EGU25-15027, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-15027
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Scaling Cosmic Ray Neutron Flux for Enhanced Environmental Monitoring
Roland Baatz1, Patrick Davies2, Paolo Nasta3, Paul Schattan4, Emmanuel Quansah2, Leonard Amekudzi2, and Heye Bogena5
Roland Baatz et al.
  • 1Leibniz Zentrum für Agrarlandschaftsforschung (ZALF) e.V., Müncheberg, Germany
  • 2Department of Meteorology and Climate Science, KNUST, Kumasi-Ghana
  • 3Department of Agricultural Sciences, Division of Agricultural, Forest and Biosystems Engineering, University of Naples Federico II, Portici (Naples), Italy
  • 4Institut für Geographie, Innrain 52f, Innsbruck, Austria
  • 5Institute of Bio- and Geosciences, Agrosphere (IBG-3), Forschungszentrum Jülich GmbH, Jülich, Germany

Cosmic Ray Neutron Sensors (CRNS) are pivotal in measuring field-scale soil moisture, but uncertainties persist due to traditional methods of scaling parameter estimation, which often fail to consider site- and sensor-specific factors. This study integrates novel, data-driven approaches to refine scaling parameters for atmospheric pressure, air humidity and incoming cosmic ray intensity (β, ψ, ω) using measurement data. We demonstrate the strong potential for considerable improvents in the accuracy of CRNS-derived soil moisture estimates. Additionally, barometric correction in CRNS but also in neutron monitors is critical to account for local atmospheric density variations to minimize errors in soil moisture estimation and incoming cosmic ray intensity. Our analysis of CRNS and Neutron Monitor data from global stations reveals significant variability in barometric coefficients (β), influenced by geographical and atmospheric factors. The findings underscore the necessity for tailored scaling and correction methods to optimize CRNS applications in hydrology, agriculture, and climate research. Enhanced parameter estimation reduced RMSE by up to 25%, demonstrating potential for improved environmental decision-making and modeling accuracy.

How to cite: Baatz, R., Davies, P., Nasta, P., Schattan, P., Quansah, E., Amekudzi, L., and Bogena, H.: Scaling Cosmic Ray Neutron Flux for Enhanced Environmental Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15027, https://doi.org/10.5194/egusphere-egu25-15027, 2025.