HR: 0800h
AN: GP11B-0832 [Abstracts]
TI: Local Reversal Durations and Inverse Magnetic Field Patches in
Geodynamo Simulations
AU: * Wicht, J
EM: wicht@linmpi.mpg.de
AF: Johannes Wicht, Max-Planck-Institut fuer Sonnensystemforschung
Max-Planck-Strasse 2, Katlenburg-Lindau, Ni 37191
Germany
AB:
Paleomagnetists commonly infer reversal properties based
on records from one site only.
In an attempt to gain more global information about geomagnetic
field reversals Bradford Clement (Nature, 2004) analyses the
latitude dependence of reversal durations in several paleomagentic
records. He finds that the field transitions takes signifincantly
longer close to the poles than near the equator.
Such a piece of information is important for testing numerical
geodynamo simulations. Many simulated reversals show a comparable
latitudinal dependence. These models offer the opportunity to
identify the cause of such an effect. I have tried to link the
reversal duration to the transitional magnetic field at the core-mantle
boundary. Unfortunately, the connection is complex.
Reversals tend to last longer then average where the first inverse patches appear
at the core-mantel boundary.
They are shorter than average where secondary inverse patches tilt over
an already weak core-mantel boundary field.
Any equatorial and large scale azimuthal transitional field asymmetries
can be identified in a global map of reversal duration.
It has been speculated that the intensifying inverse patches at the Earth's
core-mantel boundary may constitute the start of a field reversal.
So far, they are too weak to lead to significant changes in field inclination.
This, however, may change if the inverse patches close to the equator
move to higher latitudes. Such a behavior is frequently found in
dynamo simulations and indeed can mark the start of a field
reversal. However, more often the inverse patches disappear again
causing only slight oszillations in inclination.
UR: http://www.linmpi.mpg/~Wicht/Reversals
DE: 1510 Dynamo theories
DE: 1513 Geomagnetic excursions
DE: 1535 Reversals (process, timescale, magnetostratigraphy)
DE: 1545 Spatial variations (all harmonics and anomalies)
SC: Geomagnetism and Paleomagnetism [GP]
MN: 2004 AGU Fall Meeting