Abstract
The very long wavelength (i.e. in the degree range ℓ = 1–8) dynamic topography at the Earth's surface, estimated by isostatic reduction of the observed topography, is shown to be in good agreement with the topography predicted by a model of viscous flow in the mantle. This flow model was previously derived by independent consideration of the observed nonhydrostatic geoid and is based upon a recent model of large‐scale seismic shear velocity heterogeneity in the mantle. Our estimate (and prediction) of the long wavelength dynamic surface topography reveals significant depressions (≈ 2–3 km) of the continental shields relative to their hydrostatic reference positions.
| Original language | English |
|---|---|
| Pages (from-to) | 225-228 |
| Number of pages | 4 |
| Journal | Geophysical Research Letters |
| Volume | 20 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - 1 Jan 1993 |
| Externally published | Yes |
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