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The Cosmic-ray Soil Moisture Observation System (Cosmos) for estimating the crop water requirement: new approach

Ragab, R. ORCID: https://orcid.org/0000-0003-2887-7616; Evans, J.G. ORCID: https://orcid.org/0000-0003-4194-1416; Battilani, A.; Solimando, D.. 2017 The Cosmic-ray Soil Moisture Observation System (Cosmos) for estimating the crop water requirement: new approach. Irrigation and Drainage, 66 (4). 456-468. 10.1002/ird.2152

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Abstract/Summary

Soil moisture is a crucial parameter to determine the crop water requirement for irrigation. The soil moisture deficit (SMD) of the root zone is an indicator that can be used to determine the exact crop water requirement. Application of the recent technology of COsmic-ray Soil Moisture Observation System (Cosmos) provides continuous, integrated, area-based values, with a measurement radius of up to 400 m, whilst being non-invasive. In a field experiment in Italy, the Cosmos probe was used over a mixed crop area during the cropping seasons of 2014 and 2015. The results showed that soil moisture values obtained by Cosmos were comparable with those obtained for the top 0–60 cm layer soil moisture measured by sensors, soil cores, profile probes and with values simulated by the SALTMED model. This indicates that the Cosmos probe's effective depth of sensing is within the top 0–60 cm. Knowing that almost 80% of the crop root system is accommodated within the top 0–60 cm, the Cosmos measurement could be useful for monitoring the soil water status and SMD in the root zone in irrigated agriculture. The Cosmos system could be made operational for irrigation managers to determine when and how much to irrigate

Item Type: Publication - Article
Digital Object Identifier (DOI): 10.1002/ird.2152
UKCEH and CEH Sections/Science Areas: Acreman
Rees (from October 2014)
ISSN: 1531-0353
Additional Keywords: crop water requirement, Cosmos, soil moisture deficit, soil moisture measurement, SALTMED model, irrigation requirement
NORA Subject Terms: Hydrology
Agriculture and Soil Science
Date made live: 30 Oct 2017 12:23 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/518160

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