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Paleointensity behavior in Barremian–Cenomanian (Cretaceous)

Authors: A. Yu. Kurazhkovskii;

Paleointensity behavior in Barremian–Cenomanian (Cretaceous)

Abstract

Fragmentary knowledge on geomagnetic field intensity in Barremian–Cenomanian stageobtained from sediment rocks is summarized. Three types of periodical variations arerevealed in the paleointensity behavior. The types differ by the amplitude and duration(tens of millennia, hundreds of millennia and more than million years). It is foundthat in all the magnetopolar intervals an alternating of quiet and burst-like regimes ofmagnetic field generation is observed, the regimes differing by the oscillation amplitudeand mean values of the paleointensity. It is demonstrated that the mean values of thepaleointensity of quiet regimes of geomagnetic field generation were (0.5–0.8) H

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average
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