TY - JOUR
T1 - Microplate motions in the hotspot reference frame
AU - Cuffaro, Marco
AU - Jurdy, Donna M.
PY - 2006/8
Y1 - 2006/8
N2 - We have computed motions of the major plates (seven large plates and seven medium-sized plates) and 38 microplates relative to the hotspot reference frame, and present velocities of these 52 plates. Moreover, using updated plate boundaries for the present, we have computed new geometrical factors for plates and microplates, useful for kinematic calculations and to obtain the net-rotation of the lithosphere and plate velocities in the mean-lithosphere reference frame. Instead of a continuum or gradational distribution of the plates by size, the plates clearly partition into three groups each having their own characteristics. For the seven large plates, rotation poles generally lie in high latitudes; the seven medium-sized plates have rotation poles in a restricted equatorial area; the 38 small plates show the greatest scatter. Moreover subsets of the 52 plates reveal differing fractal behaviour: the large, middle and small groupings each have a characteristic fractal dimension, suggestive of microplate clustering. The highest angular velocities occur for some of the smallest plates, with the location of their rotation poles closeby.
AB - We have computed motions of the major plates (seven large plates and seven medium-sized plates) and 38 microplates relative to the hotspot reference frame, and present velocities of these 52 plates. Moreover, using updated plate boundaries for the present, we have computed new geometrical factors for plates and microplates, useful for kinematic calculations and to obtain the net-rotation of the lithosphere and plate velocities in the mean-lithosphere reference frame. Instead of a continuum or gradational distribution of the plates by size, the plates clearly partition into three groups each having their own characteristics. For the seven large plates, rotation poles generally lie in high latitudes; the seven medium-sized plates have rotation poles in a restricted equatorial area; the 38 small plates show the greatest scatter. Moreover subsets of the 52 plates reveal differing fractal behaviour: the large, middle and small groupings each have a characteristic fractal dimension, suggestive of microplate clustering. The highest angular velocities occur for some of the smallest plates, with the location of their rotation poles closeby.
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U2 - 10.1111/j.1365-3121.2006.00690.x
DO - 10.1111/j.1365-3121.2006.00690.x
M3 - Article
AN - SCOPUS:33746241985
SN - 0954-4879
VL - 18
SP - 276
EP - 281
JO - Terra Nova
JF - Terra Nova
IS - 4
ER -