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STANDARD - Survey Instrument Antique Center!

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From the center of the instrument to the rod the distance is<br />

c being the distance from the objective to the center of the instrument.<br />

Since (c -f/) is practically a constant it is usually denoted by the single letter c<br />

and is known as the " constant of the instrument."<br />

When the line of sight is not level, but the stadia held at right angle to it, the<br />

formula for the horizontal distance is :<br />

D = fc.a.cos n ~\- c -j- om.<br />

(2)<br />

The member om -- sin n ; for a = 24', n 45 the value of om is but 8.4', and for<br />

o = 10' , n = 10 it is 0.86' ; this shows that om in most cases may safely be omitted.<br />

Some engineers let the rodman hold the staff perpendicularly to the line of sight ;<br />

they accomplish this by different devices, as, a telescope or a pair of sights attached<br />

at right angle to the staff. This method is not practicable, as it is very difficult,<br />

especially in long distances, and with greater vertical angles for the rodman to see<br />

the exact position of the telescopes, and furthermore, in some instances it is entirely<br />

Impossible, when, for instance, the point to be ascertained is on a place where only<br />

the staff can stand, but where there is no room for the man. The only correct way<br />

to hold the staff is vertically.<br />

In this case we have the following : (Fig. 4)<br />

MF = c + GF = c + &.C.D.<br />

CD must be expressed by AB.<br />

AB = a. AGB = 2m.<br />

And finally, after many<br />

CD = 2GF tan.m.<br />

transformations :<br />

D=c.cos n-f-a.A;.cos 2n a.fc.sin 2 n tan jrn. The third member of this equation may safely be neglected, as it is very small<br />

even for long distances and large angles of elevation (for 1500', n = 45 and k= 100,<br />

it is but 0.02'). Therefore, the final formula for distances, with a stadia kept ver-<br />

tically, and with wires equi-distant from the center wire, is the following :<br />

(3)<br />

D = C.POS n-\-a.k.cos*n.<br />

The value of c.cos n is usually neglected, as it amounts to but 1 or 1.5 feet ; it is<br />

exact enough to add always 1.25' to the distance as derived from the formula<br />

(3a)<br />

D = a.&.eos'n<br />

without considering the different values of the angle n.<br />

In order to make the subtraction of the readings of the upper and lower wire<br />

quickly, place one of the latter on the division of a whole foot and count the parts

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