Although taping and theodolites are used regularly on site – total stations are
also used extensively in surveying, civil engineering and construction because
they can measure both distances and angles.
A typical total station is shown in the figure below
The appearance of the total station is similar to that of an electronic theodolite,
but the difference is that it is combined with a distance measurement component
which is fitted into the telescope.
Because the instrument combines both angle and distance measurement in the
same unit, it is known as an integrated total station which can measure horizontal
and vertical angles as well as slope distances.
Using the vertical angle, the total station can calculate the horizontal and vertical
distance components of the measured slope distance.
As well as basic functions, total stations are able to perform a number of different
survey tasks and associated calculations and can store large amounts of data.
As with the electronic theodolite, all the functions of a total station are controlled
by its microprocessor, which is accessed thought a keyboard and display.
To use the total station, it is set over one end of the line to be measured and
some reflector is positioned at the other end such that the line of sight between
the instrument and the reflector is unobstructed (as seen in the figure below).
-The reflector is a prism attached to a detail pole
-The telescope is aligned and pointed at the prism
-The measuring sequence is initiated and a signal is sent to the reflector and a
part of this signal is returned to the total station
-This signal is then analysed to calculate the slope distance together with the
horizontal and vertical angles.
-Total stations can also be used without reflectors and the telescope is pointed at
the point that needs to be measured
-Some instruments have motorised drivers and can be use automatic target
recognition to search and lock into a prism – this is a fully automated process and
does not require an operator.
-Some total stations can be controlled from the detail pole, enabling surveys to
be conducted by one person
A total station is levelled and centred in the same way as a theodolite.
Most total stations have a distance measuring range of up to a few kilometres,
when using a prism, and a range of at least 100m in reflector less mode and an
accuracy of 2-3mm at short ranges, which will decrease to about 4-5mm at 1km.
Although angles and distances can be measured and used separately, the most
common applications for total stations occur when these are combined to define
position in control surveys.
As well as the total station, site surveying is increasingly being carried out using
GPS equipment. Some predictions have been made that this trend will continue,
and in the long run GPS methods may replace other methods.
Although the use of GPS is increasing, total stations are one of the predominant
instruments used on site for surveying and will be for some time.
Developments in both technologies will find a point where devices can be made
that complement both methods.
also used extensively in surveying, civil engineering and construction because
they can measure both distances and angles.
A typical total station is shown in the figure below
but the difference is that it is combined with a distance measurement component
which is fitted into the telescope.
Because the instrument combines both angle and distance measurement in the
same unit, it is known as an integrated total station which can measure horizontal
and vertical angles as well as slope distances.
Using the vertical angle, the total station can calculate the horizontal and vertical
distance components of the measured slope distance.
As well as basic functions, total stations are able to perform a number of different
survey tasks and associated calculations and can store large amounts of data.
As with the electronic theodolite, all the functions of a total station are controlled
by its microprocessor, which is accessed thought a keyboard and display.
To use the total station, it is set over one end of the line to be measured and
some reflector is positioned at the other end such that the line of sight between
the instrument and the reflector is unobstructed (as seen in the figure below).
-The reflector is a prism attached to a detail pole
-The telescope is aligned and pointed at the prism
-The measuring sequence is initiated and a signal is sent to the reflector and a
part of this signal is returned to the total station
-This signal is then analysed to calculate the slope distance together with the
horizontal and vertical angles.
-Total stations can also be used without reflectors and the telescope is pointed at
the point that needs to be measured
-Some instruments have motorised drivers and can be use automatic target
recognition to search and lock into a prism – this is a fully automated process and
does not require an operator.
-Some total stations can be controlled from the detail pole, enabling surveys to
be conducted by one person
A total station is levelled and centred in the same way as a theodolite.
Most total stations have a distance measuring range of up to a few kilometres,
when using a prism, and a range of at least 100m in reflector less mode and an
accuracy of 2-3mm at short ranges, which will decrease to about 4-5mm at 1km.
Although angles and distances can be measured and used separately, the most
common applications for total stations occur when these are combined to define
position in control surveys.
As well as the total station, site surveying is increasingly being carried out using
GPS equipment. Some predictions have been made that this trend will continue,
and in the long run GPS methods may replace other methods.
Although the use of GPS is increasing, total stations are one of the predominant
instruments used on site for surveying and will be for some time.
Developments in both technologies will find a point where devices can be made
that complement both methods.
