Closed leuliett closed 3 months ago
I will use the same implementation as in Sentinel-6 and Jason-3 GDR-F. The coefficients you refer to are there expanded into 2D grids. A file poletide_aux.nc has already been put in $RADSROOT/altim/data for that purpose.
With commit ad3b7ef the issue is fixed in code.
Will still need to be applied to all RADS data.
The following mission data have been fully updated with the pole tide fix:
Closing this in favour of #204
Update the pole tide solution to S. Desai pole tide with new IERS linear mean pole.
1) The secular pole computation in poletide.f90 needs to be updated: ! Remove GIA contribution to polar motion (Desai, 2015) poletab(i)%xpole = x - (0.05097d0 + 0.00062d0 t) poletab(i)%ypole = y - (0.33449d0 + 0.00348d0 t)
GDR-F is using IERS Conventions (2010) v1.3.0, Chapter 7.1.4: The coordinates of that secular pole designated (xs, ys) and are given in milliarcseconds by xs = 55.0+1.677∗(t−2000), ys = 320.5+3.460∗(t−2000), where t is the date in years of 365.25 days.
References: IERS Conventions (2010) v1.3.0, Chapter 6 and 7: https://iers-conventions.obspm.fr/conventions_versions.php#official_target
Desai, S., Wahr, J., Beckley, B., 2015, “Revisiting the pole tide for and from satellite altimetry,“ J. Geod., 89, 1233-1243, doi:10.1007/s00190-015-0848-7.
2) A more complete implementation of the pole tide would include more harmonics than the degree-2 values in poletide.f90 Approximately 90% of the variance of the ocean pole tide potential is provided by the degree n = 2 spherical harmonic components, with the next largest contributions provided by the degree n = 1 and n = 3 components, respectively (see Figure 6.1). Expansion to spherical harmonic degree n = 10 provides approximately 99% of the variance. However, adequate representation of the continental boundaries will require a spherical harmonic expansion to high degree and order.
The full set of coefficients is available at: ftp://tai.bipm.org/iers/conv2010/chapter6/desaiscopolecoef.txt