WELDON'S RANGE FINDER.

Colonel Weldon has recently considerably modified and improved his

ingenious range finder, and we illustrate herewith from _Engineering_

the form in which it is now manufactured. It consists of a metal box,

the lid of which is shown open in the engraving, and on this lid are

fitted three prisms which are the essential constituents of the

instrument. When the lid is closed, these, with the compass and level,

also attached to the lid, lie inside the metal box, and are thus

thoroughly protected. The upper prism marked 1 is a right-angled one

and is mounted with the right angle outward; looking into the

left-hand corner of this prism one will see in it, by double

reflection, objects lying on one's right hand. Below this is a second

prism with a principal angle of 88 deg. 51 min. 15 sec., and below

this a third with a principal angle of 74 deg. 53 min. 15 sec.

A level and a compass are also mounted on the lid as shown. To use the

instrument the observer stands so that the object the range of which

is required lies on his right hand, and looking into the left-hand

corner of the upper prism views it there by double reflection from the

internal faces of the prism. At the same time looking through the

opening shown in the lid below the prism he selects some object, which

appears nearly in line with the image seen in the prism. He then

shifts his position till these two images coincide, in which case

lines joining him with the two objects will make right angles with

each other. In Fig. 2, O is the object whose range is required, D the

object seen by direct vision, and A the position of the observer. The

observer now marks his position on the ground, and shifting the

instrument looks into the left-hand corner of the second prism, when

he again sees the image of the object, whose range is required, by

double reflection, but lying now to the right of the object, D. He

then retires, keeping in line with A and D, till he reaches B, when

the two images again coincide; the lines joining them and the observer

now make an angle of 88 deg. 51 min. 15 sec. Then in the triangle,

OBA, OA = tan 88 deg. 51 min. 15 sec. X A B = 50 AB. The length AB is

easily paced, and the distance OA is 50 times this length.

A longer base, and probably greater accuracy, can be obtained by using

the second prism only, as indicated in Fig. 3, in which case the

distance of the object is 25 times the distance BC. This second prism

is, however, best adapted for predicting the range of moving objects.

Three observers are required. Two of them have finders, while the

other measures the distance between the two. The first two observers

separate, and No. 2 takes a position such that the object is reflected

to one side of observer No. 1, whom he views by direct vision. As the

object continues to move, its image gets nearer and nearer No. 1, who

during the whole of the time moves a little to one side or the other,

so as to keep the image of the object constantly in line with No. 2.

Just as the image of the object gets very near No. 1, No. 2 calls out

"Ready," the distance between the two observers is taken by the third,

and when the image of the object actually falls on No. 1 its distance

is just 25 times the distance between them, and the guns set to this

range are fired by word of command from No. 2.

[Illustration: FIG. 2. & FIG. 3.]

By using the third prism in conjunction with the second a still longer

base of one-fourth the distance of the object can be employed. The

range finder can also be used as a depleidoscope for transit

observations. For this purpose it is mounted on a block of wood by

means of elastic band and leveled by the level on its lid, being at

the same time set in the meridian of the place. The lid is opened to

make an angle with the horizon equal to the latitude of the place of

observation. On looking into the upper prism two images of the sun

will be seen on each side of the apex of the prism, which gradually

approach each other as the sun nears the meridian, and finally

coincide as it passes it, the time of which being noted gives the

longitude of the place.

Extensive trials of the instrument have been made both in this country

and in India, which agree in showing that the average error in using

the instrument is about 2½ to 3½ per cent.

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Scientific American Supplement, No. 829, November 21, 1891 · 第 30 / 66 题