Theodolite: It was invented by Roemer, a Danish astronomer in 1690.
The instrument was used to observe the passage (transit) of stars across any
portion of the celestial meridian. About a century later it was modified to
suit the surveying requirements.
It is a most precise instrument
designed for the measurement of horizontal and vertical angles and has wide
applicability in surveying such as laying of horizontal angles, locating points
on line, prolonging survey lines, establishing grades, etc.
Figure shows three assemblies of
theodolite
|
Following three axis of
theodolite should always be perfectly perpendicular to each other, and by
considering this permanent adjustment of theodolite carried out.
1. Vertical
axis
2. Horizontal
axis
3. Line
of sight
Theodolite may be classified as:
1. Transit
theodolite
2. Non-transit
theodolite
Transit
theodolite is one in which the line of sight can be reversed by revolving the
telescope through 180◦ in the vertical plane.
Non-transit
theodolite are either plain theodolites or Y-theodolite in which the telescope
cannot be transited. The transit theodolite is mainly used and Y-theodolites
have now become obsolete.
Purposes for which a theodolite
can be used:
1. Measuring
the horizontal angles
2. Measuring
the vertical angles
3. Measuring
the deflection angles
4. Measuring
the magnetic bearings
5. Finding
the vertical height of an object
6. Measuring
the horizontal distance between two points
7. Finding
the difference of elevation between various points
8. Ranging
a line
Terms used in Theodolite
surveying:
1. Centering:
it involves setting the theodolite such that its vertical axis passes through
the station mark on the ground. It is done by means of a plumb line attached to
a hook below the instrument, or by optical plummet, if available. (Optical
plummet substitutes for a plumb bob when centering the instrument.)
2. Levelling:
The operation of levelling involves the plates being made horizontal with the
aid of bubble tubes or plate levels attached to them.
3. Transiting
(or plunging or reversing): It is a process of turning the telescope over the
horizontal axis through 180◦ in a vertical plane, making its upside down and
pointing in the opposite direction.
4. Face
left (bubble up): if the vertical circle is to the left of the observer when
sighting from the eyepiece end. The angle measured in this position is called a
face left observation. The bubble tube attached to the instrument lie above it.
5. Face
right (bubble down): if the vertical circle is to the right of the observer
when sighting from the eyepiece end. The angle measured in this position is
called a face right observation. The bubble tube attached to the instrument lie
below it.
6. Changing
face: it is the process of changing face from right to left. The face of
theodolite is changed by transiting the telescope first and then turning it
through 180◦.
7. Right
swing: it is made by turning the telescope to the right (or clockwise) in the
horizontal plane. The reading on the horizontal circle then increases.
8. Left
swing: it is made by turning the telescope to the left (or anti clockwise) in
the horizontal plane. The reading on the horizontal circle then decreases.
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