Publication | Open Access
Apparent and true polar wander and the geometry of the geomagnetic field over the last 200 Myr
975
Citations
84
References
2002
Year
EngineeringPaleoceanographyTrue Polar WanderSolar-terrestrial InteractionEarth ScienceGeophysicsPlanetary MagnetosphereGeodesyMarine GeologyGeomagnetismLast 200GeologyIndian Hot SpotsPaleoclimatologySpace WeatherMagnetospheric PlasmaTectonicsHot Spot TracksGeomagnetic FieldPolar ScienceMagnetic FieldHot Spot Apw
The study uses updated kinematic models and selected paleomagnetic data to construct a master apparent polar wander path and compares paleomagnetic and hotspot APWs to derive a new determination of true polar wander. The authors construct new APWPs for major plates over the last 200 Myr, revealing a persistent 3 % quadrupole moment, episodic true polar wander with standstills and fast tracks lasting tens of millions of years at 30–50 km/Myr, a total TPW of ~30°, no evidence for superfast TPW, and global consistency between hotspot and paleomagnetic TPW that current models still fail to fully explain.
We have constructed new apparent polar wander paths (APWPs) for major plates over the last 200 Myr. Updated kinematic models and selected paleomagnetic data allowed us to construct a master APWP. A persistent quadrupole moment on the order of 3% of the dipole over the last 200 Myr is suggested. Paleomagnetic and hot spot APW are compared, and a new determination of “true polar wander” (TPW) is derived. Under the hypothesis of fixed Atlantic and Indian hot spots, we confirm that TPW is episodic, with periods of (quasi) standstill alternating with periods of faster TPW (in the Cretaceous). The typical duration of these periods is on the order of a few tens of millions of years with wander rates during fast tracks on the order of 30 to 50 km/Myr. A total TPW of some 30° is suggested for the last 200 Myr. We find no convincing evidence for episodes of superfast TPW such as proposed recently by a number of authors. Comparison over the last 130 Myr of TPW deduced from hot spot tracks and paleomagnetic data in the Indo‐Atlantic hemisphere with an independent determination for the Pacific plate supports the idea that, to first order, TPW is a truly global feature of Earth dynamics. Comparison with numerical modeling estimates of TPW shows that all current models still fail to some extent to account for the observed values of TPW velocity and for the succession of standstills and tracks which is observed.
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