OMP Level 2A 10-Days atmospheric dealiasing model

OMP Level 2A 10-Days atmospheric dealiasing model

Description of the solutions

The ERA-Interim and TUGO dealiasing products enable the estimation of spatial and temporal variations in the gravitational potential of the atmosphere (ERA-Interim) and the ocean (TUGO) in 3D. The mean value of the original grids, calculated over a 10-year period (2001–2010), was subtracted from the time series, so that the OMP dealiasing products represent only the time-varying component of the gravitational pull of the atmosphere and ocean masses. Geopotential anomalies due to atmospheric mass redistributions were calculated from the ECMWF’s ERA-Interim reanalysis (60 model levels, every 3 hours).

The dealiasing models were calculated by Pascal Gégout (GET/CNRS), by integrating the gravitational potential at each level of the atmospheric reanalysis to obtain the total gravitational effect outside the atmospheric masses. This is why we refer to “3D” gravitational potential.

The response of the solid Earth to this time-varying atmospheric and oceanic potential was accounted for using Love numbers kp (see here). The 10-days dealiasing models are obtained by averaging the 3-hour products, taking into account the arcs used for the production of the geopotential solutions. An example of a 10-day dealiasing model is shown in Figure 1. 

Files description

The time series of atmospheric dealiasing models is provided in the form of spherical harmonic coefficients up to degree and order 90, excluding degrees 0 and 1 (8,277 coefficients). The coefficients for degrees 0 and 1 appear in the files with a value of zero. The solutions are distributed in ASCII files, with the coefficients sorted according to the extended GRACE format, which is an extension of the original GRACE gravity model format (document GR-GFZ-FD-001 GRACE 327-732 (v1.1), November 27, 2003, available here), sorted in ascending order of degree and order. An example file is provided below.

Example file: GAA 2014-01-02 RL0005 Model FIRST GAA-2_2013362-2014006_0010_GRGS_0090_0003. SHM CNES / GRGS YYYYMMDD EARTH 0.3986004415E+15 0.6378136460E+07 SHM 90 90 0.00 fully normalized not applicable GRCOF2 0 0 0.000000000000E+00 0.000000000000E+00 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 1 0 0.000000000000E+00 0.000000000000E+00 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 1 1 0.000000000000E+00 0.000000000000E+00 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 2 0 0.106720334019E-09 0.000000000000E+00 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 2 1 0.962160295167E-10 0.522538168260E-10 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 2 2 -.131141395134E-09 0.115199498788E-09 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 3 0 -.205593048067E-09 0.000000000000E+00 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 3 1 -.604262891804E-10 0.187805159783E-10 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn . . . GRCOF2 90 89 0.279197692377E-14 0.382340788923E-14 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn GRCOF2 90 90 -.192059559087E-14 -.118555283387E-15 0.0000E+00 0.0000E+00 20131228.0000 20140107.0000 nnnn

Using the solutions

In order to use these solutions, it is necessary to express the gravitational potential at every point on Earth. The Earth’s gravitational potential is expressed as follows:


Where rφ, and λ are, respectively, the radius, latitude, and longitude of the considered point, Clm and Slm are the harmonic coefficients of the solution, G is the universal gravitational constant, M is the mass of the Earth, a is the Earth’s equatorial radius, P̅lm is the associated Legendre function of degree l and order m.

Generally, the gravitational potential is expressed at the Earth’s surface. Since the models are based on the GRACE/-FO geopotential solutions, they must be expressed in the same way—that is, generally as variations in a thin layer of water on the Earth’s surface. In this case, the previous equation becomes, when calculated up to a maximum degree Lmax:

Where:

– ΔHW(φλ) is the equivalent water height at latitude φ and longitude λ,
a is the Earth’s average radius,
ρE is the average Earth density,
ρw is the water density,
kl is the Load Love Number (LLN) at any harmonic degree l,
– Y̅lm are the Legendre polynomial functions for any degree l and order m, in complex notation,
– ΔC̅lm are the increments, relative to a reference gravitational solution, of the complex spherical harmonic coefficients of the solution.

More details about the method can be found in Ditmar (2018).

Dataset identifier

10.24400/170160/SAGSA_GGM_GAA_10DAYS_RL0005

Characteristics

Product typeStokes coefficients
FormatASCII files
License(CCBY)
Start of production01/04/2002
End of production01/05/2017
CoverageGlobal
Coverage typeSpherical harmonics
Spatial resolutionMaximum degree: 90
Time resolution10-days models
Mission(s)None
Instrument(s) / Captor(s)None

Citation

F. LYARD and P. GEGOUT. Atmospheric dealiasing gaa 10 days, 2025a. URL https://geodes.cnes.fr/projects/l2a_omp_sagsa_ggm_gaa_10days/.

Bibliography

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