STANDARD - Survey Instrument Antique Center!
STANDARD - Survey Instrument Antique Center!
STANDARD - Survey Instrument Antique Center!
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58<br />
To adjust the line of collimatioii in Erecting and<br />
Inverting Telescopes.<br />
NOTE: To adjust the line of collimation in a telescope showing objects<br />
erect, follow the simple rule that the diaphragm bearing the wires must be moved<br />
in the direction in which the error is observed (as if to increase the error) ;<br />
in telescopes showing objects inverted the wires must be moved in the direction<br />
lessening the error observed. See diagrams below.<br />
Erecting Telescope.<br />
FIG.I Fio.2<br />
To move the horizontal wire for collimation explained above it must be understood<br />
that the dotted line in the upper half of the field or view, Fig. 1, shows the horizontal<br />
wire where it is actually situated on the reticule, but that through the reversing<br />
action of the erecting eye-piece the cross-wire image is reversed and therefore<br />
the horizontal wire is seen in the lower half as shown in the diagram. Therefore, if<br />
the horizontal wire seen in the lower half of the diagram must be moved upwards,<br />
then contrary to the appearance, screw A must be loosened, and B tightened an<br />
equal amount in order to bodily move the wire reticule towards the center of the<br />
stationary field of view (indicated by the dotted intersection) until one-half of<br />
the error is corrected when the wire will be adjusted and appear in the center of the<br />
field of view, provided the optical axis of the eye-piece has been previously centered.<br />
To move the vertical wire for collimation explained on page 54, remember<br />
that the dotted line at the left, Fig. 2, shows the vertical wire where it is actually<br />
situated on the reticule, but that through the reversal of the cross-wire image by<br />
the use of an erecting eye-piece it is now seen at the right in the field of view in the<br />
diagram; therefore, adjusting screw A must be loosened and B tightened an equal<br />
amount in order that the reticule will bodily move towards B, when the vertical<br />
wire seen at the right will pass towards the center of the stationary field of view<br />
(indicated by the dotted intersection) until one-quarter of the error observed is<br />
removed, when the wire will be in complete adjustment at the optical axis.<br />
Inverting Telescope.<br />
RG.3<br />
FlG.4<br />
To move the horizontal wire for collimation, page 54, the observed error must<br />
be corrected by moving the wire reticule one-half the amount hi the direction it is<br />
lessened, when the telescope is revolved in improvised wyes as in a wye level. Thus,<br />
Fig. 3, if the wire must be moved down, A must be loosened and B tightened an equal<br />
amount.<br />
To move the vertical wire for collimation explained above, the observed error<br />
must be corrected by moving the wire recticule one-quarter of the amount in the<br />
direction it is lessened. Therefore, if the wire must come to the right, A, Fig. 4, must<br />
be loosened, and B tightened an equal amount until the object is attained.<br />
B