THEODOLITE SURVEYING IN ENGINEERING PDF FILE

THEODOLITE SURVEYING
THEODOLITE SURVEYING 1

So far we have been measuring horizontal
angles by using a Compass with respect to meridian,
which is less accurate and also it is not possible to
measure vertical angles with a Compass.
So when the objects are at a considerable
distance or situated at a considerable elevation or
depression ,it becomes necessary to measure horizontal
and vertical angles more precisely. So these
measurements are taken by an instrument known as a
theodolite.
2

The system of surveying in which the angles are
measured with the help of a theodolite, is called
Theodolite surveying.
3

THEODOLITE
The Theodolite is a most accurate surveying
instrument mainly used for :
• Measuring horizontal and vertical angles.
• Locating points on a line.
• Prolonging survey lines.
• Finding difference of level.
• Setting out grades
• Ranging curves
• Tacheometric Survey
4

TRANSIT VERNIER THEODOLITE

Fig. Details if Upper & Lower Plates.

CLASSIFICATION OF THEODOLITES
Theodolites may be classified as ;
A.
i) Transit Theodolite.
ii) Non Transit Theodolite.
B.
i) Vernier Theodolites.
ii) Micrometer Theodolites.
8

A. Transit Theodolite: A theodolite is called a transit
theodolite when its telescope can be transited i.e
revolved through a complete revolution about its
horizontal axis in the vertical plane, whereas in a-
Non-Transit type, the telescope cannot be
transited. They are inferior in utility and have now
become obsolete.
9

B. Vernier Theodolite: For reading the graduated
circle if verniers are used ,the theodolite is called as a
Vernier Theodolite.
Whereas, if a micrometer is provided to read
the graduated circle the same is called as a
Micrometer Theodolite.
Vernier type theodolites are commonly used .
10

SIZE OF THEODOLITE
A theodolite is designated by diameter of the
graduated circle on the lower plate.
The common sizes are 8cm to 12 cm while 14 cm to
25 cm instrument are used for triangulation work.
Greater accuracy is achieved with larger
theodolites as they have bigger graduated circle with
larger divisions hence used where the survey works
require high degree of accuracy.
11

DESCRIPTION OF A
DESCRIPTION OF A
A Transit vernier theodolite essentially consist of the
following :
1. Levelling Head. 6. T- Frame.
2. Lower Circular Plate. 7. Plumb –bob.
3. Upper Plate. 8. Tripod Stand.
4. Telescope.
5. Vernier Scale.
12

TERMS USED IN MANIPULATING A TRANSIT VERNIER THEODOLITE.
TERMS USED IN MANIPULATING A TRANSIT VERNIER THEODOLITE.
1.Centering : Centering means setting the
theodolite exactly over an instrument- station
so that its vertical axis lies immediately above
the station- mark. It can be done by means of
plumb bob suspended from a small hook
attached to the vertical axis of the theodolite.
The centre shifting
arrangement if provided with the instrument
helps in easy and rapid performance of the
centring.
13

TERMS USED IN MANIPULATING A
TRANSIT VERNIER THEODOLITE.
2. Transiting :
Transiting is also known as plunging or
reversing. It is the process of turning the
telescope about its horizontal axis through 1800
in the vertical plane thus bringing it upside
down and making it point , exactly in opposite
direction.
14

3. Swinging the telescope
It means turning the telescope about its
vertical axis in the horizontal plane.
A swing is called right or left according as the
telescope is rotated clockwise or counter
clockwise.
15

4. Face Left
If the vertical circle of the instrument is on
the left side of the observer while taking a
reading ,the position is called the face left and
the observation taken on the horizontal or
vertical circle in this position, is known as the
face left observation
16

5. Face Right
If the vertical circle of the instrument is on
the right side of the observer while taking a
reading ,the position is called the face right and
the observation taken on the horizontal or
vertical circle in this position, is known as the
face right observation.
17

6. Changing Face
It is the operation of bringing the vertical
circle to the right of the observer ,if originally it
is to the left , and vice – versa.
It is done in two steps; Firstly revolve the
telescope through 1800 in a vertical plane and
then rotate it through 1800 in the horizontal
plane i.e first transit the telescope and then
swing it through 1800.
18

7. Line of Collimation
LINE OF
COLLIMATION
DIAPHRAGM
TELESCOPE
It is also known as the line of sight .It is an
imaginary line joining the intersection of the
cross- hairs of the diaphragm to the optical
centre of the object- glass and its continuation.
19

8. Axis of the telescope
AXIS OF THE TELESCOPE
TELESCOPE
It is also known an imaginary line joining the
optical centre of the object- glass to the centre
of eye piece.
OBJECT GLASS
.
20

9. Axis of the Level Tube
It is also called the bubble line.
It is a straight line tangential to the longitudinal
curve of the level tube at the centre of the tube.
It is horizontal when the bubble is in the centre.
21

10. Vertical Axis
It is the axis about which the telescope can be
rotated in the horizontal plane.
11. Horizontal Axis
It is the axis about which the telescope can be
rotated in the vertical plane.
It is also called the trunion axis.
22

ADJUSTMENT OFA THEODOLITE
The adjustments of a theodolite are of two kinds :-
1. Permanent Adjustments.
2. Temporary Adjustments.
1) Permanent adjustments: The permanent
adjustments are made to establish the relationship
between the fundamental lines of the theodolite and ,
once made , they last for a long time. They are essential
for the accuracy of observations.
23

1. Permanent adjustments: The permanent
adjustments in case of a transit theodolites are :-
i) Adjustment of Horizontal Plate Levels. The axis of
the plate levels must be perpendicular to the vertical
axis.
ii) Collimation Adjustment. The line of collimation
should coincide with the axis of the telescope and
the axis of the objective slide and should be at right
angles to the horizontal axis.
iii) Horizontal axis adjustment. The horizontal axis
must be perpendicular to the vertical axis.
24

1. Permanent adjustments (contd.):
iv) Adjustment of Telescope Level or the Altitude Level
Plate Levels. The axis of the telescope levels or the
altitude level must be parallel to the line of
collimation.
v) Vertical Circle Index Adjustment. The vertical
circle vernier must read zero when the line of
collimation is horizontal.
25

2. Temporary Adjustment
The temporary adjustments are made at each set
up of the instrument before we start taking
observations with the instrument. There are three
temporary adjustments of a theodolite:-
i) Centering.
ii) Levelling.
iii) Focussing.
26

MEASUREMENT OF HORIZONTALANGLES:
There are three methods of measuring horizontal
angles:-
i) Ordinary Method.
ii) Repetition Method.
iii) Reiteration Method.
27

MEASUREMENT OF HORIZONTAL ANGLES:
MEASUREMENT OF HORIZONTAL ANGLES:
i) Ordinary Method. To measure horizontal angle AOB:-
i) Set up the theodolite at station point O
and level it accurately.
ii) Set the vernier A to the zero or 3600 of
the horizontal circle. Tighten the
upper clamp.
iii) Loosen the lower clamp. Turn the
instrument and direct the telescope
towards A to bisect it accurately with
the use of tangent screw. After
bisecting accurately check the reading
which must still read zero. Read the
vernier B and record both the
readings.
o
A B
HORIZONTAL ANGLE AOB
28

iv) Loosen the upper clamp and turn the
telescope clockwise until line of sight
bisects point B on the right hand side.
Then tighten the upper clamp and
bisect it accurately by turning its
tangent screw.
v) Read both verniers. The reading of the
vernier a which was initially set at
zero gives the value of the angle AOB
directly and that of the other vernier
B by deducting 1800 .The mean of the
two vernier readings gives the value of
the required angle AOB.
o
A B
29

vi) Change the face of the instrument
and repeat the whole process. The
mean of the two vernier readings gives
the second value of the angle AOB
which should be approximately or
exactly equal to the previous value.
vii) The mean of the two values of the
angle AOB ,one with face left and the
other with face right ,gives the
required angle free from all
instrumental errors.
o
A B
30

This method is used for very accurate
work. In this method ,the same angle
is added several times mechanically
and the correct value of the angle is
obtained by dividing the accumulated
reading by the no. of repetitions.
The No. of repetitions made usually in
this method is six, three with the face
left and three with the face right .In
this way ,angles can be measured to a
finer degree of accuracy than that
obtainable with the least count of the
vernier.
o
A B
31

To measure horizontal angle by
repetitions:-
i) Set up the theodolite at starting point
O and level it accurately.
ii) Measure The horizontal angle AOB.
iii) Loosen the lower clamp and turn the
telescope clock – wise until the object
(A) is sighted again. Bisect B
accurately by using the upper tangent
screw. The verniers will now read the
twice the value of the angle now.
o
A B
32

ii) Repetition Method contd...
iv) Repeat the process until the angle is
repeated the required number of times
(usually 3). Read again both verniers .
The final reading after n repetitions
should be approximately n X (angle).
Divide the sum by the number of
repetitions and the result thus obtained
gives the correct value of the angle AOB.
v) Change the face of the instrument.
Repeat exactly in the same manner and
find another value of the angle AOB. The
average of two readings gives the
required precise value of the angle AOB.
o
A B
33

o
A
B
Reiteration Method
C
D
This method is another precise and
comparatively less tedious method
of measuring the horizontal angles.
It is generally preferred when
several angles are to be measured
at a particular station.
This method consists in measuring
several angles successively and
finally closing the horizon at the
starting point. The final reading of
the vernier A should be same as its
initial reading.
34

o
A
B
Reiteration Method
C
D
…If not ,the discrepancy is equally
distributed among all the
measured angles.
Procedure
Suppose it is required to measure
the angles AOB,BOC and COD.
Then to measure these angles by
repetition method :
i) Set up the instrument over
station point O and level it
accurately.
35

o
A
B
Reiteration Method
C
D
Procedure
ii) Direct the telescope towards
point A which is known as
referring object. Bisect it
accurately and check the reading
of vernier as 0 or 3600 . Loosen the
lower clamp and turn the telescope
clockwise to sight point B exactly.
Read the verniers again and The
mean reading will give the value of
angle AOB.
iii) Similarly bisect C & D
successively, read both verniers at-
36

iii) Reiteration Method (contd.).
o
A
B
Reiteration Method
C
D
Procedure. each bisection, find the
value of the angle BOC and COD.
iv) Finally close the horizon by sighting
towards the referring object (point A).
v) The vernier A should now read 3600.
If not note down the error .This error
occurs due to slip etc.
vi) If the error is small, it is equally
distributed among the several angles .If
large the readings should be discarded
and a new set of readings be taken.
37

MEASUREMENT OF VERTICAL ANGLES:
Vertical Angle : A vertical angle is an angle between the
inclined line of sight and the horizontal. It may be an
angle of elevation or depression according as the object is
above or below the horizontal plane.
A
B
O O
A
B
A
B
O
HORI. LINE
HORI. LINE
β
HORI. LINE
VERTICAL ANGLE
Fig.a
Fig. b Fig. c
AOB= α+ β
AOB= α - β
38
β
β
α
α
α

To Measure the Vertical Angle of an object A at a station O:
(i) Set up the theodolite at station point O and level it
accurately with reference to the altitude bubble.
(ii) Set the zero of vertical vernier exactly to the zero of the
vertical circle clamp and tangent screw.
(iii) Bring the bubble of the altitude level in the central position
by using clip screw. The line of sight is thus made horizontal
and vernier still reads zero.
(iv) Loosen the vertical circle clamp screw and direct the
telescope towards the object A and sight it exactly by using
the vertical circle tangent screw.
39

(v) Read both verniers on the vertical circle, The mean of
the two vernier readings gives the value of the required
angle.
(vi) Change the face of the instrument and repeat the
process. The mean of of the two vernier readings gives the
second value of the required angle.
(vii) The average of the two values of the angles thus
obtained, is the required value of the angle free from
instrumental errors.
40

For measuring Vertical Angle between two points A &B
i) Sight A as before , and take the mean of the two vernier
readings at the vertical circle. Let it be α
ii) Similarly, sight B and take the mean of the two vernier
readings at the vertical circle. Let it be
iii) The sum or difference of these dings will give the value of the
vertical angle between A and B according as one of the points is
above and the other below the horizontal plane. or both points
are on the same side of the horizontal plane Fig b & c
41
β

READING MAGNETIC BEARING OF A LINE
To find the bearing of a line AB as shown in fig .below
i) Set up the instrument over A and level it accurately
ii) Set the vernier to the zero of the horizontal circle.
N
A
B
Fig.
Magnetic Bearing of a Line
iii) Release the magnetic needle and loosen the
….. lower clamp.
iv) Rotate the instrument till magnetic needle
points to North. Now clamp the lower clamp with
the help of lower tangent screw .Bring the needle
exactly against the mark in order to bring it in
magnetic meridian. At this stage the line of sight
will also be in magnetic meridian.
42

iv) Now loose the upper clamp and point the
telescope towards B .With the help of upper
tangent screw ,bisect B accurately and read both
the verniers .The mean of the two readings will be
recorded as magnetic bearing of line.
N
A
B
Fig.
Magnetic Bearing of a Line
v) Change the face of the instrument
for accurate magnetic bearing of the
line and repeat .the mean of the two
values will give the correct bearing of
the line AB.
43

PROLONGING A STRAIGHT A LINE
There are two methods of prolonging a given line such as AB
(1) Fore sight method ,and (2) Back Sight Method
Fig.
(1)Fore Sight Method. As shown in the fig. below
A B C D Z
i) Set up the theodolite at A and level it accurately .Bisect the
point b correctly. Establish a point C in the line beyond B
approximately by looking over the top of the telescope and
accurately by sighting through the telescope.
ii) Shift the instrument to B ,take a fore sight on C and establish
a point D in line beyond C.
iii) Repeat the process until the last point Z is reached.
44

(2) Back Sight Method. As shown in the fig. below
A B C D Z
i) Set up the instrument at B and level it accurately .
ii) Take a back sight on A.
iii) Tighten the upper and lower clamps, transit the telescope
and establish a point C in the line beyond B.
iv) Shift the theodolite to C ,back sight on B transit the telescope
and establish a point D in line beyond C. Repeat the process
until the last point ( Z) is established.
C’
D’
45

(2) Back Sight Method.(contd.) As shown in the fig. below
A B C D Z
Now if the instrument is in adjustment, the points
A,B,C,D and Z will be in one line, which is straight but if
it is not in adjustment i.e. line of collimation is not
perpendicular to the horizontal axis ,then C’, D’ and Z’
will not be in a straight line.
C’
D’
46

Double reversing Method
A B C D Z
When the line is to be prolonged with high precision
or when the instrument is in imperfect adjustment, the
process of double sighting or double reversing, is used.
Suppose the line AB is to be prolonged to a point Z.
Procedure: As shown below:
C1
C2
D1
D2
Double Sighting / Reversing Method
47

Double reversing Method
i) Set up the theodolite at B and level it accurately.
ii) With the face of instrument left, back sight on A and
…. clamp both the upper and lower motions.
iii) Transit the telescope and set a point C1 ahead in line.
A B C D Z
C1
C2
D1
D2
48

Double reversing Method (contd.)
iv) Loosen the lower clamp ,revolve the telescope in the
horizontal plane and back sight on A .Bisect A exactly by
using the lower clamp and its tangent screw. Now the face of
instrument is right.
v) Transit the telescope and establish a point C2 in line
beside the point C1.
A B C D Z
C1
C2
D1
D2
49

vi) The exact position of the true point C must be mid-way
…..between C1 and C2 .
vii) Measure C1 C2 and establish a point C exactly mid-way,
….which lies on the true prolongation of AB.
A B C D Z
C1
C2
D1
D2
Fig. Double Sighting / Reversing Method
50

viii) Shift the instrument to C, double sight on B ,establish the
…..point D1 and D2 and locate the true point D as before .
ix) Continue the process until the last point Z is established.
A B C D Z
C1
C2
D1
D2
51

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