• Aucun résultat trouvé

Modelling SMOS brightness temperature by use of coupled SVAT and radiative transfer models over the Valencia Anchor Station

N/A
N/A
Protected

Academic year: 2021

Partager "Modelling SMOS brightness temperature by use of coupled SVAT and radiative transfer models over the Valencia Anchor Station"

Copied!
2
0
0

Texte intégral

(1)

HAL Id: hal-02754451

https://hal.inrae.fr/hal-02754451

Submitted on 3 Jun 2020

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.

Modelling SMOS brightness temperature by use of coupled SVAT and radiative transfer models over the

Valencia Anchor Station

Silvia Enache Juglea, Yann H. Kerr, Arnaud Mialon, E. Lopez-Baeza, Aurelio Cano, J.-C. Calvet, Al Bitar Ahmad, Jean-Pierre Wigneron

To cite this version:

Silvia Enache Juglea, Yann H. Kerr, Arnaud Mialon, E. Lopez-Baeza, Aurelio Cano, et al.. Modelling SMOS brightness temperature by use of coupled SVAT and radiative transfer models over the Valencia Anchor Station. EGU General Assembly, Apr 2009, Vienne, Austria. �hal-02754451�

(2)

Geophysical Research Abstracts, Vol. 11, EGU2009-2017, 2009 EGU General Assembly 2009

© Author(s) 2009

Modelling SMOS brightness temperature by use of coupled SVAT and radiative transfer models over the Valencia Anchor Station

S. JUGLEA (1), Y. KERR (1), A. MIALON (1), E. LOPEZ-BAEZA (2), A. CANO (2), J.C. CALVET (3), A.

ALBITAR (1), and J.P. WIGNERON (4)

(1) Cesbio, Toulouse, France , (2) Universitat de Valencia, Valencia, Spain, (3) Météo-France/CNRM , Toulouse, France, (4) EPHYSE - INRA , Bordeaux, France

Soil moisture is a key variable that controls water and heat energy interactions occurring at the land atmosphere interface. This parameter, very important for the weather and climate modelling, is not well monitored at a global scale. A number of experiments have shown the high potential of L-band microwave radiometry for monitoring surface soil moisture. In this context, the SMOS (Soil Moisture and Ocean Salinity) mission was designed to observe soil moisture over continental surfaces as well as ocean salinity. Due to be launched in summer 2009, it will provide global soil moisture maps every 3 days at least, with an average spatial resolution of 40 km x 40 km.

The VAS (Valencia Anchor Station) experimental site, in Spain, is a cornerstone of the SMOS Cal/Val plan. It is a semiarid environment and is characterized by an extensive set of measurements at different levels (in the atmosphere and in the soil) in order to derive surface energy fluxes.

In the framework of SMOS preparation, the research presented here deals with the use of surface variables from the VAS site to simulate passive microwave brightness temperature so as to have Satellite “match ups” for CalVal and to test retrieval algorithms.

First, ground and meteorological measurements from the VAS site are used to simulate soil moisture using a Soil-Vegetation-Atmosphere-Transfer (SVAT) model (ISBA) from Météo France. In order to validate this ap- proach, a point to point comparison with ground measurements has been done. We obtain a very good agreement between the simulated and measured soil moisture and we find that, as expected, the simulated soil moisture is mostly driven by precipitation patterns. Then, we propose a spatialization method using all the available data in order to have soil moisture estimates representative of a SMOS pixel. The results are compared with remotely sensed data such as soil moisture from AMSR-E. An amplitude difference between both soil moisture data is observed but also a good agreement in terms of temporal variability. Discrepancies appear mostly during the growing season, the AMSR-E signal being strongly influenced by the vegetation. Better correlation is obtained using polarization ratio which has often been used to study soil moisture.

The second step consists in using output data from ISBA model to simulate the surface emission through the use of radiative transfer models (L-MEB - L-band Microwave Emission of the Biosphere model). Parame- terization has been done in order to simulate brightness temperature at C and X-band. A very high correlation coefficient (more than 0.90) has been obtained when comparing with AMSR-E data at 6.9 (C-band) GHz and 10.7 (X-band) GHz.

We will present also the first simulation in L-band which will help better understanding of the exact signification of the SMOS signal and thus give a first insight of the SMOS data.

Références

Documents relatifs

The objective of this paper is to investigate the benefit of applying the PERSIANN database to reproduce the high temporal and spatial heterogeneity of soil moisture fields at

Based on this conclusion, a simple model had been built to obtain open water maps over the Amazon and Congo basin from SMOS brightness temperature at a coarse spatial resolution (25

The Mediterranean Ecosystem L-Band characterisation EXperiment (MELBEX3) to monitor SMOS validation conditions at Valencia Anchor Station in 2010 and 2011.. Maciej

A control area of 10 x 10 km 2 has been chosen where a network of ground soil moisture measuring stations has being set up based on the definition of homogeneous

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

Band brighness temperature simulated from coupled SVAT model and radiative transfer model over the Valencia Anchor Station.. European Geosciences Union General Assembly, Apr

(1) Departamento de Fisica de la Tierra y Termodinamica Facultad de Fisica Universidad de Valencia, Spain, (2) INRA - Institut National de la Recherche Agronomique, France, (3)

Figure 6.16 Comparaison entre la température de brillance verticale (à gauche) et horizontale (à droite) issues du produit AMSR-E à 6.9 GHz et la température de brillance simulée