Abstract

GRACE spherical harmonics are well-adapted for representation of hydrological signals in river drainage basins of large size such as the Amazon or Mississippi basins. However, when one needs to study smaller drainage basins, one comes up against the low spatial resolution of the solutions in spherical harmonics. To overcome this limitation, we propose a new approach based on Slepian functions which can reduce the energy loss by integrating information in the spatial, spectral and time domains. Another advantage of these regionally-defined functions is the reduction of the problem dimensions compared to the spherical harmonic parameters. This also induces a drastic reduction of the computational time. These Slepian functions are used to invert the GRACE satellite data to restore the water mass fluxes of different hydro-climatologic environments in Africa. We apply them to two African drainage basins chosen for their size of medium scale and their geometric specificities: the Congo river basin with a quasi-isotropic shape and the Nile river basin with an anisotropic and more complex shape. Time series of Slepian coefficients have been estimated from real along-track GRACE geopotential differences for about ten years, and these coefficients are in agreement with both the spherical harmonic solutions provided by the official centers CSR, GFZ, JPL and the GLDAS model used for validation. The Slepian function analysis highlights the water mass variations at sub-basin scales in both basins.

Highlights

  • Since 2002, the Gravity Recovery and Climate Experiment (GRACE) launched by NASA and DLR belongs to a new generation of Low-Earth Orbiter (LEO) satellites that improves the resolution of the gravity field to 300–400 km [1,2]

  • This analysis was applied to two African basins, Congo and Nile, respectively, according to their surface area which are quite close to ~4 and ~3 million km2

  • Another key point is the shape of these two basins, the first one, the Congo basin, has an isotropic shape ratio while the second, the Nile basin, presents a strongly latitudinal anisotropic shape, which will allow us to examine the impact of the shape and size on the parameterization of both K/Kopt and L

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Summary

Introduction

Since 2002, the Gravity Recovery and Climate Experiment (GRACE) launched by NASA and DLR belongs to a new generation of Low-Earth Orbiter (LEO) satellites that improves the resolution of the gravity field to 300–400 km [1,2]. SH are a basis of orthogonal functions on the entire Earth sphere and are not adapted to study restricted areas or localized structures, e.g., medium- to small-scale watersheds that cause a loss of their orthogonality. Without this orthogonality condition, any regional decomposition is not unique and cannot be ensured.

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