NASA NTRS · 20030067893
Improvement in Geoid Models for Ocean Circulation Studies
Abstract
At wavelengths of 500 km and longer, the GRACE GGM01 Model produces a significantly better marine geoid than any previous model. This conclusion follows from evaluating the geostrophic currents determined by combining the model with a mean sea surface from altimetry. The agreement with currents computed from a traditional hydrographic map is very close, which suggests that one of the primary missions of the TOPEX/POSEIDON mission, to determine the absolute dynamic ocean topography, may soon be met. This solution has been made available to the public at http://www.csr.utexs.edu/grace/gravity. The results reported in this paper have been presented at the 2003 EGS-AGU-EUG Joint Assembly. Two articles are currently being prepared for Geophysical Research Letters to summarize these results.
Keep this discovery
Explore connections, maps & timelines
Tapley, Byron D., Chambers, Don P., Poole, Steve, Ries, John c.. 2003-08-17. Improvement in Geoid Models for Ocean Circulation Studies. https://ntrs.nasa.gov/citations/20030067893
Cite the original work for its findings. Save a collection to share your selection of sources.