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| Online-Ressource |
Verfasst von: | Köhli, Markus [VerfasserIn]  |
| Weimar, Jannis [VerfasserIn]  |
| Schmidt, Ulrich [VerfasserIn]  |
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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Lokale URL UB: | Zum Volltext |
Soil moisture and air humidity dependence of the above-ground cosmic-ray neutron intensity / Köhli, Markus [VerfasserIn]; 28 January 2021 (Online-Ressource)
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