Mathematics – Logic
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmgp51b..06t&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #GP51B-06
Mathematics
Logic
1510 Dynamo: Theories And Simulations, 1513 Geomagnetic Excursions, 1560 Time Variations: Secular And Longer, 4910 Astronomical Forcing
Scientific paper
Paleomagnetic directions, relative paleointensities (RPI) and authigenic 10Be/9Be ratio were measured along sedimentary clayey-carbonate sequences in high accumulation rate sites of the Portuguese margin (0-400 ka BP) and West-Equatorial Pacific (600-1300 ka BP. Series of high and low RPI features are placed on the chronological scale using C-14 ages, using correlations with of delta O-18 records with the Greenland ice cores and SPECMAP records, and using the ages of polarity reversals. During the time intervals of dramatically low RPI anomalous paleodirections document excursions or polarity reversals. Significant peaks of the authigenic 10Be/9Be ratio point in stratigraphic layers recording all low RPI phases. Plotted against RPI data the 10Be/9Be ratios statistically follow the expected power law (Elsasser et al. ,1958 and Lal, 1988), which strongly establishes the unique and direct link between the recorded cosmogenic enhancement and dipole moment loss, allowing us to univocally interpret our 10Be/9Be ratio and RPI records in terms of geomagnetic dipole moment lows and highs (DML and DMH) alternation. delta O-18 records of the same cores (e.g. Abreu et al. 2004), provide the frame to interpret dipole moment variations in a paleoclimatic context within strict stratigraphic terms. We note that most DML of the last 400 ka fall in the end of interglacial stages, while DMH are rather related with full glacials. We then confirm this coincidence, though whithout strict stratigraphic control, by comparing the SINT-800 curve (Guyodo and Valet, 1999) and the S. E. Pacific near Sea Floor mag. record (Gee et al., 2000), with the highest resolution 18O record yet available (Bassinot et al. 1994). Complex Wavelet analyses using modulus and phase reveal that the geomagnetic moment proxy records contain a maximum power for periods between 30 and 100 ka. DML do not occur in any fixed eccentricity context, but several DML fall at the time of obliquity minima. The comparison of phases of the SINT-800 and Indian Ocean 18O records, at the 100 ka period, indicates that the ice volume fluctuations lead the geomagnetic moment fluctuations. These observations shed the light on mechanical couplings via Earth's rotation rate and/or orbital changes : 1) Alternations of ice accretion/melting at high and mid-latitude may have resulted in acceleration/deceleration of the Earth's rotation (Doake, 1977), although the mass of the 130 m equivalent sea level only represents 7 ppm of the Earth mass. However, acceleration/braking effects generated by tides friction on large/reduced continental platform at low/high sea level conditions (in glacial/interglacial conditions resp.)may have contribute. A coupling between Earth's rotation and geomagnetic regime was suggested for the 20th century (Courtillot and Le Mouel, 1984; Jing, 1992). An alternative - or complementary- explanation can be envisaged: lots of DML occured at the time of low obliquity, i.e. at the time of low angle precession, (rejoining Fuller's (2006)observation and re-introducing the long standing debate about possible forcing by astronomical precession on the geodynamo (Malkus, 1963,1968, Rochester, 1976). It has to be emphasized that because deglaciation are explained by maximum summer insolation of the Northern hemisphere (i.e. at high obliquity), dipole lows occurring at low obliquity, would logically lagg the deglaciation by obliquity period (20.5 ka), and thus occur near the end of interglacials.
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