Surveying
by using Digital Theodolite
South
ET-05 Electronic
A theodolite is a telescope mounted
to very sensitive horizontal and vertical protractors. It is capable of
measuring angles and, when used in conjunction with graduated reference
objects, distances with a high degree of accuracy.
1 Setup
1.1 Tripod setup
In this section we learn how to set
up the tripod and roughly center and level it over a small positioning mark,
such as a divot in a penny glued to the _oor, a nail head, or any other small
_xed object.
a. Place the tripod over the
positioning mark, setting the legs at a convenient height, and roughly center
and level the tripod head by eye.
b. Suspend the plumb bob included
in the theodolite box from the hanger beneath the tripod head.
c. Readjust the tripod to center
the plumb bob over the positioning mark by moving all three tripod feet by the
same amount in the same direction.
d. Firmly _x the tripod feet in
position. If necessary, adjust the heights of the tripod legs to re-center the tripod
within 1 cm of the reference mark.
e. Tighten the leg clamps on the
tripod.
Figure 1: Theodolite-in-a-box.
1.2 Theodolite
setup
In this section we learn how to
unpack, set up, center, and level the theodolite.
1.2.1 Seating and centering
the theodolite
a) Examine how the tripod is seated
in its box. See Fig. 1.
b) Lift the theodolite out of its
box by the handle never by the telescope.
c) Place the theodolite on the
tripod head and screw in the centering screw while holding onto the handle.
Leave the centering screw just loose enough that the theodolite can still slide
around the tripod head.
d) Looking through the optical
plummet, focus the centering index mark. Slide the theodolite on the tripod
head until the reference mark is centered in the optical plummet.
e) Fully tighten the centering
screw. Look through the optical plummet again and adjust the theodolite foot
screws for _ne alignment with the reference mark.
1.2.2 Leveling the
theodolite
A. Referring to Fig. 2, roughly level
the instrument using the circular level:
1. Turn the leveling screws A and B
in opposite directions to center the bubble along the AB axis.
2. Turn leveling screw C to bring
the bubble to the center of the circular level.
B. Referring to Fig. 3, precisely
level the instrument using the plate level.
1. Free the horizontal motion clamp
and rotate the instrument horizontally until the plate level is parallel with
line AB.
2. Bring the bubble to the center
of the plate level by turning screws A and B in opposite directions.
3. Rotate the instrument by 90◦
around its vertical axis and turn screw C to center the bubble once more.
4. Repeat procedures i. and ii. for
each 90◦ rotation of the instrument and check that the bubble is correctly
centered for all four points. If after 180◦ of rotation, the bubble is of
center, remove half the error in the bubble centering. Check that when you have
swung another 180◦ back to the initial point, the bubble offset is the same as
the offset you allowed to remain in the 180◦ rotated position.
Once the theodolite is leveled,
double check the optical plummet to make sure that it is still centered. If
not, repeat the procedure in section 1.2.1 (d) through all of section 1.2.2.
Figure
2: Diagram for rough leveling with the circular level.
Figure 3: Diagram for _ne
leveling with the plate level.
2
Measurements
In
this section we learn how to take accurate readings of horizontal and vertical
angles using a theodolite.
a.
Determine how many reference points you will need to measure, and make sure
that their horizontal and vertical positions are clearly marked. In order of
measurement, these reference points will be referred to as X, Y and Z in these
instructions.
b.
Turn on the theodolite by pressing the green power key.
2.1
Horizontal measurement
To avoid
confusion, all horizontal angle measurements should be completed before taking
vertical angle measurements.
(a) Take face-left angle measurements.
1. Rotate
the telescope about the turning axis until the instrument is in face-left
position.
2. Press
the OSET key and rotate the telescope horizontally to give a reading between 0◦
and 1◦.
3. Press
HOLD to lock this value.
4. After
making sure no one is in the telescope line of sight, press the laser on button
on top of the telescope. Free the horizontal and vertical clamps and swing the
laser spot to reference point X.3
5.
Roughly align the laser spot and focus it using the focusing ring on the
telescope. Tighten the horizontal and vertical clamps. Turn o_ the laser.
6. Place
a blank sheet of paper in front of the telescope, and, looking through the
telescope, focus the crosshairs using the eyepiece.
7. Remove
the paper and focus the telescope on the reference object using the focusing
ring.
8. Check
for parallax by moving your head up and down and left to right. If the
crosshairs move, refocus the crosshairs, and refocus the reference object as
described above.
9.
Looking through the telescope, home in on the reference object using the
slow-motion screws. For horizontal angle measurements, the vertical crosshair
must be perfectly aligned with the reference point, but the horizontal
crosshair need not be, as long as approximately the same part of the vertical
crosshair is used for each horizontal measurement.
10. Check
the telescope pointing, book the horizontal angle reading, and check the
booking.
11.
Release the HOLD key (only applies to the very first reading).
12.
Repeat steps 4 to 10 for reference points Y, Z, etc.
(b) Take face-right angle measurements to complete a
round of angles.
1. Rotate
the telescope about the turning axis until the instrument is in face-right
position.
2. Repeat
steps (a) 4 - 10 in the face-right position. Now you've booked a series of
angles between 0◦ and 360◦ and a series between 360◦ and 720◦. This completes a
round of angles.
(c) Take at least one more round of angles using
an initial horizontal reading between 90◦ and 91◦ for the second round, 180◦
and 181◦ for the third round, etc. If you take only two rounds of angles, make
sure that the readings agree within twice the precision of the theodolite.
(d) Once the desired precision is achieved, take the mean value of the measured
angles.
2.2 Vertical
measurement
The vertical angle scale is
referenced absolutely to the ground, so it is impossible to use different
initial readings for the multiple rounds of angles.
(a) Take face-left angle
measurements.
1. Rotate the telescope
about the turning axis until the instrument is in face-left position.
2. After making sure no one is in
the telescope line of sight, press the laser on button on top of the telescope.
Free the horizontal and vertical clamps and swing the laser spot to reference
point X.
3. Roughly align the laser spot and
focus it using the focusing ring on the telescope. Tighten the horizontal and
vertical clamps. Turn o_ the laser.
4. Place a blank sheet of paper in
front of the telescope, and, looking through the telescope, focus the crosshairs
using the eyepiece.
5. Remove the paper and focus the
telescope on the reference object using the focusing ring.
6. Check for parallax by moving
your head up and down and left to right. If the crosshairs move, refocus the
crosshairs, and refocus the reference object as described above.
7. Looking through the telescope,
home in on the reference object using the slow-motion screws. For vertical
angle measurements, the horizontal crosshair must be perfectly aligned with the
reference point, but the vertical crosshair need not be, as long as
approximately the same part of the horizontal crosshair is used for each
vertical measurement.
8. Check the telescope pointing,
book the vertical angle reading, and check the booking.
9. Repeat steps ii. to viii. for reference
points Y, Z, etc.
(b) Take face-right
angle measurements to complete a round of angles.
1. Rotate the telescope about the
turning axis until the instrument is in face-right position.
2. Repeat steps (a) ii. - ix. in
the face-right position. This completes a round of angles.
(c) Take at least one
more round of angles. If you take only two rounds of angles, make sure that the
readings agree within twice the precision of the theodolite.
(d) Once desired
precision is achieved, take the mean value of the angles measured.
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