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Reflecting Level," invented by Colonel Burel; a description of which, is given in the second volume of "Professional Papers of the Royal Engineers."

The principle upon which this instrument acts is implied by its name. In a plane mirror the rays are reflected as though they diverged from a point behind the mirror, situated at precisely the same distance in rear of its surface, as the object itself is in front. If the mirror be vertical, the eye and its image are on the same horizontal line; and any object coinciding with these is necessarily on the same level. It appears then only requisite to ensure the verticality of a small piece of common looking-glass set in a frame of wood or metal, to be able without further assistance to trace contour lines in every direction, or to take a section on any given line. The mirror AB, described in the paper alluded to, is only one inch square, fixed against a vertical plate of metal weighing about 1lb., and suspended from a ring m, by a twisted wire n, so that it may hang freely, but not turn round on its axis of suspension. It can either be used for sketching in the field, being held by this ring at arm's length; or fixed, for greater accuracy, in a frame which fits upon the top of the legs of a theodolite, with a bar of metal like a bent lever, pressing so slightly against it from below, that it may check any tendency to oscillation, and at the same time not prevent the mirror from adjusting itself vertically by its own. weight. The accompanying sketch will render this description more intelligible.

The required verticality of the plane of the mirror is thus ascertained: a level spot of ground is chosen, where it is suspended in its frame (or any temporary stand) 40 or 50 yards from a wall, and the prolongation of the line of sight from the eye to its image, coinciding with a fine silk thread across the centre of the mirror, is marked on the wall, which is visible through a

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small opening p, in the metal frame. The mirror is then turned round, and the observer, placed between it and the wall, with his back to the latter, notes the spot where the image of his eye

coincides with the reflected wall above or below the former mark. The mean distance between these two points is assumed and marked; and, by turning the screw r, the centre of gravity of the mirror is altered until the image of the eye coinciding as before with the silk thread agrees also with this central mark on the wall. It would perhaps be a better plan to send an assistant some distance behind the mirror with a levelling-staff, the vane of which could be raised or lowered to coincide with the line of sight; on reversing the mirror (the staff remaining stationary) the vane would be again moved, until its refleted zero mark is cut by the thread on a level with the image of the eye, and finally, the mirror adjusted by the screw, to the mean between these two heights; this method admits, apparently, of greater nicety than a chalk mark on a rough wall.

The reflecting-level is not generally known in this country; but for many purposes it is superior to any other description of instrument, particularly for tracing contour lines on the ground in a military sketch. It is peculiarly simple in its construction; is easily managed, easily adjusted, is not liable to have this adjustment deranged, or to be injured by a fall; is from its size, more portable than any other instrument, and can be used either held at an arm's length, or at a distance of several feet; in which position, the length of the line of sight ensures the greatest accuracy.

The levelling-staff, a necessary accompaniment to each of the species of levelling instruments described, was formerly made with a sliding vane to move up and down a staff graduated to feet and decimals, or feet and inches: this was effected by a string and pulley, or the staff itself was made in two or three pieces, each of the upper pieces sliding in a groove in the one next below it. For any height less than the length of the first piece (generally about 6 feet) the vane was slid up or down with the hand; but for a greater height, the second piece, with the vane at the top, was moved up bodily till the centre of the vane was cut by the line of the optical axis of the instrument, when the height was read on another scale graduated downwards from the top on the side of the lower joint of the staff. A description of staff was however introduced some years ago by Mr. Gravatt, and has been since improved upon, on which the divisions (in feet and decimals) are

marked so distinctly that they can be read by the observer without the use of a vane, or the necessity of trusting to an assistant; the figures are inverted to suit the inverting telescopes now generally used, and instead of moving about a heavy iron tripod on which to rest the staff, a species of shoe with a hinge is attached to it, which allows the face to be turned round in any required direction without the staff being moved off the ground. Though much more convenient, and less liable to mistakes in reading than the old species of staff, the same degree of accuracy cannot be obtained with it.

To proceed to the method of using the spirit-level or other instrument for tracing horizontal lines, and also of keeping the field-book in levelling for sections. In the system formerly pursued, the instrument was set up at one end of the line A, of which a section was required; and having ascertained the accuracy of its adjustments, and levelled it by the plate-screws, an assistant was sent forward with the levelling-staff to the first station, and the difference between the height of the vane when intersected by the cross wires of the telescope, and the height of the optical axis of the instrument from the ground, gave of course the difference of level between these two points. The distance was then measured and entered in the field-book, and the level moved on to the first station, the staff being sent on to the second, where the same process was repeated.

It is self-evident that this manner of levelling is vitiated by the

errors of curvature and refraction, which, if not allowed for in a long section, would in the end produce a considerable error. But the necessity for these corrections is avoided by simply placing the instrument half-way between the two stations, and either in the line of section, or on one side of it.

Thus the level * being set up, as in the figure at a, the difference between the reading on the staff set at the back station A, and at


the forward station (1), gives at once the difference of level between the ground at these points, without any correction for refraction or curvature, and also without taking into account the height of the instrument; a slight error in the line of collimation of the telescope also does not impair the results, as the elevation or depression of the optical axis would have the same effect on both staves; whereas in levelling entirely by the forward station, the least error in the adjustment of the instrument is fatal to the accuracy of the section, being always carried on, whether additive or subtractive. This assertion, however, supposes the instrument to be exactly equidistant from the two stations, which in ground having a great inclination is often impossible; nevertheless, by good management, any reference to the table of curvature and refraction may generally be avoided, and if this correction is necessary, it should be made merely for the difference between the distances.

In keeping the detail in the field, the horizontal and vertical distances are sometimes written on a sort of rough diagram, as recommended in levelling by angles of elevation and depression with the theodolite; but the most general and best plan is to enter all the dimensions in the field-book, particularly if the distance to be levelled is considerable, and references are made to benchmarks. There are slight differences in the modes in which this field-book is kept; but the following example, with the description

* By having two assistants, with levelling-staves, one for the back and the other for the forward station, much time may be saved.

below, will show the usual method of entering the details, so as to render them at once available for transferring to paper * :— :

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This table almost explains itself: the first column headed “Distances," contains the distances measured between each place where the staff is put upt. The second and third columns are for the readings of the staff at each back and forward station, the differences between each of which are entered under the fourth and fifth columns, headed + and under the two last, headed "Rise" and "Fall," are carried out the total rise or fall of each place where the staff was placed, above or below the starting point.-The bench-mark at the end of the fourth station being in the line of the section, the distance is entered as usual; but that at the seventh, being out of this line, and its level merely ascertained for a future reference, there is no dimension entered in the column of "Distances," so that it is not plotted in the section.

* For more detailed instructions on the method of levelling for and plotting sections see Mr. Simms' work. Where very great accuracy is required, the level is always read over a second time, the instrument being thrown out of adjustment and readjusted—a certain amount of difference only is allowed-about 003 ft. A levelling staff, with an improved vane, is also used, instead of the now common staff without a vane.

+ Where only lineal distances or sectional areas are required, a chain of feet is the most convenient for use, instead of the Gunter's chain used for determining superficial areas in


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