Geomagnetic moment instability between 0.6 and 1.3 Ma from cosmonuclide evidence

The reliability of paleomagnetic records as proxies of the geomagnetic field intensity is still a matter of controversy since volcanic materials hardly provide continuous records, and marine sediments are suspected to carry a remanence biased by post-depositional realignments and/or by overprints. Such long standing debate emphasizes the need for the development of methods independent from paleomagnetism to decipher geomagnetic intensity variations. High resolution measurements of authigenic (10)Be/(9)Be along with a detailed sedimentary record of directional and relative paleointensity variations evidence, over the 0.6-1.3 Ma time interval, frequent and recurrent excursions or short events in the late Matuyama and the early Brunhes epochs, among which two Brunhes-Matuyama reversal precursors and an intra-Jaramillo excursion. The results of this study confirm the idea of a highly unstable geomagnetic field as suggested by paleomagnetic evidences.

Keyword(s)

geomagnetic excursions and reversals, paleointensity, geomagnetic moment, authigenic (10)Be/(9)Be, cosmogenic isotope production, marine sedimentary archives

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Carcaillet JT, Thouveny N, Bourles DL (2003). Geomagnetic moment instability between 0.6 and 1.3 Ma from cosmonuclide evidence. Geophysical Research Letters. 30 (15). 5.1-5.4. https://doi.org/10.1029/2003GL017550, https://archimer.ifremer.fr/doc/00226/33708/

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