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Verfasst von:Köhli, Markus [VerfasserIn]   i
 Weimar, Jannis [VerfasserIn]   i
 Schmidt, Ulrich [VerfasserIn]   i
Titel:Soil moisture and air humidity dependence of the above-ground cosmic-ray neutron intensity
Verf.angabe:Markus Köhli, Jannis Weimar, Martin Schrön, Roland Baatz and Ulrich Schmidt
E-Jahr:2021
Jahr:28 January 2021
Umfang:15 S.
Teil:volume:2
 year:2021
 day:28
 month:01
 elocationid:544847
 extent:15
Fussnoten:Gesehen am 31.03.2021
Titel Quelle:Enthalten in: Frontiers in water
Ort Quelle:Lausanne : Frontiers Media, 2019
Jahr Quelle:2021
Band/Heft Quelle:2(2021) vom: 28. Jan., Artikel-ID 544847
ISSN Quelle:2624-9375
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.
DOI:doi:10.3389/frwa.2020.544847
URL:Kostenfrei: Volltext ; Verlag: https://doi.org/10.3389/frwa.2020.544847
 Kostenfrei: Volltext: https://www.frontiersin.org/articles/10.3389/frwa.2020.544847/full
 DOI: https://doi.org/10.3389/frwa.2020.544847
Datenträger:Online-Ressource
Sprache:eng
Sach-SW:Air humidity
 Cosmic-ray neutron sensing
 MCNP
 monte carlo
 neutron
 soil moisture
 URANOS
K10plus-PPN:1752980514
Verknüpfungen:→ Zeitschrift
 
 
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