LEVELLING In Surveying
Levelling
is a
branch of surveying, the
object of which is to
1.
Find the elevation of a given
point with respect to the given or assumed datum.
2.
Establish a point at a given
elevation with respect to the given or assumed datum.
Levelling is the measurement of geodetic height using an
optical levelling instrument and a level staff or
rod having a numbered scale. Common levelling instruments include the spirit level,
the dumpy level,
the digital level, and the laser level.
v Method Of Levelling
:-
1. Rise and fall method
2. Height of collimation method
1. Rise and fall
method :-
In this method,
the difference of level between two consecutive points for each setting of the
instrument, is obtained by comparing their staff readings. The difference
between their staff readings indicates a rise if the back staff
reading is more than the fore sight and a fall if it is less
than the fore sight. The algebraic sum of rises and falls, gives the difference
in level between the starting and closing points
.
2. Height of collimation method :-
In this
method height of the instrument is calculated for the first setting of instrument
by adding the back sight to the reduced level of the given Bench Mark. The
reduced level of the first station is obtained by subtracting its fore sight
from the instrument height (H.I.).
Arithmetical
checks :-
∑ B.S.-
∑ F.S. =∑ Rise - ∑ Fall = Last R.L. – First R.L.
v Comparison of Line of Collimation
Method with Rise and Fall Method :-
Height of collimation method
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Rise and fall method
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1. It is more rapid and saves a considerable time and labour.
2. It is well adopted for reduction of
levels for construction work such as longitudinal or cross section levelling
operations.
3. There is no check on reduction of R.L.S.
of intermediate stations.
4. There are only two arithmetical
check i.e.,, the difference between the sum of the back
sights and the sum of the fore sights must be equal to the difference in R.L.
of the last station and first station.
5. Errors if any in intermediate sights are
not detected.
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1. It is laborious as the staff reading of
each station is compared, to get a rise or fall.
2. It is well adopted for determining the
difference in levels of two points where precision is required.
3. There is a complete check on the
reduction of R.Ls. of intermediate stations.
4. There are three arithmetical
checks i.e. the difference between the sum of the back
sights and the sum of the fore sights must be equal to the difference between
the sum of the rises and the sum of the falls as well as it must be equal to
the difference in R.Ls. of the last station and first station.
5. Errors in intermediate sights are noticed
as these are used for finding out the rises or falls.
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v Sprit
level:-
The spirit level is
on a tripod with sight lines to the two points whose height difference is to be
determined. A graduated leveling staff or rod is held vertical on each point;
the rod may be graduated in centimetres and fractions or tenths and hundredths
of a foot. The observer focuses in turn on each rod and reads the value.
Subtracting the "back" and "forward" value provides the
height difference.
v Refraction and curvature :-
The curvature of the earth means that a line of sight that is
horizontal at the instrument will be higher and higher above a spheroid at
greater distances. The effect may be significant for some work at distances
under 100 meters.
The line of sight is horizontal at the instrument, but is not
a straight line because of refraction in the air. The change of air density
with elevation causes the line of sight to bend toward the earth.
The combined correction for refraction and curvature is
approximately.
For precise work these effects need to be calculated and
corrections applied. For most work it is sufficient to keep the foresight and
back sight distances approximately equal so that the refraction and curvature
effects cancel out. Refraction is generally the greatest source of error in
leveling. For short level lines the effects of temperature and pressure are
generally insignificant, but the effect of the temperature gradient dT / dh can lead to errors.
vDumpy level :-
The dumpy level was developed by English
civil engineer William Gravatt, while surveying the route
of a proposed railway line form London to Dover. More compact and hence both
more robust and easier to transport, it is commonly believed that dumpy
levelling is less accurate than other types of levelling, but such is not the
case. Dumpy levelling requires shorter and therefore more numerous sights, but
this fault is compensated by the practice of making foresights and back sights
equal.
Precise level designs were often used for large leveling
projects where utmost accuracy was required. They differ from other levels in
having a very precise spirit level tube and a micrometer adjustment to raise or
lower the line of sight so that the crosshair can be made to coincide with a
line on the rod scale and no interpolation is required.
v Wye
level :-
The wye level is the oldest
and bulkiest of the older style optical instruments. A low-powered telescope is
placed in a pair of clamp mounts, and the instrument then leveled using aspirit level, which is mounted
parallel to the main telescope.
Automatic level:- Automatic levels make use of
a compensator that ensures that the line of sight remains horizontal once the
operator has roughly leveled the instrument (to within maybe 0.05 degree). The
surveyor sets the instrument up quickly and doesn't have to relevel it
carefully each time he sights on a rod on another point. It also reduces the
effect of minor settling of the tripod to the actual amount of motion instead
of leveraging the tilt over the sight distance. Three level screws are used to
level the instrument.
1.
Gun sight
2.
Circular level (pond bubble)
3.
Levelling Screw
4.
Base Plate
5.
Objective Lens
6.
Focusing Knob
7. Horizontal fine motion screw
8. Horizontal circle window
9. Horizontal circle setting ring
10. Reticle
adjusting screw cover
11.Eyepiece
v Setting
up an automatic level :-
Set up
the tripod at just above chest height. Make sure it is stable, and mount the
level on the top. Adjust the leveling screws until the pond bubble is
centralised. As long as the pond bubble is central, the automatic compensators
are able to finely level the instrument. To ensure.
This
is the case, whilst looking through the scope, gently tap the level. The view
will waver for a few moments before steadying. If this does not happen, the
instrument is not level enough for the compensators to cope, and needs
adjustment.
v
Sighting
:-
Sight towards the staff using the
gun sight. Look through the eyepiece and focus the reticle by gradually turning
the reticle focusing ring anti-clockwise. Turn the focusing knob to focus on
the staff. Turn the fine motion screw to centre the staff in the field of view.
Turn the focusing knob to eliminate parallax between the staff and reticle.
v
Reading the staff :-
The staff starts at zero, on the ground. Every
10 cm is a number, showing ( in meters to one decimal) the height of the
bottom of what appears to be a stylised E (even numbers) or 3 (odd numbers),
5 cm high. The stems of the E or 3 and the gaps between them are each 10mm
high. These 10mm increments continue up to the next 10 cm mark.
To read the staff, take the number shown below
the reticle. Count the number of whole 10mm increments between the whole number
and the reticle. Then estimate the number of mm between the last whole 10mm
block and the center of the reticle. The diagram above shows 4 readings:- 1.950,
2.000, 2.035 and 2.087.
The person holding the staff should end heavour
to hold it as straight as possible. The leveller can easily see if it is tilted
to the left or right, and should correct the staff-holder. However, it cannot
easily be seen that the staff is tilted towards or away from the leveller. In
order to combat this possible source of error, the staff should be slowly
rocked towards and away from the leveller. When viewing the staff, the reading
will thus vary between a high and low point. The correct reading is the lowest
value.
Digital levels electronically read a bar-coded scale on the staff. These instruments usually include data recording capability. The automation removes the requirement for the operator to read a scale and write down the value, and so reduces blunders. It may also compute and apply refraction and curvature corrections.
v Laser level :-
Laser levels project
a beam which is visible and/or detectable by a sensor on the leveling rod. This
style is widely used in construction work but not for more precise control
work. An advantage is that one person can perform the levelling independently,
whereas other types require one person at the instrument and one holding the
rod.
The sensor can be mounted on
earth-moving machinery to allow automated grading.
v Level staff :-
A level staff, also called levelling rod, is a graduated wooden or aluminium rod, used with a levelling
instrument to determine the difference in height between points or heights of points
above a datum surface. It cannot be used without a leveling instrument.
v Reading a rod :-
In the
photograph on the right, both a metric (left) and imperial (right) levelling
rod are seen. This is a two-sided aluminum rod, coated white with markings in
contrasting colours. The imperial side has a bright yellow background
The imperial graduations are
in feet (large red numbers), tenths of a foot (small black numbers) and
hundredths of a foot (unnumbered marks or spaces between the marks). The tenths
of a foot point is indicated by the top of the long mark with the upward sloped
end. The point halfway between tenths of a foot marks is indicated by the
bottom of a medium length black mark with a downward sloped end. Each mark or
space is approximately 3mm, yielding roughly the same accuracy as the metric
rod.
v Levelling
procedure :-
A typical procedure is to set up the instrument within 100
meters (110 yards) of a point of known or assumed elevation. A rod or staff is
held vertical on that point and the instrument is used manually or
automatically to read the rod scale. This gives the height of the instrument
above the starting (back sight) point and allows the height of the instrument
(H.I.) above the datum to be computed.
The rod is then held on an unknown point and a reading is
taken in the same manner, allowing the elevation of the new (foresight) point
to be computed. The procedure is repeated until the destination point is
reached. It is usual practice to perform either a complete loop back to the
starting point or else close the traverse on a second point whose elevation is
already known. The closure check guards against blunders in the operation, and
allows residual error to be distributed in the most likely manner among the
stations.
Some instruments provide three crosshairs which allow stadia measurement of the foresight
and back sight distances. These also allow use of the average of the three
readings (3-wire leveling) as a check against blunders and for averaging out
the error of interpolation between marks on the rod scale.
The two main types of levelling are single-levelling as
already described, and double-levelling (Double-rodding). In double-levelling,
a surveyor takes two foresights and two back sights and makes sure the
difference between the foresights and the difference between the backsights are
equal, thereby reducing the amount of error. Double-levelling costs twice
as much as single-levelling.
v Safety and precautions in leveling :-
While leveling, the following precautions
should be taken:
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