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Cosmic-ray neutron sensing for the estimation of soil moisture ; Cosmic-Ray Neutron Sensing zur Messung der Bodenfeuchte

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  • معلومة اضافية
    • الموضوع:
      2024
    • Collection:
      University of Potsdam: publish.UP
    • نبذة مختصرة :
      Water stored in the unsaturated soil as soil moisture is a key component of the hydrological cycle influencing numerous hydrological processes including hydrometeorological extremes. Soil moisture influences flood generation processes and during droughts when precipitation is absent, it provides plant with transpirable water, thereby sustaining plant growth and survival in agriculture and natural ecosystems. Soil moisture stored in deeper soil layers e.g. below 100 cm is of particular importance for providing plant transpirable water during dry periods. Not being directly connected to the atmosphere and located outside soil layers with the highest root densities, water in these layers is less susceptible to be rapidly evaporated and transpired. Instead, it provides longer-term soil water storage increasing the drought tolerance of plants and ecosystems. Given the importance of soil moisture in the context of hydro-meteorological extremes in a warming climate, its monitoring is part of official national adaption strategies to a changing climate. Yet, soil moisture is highly variable in time and space which challenges its monitoring on spatio-temporal scales relevant for flood and drought risk modelling and forecasting. Introduced over a decade ago, Cosmic-Ray Neutron Sensing (CRNS) is a noninvasive geophysical method that allows for the estimation of soil moisture at relevant spatio-temporal scales of several hectares at a high, subdaily temporal resolution. CRNS relies on the detection of secondary neutrons above the soil surface which are produced from high-energy cosmic-ray particles in the atmosphere and the ground. Neutrons in a specific epithermal energy range are sensitive to the amount of hydrogen present in the surroundings of the CRNS neutron detector. Due to same mass as the hydrogen nucleus, neutrons lose kinetic energy upon collision and are subsequently absorbed when reaching low, thermal energies. A higher amount of hydrogen therefore leads to fewer neutrons being detected per unit time. Assuming ...
    • File Description:
      application/pdf
    • Relation:
      https://publishup.uni-potsdam.de/frontdoor/index/index/docId/63646; urn:nbn:de:kobv:517-opus4-636465; https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-636465; https://doi.org/10.25932/publishup-63646; https://publishup.uni-potsdam.de/files/63646/rasche_diss.pdf
    • الرقم المعرف:
      10.25932/publishup-63646
    • الدخول الالكتروني :
      https://publishup.uni-potsdam.de/frontdoor/index/index/docId/63646
      https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-636465
      https://doi.org/10.25932/publishup-63646
      https://publishup.uni-potsdam.de/files/63646/rasche_diss.pdf
    • Rights:
      https://creativecommons.org/licenses/by/4.0/ ; info:eu-repo/semantics/openAccess
    • الرقم المعرف:
      edsbas.D3F8F01E