The biaxial level compensation mechanism has a wider adjusting range of ±6′ which is twice as wide, compared with previous models. This enables highly accurate measuring performance.

The auto-pointing accuracy* with the standard prism is 1″ (1mm@200m), and 4″ (1mm@50m) with a reflective sheet.
* Auto-pointing accuracy is verified using the methods specified by ISO 17123-3.

Prisms or sheet target can be located easily in dim lighting conditions using the high-intensity white LED built into the telescope.

Provides protection from dust and driving rain as well as other inclement weather conditions. Operates in temperatures from -20 to +50ºC.

A library of special control commands can be provided in order to establish remote operation functionality in your own monitoring system.

*Please contact us for the details of the special commands.

This function is ideal for structural monitoring applications to make initial setup easy and fast.
The NET series automatically searches within the predetermined area to quickly measure the reflectors as initial positions for subsequent routine measurements.
This function works even in low light or dark conditions where the reflectors cannot be clearly seen by the human eye and provides greatly increased efficiency in initial reflector search.

*This function is not included in on-board software, and need to be implemented in the user’s own system using opened command.

The NET series incorporates an advanced auto-pointing algorithm* optimized for monitoring applications. The NET series automatically sights the prism closest to the telescope center regardless of the distance from the instrument. This works even if multiple prisms or other reflective objects are in the field of view.
This feature dramatically enhances the reliability in periodic monitoring of predetermined prism locations.

* With a regular auto-pointing algorithm, the instrument normally sights the nearest target with the strongest reflection.