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Case G Reversal
Case H Reversal
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Simulations—Case H Reversal

The tomographic simulation also produced two reversals, the first of which is shown here (zoom to enlarge). On the left (a & c), the dipole moment (normalized by Earth -radius cubed) and the true-dipole path are plotted versus time step (100 yr), each fifth step between 1680 and 1725 corresponding to letters F-O. On the right are plotted (b) axial and inclined dipole intensity, total-field intensity (left axis) and reversal angle (right axis) and (d) VGP path for the site indicated by the star. The 2.5 kyr duration, as defined by the dipole intensity, is similar to the previous example, but the non-axial-dipole field is much more active (see next figure), giving rise to greater variation in transition signature over the globe. The prominent excursion in direction (H-I-J-K) after the initial switch in polarity reminds one of the Steens Mountain reversal record. (Click to enlarge)


The onset of the reversal was marked by the rapid growth of two enormous nondipole-field flux patches of opposite sign. These reversed the field at high northern latitudes, and temporarily as well at equatorial latitudes between longitudes 90 and 300 east.


Links: Case G Reversal | VGP Preference? | Case C Excursion | References | Simulations


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