Publication Details |
Category | Text Publication |
Reference Category | Journals |
DOI | 10.3389/frwa.2020.544847 |
Licence | |
Title (Primary) | Soil moisture and air humidity dependence of the above-ground cosmic-ray neutron intensity |
Author | Köhli, M.; Weimar, J.; Schrön, M.; Baatz, R.; Schmidt, U. |
Source Titel | Frontiers in Water |
Year | 2021 |
Department | MET |
Volume | 2 |
Page From | art. 544847 |
Language | englisch |
Topic | T5 Future Landscapes |
Keywords | monte carlo, neutron, soil moisture, Air humidity, Cosmic-ray neutron sensing, MCNP, URANOS |
UFZ wide themes | MOSES; |
Abstract | Investigations of neutron transport through air and soil by Monte Carlo simulations led to major advancements towards a precise interpretation of measurements, especially they improved the understanding of the cosmic-ray neutron footprint. Up to now, the conversion of soil moisture to a detectable neutron count rate relies mainly on the equation presented by Desilets et al. (2010). While in general a hyperbolic expression can be derived from theoretical considerations, their empiric parameterisation needs to be revised for two reasons. Firstly, a rigorous mathematical treatment reveals that the values of the four parameters are ambiguous because their values are not independent. We find a 3-parameter equation with unambiguous values of the parameters which is equivalent in any other respect to the 4-parameter equation. Secondly, high-resolution Monte-Carlo simulations revealed a systematic deviation of the count rate to soil moisture relation especially for extremely dry conditions as well as very humid conditions. That is a hint, that a smaller contribution to the intensity was forgotten or not adequately treated by the conventional approach. Investigating the above-ground neutron flux by a broadly based Monte-Carlo simulation campaign revealed a more detailed understanding of different contributions to this signal, especially targeting air humidity corrections. The packages MCNP and URANOS were used to derive a function able to describe the respective dependencies including the effect of different hydrogen pools and the detector-specific response function. The new relationship has been tested at two exemplary measurement sites and its remarkable performance allows for a promising prospect of more comprehensive data quality in the future. |
Persistent UFZ Identifier | https://www.ufz.de/index.php?en=20939&ufzPublicationIdentifier=23969 |
Köhli, M., Weimar, J., Schrön, M., Baatz, R., Schmidt, U. (2021): Soil moisture and air humidity dependence of the above-ground cosmic-ray neutron intensity Front. Water 2 , art. 544847 10.3389/frwa.2020.544847 |