ASYMMETRY IN THE REVERSAL RATE BEFORE AND AFTER THE CRETACEOUS NORMAL POLARITY SUPERCHRON

dc.contributor.authorMcFadden P.L.
dc.contributor.authorMerrill R.T.
dc.date.accessioned2020-12-14T10:49:47Z
dc.date.available2020-12-14T10:49:47Z
dc.date.issued1997
dc.description.abstractThe geomagnetic reversal chronology shows a decreasing reversal rate, λ, from about 160 Ma to about 118 Ma, a cessation in the reversal process (the Cretaceous Normal Polarity Superchron) until about 83 Ma, and then an increasing λ until recent times. Visually, the rate of decrease in λ leading into the superchron appears larger than the rate of increase in λ following the superchron. Statistical tests developed here confirm the visual perception of an asymmetry in the rate of change in λ. This asymmetry could be caused by a relatively rapid breakdown of D'', with thermal energy being advected away followed by a slower thickening of the layer through thermal conduction. However, in the absence of good thermal models as to how different core-mantle boundary conditions affect the geodynamo there are probably many apparently viable speculations as to the origin of the observed rate asymmetry.
dc.identifierhttps://elibrary.ru/item.asp?id=267760
dc.identifier.citationEarth and Planetary Science Letters, 1997, , 1, 43-47
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/20781
dc.subjectDYNAMOS
dc.subjectREVERSALS
dc.subjectCORE-MANTLE BOUNDARY
dc.subjectPALEOMAGNETISM
dc.titleASYMMETRY IN THE REVERSAL RATE BEFORE AND AFTER THE CRETACEOUS NORMAL POLARITY SUPERCHRON
dc.typeСтатья

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