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201.
We present high-precision Mg isotope data for most classes of basaltic meteorites including eucrites, mesosiderite silicate clasts, angrites and the ungrouped Northwest Africa (NWA) 2976 measured by pseudo-high-resolution multiple-collector inductively coupled plasma mass spectrometry and utilising improved techniques for chemical purification of Mg. With the exception of the angrites Angra dos Reis, Lewis Cliff (LEW) 86010, NWA 1296 and NWA 2999 and the diogenite Bilanga, which have either been shown to have young ages by other dating techniques or have low Al/Mg ratios, all bulk samples of basaltic meteorites have 26Mg excesses (δ26Mg∗=+0.0135 to +0.0392‰). The 26Mg excesses cannot be explained by analytical artefacts, cosmogenic effects or heterogeneity of initial 26Al/27Al, Al/Mg ratios or Mg isotopes in asteroidal parent bodies as compared to Earth or chondrites. The 26Mg excesses record asteroidal melting and formation of basaltic magmas with super-chondritic Al/Mg and confirm that radioactive decay of short-lived 26Al was the primary heat source that melted planetesimals. Model 26Al-26Mg ages for magmatism on the eucrite/mesosiderite, angrite and NWA 2976 parent bodies are 2.6-3.2, 3.9-4.1 and 3.5 Myr, respectively, after formation of calcium-aluminium-rich inclusions (CAIs). However, the validity of these model ages depends on whether the elevated Al/Mg ratios of basaltic meteorites result from magma ocean evolution on asteroids through fractional crystallisation or directly during partial melting. Mineral isochrons for the angrites Sahara (Sah) 99555 and D’Orbigny, and NWA 2976, yield ages of and , respectively, after CAI formation. Both isochrons have elevated initial δ26Mg∗ values. Given the brecciated and equilibrated texture of NWA 2976 it is probable that its isochron age and elevated initial δ26Mg∗(+0.0175±0.0034‰) reflects thermal resetting during an impact event and slow cooling on its parent body. However, in the case of the angrites the marginally elevated initial δ26Mg∗(+0.0068±0.0058‰) may reflect either δ26Mg∗ ingrowth in a magma ocean prior to eruption and crystallisation or in an older igneous protolith with super-chondritic Al/Mg prior to impact melting and crystallisation of these angrites, or partial internal re-equilibration of Mg isotopes after crystallisation. 26Al-26Mg model ages and an olivine + pyroxene + whole rock isochron for the angrites Sah 99555 and D’Orbigny are in good agreement with age constraints from 53Mn-53Cr and 182Hf-182W short-lived chronometers, suggesting that the 26Al-26Mg feldspar-controlled isochron ages for these angrites may be compromised by the partial resetting of feldspar Mg isotope systematics. Even when age constraints from the 26Al-26Mg angrite model ages or the mafic mineral + whole rock isochron are considered, the relative time difference between Sah 99555/D’Orbigny crystallisation and CAI formation cannot be reconciled with Pb-Pb ages for Sah 99555/D’Orbigny and CAIs, which are ca. 1.0 Myr too old (angrites) or too young (CAIs) for reasons that are not clear. This discrepancy might indicate that 26Al was markedly lower (ca. 40%) in the planetesimal- and planet-forming regions of the proto-planetary disc as compared to CAIs, or that CAI Pb-Pb ages may not accurately date CAI formation, which might be better dated by the 182Hf-182W and 26Al-26Mg chronometers as 4568.3±0.7 (Burkhardt et al., 2008) and (herein), respectively, when mapped onto an absolute timescale using Pb-Pb ages for angrites. 相似文献
202.
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204.
The stability of the Atlantic thermohaline circulation against meltwater input is investigated in a coupled ocean-atmosphere
general circulation model. The meltwater input to the Labrador Sea is increased linearly for 250 years to a maximum input
of 0.625 Sv and then reduced again to 0 (both instantaneously and linearly decreasing over 250 years). The resulting freshening
forces a shutdown of the formation of North Atlantic deepwater and a subsequent reversal of the thermohaline circulation of
the Atlantic, filling the deep Atlantic with Antarctic bottom water. The change in the overturning pattern causes a drastic
reduction of the Atlantic northward heat transport, resulting in a strong cooling with maximum amplitude over the northern
North Atlantic and a southward shift of the sea-ice margin in the Atlantic. Due to the increased meridional temperature gradient,
the intertropical convergence zone over the Atlantic is displaced southward and the westerlies in the Northern Hemisphere
gain strength. We identify four main feedbacks affecting the stability of the thermohaline circulation: the change in the
overturning circulation of the Atlantic leads to longer residence times of the surface water in high-northern latitudes, which
allows them to accumulate more precipitation and runoff from the continents. As a consequence the stratification in the North
Atlantic becomes more stable. This effect is further amplified by an enhanced northward atmospheric water vapour transport,
which increases the freshwater input into the North Atlantic. The reduced northward oceanic heat transport leads to colder
sea-surface temperatures and an intensification of the atmospheric cyclonic circulation over the Norwegian Sea. The associated
Ekman transports cause increased upwelling and increased freshwater export with the East Greenland Current. Both the cooling
and the wind-driven circulation changes largely compensate for the effects of the first two feedbacks. The wind-stress feedback
destabilizes modes without deep water formation in the North Atlantic, but has been neglected in almost all studies so far.
After the meltwater input stops, the North Atlantic deepwater formation resumed in all experiments and the meridional overturning
returned within 200 years to a conveyor belt pattern. This happened although the formation of North Atlantic deep water was
suppressed in one experiment for more than 300 years and the Atlantic overturning had settled into a circulation pattern with
Antarctic bottom water as the only source of deep water. It is a clear indication that cooling and wind-stress feedback are
more effective, at least in our model, than advection feedback and increased atmospheric water vapour transport. We conclude
that the conveyor belt-type thermohaline circulation seems to be much more stable than hitherto assumed from experiments with
simpler models.
Received 31 January 1996/Accepted 22 August 1996 相似文献
205.
Abstract. Cladocora caespitosa is a relatively common, colonial, symbiotic, scleractinian coral in the Mediterranean Sea. It inhabits a wide ecological range: hard and soft bottoms, shallow waters or depths to about 50m, calm water or sites exposed to strong currents and wave action. The present study compares the distribution of this coral at two sites, one shallow (3m — wave exposed) and one deeper (12m — soft bottom).
Different parameters including dry weight, volume, and skeletal growth rates were investigated. The polyp biomass, carbon content, and overall area of fully expanded polyps were also measured. Equations are given for the relationship of skeleton diameter to polyp tissue dry weight as well as skeleton diameter to the possible filter area of fully expanded polyps.
C. caespitosa harbors a rich community of vagile and sessile organisms within the skeleton. The cryptofauna was sorted to higher taxonomic levels and their biomass determined. Several highly significant linear relationship were found between skeleton dry weight, volume and cryptofauna biomass. Thus, the determination of colony volume allows the prediction of cryptofauna biomass.
The interstitial space is dominated by sponges - many of them borers - which erode the corallites close to the living tissue until they break off from the colony. At the deeper sampling site, 26% of all colonies are smaller than 2 cm and 48% are smaller than 5 cm. The fragmentation process is discussed with respect to reproduction. 相似文献
Different parameters including dry weight, volume, and skeletal growth rates were investigated. The polyp biomass, carbon content, and overall area of fully expanded polyps were also measured. Equations are given for the relationship of skeleton diameter to polyp tissue dry weight as well as skeleton diameter to the possible filter area of fully expanded polyps.
C. caespitosa harbors a rich community of vagile and sessile organisms within the skeleton. The cryptofauna was sorted to higher taxonomic levels and their biomass determined. Several highly significant linear relationship were found between skeleton dry weight, volume and cryptofauna biomass. Thus, the determination of colony volume allows the prediction of cryptofauna biomass.
The interstitial space is dominated by sponges - many of them borers - which erode the corallites close to the living tissue until they break off from the colony. At the deeper sampling site, 26% of all colonies are smaller than 2 cm and 48% are smaller than 5 cm. The fragmentation process is discussed with respect to reproduction. 相似文献