80 research outputs found
Paleomagnetic record of basaltic volcanism from Pukaki and Onepoto maar lake cores, Auckland Volcanic Field, New Zealand
The Auckland Volcanic Field contains several maars that formed after the last interglacial and subsequently filled with sediment. Two of these maars, Pukaki and Onepoto, were recently cored as part of the Auckland Maar Lakes Project. The tephra stratigraphy of the cores indicates that sediment accumulated relatively slowly in both maars until the Holocene when ocean waters breached the craters and they filled up quite rapidly. Using u-channels, we collected 23 m of pre-Holocene lacustrine sediment from the Pukaki 1-01 core and 15 m from the Onepoto core. Paleomagnetic measurements were performed on these at the University of California, Davis. Environmental magnetic records from both cores provide insights in particular about the eruptive history of the Auckland Volcanic Field. The lack of a tephrostratigraphic control in the lower portion of the cores, and the lack of similar trends in the magnetic parameters, prevented a complete core correlation. The main finding is that local basaltic tephra layers visible in the cores show up as spikes in the concentration dependent magnetic parameters, suggesting that other spikes represent tephra layers that are not as easily discerned
Paleomagnetic record of basaltic volcanism from Pukaki and Onepoto maar lake cores, Auckland Volcanic Field, New Zealand
The Auckland Volcanic Field contains several maars that formed after the last interglacial
and subsequently filled with sediment. Two of these maars, Pukaki and Onepoto, were
recently cored as part of the Auckland Maar Lakes Project. The tephra stratigraphy of the
cores indicates that sediment accumulated relatively slowly in both maars until the
Holocene when ocean waters breached the craters and they filled up quite rapidly. Using u-channels, we collected 23 m of pre-Holocene lacustrine sediment from the Pukaki 1-01 core and 15 m from the Onepoto core. Paleomagnetic measurements were performed on
these at the University of California, Davis. Environmental magnetic records from both cores provide insights in particular about the eruptive history of the Auckland Volcanic Field. The lack of a tephrostratigraphic control in the lower portion of the cores, and the lack of similar trends in the magnetic parameters, prevented a complete core correlation.
The main finding is that local basaltic tephra layers visible in the cores show up as spikes in the concentration dependent magnetic parameters, suggesting that other spikes represent tephra layers that are not as easily discerned
Data report: paleomagnetic and environmental magnetic properties of sediments from site 1202 (kuroshio current)
We present paleomagnetic and mineral magnetic results from ocean
sediments from the southern Okinawa Trough (west Pacific). We obtained
samples from two holes from Ocean Drilling Program Site 1202
and determined the natural remanent magnetization, magnetic susceptibility,
anhysteretic remanent magnetization (ARM), hysteresis properties,
and thermomagnetic behavior. Hole 1202A was studied between
100 and 120 meters below seafloor (mbsf) and Hole 1202B between 0
and 140 mbsf, both at 1-cm resolution. Hysteresis properties and thermomagnetic
behavior were measured on selected samples. The measurements
show a stable magnetization carried by pseudo-singledomain-
sized low-titanium magnetite. Magnetic inclinations are predominantly
positive and record the Brunhes (C1n) normal polarity
chron. Susceptibility and ARM, as well as the environmentally significant
rock magnetic ratios (ARM/k and ARM30 mT/ARM0 mT), reflect
changes in sediment input from Taiwan and the East China Sea continental
shelf changes in the path of the Kuroshio Current and changes
in climatic conditions
Reversal-field memory in magnetic hysteresis
We report results demonstrating a singularity in the hysteresis of magnetic
materials, the reversal-field memory effect. This effect creates a
nonanalyticity in the magnetization curves at a particular point related to the
history of the sample. The microscopic origin of the effect is associated with
a local spin-reversal symmetry of the underlying Hamiltonian. We show that the
presence or absence of reversal-field memory distinguishes two widely studied
models of spin glasses (random magnets).Comment: 3 pages, 5 figures. Proceedings of "2002 MMM Conferece", Tampa, F
Reversal-Field Memory in the Hysteresis of Spin Glasses
We report a novel singularity in the hysteresis of spin glasses, the
reversal-field memory effect, which creates a non-analyticity in the
magnetization curves at a particular point related to the history of the
sample. The origin of the effect is due to the existence of a macroscopic
number of "symmetric clusters" of spins associated with a local spin-reversal
symmetry of the Hamiltonian. We use First Order Reversal Curve (FORC) diagrams
to characterize the effect and compare to experimental results on thin magnetic
films. We contrast our results on spin glasses to random magnets and show that
the FORC technique is an effective "magnetic fingerprinting" tool.Comment: 4 pages, 6 figure
Preliminary Integrated Chronostratigraphy of the AND-2A Core, ANDRILL Southern McMurdo Sound Project, Antarctica
We use all available chronostratigraphic constraints – biostratigraphy, magnetostratigraphy,
radioisotopic dates, strontium-isotope stratigraphy, and correlation of compositional and physical properties
to well-dated global or regional records – to construct a preliminary age model for ANDRILL SMS Project’s
AND-2A drillcore (77°45.488’S, 165°16.605’E, 383.57 m water depth). These diverse chronostratigraphic
constraints are consistent with each other and are distributed throughout the 1138.54 m-thick section,
resulting in a well-constrained age model. The sedimentary succession comprises a thick early and middle
Miocene section below 224.82 mbsf and a condensed middle/late Miocene to Recent section above
this. The youngest sediments are Brunhes age (<0.781 Ma), as confirmed by a radioisotopic age of
0.691±0.049 Ma at 10.23 mbsf and the occurrence of sediments that have normal magnetic polarity down
to ~31.1 mbsf, which is interpreted to be the Brunhes/Matuyama reversal (0.781 Ma). The upper section
is punctuated by disconformities resulting from both discontinuous deposition and periods of extensive
erosion typical of sedimentary environments at the margin of a dynamic ice sheet. Additional breaks in
the section may be due to the influence of tectonic processes. The age model incorporates several major
hiatuses but their precise depths are still somewhat uncertain, as there are a large number of erosional
surfaces identified within the stratigraphic section. One or more hiatuses, which represent a total 7 to 8
million years of time missing from the sedimentary record, occur between about 50 mbsf and the base of
Lithostratigraphic Unit (LSU) 3 at 122.86 mbsf. Similarly, between about 145 mbsf and the base of LSU
4 at 224.82 mbsf, one or more hiatuses occur on which another 2 to 3 million years of the sedimentary
record is missing. Support for the presence of these hiatuses comes from a diatom assemblage that
constrains the age of the core from 44 to 50 mbsf to 2.06-2.84 Ma, two radioisotopic dates (11.4 Ma)
and a Sr‑isotope date (11.7 Ma) that indicate the interval from 127 to 145 mbsf was deposited between
11.4 and 11.7 Ma, and three diatom occurrence datums from between 225.38 and 278.55 mbsf that
constrain the age of this upper part of Lithostratigraphic Unit (LSU) 5 to 14.29 - 15.89 Ma. Below the
boundary between LSU 5 and 6 sedimentation was relatively continuous and rapid and the age model is
well-constrained by 9 diatom datums, seven 40Ar-39Ar dates, one Sr-isotope date, and 19 magnetozones.
Even so, short hiatuses (less than a few hundred thousand years) undoubtedly occur but are beyond
the resolution of current chronostratigraphic age constraints. Diatom first and last occurrence datums
provide particularly good age control from the top of LSU 6 down to 771.5 mbsf (in LSU 10), where
the First Occurrence (FO) of Thalassiosira praefraga (18.85 Ma) is observed. The diatom datum ages
are supported by radioisotopic dates of 17.30±0.31 Ma at 640.14 mbsf (in LSU 9) and 18.15±0.35 and
17.93±0.40 Ma for samples from 709.15 and 709.18 mbsf (in LSU 10), respectively, and 18.71±0.33 Ma
for a sample from 831.67 mbsf (in LSU 11). The sediments from 783.69 mbsf to the base of the hole
comprise two thick normal polarity magnetozones that bound a thinner reversed polarity magnetozone
(958.59 - 985.64 mbsf). This polarity sequence most likely encompasses Chrons C5En, C5Er, and C6n
(18.056 - 19.772 Ma or slightly older given uncertainties in this section of the geomagnetic polarity
timescale), but could be also be Chrons C6n, C6r, and C6An.1n (18.748 - 20.213 Ma). Either polarity
sequence is compatible with the 40Ar–39Ar age of 20.01±0.35 Ma obtained from single-grain analyses of
alkali feldspar from a tephra sample from a depth of 1093.02 mbsf, although the younger interpretation
allows a better fit with chronostratigraphic data up-core. Given this age model, the mean sedimentation
rate is about 18 cm/k.y. from the top of LSU 6 to the base of the hole.Published221-2202.2. Laboratorio di paleomagnetismoN/A or not JCRreserve
An abrupt weakening of the subpolar gyre as trigger of Little Ice Age-type episodes
We investigate the mechanism of a decadal-scale weakening shift in the strength of the subpolar gyre (SPG) that is found in one among three last millennium simulations with a state-of-the-art Earth system model. The SPG shift triggers multicentennial anomalies in the North Atlantic climate driven by long-lasting internal feedbacks relating anomalous oceanic and atmospheric circulation, sea ice extent, and upper-ocean salinity in the Labrador Sea. Yet changes throughout or after the shift are not associated with a persistent weakening of the Atlantic Meridional Overturning Circulation or shifts in the North Atlantic Oscillation. The anomalous climate state of the North Atlantic simulated after the shift agrees well with climate reconstructions from within the area, which describe a transition between a stronger and weaker SPG during the relatively warm medieval climate and the cold Little Ice Age respectively. However, model and data differ in the timing of the onset. The simulated SPG shift is caused by a rapid increase in the freshwater export from the Arctic and associated freshening in the upper Labrador Sea. Such freshwater anomaly relates to prominent thickening of the Arctic sea ice, following the cluster of relatively small-magnitude volcanic eruptions by 1600 CE. Sensitivity experiments without volcanic forcing can nonetheless produce similar abrupt events; a necessary causal link between the volcanic cluster and the SPG shift can therefore be excluded. Instead, preconditioning by internal variability explains discrepancies in the timing between the simulated SPG shift and the reconstructed estimates for the Little Ice Age onset
The Sariçiçek Howardite Fall in Turkey: Source Crater of HED Meteorites on Vesta and İmpact Risk of Vestoids
The Sariçiçek howardite meteorite shower consisting of 343 documented stones
occurred on 2 September 2015 in Turkey and is the first documented howardite fall. Cosmogenic
isotopes show that Sariçiçek experienced a complex cosmic ray exposure history, exposed during
~12–14 Ma in a regolith near the surface of a parent asteroid, and that an ~1 m sized meteoroid
was launched by an impact 22 ± 2 Ma ago to Earth (as did one third of all HED meteorites). SIMS
dating of zircon and baddeleyite yielded 4550.4 ± 2.5 Ma and 4553 ± 8.8 Ma crystallization ages
for the basaltic magma clasts. The apatite U-Pb age of 4525 ± 17 Ma, K-Ar age of ~3.9 Ga, and
the U,Th-He ages of 1.8 ± 0.7 and 2.6 ± 0.3 Ga are interpreted to represent thermal metamorphic
and impact-related resetting ages, respectively. Petrographic, geochemical and O-, Cr- and Tiisotopic
studies confirm that Sariçiçek belongs to the normal clan of HED meteorites. Petrographic
observations and analysis of organic material indicate a small portion of carbonaceous chondrite
material in the Sariçiçek regolith and organic contamination of the meteorite after a few days on
soil. Video observations of the fall show an atmospheric entry at 17.3 ± 0.8 kms-1 from NW,
fragmentations at 37, 33, 31 and 27 km altitude, and provide a pre-atmospheric orbit that is the
first dynamical link between the normal HED meteorite clan and the inner Main Belt. Spectral data
indicate the similarity of Sariçiçek with the Vesta asteroid family (V-class) spectra, a group of
asteroids stretching to delivery resonances, which includes (4) Vesta. Dynamical modeling of
meteoroid delivery to Earth shows that the complete disruption of a ~1 km sized Vesta family
asteroid or a ~10 km sized impact crater on Vesta is required to provide sufficient meteoroids ≤4
m in size to account for the influx of meteorites from this HED clan. The 16.7 km diameter Antonia
impact crater on Vesta was formed on terrain of the same age as given by the 4He retention age of
Sariçiçek. Lunar scaling for crater production to crater counts of its ejecta blanket show it was
formed ~22 Ma ago
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