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STANDARD - Survey Instrument Antique Center!

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21<br />

applied with an adjusting pin about one and one half inches long, and held between<br />

the thumb and forefinger, will then make a perfect contact. For instance, after the<br />

it is<br />

opposing capstan-heade I screws of the cross-wire reticule have come to a bearing,<br />

only necessary to give them each a slight turn, say from 20 to 30 (with the usual pitch<br />

of these screws) in order to insure such a tightness that a moderate pressure of the<br />

finger upon these screws, or an accidental gliding of the hand over them, cannot change<br />

their relative position. On the other hand, if one pair of these opposing screws be<br />

in all likeli-<br />

fastened tightly during the tentative process of adjustment, there will be,<br />

hood, at the end, an excessive strain exerted upon the pair of opposing screws at right<br />

angles, which will make itself felt at any change of temperature, or whenever any<br />

external pressure may be momentarily applied to them. Jt is but natural that these<br />

continual changes in the resultant pressure must affect the adjustments in a like man-<br />

ner. To obviate such changes the procedure should be as follows :<br />

Having placed approximately in position the principal wire of an instrument : viz.,<br />

in a transit, the vertical wire in a plane perpendicular to the horizontal axis of revolu-<br />

tion, in a level, the horizontal wire in a plane perpendicular to the vertical axis<br />

of revolution, the other wire should be approximately adjusted for collimation,<br />

with the capstan-headed screws only moderately tightened. This accomplished, the<br />

capstan -headed screws of each pair in succession should be unscrewed about one-<br />

quarter turn, and again screwed tight the same amount. Now if the two pairs of<br />

opposing screws have exerted no undue strain upon themselves, the telescope tube, or the<br />

wire reticule, the principal wire will still be in the perpendicular plane ; but if the screws<br />

have been used too much the wire will have slightly moved out of the perpendicular<br />

plane. Therefore all four capstan-headed screws will have to be released again, say<br />

about | turn, so that they may be moved simultaneously until the principal wire is<br />

again in a plane perpendicular to the axis of revolution, and then each pair in succession<br />

must be again tightened an equal amount. The adjustment of the wires lor collimation<br />

must now be made in turn the less important wire should always be taken<br />

up first by slightly releasing the capstan-headed screw away 1 from which the wire<br />

must be moved, and tightening the opposite screw the same amount, and repeating<br />

this process until the adjustment is gradually perfected. If during this operation either<br />

or both of these wires Lave become so much displaced that the capstan-headed screws<br />

have to be moved more than a quarter turn, it would be advisable to slightly release all<br />

four of them again, in succession, and commence anew.<br />

It should be said here, that the force applied by the capstan-headed screws<br />

cannot break or affect the tightness of the wires in any case, since the reticule, as<br />

made by us, although very light in weight, is of a very stiff form. Too great pressure<br />

exerted by the capstan-headed screws against the outer tube of the telescope may,<br />

however, change die form of the main tube, thereby affecting the true fitting of the<br />

object-slide, and creating friction of so serious a nature as to lead to the fretting of the<br />

object slide mentioned in other paragraphs.<br />

In following the above-described course, the cross-wire reticule occupies a position<br />

in the telescope free from any excessive side strain the result of which is found in the<br />

;<br />

greater permanency of these adjustments and ; although it may require a little more time<br />

for an inexperienced person to make the adjustments in this manner, the satisfaction<br />

derived from their greater permanency will more than recompense for the extra time<br />

spent on them. The adjustments should be made at leisure, and should not be<br />

meddled with, unless they appear to be permanently deranged; when, ordinarily,<br />

the adjustments will merely require a very slight turn of the capstan-headed screws<br />

and opposing nuts in the proper direction. 2<br />

Unequal exposure of the instrument to the<br />

sun, or exposure to sudden changes of temperature, may for a time expand some<br />

parts more than others, so that the instrument may seem to be slightly out of adjustment.<br />

In such a case it would be better to stop temporarily and cover the<br />

instrument with a bag to allow the temperature to become equalized, instead of attempting<br />

adjustments that would need to be repeated when the instrument is<br />

again in a normal condition. The use of metals of different co-efficients of expansion<br />

in the construction of corresponding parts of an instrument w?ll naturally lead to a<br />

1 We refer here exclusively to the more common instruments of American manufacture, where the<br />

shoulders of the capstan-headed screws bear against ihe outer tube of the telescope, and where the adjusting<br />

threads are contained in the wire reticule. In other designs where, as in most instruments of Cont nenta<br />

><br />

Europe, the capstan-headed screws are made to butt ajrainst the wire reticule, the capstan-headed screws<br />

towards which the wire mu-t be moved, must first be loosened. In the latter case this action is identical<br />

with that of opposing nuts used for the adjustment of most telescope levels on American instruments.<br />

2 See page 58.

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