EGU21-9215
https://doi.org/10.5194/egusphere-egu21-9215
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Moisture and humidity dependence of the above-ground cosmic-ray neutron intensity revised

Markus Köhli1,2, Jannis Weimar1, Benjamin Fersch3, Roland Baatz4, Martin Schrön5, and Ulrich Schmidt1
Markus Köhli et al.
  • 1Physikalisches Institut, Heidelberg University, Heidelberg, Germany (koehli@physi.uni-heidelberg.de)
  • 2Physikalisches Institut, University of Bonn, Bonn, Germany
  • 3Karlsruhe Institute of Technology, Campus Alpin (IMK-IFU), Garmisch-Partenkirchen, Germany
  • 4Agrosphere (IBG-3), Forschungszentrum Jülich GmbH, Jülich, Germany
  • 5Department of Monitoring and Exploration Technologies, Helmholtz Center for Environmental Research (UFZ), Germany

The novel method of Cosmic-ray neutron sensing (CRNS) allows non-invasive soil moisture measurements at a hectometer scaled 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 three exemplary measurement sites and its remarkable performance allows for a promising prospect of more comprehensive data quality in the future.

How to cite: Köhli, M., Weimar, J., Fersch, B., Baatz, R., Schrön, M., and Schmidt, U.: Moisture and humidity dependence of the above-ground cosmic-ray neutron intensity revised, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-9215, https://doi.org/10.5194/egusphere-egu21-9215, 2021.

Corresponding presentation materials formerly uploaded have been withdrawn.