

has moved farther from the collodion film than the transmitted wave,

which, as a matter of fact, has been flattened out into a hyperboloid.

Exactly the same thing happens when light strikes a block of glass. We

have rays reflected from the surface, and rays transmitted through the

block, the waves which give rise to the latter moving slower than the

ones in air.

A complete discussion of all of the cases that have been studied in

this way would probably prove wearisome to the general reader. Prisms

and lenses of collodion filled with carbonic acid and hydrogen gas

have been made, and their action on the wave surface photographed.

Diffraction, or the bending of the waves around obstacles, and the

very complicated effects when the waves are reflected from corrugated

surfaces, are also well shown. I shall, however, omit further mention

of them and speak of but one other case, possibly the most beautiful of

all.

[Illustration: FIG. 8. A MUSICAL TONE.]

In all the cases that we have considered, it must be remembered that

we have been dealing with a single wave--a pulse, as it is called.

Musical tones are caused by trains of waves, the pitch of the note

corresponding to the distance between the waves, or to the rate

at which the separate pulses beat upon the drum of the ear. For

studying the changes produced by reflection, wave trains would have

been useless, owing to the confusion which would have resulted from

the superposition of the different waves. Moreover, it is doubtful

whether an ordinary musical tone could be photographed in this way;

for the distance between the waves, even in the shrillest tones, is

four or five inches, and the abrupt change in density, necessary for

the perception of the wave, is not present. It is possible, however,

to create a wave train or musical tone which can be photographed.

The reader may perhaps have noticed that on a very still night, when

walking beside a picket fence or in front of a high flight of steps,

the sounds of his footsteps are echoed from the palings as metallic

squeaks. Each picket, as the single wave caused by the footfall sweeps

along the fence, reflects a little wave; consequently a train of waves

falls on the ear, the distance between the waves corresponding to the

distance between the pickets. The closer together the pickets, the

shriller the squeak. In point of fact, the distance between the waves

in such a train is twice the distance between the palings, since they

are not struck simultaneously by the footstep wave, but in succession.

This phenomenon, of the creation of a musical tone by the reflection

of a noise, was reproduced by reflecting the crack of the spark from

a little flight of steps. In the first picture the wave is seen half

way between its origin and the reflecting surface. In the second it

has struck the top stair, which is giving off its echo, the first wave

of our artificially constructed musical tone. In the third we find the

original wave at the sixth step, with a well-developed train of five

waves rising from the flight. The following three pictures show the

further development of the wave train. The height of each step was

about a quarter of an inch; consequently the distance between the waves

was half an inch. This would correspond to a note about three octaves

above the highest ever used in music.

[Illustration: FIG 9. THE REFLECTION INSIDE THE HOLLOW SPHERE.]

While experimenting with the complete circular mirror, which, it will

be remembered, gave the most complicated forms, it occurred to me that

a very vivid idea of how these curious wave surfaces are produced

could be obtained by preparing a complete series in proper order on

a kinetoscope film, and then projecting them in succession on the

screen. The experimental difficulties were, however, too great to make

it seem worth while to attempt to obtain a series of pictures of the

actual waves, it being very difficult to accurately regulate the time

interval between the two sparks. The easier method of making a large

number of geometrical constructions, and then photographing them in

succession on the film, was accordingly adopted. Three complete sets

of drawings, to the number of about one hundred each, were prepared for

three separate cases of reflection;--viz.: the entrance of a plane wave

into a hemispherical mirror, the passage of a spherical wave out from

the focus of a hemispherical mirror, and the multiple reflection of a

spherical wave inside of a complete spherical mirror. Special methods

were devised for simplifying the constructions, and much less labor was

required in the preparation of the diagrams than one would suppose. The

results fully justified the labor, the evolutions of the waves being

shown in a most striking manner. These films I exhibited before the

Royal Society in February last, and a more complete description of the

manner of preparing them may be found in the Proceedings of the Society.

A portion of one of these series is reproduced, about one in four or

five of the separate diagrams being given. The series runs from left to

right in horizontal rows. When projected on the screen, the spherical

wave is seen gradually to expand from the focus point, like a swelling

soap bubble; it strikes the surface, and the bowl-shaped echo bounces

off and follows the unreflected portion across the field; these two

portions are then reflected in turn, and the curiously looped wave

flies back and forth across the mirror, changing continuously all the

time, and becoming more complicated at each reflection. These diagrams

should be compared with the photographs shown in the fourth series.

One must not suppose that these beautiful forms exist only in the

laboratory. Every time we speak, spherical waves bounce off the floor,

ceiling and walls of the room, while in any ordinary bowl or basin

the curious crater-shaped echoes are formed. Glance once more at the

wave surfaces produced within a hollow sphere, and try to imagine the

complexity of the aerial vibrations caused by a fly buzzing around in

an empty water-caraffe! The photographs enable us to realize what is

going on around us all the time--this our perceptions are fortunately

too dull to perceive. Life would be a nightmare if we were obliged to

see the myriads of flying sound waves bounding and rebounding about

us in every direction, and combining into grotesque and ever-changing

forms. It is just as well, on the whole, that the light of the electric

spark and the delicate optical device of Toepler are necessary to bring

them into view.

The Popular Science Monthly, August, 1900 Vol. 57, May, 1900 to October, 1900 · 第 10 / 34 题