Home    Printable version    Sitemap    Glossary    Contacts

AltimetryData flowProcessingGeophysical corrections dry troposphere | electromagnetic bias | inverse barometer | ionosphere | ocean tide | pole tide | wet troposphere Wet troposphere correction

The wet troposphere correction is the correction for the path delay in the radar return signal due to liquid water in the atmosphere. It is calculated from radiometer measurements and meteorological models.

Its order of magnitude is about 0 to 50 cm with an annual cycle amplitude of up to 20 cm.

It is usually computed over oceans with simultaneous radiometric measurements (see the Jason-1 Microwave Radiometer (JMR)). But, such radiometric measurements generally fail over land or near the coasts and may be superseded by a correction computed from meteorological model outputs (usually the NCEP or ECMWF models).
In addition to its limited geographical coverage, this correction suffers, in Topex/Poseidon MGDR products, from the fact that the altitude of the water body is not taken into account: the atmosphere column reaches the sea level everywhere and is thus too thick!

wet troposphere correction from NCEP models
Amplitude in metres of the wet troposphere correction computed from the NCEP model during Topex/Poseidon cycle 300. (Credits CLS/Legos)

An error of 10 m in the thickness of the atmosphere column corresponds to an error of 1 mm in the correction. Consequently the correction is often overestimated for non-ocean areas. When this correction from meteorological models takes into account the surface altitude with a DEM (Digital Elevation Model), it's not so optimal.

Therefore, the precise estimation of the altitude of the reflecting continental surface appears as the key factor for an accurate computation of the propagation delay through the troposphere. Some projects are underway to improve this wet troposphere correction near the coasts and over land using the altitude value deduced from altimetric measurement itself.

Further information:


All rights reserved, copyright © 2006-2011
Tutorial produced by CLS under contract to ESA and CNES