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URANOS - The Ultra Rapid Adaptable Neutron-Only Simulation for Environmental Research

M. Köhli 1, M. Schrön 2, S. Zacharias 2, P. Dietrich 2, and U. Schmidt 1

1 Physics Institute, Heidelberg University,
2 Department of Monitoring and Exploration Technologies, UFZ Leipzig

Cite as (preliminary):
Köhli, M., Schrön, et al., 2015, "Footprint characteristics revised for field-scale soil moisture monitoring with cosmic-ray neutrons", Water Resources Research, 51, 5772-5790, doi:10.1002/2015WR017169


The Monte-Carlo code URANOS was specifically tailored to address the open questions of cosmic-ray neutron sensing for environmental applications (Köhli et al. 2015). The model's designated purpose is the precise description of neutron interactions in nuclear physics, where it is used as a tool to study the response of detectors for time-of-flight based interferometric methods (see Köhli et al. 2016). Recently, the response functions of cosmic-ray neutron detectors have been analysed with URANOS (Köhli et al. 2018). The model is able to predict the response of cosmic-ray neutrons to user-defined and spatially variable conditions in the soil, atmosphere, and biosphere (Schrön et al. 2018a, 2018b). URANOS is very efficient, as it only accounts for the most relevant neutron interaction processes, namely elastic collisions, inelastic collisions, absorption, and evaporation. The main model features are:

  • tracking of particle histories from creation to detection (ray-tracing),
  • detector representation as layers or cylinders,
  • automatic model and material setup based on color codes in 2D bitmap images

Using ENDF/B-VII and JENDL-HE, the model refers to the same physics database as other particle transport codes, like MCNP or Geant4. Nevertheless, this software should be considered as research in progress.

User community

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Publications using URANOS

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URANOS was developed for the project "Neutron Detectors for the MIEZE method" funded by the German Federal Ministry of Education and Research (BMBF), grant identifier: 05K10VHA. Source code and support for URANOS can be provided by M. Köhli. The research was funded and supported by Terrestrial Environmental Observatories (TERENO), which is a joint collaboration program involving several Helmholtz Research Centers in Germany.