Reversals Of The Magnetic Field, Mantle Convection And Tectonics

Key variable heat transfer

“The key variable is the heat flow. A cooler mantle accelerates the flow of heat from the hot core of the Earth, and in this way alters the also heat-driven convection in the Earth’s core”, said Bernhard Steinberger of the GFZ German Research Centre for Geosciences. “Ocean floor sinking into the mantle due to tectonic processes can lead to cooling in the mantle. They cause at these sites an increased heat flow into the cooler parts, namely until they have been heated to the ambient temperature.” That might take several hundred million years, however.

Video: Calculated current distribution of heat flow at the core-mantle boundary

http://youtu.be/bP_BZQv0dM8

Conversely, the hot core of the Earth leads to the ascent of heated rocks in form of large bubbles, so-called mantle plumes that separate from the core-mantle boundary and make their way up to the surface of the earth. This is how Hawaii came into existence. This increases the local heat flux out of the earth’s core and in turn modifies the generator of the geomagnetic field.

Reversals of the magnetic field 

In the Earth’s history, polarity reversals of the geomagnetic field are nothing extraordinary. The most recent took place only 780 000 years ago, geologically speaking a very short period of time. The research team was able to determine that in the period of 200 to 80 million years before present, reversals initially happened more often, namely up to ten times in hundred million years. “Surprisingly, these reversals stopped about 120 million years ago and were absent for nearly 40 million years,” explains GFZ scientist Sachs. Scientists presume that the reason for this is a concurrent reorientation of the whole mantle and crust with a shift in the geographic and magnetic poles of about 30°. Known as “true polar wander”, thisprocess is caused by a change in density distribution in the mantle. If it increases the heat flux in equatorial regions, it would presumably lead to more frequent field reversals, if it decreases it, the field reversal might not occur.

Looking to the future

According to current knowledge, therefore, an influence of plate tectonics and mantle convection on the Earth’s magnetic field seems quite possible. The article also shows, however, that further research is still needed for a better understanding of these relationships. In particular, more episodes of “true polar wander” should be derived from paleomagnetic data, and it should be determined whether these are usually associated with an altered behavior of the magnetic field (e.g. frequency of field reversal). Also, future models for the generation of the geomagnetic field should investigate the influence of the spatial and temporal variation of the heat flux at the core-mantle boundary in more detail.

Contacts and sources:
F.Ossing
Helmholtz Association of German Research Centres