Radium and barium at GEOSECS stations in the Atlantic and Pacific     

L.H. Chan  J.M. Edmond  R.F. Stallard  W.S. Broecker  Y.C. Chung  R.F. Weiss  T.L. Ku 《Earth and Planetary Science Letters》1976,32(2):258-267

²²⁶Ra and Ba show a general linear correlation in the oceanic water column within the uncertainties of the data: the slope of the line is about 4.6 nanomoles (nmoles) Ra/mole Ba, the intercept being at about 4 nmoles Ba/kg. This demonstrates the usefulness of Ba as a “chemical analogue” of Ra. Box-model calculations indicate that the average deep-water excess of Ra over Ba should be about 10% relative to the surface. This is consistent with the observations outside the deep northeast Pacific. However, the uncertainties in the data are such that the regional variation in the primary input cannot be resolved. In the deep waters of the North Pacific there is in fact a large excess of Ra relative to Ba. The one detailed profile presently available (204) can be explained consistently by a simple vertical advection-diffusion model.  相似文献   

Fluxes of metals to a manganese nodule radiochemical,chemical, structural,and mineralogical studies     

Willard S. Moore  Teh-Lung Ku  J. Douglas Macdougall  Virginia Mee Burns  Roger Burns  Jack Dymond  Mitchel W. Lyle  David Z. Piper 《Earth and Planetary Science Letters》1981,52(1):151-171

Fluxes of metals to the top and bottom surfaces of a manganese nodule were determined by combining radiochemical (²³⁰Th,²³¹Pa,²³²Th,²³⁸U,²³⁴U) and detailed chemical data. The top of the nodule had been growing in its collected orientation at 4.7 mm Myr^?1 for at least 0.5 Myr and accreting Mn at 200 μg cm^?2 kyr^?1. The bottom of the nodule had been growing in its collected orientation at about 12 mm Myr^?1 for at least 0.3 Myr and accreting Mn at about 700 μg cm^?2 yr^?1. Although the top of the nodule was enriched in iron relative to the bottom, the nodule had been accreting Fe 50% faster on the bottom.²³²Th was also accumulating more rapidly in the bottom despite a 20-fold enrichment of²³⁰Th on the top.The distribution of alpha-emitting nuclides calculated from detailed radiochemical measurements matched closely the pattern revealed by 109-day exposures of alpha-sensitive film to the nodule. However, the shape and slope of the total alpha profile with depth into the nodule was affected strongly by²²⁶Ra and²²²Rn migrations making the alpha-track technique alone an inadequate method of measuring nodule growth rates.Diffusion of radium in the nodule may have been affected by diagenetic reactions which produce barite, phillipsite and todorokite within 1 mm of the nodule surface; however, our sampling interval was too broad to document the effect. We have not been able to resolve the importance of nodule diagenesis on the gross chemistry of the nodule.  相似文献   

Meridional distribution of²²⁶Ra in the eastern Pacific along GEOSECS cruise tracks     

T.L. Ku  C.A. Huh  P.S. Chen 《Earth and Planetary Science Letters》1980,49(2):293-308

We present the distribution of²²⁶Ra in eight vertical profiles from the eastern Pacific. The profiles are located along a meridional trend near 125°W, from 43°S to 29°N. Surface²²⁶Ra concentrations are about 7 dpm/100 kg, except for the two stations south of 30°S where the higher values are due to the Antarctic influence. Deep waters show a distinctive south-to-north increase in the²²⁶Ra content, from about 26 to 41 dpm/100 kg near the bottom. Unlike in the Atlantic and Antarctic Oceans, the effect of²²⁶Ra injection from bottom sediments is clearly discernible in the area. The presence of this primary²²⁶Ra can be traced up to at least 1–1.5 km above the ocean floor, making this part of the sea bed among the strongest source regions for the oceanic²²⁶Ra. Numerical solutions of a two-dimensional vertical advection-diffusion model applied to the deep (1.2–4 km)²²⁶Ra data give the following set of best fits: upwelling velocity(V_z) = 3.5m/yr, vertical eddy diffusivity(K_z) = 0.6cm²/s, horizontal (north-south) eddy diffusivity(K_y) = 1 × 10⁷cm²/s, and water-column regeneration flux of²²⁶Ra(J) = 3.3 × 10^?5dpmkg^?1yr^?1 as an upper limit. These parametric values are in general agreement with one-dimensional (vertical) model fits for the Ra-Ba system. However, consideration of²²⁶Ra balance leads us to suspect the appropriateness of describing the vertical exchange processes in the eastern Pacific with constantV_z and K_z. If future modeling is attempted, it may be preferable to treat the area as a diffusion-dominant mixing regime with depth-dependent diffusivities.  相似文献   

Radium and thorium isotopes in the surface waters of the East Pacific and coastal Southern California     

Kevin G. Knauss  Teh-Lung Ku  Willard S. Moore 《Earth and Planetary Science Letters》1978,39(2):235-249

A fiber extraction technique is used to concentrate Ra and Th isotopes from 1000 liters or more of seawater. Natural²²⁶Ra and²³⁴Th are used as yield tracers. In the equatorial Pacific the²²⁸Ra activity of surface water varies from 20 to 1 dpm/1000 kg and generally decreases away from continental shelf areas. Across the Peru Current System, this decrease is modeled as one-dimensional diffusion and indicates the possibility of two flow regimes with distinct characteristic mixing lengths and apparent eddy diffusivities of 10⁵ and 10⁷ cm²/s. The perturbing effects of advection and equatorial upwelling west of the Galapagos Islands are noted. Off the coast of Southern California a vertical²²⁸Ra distribution gives an apparent diffusivity of 1.6 cm²/s for the upper thermocline.²²⁶Ra concentrations near the coast appear to be higher than the open ocean values at comparable depths, which may reflect supply of this isotope from continental shelf sediments and/or upwelling. The insoluble daughter/soluble parent activity ratios²²⁸Th/²²⁸Ra and²³⁴Th/²³⁸U in the equatorial Pacific surface water display latitudinal trends which may be correlated with productivity variations. Near the coast of California these ratios reflect the differing oceanographic conditions north and south of Pt. Conception indicating a mean chemical removal time constant on the order of 4 months for Th and other highly reactive elements within the Southern California Bight. The²³²Th content of seawater sampled is less than 0.1 μg/1000 1; most of the published values for seawater²³²Th could well be too high. A comparison of the two methods of determining²²⁸Ra (via²²⁸Ac and via²²⁸Th) made on 64 seawater samples shows that the time delay required by the²²⁸Th method is more than compensated by its better analytical simplicity and precision.  相似文献   

A method for quantitative evaluation of carbonate dissolution in deep-sea sediments and its application to paleoceanographic reconstruction     

Teh-Lung Ku  Tadamichi Oba 《Quaternary Research》1978,10(1):112-129

A method is proposed by which the degree of attrition of the tests of certain foraminifera species, such as Globorotalia menardii and Globorotalia tumida, is used to “scale” the amount of CaCO₃ that has been dissolved from sediment. The scale is calibrated experimentally in the laboratory. The method has been applied to three calcareous cores from the Pacific and the Indian Oceans. It is shown that the original CaCO₃ contents in these cores were high (82–95%) and relatively uniform compared to the present down-core values. About 65 to 85% of the originally deposited CaCO₃ has been dissolved, corresponding to dissolution rates on the order of 0.1-0.3 moles/cm²/yr. These results indicate that appreciable solution could have occurred on sea floor rich in calcareous sediments and that the variation in CaCO₃ content in a core may have resulted largely from dissolution. The difference in the degree of solution between glacial and interglacial sediments in these cores is not so distinct, with ? 10% less intense dissolution during glacial times on the average. However, the dissolution minimum occurring around the late Wisconsin glaciation (10,000–20,000 yr B.P.) previously noted in several cores elsewhere is confirmed. At that time, near the site of core M70 PC-20 in the southwest Pacific, the $\text{CO}{}_3{}^{\mathrm{2?}}$ concentration of the bottom water is estimated to have been approximately 5% higher than the present value, and the calcite lysocline was about 300 m deeper. To evaluate possible variations in CaCO₃ deposition rate across the glacial-interglacial transitions requires precise age control, which the present study lacks.  相似文献   

Hydrogeochemical Anomalies in the Springs of the Chiayi Area in West-central Taiwan as Possible Precursors to Earthquakes   总被引：1，自引：0，他引：1  

S. R. Song  W. Y. Ku  Y. L. Chen  C. M. Liu  H. F. Chen  P. S. Chan  Y. G. Chen  T. F. Yang  C. H. Chen  T. K. Liu  M. Lee 《Pure and Applied Geophysics》2006,163(4):675-691

Water samples from both hot and artesian springs in Kuantzeling in west-central Taiwan have been collected on a regular basis from July 15, 1999 to the end of August 2001 to measure cation and anion concentrations as a tool to detect major earthquake precursors. The data identify chloride and sulfate ion anomalies few days prior to major quakes and lasting a few days afterward. These anomalies are characterized by increases in Cl^- concentrations from 34.9% to 41.2% and 71.5% to 138.1% as well as increases in SO₄^2- concentrations from 232.7% to 276.8% and 100.0% to 155.1% above the means in both hot and artesian springs. The occurrence of these anomalies is probably explained first as stress/strain-induced pressure changes in the subsurface water systems which then generate precursory limited geochemical discharges at the levels of subsurface reservoirs. Therefore, finally leading to the mixing of previously separated subsurface water bodies occurs. This suggests that the hot and artesian springs in the Kuantzeling area are possible ideal sites for recording strain changes serving well as earthquake precursors.  相似文献   

Circumstellar Shells of the Mass-Losing Asymptotic Giant Branch Stars: Limits for the Dust-Driven Winds     

Arñas Kučinskas 《Astrophysics and Space Science》1998,262(2):127-143

We investigated whether the radiation pressure on dust grains alone may account for driving winds in semiregular, irregular and non-variable AGB stars. A simple theoretical model is employed to calculate the limits for the radiatively driven winds and to compare theoretical predictions with observations. Present analysis indicates, that for most of the objects in the studied sample of 67 oxygen-rich and 40 carbon-rich mass-losing AGB stars radiation pressure on dust grains alone is not effective enough to drive the observed circumstellar outflows.  相似文献   

10Be distribution and uranium-series dating of salt samples from salt playae in the Chaidamu Basin,Qinghai, northwest China     

Liang Zhuocheng  Teh-Lung Ku 《中国地球化学学报》1987,6(3):257-263

The distributions of cosmogenic nuclide¹⁰Be in the upper and lower salt units from a core (36.4°N, 94.5°E) in the Chaidamu Basin, Qinghai, China have been measured by means of accelerator-mass spectrometer. The comparison of these¹⁰Be results measured on salt and detritus fractions shows that the geochemical behaviour of¹⁰Be is detritus-phile. In this area¹⁰Be influx is different in the past tens of thousands of years, which is suggested to be related to climatic fluctuations during late Pleistocene. It seems that¹⁰Be influx is higher in the humid climate environnent than in the dry climate environment. The²³⁰Th-age estimates of two salt units have been determined. The corrected ages of the lower unit show a climate shift from humid to dry at about 50 Ka ago in this area.  相似文献   

Growth of a manganese nodule from Peru Basin: A radiochemical anatomy     

J.L Reyss  N Lemaitre  T.L Ku  V Marchig  J.R Southon  D.E Nelson  J.S Vogel 《Geochimica et cosmochimica acta》1985,49(11):2401-2408

Attempts have been made to study the entire growth history of a manganese nodule from the northern part of Peru Basin in the Pacific using radiochemical profiles of ${}^{230}\text{Th}{}^{232}\text{Th}$, ${}^{227}\text{Th}{}^{230}\text{Th}$, and ${}^{10}\text{Be}{}^9\text{Be}$. Combined with the observations on Fe-Mn contents and textural variation, the radiochemical data indicate that the nodule grew more or less concentrically throughout most of its existence since it formed 1.5 my ago, receiving Mn from both bottom water and pore water. This condition appeared to have changed about 180 ky ago when the growth became asymmetric in that the top and bottom sides became fixed in their relative positions on the sea floor. Since then, the bottom side accreted with a fast rate of close to 200 mm/my, apparently fueled by the supply of diagenetically remobilized Mn in pore water from the sediment substrate. In the meantime, the top side accumulated at about 6 mm/my, a value which is in the normal range for deep-sea nodules having their Mn supplied from the hydrogenous source.  相似文献   

Transport ofBe andBe in the ocean     

P. Sharma  R. Mahannah  W.S. Moore  T.L. Ku  J.R. Southon   《Earth and Planetary Science Letters》1987,86(1)

Beryllium isotopes (¹⁰Be and⁹Be) have been measured in suspended particles of < 1 mm size collected by mid-water sediment traps deployed in the eastern Pacific at MANOP sites H (6°32′N, 92°50′W, water depth 3600 m) and M (8°50′N, 104°00′W, 3100 m). For comparison, surface sediments from box cores taken from the two sites were also studied. The concentrations of¹⁰Be and⁹Be in sediment-trap particles are about an order of magnitude smaller than those in the bottom sediments which contain about 8 × 10⁹ and 6 × 10¹⁶ atoms g⁻¹ of¹⁰Be and⁹Be, respectively. The sediment trap samples collected from 50 m off the bottom showed significant (26–63%) contributions from resuspended bottom sediments. The¹⁰Be/⁹Be ratio in trap samples varies from 3 to 20 × 10⁻⁸. The variation may partly result from varied proportion of authigenic/detrital material. The fluxes of both isotopes exhibit a very strong seasonality. The fluxes of¹⁰Be into the traps at about 1500 m are estimated as 9 × 10⁵ and 4 × 10⁵ atoms cm⁻² a⁻¹ at sites H and M respectively. These values are to be compared with the fluxes into the sediments of 4–5 × 10⁵ atoms cm⁻² a⁻¹ at both locations. Good correlations exist between¹⁰Be,⁹Be and²⁷Al indicating that the primary carrier phase(s) for the beryllium isotopes in the water column may be aluminosilicates.  相似文献