Reflections from a randomly grooved interface: ultrasonic modelling and finite-diff erence calculation1     

Craig A. Schultz  M. Nafi Tokcz 《Geophysical Prospecting》1995,43(5):581-594

This study utilizes ultrasonic water tank modelling to examine the complexities which can result when seismic energy is diffracted by even a simple 3D interface structure. Ultrasonic laboratory modelling is carried out in our in-house water tank, using an aluminum block to simulate very simple ocean-bottom topography. The topography consists of parallel depressions which simulate valleys running parallel to a mid-ocean spreading ridge. This study shows that the phase and amplitude of primary ocean-bottom reflections can vary strongly with the azimuth of propagation. The trailing energy coda also varies dramatically as a function of propagation direction, showing the importance of developing a seismic model which includes the full 3D azimuthal distribution of interface structure.  相似文献   

Enhanced backscattering of seismic waves from a highly irregular, random interface: P-SV case     

Craig A. Schultz  M. Nafi. Toksöz 《Geophysical Journal International》1994,117(3):783-810

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Radiogenic, fissiogenic and nucleogenic noble gases in zircons     

E.H. Hebeda  L. Schultz  M. Freundel   《Earth and Planetary Science Letters》1987,85(1-3)

The concentrations and isotopic compositions of argon, krypton and xenon have been determined in a grain size suite of zircons separated from pyroxene syenite of the Botnavatn Igneous Complex, southwestern Norway. The UPb systematics of these zircons has been studied previously.Kr and Xe are mixtures of fissiogenic gas from the spontaneous fission of²³⁸U and a component with atmospheric isotopic composition. From correlation diagrams the fissiogenic component is determined to be:⁸³Kr :⁸⁴Kr :⁸⁶Kr = (4.6 ± 1.3) : (11.0 ± 2.0) : 100 and¹²⁹Xe :¹³¹Xe :¹³²Xe :¹³⁴Xe :¹³⁶Xe = (0.6 ± 0.3) : (8.8 ± 0.2) : (56.8 ± 0.3) : (82.8 ± 0.4) : 100. The fissiogenic¹³⁶Xe/⁸⁶Kr is 6.0 ± 0.4.The Ar isotopic composition shows radiogenic⁴⁰Ar and a small excess of³⁸Ar. The excess³⁸Ar of about 1 × 10⁻¹¹ cm³ STP/g can be explained by reactions of α-particles with chlorine. Asymmetric fission of²³⁸U which has been postulated to cause argon isotope anomalies in U-rich minerals is unnecessary to explain the observed³⁸Ar concentrations.UXe ages are (1.19 ± 0.07) Ga, in agreement with UPb ages. However, if the recoil loss of fissiogenic Xe is considered the UXe ages of these zircons are about 1.53 Ga, which is comparable with the KAr ages and some RbSr ages observed in basement rocks in this region. The uncertainty of the product of fission yield times spontaneous fission decay constant of²³⁸U prevents to decide which age is the true crystallization age.  相似文献   

Magnetorotational instability in Taylor-Couette flows between cylinders with finite electrical conductivity     

G. Rüdiger  M. Schultz  F. Stefani  R. Hollerbach 《地球物理与天体物理流体动力学》2018,112(4):301-320

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Anomalous Fresh Water Lens Morphology on a Strip Barrier Island     

C. Ruppel  G. Schultz  S. Kruse 《Ground water》2000,38(6):872-881

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Environmental estrogens: dose–response relationships for vitellogenin formation and reproductive toxicity in male rainbow trout     

I. R. Schultz  P. N. N. L. Battelle  W. A. Richland  A. S. Drum  M. S. L. Battelle  W. A. Sequim  W. L. Hayton  G. A. Orner 《Marine environmental research》2000,50(1-5)

The appearance of the egg-yolk protein vitellogenin (Vg) in plasma of male fish is a sensitive indicator of exposure to estrogenic compounds. We have been studying the kinetics of Vg formation and excretion in rainbow trout with a goal towards developing an integrated pharmacokinetic–pharmcodynamic (PK–PD) model to quantitatively relate cumulative estrogenic exposure of fish to the expression and appearance of Vg in plasma. We administered graded doses of ethynylestradiol (EE2), o,p-DDT, DDD and DDE and octylphenol to male rainbow trout via a dorsal aortic cannula which allowed repetitive blood sampling from individual fish for up to 48 days after injection. The plasma concentrations of the xenobiotics and Vg were simultaneously quantified using ELISA and GC–MS or GC–ECD. In separate experiments, sexually mature trout were exposed to graded water concentrations of EE2 for 3 months and various parameters indicative of the functional status of the male reproductive system determined. These parameters included tissue-somatic indices, histopathological evaluation, spermatocrit, sperm motility (quantified using computer-assisted-motion analysis) and viability of semen based on fertilization assays using eggs harvested from untreated trout. Results from fertilization assays indicated that 12 week exposure to EE2 concentrations of 10 and 100 ng/l caused a 50% reduction in the fertilization rate of semen harvested from exposed trout. PK–PD modeling strategies proved valuable tools for linking chemical exposures to Vg formation.  相似文献   

A dual sensor device to estimate fluid flow velocity at diffuse hydrothermal vents     

J. Sarrazin  P. Rodier  M.K. Tivey  H. Singh  A. Schultz  P.M. Sarradin 《Deep Sea Research Part I: Oceanographic Research Papers》2009,56(11):2065-2074

Numerous attempts have been made over the last thirty years to estimate fluid flow rates at hydrothermal vents, either at the exit of black smoker chimneys or within diffuse flow areas. In this study, we combine two methods to accurately estimate fluid flow velocities at diffuse flow areas. While the first method uses a hot film anemometer that performs high-frequency measurements, the second allows a relatively rapid assessment of fluid flow velocity through video imagery and provides in situ data to calibrate the sensor. Measurements of flow velocities on hydrothermal diffuse flow areas were obtained on the Mid-Atlantic Ridge (MAR). They range from 1.1 to 4.9 mm/s at the substratum level, in low-temperature (4.5–16.4 °C) diffuse flow areas from the Tour Eiffel sulfide edifice. A strong correlation was observed between fluid flow velocities and temperature, supporting the possible use of temperature as a proxy to estimate the flow rates in diffuse flow areas where such a simple linear flow/temperature relation is shown to dominate.  相似文献   

First record of stereospondyls (Tetrapoda,Temnospondyli) in the Upper Triassic of Southern Brazil     

Sérgio Dias-da-Silva  Eliseu Vieira Dias  Cesar Leandro Schultz 《Gondwana Research》2009,15(1):131-136

Stereospondyls survived the Permo-Triassic extinctions in a refuge probably located in the landmass that nowadays comprises Australia. Subsequently, they radiated to other parts of Pangaea, reaching their highest distribution and diversification during the Early Triassic. An incomplete interclavicle from the Caturrita Formation represents their first record in the Upper Triassic of Brazil. Previously, Upper Triassic South American stereospondyls were restricted to Argentina. This new record reinforces a former hypothesis that suggests the presence of a more diverse stereospondyl fauna in South America during the Late Triassic than previously assumed. Additionally, the presence of a stereospondyl and a phytosaur in the Caturrita Formation reinforces the hypothesis of a change to more humid climatic conditions in the Paraná Basin during the Upper Triassic. The record of Early Triassic stereospondyls in South America suggests that they first colonized Brazil and/or Uruguay, spreading from South Africa during the Early Triassic, subsequently reaching Argentina. Up till now, there is no record of Middle Triassic stereospondyls in either Argentina and Brazil, probably due to either taphonomic bias or insufficient prospecting. Despite the lack of direct evidence, one should not dismiss an earlier stereospondyl colonization of Argentina still during the Early or Middle Triassic.  相似文献   

Itqiy: A study of noble gases and oxygen isotopes including its terrestrial age and a comparison with Zakłodzie     

Andrea Patzer  Dolores H. Hill  William V. Boynton  Luitgard Franke  Ludolf Schultz  A. J. Timothy Jull  Lanny R. McHargue  Ian A. Franchi 《Meteoritics & planetary science》2002,37(6):823-833

Abstract— We report noble gas, oxygen isotope, ¹⁴C and ¹⁰Be data of Itqiy as well as noble gas, ¹⁴C and ¹⁰Be results for Zak?odzie. Both samples have been recently classified as anomalous enstatite meteorites and have been compared in terms of their mineralogy and chemical composition. The composition of enstatite and kamacite and the occurrence of specific sulfide phases in Itqiy indicate it formed under similar reducing conditions to those postulated for enstatite chondrites. The new results now seem to point at a direct spatial link. The noble gas record of Itqiy exhibits the presence of a trapped subsolar component, which is diagnostic for petrologic types 4–6 among enstatite chondrites. The concentration of radiogenic ⁴He is very low in Itqiy and indicates a recent thermal event. Its ²¹Ne cosmic‐ray exposure age is 30.1 ± 3.0 Ma and matches the most common age range of enstatite chondrites (mostly EL6 chondrites) but not that of Zak?odzie. Itqiy's isotopic composition of oxygen is in good agreement with that observed in Zak?odzie as well as those found in enstatite meteorites suggesting an origin from a common oxygen pool. The noble gas results, on the other hand, give reason to believe that the origin and evolution of Itqiy and Zak?odzie are not directly connected. Itqiy's terrestrial age of 5800 ± 500 years sheds crucial light on the uncertain circumstances of its recovery and proves that Itqiy is not a modern fall, whereas the ¹⁴C results from Zak?odzie suggest it hit Earth only recently.  相似文献   

Noble gases in enstatite chondrites II: The trapped component     

Andrea Patzer  Ludolf Schultz 《Meteoritics & planetary science》2002,37(4):601-612

Abstract— The trapped noble gas record of 57 enstatite chondrites (E chondrites) has been investigated. Basically, two different gas patterns have been identified dependent on the petrologic type. All E chondrites of type 4 to 6 show a mixture of trapped common chondritic rare gases (Q) and a subsolar component (range of elemental ratios for E4–6 chondrites: ³⁶Ar/¹³²Xe = 582 ± 270 and ³⁶Ar/⁸⁴Kr = 242 ± 88). E3 chondrites usually contain Q gases, but also a composition with lower ³⁶Ar/¹³²Xe and ³⁶Ar/⁸⁴Kr ratios, which we call sub‐Q (³⁶Ar/¹³²Xe = 37.0 ± 18.0 and ³⁶Ar/⁸⁴Kr = 41.7 ± 18.1). The presence of either the subsolar or the sub‐Q signature in particular petrologic types cannot be readily explained by parent body metamorphism as postulated for ordinary chondrites. We therefore present a different model that can explain the bimodal distribution and composition of trapped heavy noble gases in E chondrites. Trapped solar noble gases have been observed only in some E3 chondrites. About 30% of each group, EH3 and EL3 chondrites, amounting to 9% of all analyzed E chondrites show the solar signature. Notably, only one of those meteorites has been explicitly described as a regolith breccia.  相似文献