FlexLine Total Stations

For Basic to Advanced Users with the Need for Flexibility and Performance.

To ensure that you stay one-step-ahead, Leica Geosystems has developed a new generation of Total Stations using latest technology, the Leica FlexLine. For the first time, hardware and software options can be simply selected so that the FlexLine Total Station exactly meets your requirements.

Construction Products Comparison Booklet

Leica FlexLine Total Stations provide complete flexibility in configuring each Total Station. The following table shows the standard () and optional (o) features for each Total Station within the FlexLine family.
 

	Leica TS02	Leica TS06	Leica TS09
High accuracy instrument
1” angular accuracy
1 mm + 1.5 ppm distance measurement accuracy
Distance measurement
Prism, 3500 m range
Non-Prism: 30 m FlexPoint incl. Laserpointer	o
Non-Prism: >400 m PinPoint – Power	o	o	o
Non-Prism: >1000 m PinPoint – Ultra	o	o	o
Data storage/Communication
Internal memory
Enhanced Internal memory
Removable USB memory stick, mini-USB port	o	o
Integrated Bluetooth® wireless technology	o	o
Keyboard
Alpha-numerical	o
Second Keyboard	o	o
1-functionTrigger key
2-functionTrigger key
FlexField Onboard Software
Orientation & Surveying, Stake Out, Resection, Height Transfer, Construction, Area (Plan & Surface), Volume calculation, Tie Distance (MLM), Remote Height, Hidden Point, Offset, Reference Line
Reference Arc, Reference Plane, COGO, Road 2D	o
Roadworks 3D, TraversePRO		o
Emitting Guide Light (EGL)
Emitting Guide Light (EGL) for stake out	o	o
Arctic Version
Temperature -35° C (operation)	o	o	o

A total station is an electronic/optical instrument used in modern surveying. It is also used by archaeologists to record excavations as well as by police, crime scene investigators, private accident reconstructionists and insurance companies to take measurements of scenes. The total station is an electronic theodolite (transit) integrated with an electronic distance meter (EDM) to read distances from the instrument to a particular point. Some models include internal electronic data storage to record distance, horizontal angle, and vertical angle measured, while other models are equipped to write these measurements to an external data collector, which is a hand-held computer.

Angles and distances are measured from the total station to points under survey, and the coordinates (X, Y, and Z or northing, easting and elevation) of surveyed points relative to the total station position are calculated using trigonometry and triangulation.

Data can be downloaded from the total station to a computer and application software used to compute results and generate a map of the surveyed area.

Some total stations also have a GNSS interface which combines the advantages of these two technologies (GNSS - line of sight not required between measured points; Total Station - high precision measurement especially in the vertical axis compared with GNSS) and reduce the consequences of each technology's disadvantages (GNSS - poor accuracy in the vertical axis and lower accuracy without long occupation periods; Total Station - requires line of sight observations and must be set up over a known point or with line of sight to 2 or more points with known location).

Most modern total station instruments measure angles by means of electro-optical scanning of extremely precise digital bar-codes etched on rotating glass cylinders or discs within the instrument. The best quality total stations are capable of measuring angles to 0.5 arc-second. Inexpensive "construction grade" total stations can generally measure angles to 5 or 10 arc-seconds.

Measurement of distance is accomplished with a modulated microwave or infrared carrier signal, generated by a small solid-state emitter within the instrument's optical path, and refected by a prism reflector or the object under survey. The modulation pattern in the returning signal is read and interpreted by the computer in the total station. The distance is determined by emitting and receiving multiple frequencies, and determining the integer number of wavelengths to the target for each frequency. Most total stations use purpose-built glass Porro prism reflectors for the EDM signal. A typical total station can measure distances with an accuracy of about 1.5 millimetres + 2 parts per million over a distance of up to 1,500 metres.

Reflectorless total stations can measure distances to any object that is reasonably light in color, to a few hundred meters.

Robotic total stations allow the operator to control the instrument from a distance via remote control. This eliminates the need for an assistant staff member as the operator holds the reflector and controls the total station from the observed point.

Content Acknowledgements: Wikipedia