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Amit and Olson (2015) proposed that the extreme variability in the recorded geomagnetic reversal frequency, from hyper-reversing periods to superchrons, may be explained by lower mantle piles with a fixed lateral pattern but time-dependent height.
The Frz two-component system regulates the cell reversal frequency, and frz mutants only rarely reverse (Blackhart and Zusman, 1985).
In contrast, the dynamo model with time-dependent CMB heat flux shows larger reversal frequency fluctuations including superchrons and rather hyper-reversing periods.
For example, we have shown that the Frz signal transduction pathway regulates both vegetative swarming and developmental aggregation by controlling the reversal frequency of cells.
Higher air inlet velocity, staggered cell arrangement or a periodic reversal airflow of high reversal frequency results in a more uniform temperature distribution in the module.
The reversal frequency increases approximately linearly beyond onset.
Figure 10 shows comparison of the reversal frequency of the dynamo models of Olson et al. (2013) with the observed paleomagnetic reversal frequency record (Gradstein et al. 2012).
The dependence of the reversal frequency on the heterogeneity amplitude is not trivial.
One direct consequence of the results of the reversal frequency studies is the possibility to invert the record of paleomagnetic reversal frequency (Gradstein et al. 2012) for time-dependent core energetics.
They show that numerical dynamo with time-dependent CMB heat flux can explain the history of geomagnetic reversal frequency.
The dynamo model with fixed CMB heat flux is characterized by weaker temporal variability in reversal frequency.
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