Evidence for a post-3.16-Ma change in Nubia^Eurasia^North America plate motions?

We combine updated GPS velocities from the Nubian (NU), Eurasian (EU), and North American (NA) plates with 500 new 3.16-Myr-average seafloor spreading rates and nine transform fault azimuths from the northern Atlantic and Arctic basin seafloor spreading centers to estimate and test for changes in th...

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Bibliographic Details
Main Authors: E. Calais A, C. Demets B, J. -m. Nocquet C
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2003
Subjects:
plate motions
GPS
Eurasia
Nubia
North America
Arctic
Nubian
Arctic Basin
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.491.7922
http://kreiz.unice.fr/data/ARTICLES/epsl_2003.pdf
Description
Summary:We combine updated GPS velocities from the Nubian (NU), Eurasian (EU), and North American (NA) plates with 500 new 3.16-Myr-average seafloor spreading rates and nine transform fault azimuths from the northern Atlantic and Arctic basin seafloor spreading centers to estimate and test for changes in the relative motion between these plates. The numerous new seafloor spreading rates and GPS velocities improve our ability to detect recent changes in the relative motions of these plates. The angular velocity vector that best fits the EU^NA GPS velocities lies significantly north of the 3-Ma-average pole, in accord with previously published geologic evidence that the EU^NA pole has migrated northward since V3 Ma. Although we also find evidence for a significant post-3-Ma change in NU^NA motion, it is less compelling because the Nubian plate GPS velocity field is sparse and NU^NA seafloor spreading rates appear to have remained steady within the 1 mm yr31 uncertainties if we systematically decrease the seafloor spreading rates to correct for outward displacement of seafloor spreading magnetic lineations. The NU^EU pole derived from GPS site velocities lies more than 30 angular degrees south of the tightly constrained 3-Ma-average estimate and predicts significantly slower and more oblique present-day NU^EU convergence in the Mediterranean. Both models for NU^EU motion pass a key test for their accuracy, namely, they correctly predict strike-slip motion along the well-mapped Gloria fault east of the Azores. The change to more oblique NU^EU motion may reflect increasing difficulty in maintaining margin-normal convergence within this continent^continent collision zone.

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