Difficulties
faced in levelling.
[1]. When staff is too near the instrument: If the levelling staff is held very near the levelling instrument, the
graduation of the staff are not visible. In such a case, a piece of white paper
moved up and down along the staff until the edge of the paper is bisected by
the line of collimation. Then the reading is noted from the staff with naked
eye. Sometime the reading is taken by looking through the object glass.
[2]. Levelling across a large pond or lake: Suppose the levelling is to be done across a very wide pond or lake.
We know that the water surface of a still
lake or pond is considered to be level. Therefore, all points on a water
surface have the same RL. Two pegs A and B are fixed on opposite banks of the
lake or pond. The top of the pegs are just flush with water surface. The level
is set up at O₁ and the RL of A is determined by taking an FS on A. The RL of B
is assumed to the equal to of A. Now the level is shifted and set up at O₂.
Then by taking a BS on peg B, levelling is continued (Fig.-L.26).
[3]. Levelling across a river: In case of following water, the surface cannot be considered level.
The water levels on the opposite edges will be different. in such a case, the
method of reciprocal levelling is adopted. Two pegs A and B are driven on the
opposite bank of the river (not flush with the water surface). The RL of A is
determined in the usual way. Then the true difference of level between A and B
is found by reciprocal levelling. Thus the RL of B is calculated, and levelling
is continued.
[4]. Levelling across a solid wall: When levelling is to be done across a solid wall, two pegs A and B are
driven on either side of the wall, just touching it. The level is set up at O₁
and a staff reading is taken on A. Let the reading be AC. Then the height of
the wall is measured by staff. Let the height be AE. HI is found out by taking a
BS on any BM or CP.
Then RL of A = HI – AC
RL of E = RL of
A + AE = RL of F (same level)
The level is shifted and set
up at O₂. The staff reading BD is noted and the height of BF is measured.
Then RL of B = RL of F
– BF
HI at O₂ = RL
of B + BD
The leveling is then continued by working out the HI of setting (Fig.-L.27).
[5]. When the BM is above line of collimation: This happens when the BM is at the bottom of a bridge girder or on the
bottom surface of a culvert. It also happens when the RLS of points above the
line of collimation have to be found out.
Suppose the BM exists on the bottom surface
of a culvert, and it is required to find out the RL of A. The level is set up
at O and is held inverted on the BM. The staff reading is taken and noted with
a negative sign. The remark “staff held inverted” should be entered in the
appropriate column. Let the BS and FS readings be -1.45 and 2.30 respectively (Fig.-L.28).
Now, height of instrument = 100.00 – 1.45
= 98.55
RL of A = 98.55 – 2.30 = 96.25
[6]. Levelling along a steep slope: While levelling along a steep slope in a hilly area, it is very
difficult to have equal BS and FS distance. In such case, the level should be
set up along a zig-zag path so the BS and FS distance may be kept equal. Let AB
the direction of levelling. I₁, I₂, …… are the position of the level and S₁,
S₂, S₃, … the position of staff (Fig.-L.29).
[7]. Levelling across a rising ground or
depression: While a levelling across high ground, the level
should not be place on top of the high ground but on the side so that the line
of collimation just passes through the apex.
While a levelling across depression, the level
should be place on the side and not at the bottom of the depression (Fig. – L.30.a and L.30.b).
The precision of levelling ascertained
according to the error of closure. The permissible limit of closing error
depends upon the nature of the work for which the levelling is to be done. The
permissible closing error is expressed as
E = C√D
Where, E = closing error in metres
C = the constant, and
D = distance in
kilometres.
The following are the permissible error of different type of
levelling:
[1]. Rough levelling E =
±0.100√D
[2]. Ordinary levelling E =
±0.025√D
[3]. Accurate levelling E =
±0.012√D
[4]. Precies levelling E =
±0.006√D
Determination
of Stadia Constant
From the theory of the telescope it is known
that
D =
(f/i) x S + (f + d)
Where, D = distance between vertical axis of the
telescope and staff.
f = focal length of object glass.
i = length of image.
S = difference of reading between
the lower and upper stadia, and
d = distance between optical
centre and vertical axis of telescope.
The quantity of (f/i) is known as the
multiplying constant and its value is usually 100. The quantity (f + d) is
called the additive constant and its value is normally zero. But sometimes its
value lies between 20 and 30 cm.
The values of constants are obtained by
computation from field measurements.
Procedure:-
[1]. A
line OA, about 250 m long, is measured on level ground.
[2].
Pegs are fixed along this line at a known interval, say 25 m (Fig.-L.31).
[3]. The
instrument is set up at O and stadia hair readings are taken at each
of the pegs.
[4].
Thus the value of D and S are known for each of the pegs.
[5].
Putting these value of D and S in equation,
D = (f/i) x S + (f + d)
We get a numbers of equations.
[6].
The equations are solved in pairs to get several values of (f/i) and
(f+d). The means of this values is taken
as a stadia constant of the
corresponding instrument.
Example: The following field
observations are made with a level.
Distance
in metre Lower stadia Upper stadia
250.00 1.445 3.945
225.00 0.930 3.180
Let us
find the multiplying and additive constant.
Solution: We know that
D = (f/i) x S + (f + d)
Let (f/i) = x and (f + d) = y
D = xS + y ………………………..(1)
Substituting
the observed values in (1), we get
250 = (3.945 – 1.445)x + y
= 2.50x + y …………(2)
225 = (3.180 – 0.930)x + y
= 2.25x + y …………(3)
Subtracting Equation (3) from Equation (2)
25 = 0.25x
or x = 25/0.25 = 100
From Equation (2),
y = 250 - 2.50 x 100 = 0
Therefore
, Multiplying constant (f/i) = 100
Additive constant
(f + d) = 0
(Next post
on “COMPUTATION OF AREA AND VOLUME”)
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