Correction Applied in Distance Measurement
Temperature Correction (Add or Subtract)
                    Ct = αL∆T
         α = 11.6x106 ; ∆T = Tf − To
      Correction Due to Pull (Add or Subtract)
                 ∆PL (PActual − Po )L
            CP =      =
                  AE           AE
   Correction Due to Sag (To be Subtracted Only)
                        ω2 L3
                Cs =
                     24(PActual )2
                                        W
         ω = Weight per tape length =
                                        L
  Correction Due To Slope (To Be Subtracted only)
                            h2
                   CSlope =
                            2S
                  H = S − CSlope
 Normal Tension – the pull used to compensate the
              correction due to sag
                   Csag = Cpull
                       0.204W√AE
                PN =
                        √PN − Po
               Sea Level Correction
                   ′
                              h
                 L = L (1 − )
                              R
              MD
   CTotal   =    (Ct )
               L
                                     TD = MD ± CTotal
               MD
  No. of Sag =
                L
                                        CTotal = Cs1 + Cs2
Probability
         Probable Error Of Single Observation
                                 ∑ V2
                  PEs = ±0.6745√
                                 n−1
                Probable Error Of The Mean
                              ∑ V2     PEs
             PEm = ±0.675 √          =
                             (
                            n n−1  )   √n
                    Standard Deviation
                                 ∑ V2
                          SD = √
                                 n−1
                         Standard Error
                                 SD
                            SE =
                                 √n
Where:
  n = no. of obsevation
  ∑ V 2 = Sum of the square of the residuals
Weighted Observation
The weights are directly proportional to the number of
observations.
                         w= n
The weights are inversely proportional to the square of
the corresponding probable errors.
                             1
                         w= 2
                             e
The errors are directly proportional to the square roots
of the distances.
                         e = √L
The errors are inversely proportional to the number of
set-ups. Degree / Angle.
                             1
                          e=
                             n
The weights are inversely proportional to the distances.
                              1
                         w=
                              L
Weighted Observation
               wo = Elevation x Weights
                             ∑ wo
                     MPv =
                              WT
                    1
Cal. Tech for w =             [MODE 3 | 4 | Shift | MODE | ↓ | 4 |AC | x = Shift 1 | 4 | 2 | =]
                    e2
Leveling
                         Elev1 + BS1 = Elev2 + FS2
Two – Peg Test
  ∆ + elev1 = elev2 + e                           ∆ + elev1 = elev2 + e
Cal. Tech.
MODE | 5 |1 | ∆ + e = elev2 − elev1 | ∆ − e = elev2 − elev1 | = | ∆= x | e = y |
  ∆ + elev1 − e = elev2 − e                  ∆ + elev1 − e1 = elev2 − e2
               Level line of Sight            LS = elev − e
    Error Due to Settlement of the Rod                       eT = e(TP)
                                                         L
                   No. of Set up            NST =
                                                      BS+FS
           No. of Turning Point                 NTP = NST − 1
Bubble sensitivity
            b−a                 S               π
  tan n θ =             θrad =           rad =
              L                R               180
Effect of Earth’s Curvature & Reflection
                          2              hcr
  hcr = 0.067k                      k=√                         k = k1 + k 2
                                        0.067
Where:   hcr = meters ;   k = kilometers
Compass Surveying
                      Magnet Declination
 True Bearing (TB) – Bearing with reference to the true direction
                     Magnetic Bearing (MB)
Traverse Surveying
Latitude – Projection of North and South Line
Departure – Projection of East and West Line.
   Lat = Dcos θ                    Dep = D sin θ            D = √Lat 2 + Dep2
Error of Closure – for a closed traverse, the sum of the latitudes and departures
should be equal to zero.
Linear Error of Closure                       Relative Error
                                                                     LEC
       LEC = √∑ Lat 2 + ∑ Dep2                                 RE =
                                                                     ∑P
Area Computation (DMD, DPD, Coordinate method)
DMD                      DPD
       DMD1 = Dep1                                  DPD1 = DMD1 (Lat1 )
 DMD2 = DMD1 + Dep1 + Dep2                          DPDn = DMDn (Lat n )
 DMDn = DMDn + Depn + Depn                               2A = ∑ DPD
    (x1 y2 − y1 x2 ) + (x2 y3 − y2 x3 ) + ⋯ + (xn y1 − yn x1 )
 A=
                                2
Balancing Survey
Compass Rule – Total Correction
               CLat/Dep            L
                          =
            CTotal Lat/Dep ∑ Lat or ∑ Dep
Transit Rule – Arithmetical Sum
               CLat/Dep       Lat or Dep
                          =
            CTotal Lat/Dep ∑ Lat or ∑ Dep
Tachymetry Survey
                                                             D = C + Ks
                                                                  f
                                                       D = c + f + (s)
                                                          (     )
                                                                  i
                                                           D = (c + f) + x
                                                       f         x              f
                                                         =s          ;   x = i (s)
                                                       i
                                                                     f x′
                                                                      =
                                                                     i s′
                                               f            x′
                                                            ′               f
                                                 =        x   = i (Scosθ)
                                               i   Scos θ
                                                           D = (c + f) + x ′
                                                              f
                                                   D = c + f + (Scosθ)
                                                      (     )
                                                              i
                                                       D = C + K(Scosθ)
Where:
    C = (c + f) = Stadia constant                            H = Dcosθ
            f
        K = = Stadia factor                                      V = Dsinθ
            i
For Continuous Rod
              S = Upper Reading − Lower Reading
                                    f          ∑K
                            K=i         ;K =
                                                   n
The Subtense Bar Method
                                                𝜃    1
                                           tan ( ) =
                                                2    𝐻
                                                       1
                                           𝐻=
                                                       𝜃
                                                  tan ( )
                                                       2
Topographic Surveys
        𝐷𝑖𝑠𝑡. 𝑜𝑛 𝑡ℎ𝑒 𝑚𝑎𝑝 𝐷𝑚𝑎𝑝                        𝐴𝑚𝑎𝑝
𝑆𝑐𝑎𝑙𝑒 =
         𝐷𝑖𝑠𝑡. 𝑜𝑛 𝑎𝑐𝑡𝑢𝑎𝑙
                         =
                           𝐷𝑎𝑐𝑡
                                        (𝑆𝑐𝑎𝑙𝑒 =  )2
                                                     𝐴𝑎𝑐𝑡
                  1                             −1 (
                                                      𝑥
           𝑆𝑐𝑎𝑙𝑒 =                      𝜃 = tan          )
                  𝑥                                 𝐷𝑎𝑐𝑡
     𝑥 = 𝐶𝑜𝑛𝑡𝑜𝑢𝑟 𝑖𝑛𝑡𝑒𝑟𝑣𝑎𝑙              400 𝑔𝑟𝑎𝑑            360°
                                  𝜃=              ; 𝜃 = 6400 𝑚𝑖𝑙𝑠
                                         360°
Photographic Surveys
                                            𝑋1   𝑓
                                               =
                                            𝑥2 𝐻 − ℎ
                                                   𝑓
                                          𝑆𝑐𝑎𝑙𝑒 =
                                                  𝐻−ℎ
                                        𝑥2 = 𝐴𝑐𝑡𝑢𝑎𝑙 𝑠𝑖𝑧𝑒
                                           ℎ𝑚𝑖𝑛 + ℎ𝑚𝑎𝑥
                                        ℎ=
                                                2
Mine Surveying
             𝑥            𝑧           𝑧
     𝑠𝑖𝑛𝛼 =         𝑥=            𝑦=
             𝑦         tan 𝜃𝑑𝑖𝑝      𝑔%
           𝑔%
 sin 𝛼 =
         tan 𝜃𝑑𝑖𝑝