The influence of water on melting of mantle peridotite   总被引：47，自引：8，他引：39  

Glenn A. Gaetani  Timothy L. Grove 《Contributions to Mineralogy and Petrology》1998,131(4):323-346

This experimental study examines the effects of variable concentrations of dissolved H₂O on the compositions of silicate melts and their coexisting mineral assemblage of olivine + orthopyroxene ± clinopyroxene ± spinel ± garnet. Experiments were performed at pressures of 1.2 to 2.0 GPa and temperatures of 1100 to 1345 °C, with up to ∼12 wt% H₂O dissolved in the liquid. The effects of increasing the concentration of dissolved H₂O on the major element compositions of melts in equilibrium with a spinel lherzolite mineral assemblage are to decrease the concentrations of SiO₂, FeO, MgO, and CaO. The concentration of Al₂O₃ is unaffected. The lower SiO₂ contents of the hydrous melts result from an increase in the activity coefficient for SiO₂ with increasing dissolved H₂O. The lower concentrations of FeO and MgO result from the lower temperatures at which H₂O-bearing melts coexist with mantle minerals as compared to anhydrous melts. These compositional changes produce an elevated SiO₂/(MgO + FeO) ratio in hydrous peridotite partial melts, making them relatively SiO₂ rich when compared to anhydrous melts on a volatile-free basis. Hydrous peridotite melting reactions are affected primarily by the lowered mantle solidus. Temperature-induced compositional variations in coexisting pyroxenes lower the proportion of clinopyroxene entering the melt relative to orthopyroxene. Isobaric batch melting calculations indicate that fluid-undersaturated peridotite melting is characterized by significantly lower melt productivity than anhydrous peridotite melting, and that the peridotite melting process in subduction zones is strongly influenced by the composition of the H₂O-rich component introduced into the mantle wedge from the subducted slab. Received: 7 April 1997 / Accepted: 9 January 1998  相似文献   

Looking Down the Light Cone: Can Deep Redshift Surveys Alone Measure the Power Spectrum?     

Andrew A. de Lai  & Glenn D. Starkman 《Monthly notices of the Royal Astronomical Society》1998,299(4):977-984

We analyse the window functions for the spherical harmonic mode estimators of all-sky, volume-limited surveys, considering evolutionary effects along the past light-cone which include the deviation of the distance scale from a linear relationship with redshift, linear peculiar velocity corrections, and linear evolution of the density perturbations. The spherical harmonic basis functions are considered, because they correspond most closely to the symmetries of typical survey geometries and of the light-cone effects we consider. Our results show substantial broadening of the windows over that expected by ignoring light-cone effects, indicating the difficulty of measuring the power spectrum independently from cosmology. We suggest that because of light-cone effects, deep redshift surveys should be analysed either in conjunction with CMBR data which determines the cosmological parameters, or by using a Bayesian likelihood scheme in which varying cosmological parameters and a simple parametrization of the primordial power spectrum are assumed as the priors, so that observed data can be mapped from redshift to real space. The derived power spectrum can then be compared with underlying models of fluctuation generation and growth in structure formation to evaluate both these models and the cosmological priors.  相似文献   

Relationship between subcellular cadmium distribution in prey and cadmium trophic transfer to a predator   总被引：1，自引：0，他引：1  

William G. Wallace  Glenn R. Lopez 《Estuaries and Coasts》1996,19(4):923-930

We tested the hypothesis that exposure-related alterations in the subcellular Cd distribution in prey relate to changes in Cd absorption by a predator. Oligochaete worms,Limnodrilus hoffmeisteri were exposed for 1 wk or 6 wk to 0.5 μg Cd 1^?1, 47 μg Cd 1^?1, or 140 μg Cd 1^?1 (including¹⁰⁹Cd as a tracer) and relationships between oligochaete subcellular Cd distribution and Cd absorption by a predator, the grass shrimp (Palaemonetes pugio), were determined. Concentration and duration of Cd exposure had direct effects on oligochaete subcellular Cd distribution. Changes in oligochaete subcellular Cd distribution were characterized by increases in both the amount and proportion of Cd bound to the cytosolic fraction. The induction of Cd-binding proteins (e.g., metallothioneins) were suspected to be responsible for these changes. We found 1∶1 relationships between the amount and percentage of Cd in oligochaete cytosol and the amount and percentage of Cd adsorbed by shrimp. These results demonstrate that only metal bound to the soluble fraction of prey is available to higher trophic levels, and that factors influencing subcellular metal distribution in prey will directly alter metal trophic transfer to predators.  相似文献   

Particle trajectories and simple models of transport in coherent vortices     

William K. Dewar  Glenn R. Flierl 《Dynamics of Atmospheres and Oceans》1985,9(3):215-252

The particle trajectories and transport effects of coherent vortices are computed and a number of advection and diffusion experiments using a time-dependent dynamical ring model are analyzed. Several features of the tracer distributions in the numerical solutions are similar to features noted in sea surface temperature images of Gulf Stream rings and are discussed from the point of view of the model. Comparisons between tracer distributions computed using the dynamic ring model and several purely kinematic ring representations demonstrate that most of the important features of ring transport are not altered by slow dynamical evolution. Loss rates from the ring trapped zone are also estimated, which permits calculation of cross-Gulf Stream chemical and biological fluxes due to ring formation. We demonstrate that the salinoty flux to the Slope Water caused by rings is comparable to that caused by the atmosphere.The transport of passive scalars produced by a series of rings moving through a channel (modeling the Slope Water region between the Shelf and the Gulf Stream) is computed. It is found that transport in the along-channel direction is enhanced by the presence of rings and is characterized by Nusselt numbers of 0(30–40). Cross-channel fluxes, while enhanced, are somewhat less affected by rings, and are generally characterized by Nusselt numbers < 0(10). The combined effect of rings on the Slope is seen to make it an anisotropic medium, with along-channel transport one to two orders of magnitude more efficient than cross-channel transport. The implications with respect to the Slope are discussed.  相似文献   

Gaseous Behavior of TCE Overlying a Contaminated Aquifer     

Donn L. Marrin  Glenn M. Thompson 《Ground water》1987,25(1):21-27

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Theoretical estimates of the westward drift     

Glenn R. Ierley 《Physics of the Earth and Planetary Interiors》1984,36(1):43-48

Virtually all dynamo models may be expected to give rise to a permanent differential rotation between mantle and core. Weak conductivity in the mantle permits small leakage currents which couple to the radial component of the magnetic field, producing a Lorentz torque. Mechanical equilibrium is achieved when a zero net torque is established at a critical rotation rate. An estimate of the drift is determined easily given the magnetic field structure predicted by any dynamo model. The result for the drift rate at the core-mantle interface along the equator is given by the product of three factors The first of these is a geometrical factor which depends only on the structural character of the field. For a variety of model fields, this factor ranges from 16 to 35. The second factor is the ratio of r.m.s. toroidal to poloidal field. This ratio is an (implicitly) adjustable parameter of both α² and α-ω dynamos, and is a measure of the relative efficiency of the generation process for each component. The third (dimensional) term is the ratio of core magnetic diffusivity to core radius, 10^?4 cm s^?1.The result is essentially independent of the value of mantle diffusivity and its effective depth. The sign of the result may be positive or negative. For α² dynamos a westward drift is produced by choosing α > 0 in the Northern Hemisphere, which constitutes a dynamical assertion about the dynamo process. For an r.m.s. toroidal field of the order of 15 Gs, based on fairly general considerations, a drift rate comparable to observation is expected.  相似文献   

Central Arctic Ocean response to Pleistocene Earth-orbital variations     

Robin F. Boyd  David L. Clark  Glenn Jones  W.F. Ruddiman  A. McIntyre  N.G. Pisias 《Quaternary Research》1984,22(1):121-128

Three central Arctic Ocean sediment cores were sampled for percentage carbonate, number of foraminifera, and texture. These three parameters were used in spectral analyses to test the idea that the ice-covered Arctic Ocean may respond to orbital forcing in a different manner than has been indicated for lower latitude ice-free oceans. The record for two of the cores represents approximately 1 my, and the record for the third, approximately 400,000 yr. The 100,000-yr frequency is well represented in all of the cores. A 40,000-yr frequency may be present, as well. An unexpected 70,000-yr frequency occurs in most of the spectra and may reflect nonlinear sedimentation rates or the combined effect of obliquity and eccentricity. The strong 100,000-yr signal confirms that, in spite of ice feedback, the Arctic Ocean has responded to orbital forcing in much the same manner as have ice-free oceans.  相似文献   

An aperture synthesis study of Saturn and its rings at 3.71-cm wavelength     

F.Peter Schloerb  Duane O. Muhleman  Glenn L. Berge 《Icarus》1979,39(2):232-250

We present aperture synthesis maps of the Saturn system at a wavelength of 3.71 cm. The data used to make the maps were obtained in May–June 1976 at the Owens Valley Radio Observatory on 13 interferometer baselines. The aperture synthesis maps contain few assumptions about the brightness structure of Saturn and the rings and, therefore, may be used to check previous model-fitting results as well as search for new unmodeled features. Generally, the maps confirm the previous model-fitting results. An exception to this is that the brightness temperature of the planet that is implied by the maps is about 4% less than that deduced from model fitting. The likely explanation of this discrepancy is that random errors on the phase of the visibility function have led to an underestimate of the planet brightness temperature in the map. Maps of the residuals to the model fits have shown that the position of Saturn given in the American Ephemeris and Nautical Almanac may be in error by about 0.25 arcsec. Maps of the residuals to model fits including a position offset show that no new features of the Saturn brightness structure are required to match the present data. In particular, no azimuthal variations in the brightness temperature of the rings were detected.  相似文献   

Three distinct regimes of volcanic tremor associated with the eruption of Shishaldin Volcano, Alaska 1999     

Glenn Thompson  Stephen R. McNutt  Guy Tytgat 《Bulletin of Volcanology》2002,64(8):535-547

Tremor signals associated with the eruption of Shishaldin Volcano on 19 and 23 April 1999 were the strongest recorded anywhere in the Aleutian Arc by the Alaska Volcano Observatory (AVO) in its 10-year history. Reduced displacements (D_R) reached 23 cm² on 19 April and 43 cm² on 23 April. During the activity, D_R and spectral data with a frequency resolution of 0.1 Hz were computed and put on the World Wide Web every 10 min. These data are analyzed here. The general temporal patterns of seismicity of these eruption events were similar, but the eruptions and their effects quite different. The 19 April event is known to have culminated in a sub-Plinian phase, which ejected ash to an altitude of 16 km. Despite higher amplitudes and the largest hotspot from satellite data, the 23 April event produced little ash reaching only 6 km altitude. For several hours prior to the sub-Plinian phase on 19 April, tremor with a peak frequency of 1.3 Hz intensified. During the sub-Plinian phase the peak frequency increased to 4-8 Hz. However, in 15 h after the eruption, three episodes of stronger tremor occurred with a lower 1.0-Hz peak, alternating with weaker tremor with a 1.3-Hz peak. These transitions correspond to D_R=~8 cm². Although these strong tremor episodes produced higher D_R levels than the sub-Plinian phase, data from a pressure sensor show that only strong Strombolian explosions occurred. The suite of observations suggests three distinct tremor regimes that may correspond to slug flow, bubbly flow, and sustained strong eruptions, or a cyclic change in source parameters (e.g., geometry, sound speed, or ascent rate). This behavior occurred at Shishaldin only during the April 1999 sequence, and we are not aware of similar behavior at other volcanoes.  相似文献   

Aspartic acid racemization in teeth from Ketef Hinnom,a late Holocene burial cave in Jerusalem: Evidence for reuse     

M. Sinibaldi  Glenn A. Goodfriend  Gabriel Barkay  S. Marchese  Emanuel Gil-av 《Geoarchaeology》1999,14(5):441-454

The Ketef Hinnom tombs, lying just outside the walls of the old city of Jerusalem, were carved out of bedrock during the 7th–5th century B.C. Several artefacts dating to the Late Hellenistic Period (ca. 100 B.C.) have also been found within the tombs. Aspartic acid (Asp) racemization in 31 samples of human tooth dentine from these tombs was analyzed in order to evaluate the possible reuse of the tombs during this later period. A range of D/L Asp values was found: a group with values averaging 0.062 and another group averaging 0.043. These D/L values are close to those expected for the two archeological age groups as calculated from (1) the kinetics of Asp racemization as established from experimental studies at higher temperatures and in vivo racemization rates, and (2) the effective annual temperature in the tombs, as measured using the Pallman method. These results thus support the later reuse of the tombs for burials. Several factors contribute to the accuracy of Asp racemization dating, including the age of the individual at death, uncertainties concerning Asp racemization kinetics, and effects of temperature history. © 1999 John Wiley & Sons, Inc.  相似文献