Magnetic lineations on the sea floor
Magnetic lineations on the sea floor#
This section was contributed by Juliane Dannberg.
The input file for this model can be found at cookbooks/magnetic_stripes/magnetic_stripes.prm.
This is a model of a mid-ocean ridge that shows how magnetic lineations are created on the sea floor as the magnetic field changes its orientation over time. The model setup is similar to the heat flow model described in Convective and conductive heat flow: Cooling of oceanic lithosphere. The only difference is that the model also has a compositional field that tracks the orientation of the magnetic field when material reaches the surface at the ridge axis in the center of the model (and correspondingly, a value of 1 or -1 is assigned to the field). As the material is advected away from the ridge axis, alternating stripes – symmetric with respect to the ridge axis – become visible.
This functionality is implemented through a new material model called magnetic stripes. This material model allows it to add a list of reversal times to the input file, that will then be used during the simulation. The input file used here contains the Earth’s reversal history of the last 83 million years.
Before the model can be run, the plugin needs to be compiled (see Running benchmarks that require code). To illustrate the stripes forming on the sea floor, a high resolution is necessary, which means that this cookbook needs longer to run than some of the others, and it may not always be feasible to run it on student laptops, or at least not during class. An animation can be found here. Slides with an introduction to the Earth’s magnetic field can be found here.