STANDARD - Survey Instrument Antique Center!
STANDARD - Survey Instrument Antique Center!
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.