Furthermore, modelling in Bernese accounts for all time-dependent parameters by a piece-wise linear, continuous representation, in particular for troposphere zenith path delay and gradient parameter, earth orientation parameters and global ionosphere models. Meeting the highest accuracy requirements, Bernese models station motions for plate movements, solid earth tides and ocean tidal loading. Sophisticated examples contained in the distribution include: The newly developed powerful Bernese Processing Engine (BPE) allows you to tailor automated processing sequences. Save time and effort processing and combining data from various receiver types in the same processing step (including establishing and use of receiver type specific antenna phase centre variations). Use of ionosphere models minimises impact of ionosphere delay on station coordinates and other parameters. Single and dual frequency data may be processed in the same estimation step. Either static or kinematic, take differential code biases for satellites and receivers into account for applications involving code observations. With Bernese, you can processes all principal observables recorded by high precision geodetic receivers (i.e., code and phase data on both carriers). Commercial users with complex applications demanding high accuracy, reliability and high productivity.Agencies responsible for maintenance of arrays of permanent GNSS receivers.Survey agencies responsible for high-accuracy GNSS surveys.Scientists researching in geodesy, meteorology and geosciences.The Bernese GNSS Software is the ideal tool for: The software is continuously in a process of development and improvement. It is used by CODE (Center for Orbit Determination in Europe) for its international (IGS) and European (EUREF/EPN) activities.
Research licences are directly supplied by the AIUB. Leica Geosystems is an exclusive re-seller of the BERNESE software for commercial applications in the field of Geomatics. The Bernese GNSS Software is a scientific, high-precision, multi-GNSS data processing software developed at the Astronomical Institute of the University of Bern (AIUB).
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