
INTERNATIONAL JOURNAL OF RESEARCH AND SCIENTIFIC INNOVATION (IJRSI)
ISSN No. 2321-2705 | DOI: 10.51244/IJRSI |Volume XII Issue IX September 2025
www.rsisinternational.org
into horizontal circle readings when the telescope is tilted, especially for steep sightings. As with horizontal
collimation error, this error is eliminated by two face measurements, or the tilting axis error a is measured in
a calibration procedure and a correction applied for this to all horizontal circle readings as before if a is too
big, the instrument should be returned to the manufacturer.
5. Vertical collimation error: A vertical collimation error exists on a total station if the 0° to 180° line in the
vertical circle does not coincide with its vertical axis. This zero-point error is present in all vertical circle
readings and like the horizontal collimation error, it is eliminated by taking FL and FR readings or by
determining.
6. Pointing errors: Pointing errors are due to both human ability to point the instrument and environmental
conditions limiting clear vision of the observed target. The best way to minimize pointing errors is to repeat
the observation several times and use the average as the results.
7. Uneven heating of the instrument: Direct sunlight can heat one side of the instrument enough to cause
small errors. For the highest accuracy, utilize an umbrella or pick a shaded spot for the instrument.
8. Vibrations: Avoid instrument locations that vibrate. Vibrations can cause the compensator to be unstable.
9. Atmospheric corrections: Meteorological data corrections to observed EDM slope distances may be
significant over longer distances. Usually for most topographic surveying over short distances, nominal
(estimated) temperature and pressure data is acceptable for input into the data collector. Instruments used to
measure atmospheric temperature and pressure must be periodically calibrated. This would include
psychrometers and barometers.
10. Optical plummet errors: The optical plummet or tri-brachs must be periodically checked for misalignment.
This would include total stations with laser plummets.
11. Adjustment of prism poles: When using prism poles, precautions should be taken to ensure accurate
measurements. A common problem encountered when using prism poles is the adjustment of the leveling
bubble. Bubbles can be examined by establishing a check station under a doorway in the office. First, mark
a point on the top of the doorway. Using a plumb bob, establish a point under the point on the doorway. If
possible, use a center punch to make a dent or hole in both the upper and lower marks. The prism pole can
now be placed into the check station and easily adjusted.
Research in Total Station Levelling
There are several studies that had been carried out to investigate the use of total station for levelling. Some of
them are described below.
The study done by Julius Geofrey, an undergraduate of Ardhi University in Tanzania, shows a comparison
between digital levelling and total station levelling. The levelling route is 7km long and consists four segments;
three 2km segments and a 1km segment. Benchmarks were established on the separation of each segment. In
addition, minor benchmarks were established in between those segments. The forward and back levelling were
run for each segment using both instruments and the loop misclosure was determined by subtracting the
computed reduced level from the known reduced level of the benchmark. The root mean squares of the observed
misclosure for each segment were in acceptable range both for the total station and digital level. However, they
found that digital level is more precise as usual. The study recommends to carry out further research on different
areas of interests with longer levelling routes in order to check the accumulation of errors in longer distances.
Another study has been done by Jongchool & Taeho, 2001, to investigate the application to levelling using total
station. This study mainly focuses on the effect of EDM error. The distance measured by EDM is expressed by
the formula;
S = U + mλ/2, where,
• U: phase shift of the reflected light wave
• λ: wavelength
• m: number of transmitted wavelengths
The device for measuring distance by light wave always should have the correction for the measured value. Here
they have studied mainly the weather correction and zero correction. Weather correction consists variables such
as refraction of atmosphere, height of sea level, refraction by projection method and difference of scale