Abstract
The evolution of structures in the Earth's convecting mantle is studied in a simple, but carefully scaled, laboratory flow. The geometrical scaling is constrained by the various geometries of convection cells possible in the Earth's interior. Two-layered mantle convection with a superposed small-scale circulation in the top is favoured here. The model flow has a Rayleigh number 104, a Prandtl number 108, and approximately axially symmetric cells with aspect ratio of unity. The rheology and boundary conditions are aimed to be dynamically similar to that occurring in the mantle. The flow is analysed on the basis on snapshots showing the progressive deformation and displacement of passive flow markers, which allow the reconstruction of velocity vectors, strain rate and vorticity. Inferences can be made about 1. (1) the progressive deformation in individual rock masses, and 2. (2) the nature of the large-scale mixing process caused by a combination of deformation and displacement in a convecting mantle. This is discussed in terms of the kinematic vorticity number. Both geological and fluid mechanical studies of low inertia flows may benefit from the new experimental technique and analyses presented here. Until now, it has been impossible to visualize and quantify the finite strains and rotation components of deformation in flowing fluids by other than numerical methods. The laboratory method advocated here is quick and involves equipment which is relatively cheap if compared with those required for numerical analyses. Basic understanding of elementary fluid dynamics is sufficient to perform innovative investigations in this new field.
| Original language | English |
|---|---|
| Pages (from-to) | 97-123 |
| Number of pages | 27 |
| Journal | Tectonophysics |
| Volume | 154 |
| Issue number | 1-2 |
| DOIs | |
| State | Published - 1 Nov 1988 |
| Externally published | Yes |
Bibliographical note
Funding Information:Uppsala University in 1984,d iscussionsw ith professor emeritusH . Ramberg,a nd continuouss u-pervision by professor C.J. Talbot. I thank Miss K. Glaersen for the word-processingo f my manuscript.A ll engineeringe, xperimentsp, hoto-graphs,p rints, preliminarya nd final line drawings were madeb y the author. The convectionp roject (1983-1987)h asbeen fundedb y the SwedishN atural ScienceR esearchC ouncil (NFR) under contract nos. G-DT 1858-101to 1858-104.
ASJC Scopus subject areas
- Geophysics
- Earth-Surface Processes