The Rigid Plate Model
The Plate Wizard rigid plate model provides:
- A detailed shapefile representing tectonic blocks on the Earth's crust with full plate definitions including rigid, deformable and oceanic plates.
- Poles of rotation are supplied back to 250 Ma for all of the plates that are defined in the shapefile. This allows reconstructions at any time interval.
New plate boundary definitions, based on present day geological structures, have been interpreted for the entire globe. Continental crust has been defined as either 'rigid', largely the cratonic interiors or 'deformable'. In the rigid model, the continental plates maintain a constant geometry through geological time.
In reality, lithospheric plates are not rigid, they undergo deformation in extensional and compressional environments. As the present day geometries of these plates are different from their palaeo-geometries, in traditional rigid plate reconstruction models this results in overlap or underfit. In the Plate Wizard deformable model, deformation has been modelled for extensional environments for the entire Atlantic margin and the Plate Wizard software uses this modelling to remove the deformation and accurately define the pre-rift geometry of these margins.
Redefining the boundaries
Utilising FRL's expertise in detailed regional modelling and the wealth of knowledge and information gained from a legacy of regional studies, new plate boundaries have been established for the entire globe.
The methods used to redefine plate boundaries include: analysis of Bouguer gravity anomalies, 3D modelling of crystalline crustal thickness, detailed geological mapping and river drainage analysis. Geophysical data, public domain datasets, and our extensive Tellus datasets (structural elements and total sediment isopach) were also used in this process.
See our Brochure for further information.
The following plate reconstructions are available for free download:
Global Rotation File
The relative motions between major tectonic plates have been determined by matching linear magnetic anomalies of similar age and combining these with palaeomagnetic, palaeobiogeographical and palaeoclimate data. Taking into consideration the geological and tectonic evolution of each region, these are then integrated into a global circuit that utilises Euler pole addition to calculate relative motions of less well-constrained plates.
