Metamorphic differentiation at Einasleigh,Northern Queensland     

Ralph Kretz 《Australian Journal of Earth Sciences》2013,60(2):561-582

Biotite‐muscovite‐garnet gneisses at Einasleigh contain quartz‐feldspar veins composed of the same minerals as found in the enclosing rock. The vein‐gneiss boundaries are commonly irregular and on a microscopic scale, gradational.

Certain amphibolite layers contain quartz‐feldspar veins composed of the same minerals as found in the amphibolite. Hornblende‐rich extraction zones surround these veins, and material balance calculations show that all or nearly all of the vein‐forming matter was locally derived. Variation in the abundance of hornblende and plagioclase in the amphibolite as a function of distance from a quartz‐feldspar vein can be expressed by error‐function curves, thus suggesting that the mineral‐segregation process was diffusion‐controlled. During the mineral rearrangement, the Na and Ca contents of plagioclase have evidently remained unchanged, but the vein hornblende has become slightly richer in Fe+3, Mg, and Ca, and poorer in Si and Al relative to hornblende in the adjacent amphibolite.

A certain biotite‐plagioclase rock forms layers and boudins in the gneisses and contains pegmatite veins composed of the same minerals as found in the host rock. The plagioclase in these veins is more sodic than that in the host rock while the biotite contains slightly more Ti and Fe+² and less Si and Mg than the biotite of the enclosing rock.

The data indicate that significant portions of the vein‐forming matter at Einasleigh were locally derived. The chemistry of some minerals has changed slightly during the segregation process, resulting possibly from different diffusion rates for the different mineral‐forming constituents.  相似文献   

Late Cenozoic paleovalley fill sequence from the Southern Liverpool Plains,New South Wales—implications for groundwater resource evaluation     

R. I. Acworth  W. A. Timms  B. F. J. Kelly  D. E. Mcgeeney  T. J. Ralph  Z. T. Larkin 《Australian Journal of Earth Sciences》2013,60(6):657-680

The Liverpool Plains in northern New South Wales contain some of the best agricultural land in Australia and are underlain by extensive smectite clay-dominated soils sourced from weathering the alkali basalts of the Liverpool Ranges. It had been thought that a relatively simple geological model explained the underlying Cenozoic sequence with salt-rich clays of the Narrabri Formation overlying sands and gravel aquifers comprising the Gunnedah Formation. Extensive groundwater modelling based upon this simple conceptualisation has been used in management plans proposed by the mining and agricultural industries. A 31.5 m core has been recovered using minimally disturbed triple-tube coring methods at Cattle Lane (Latitude –31.52° S, Longitude 150.47° E) to resolve uncertainty concerning the aquitard status of the upper layer. Recovered core has been examined and tested to determine grainsize, cation-exchange capacity, X-ray diffraction, X-ray fluorescence and microscopic examination of granular components. These measurements complement surface and borehole geophysical techniques, hydrogeological data and hydrochemical analysis of water samples recovered from a series of specially constructed piezometers adjacent to the cored hole. The sequence overlies a Late Cretaceous channel cut into Permian bedrock at 91 m depth with sands and clays below 31.5 m considered to represent various alluvial fill events mostly occurring since the Early Pliocene. Erosion of Late Eocene alkali basalts on the Liverpool Ranges, with the formation of smectite clays, pedogenic carbonates and with the addition of quartz from both eolian sources and locally derived from adjacent Triassic sandstone hills, provides the great majority of the sediment recovered from the cores. Late Pleistocene (114 ka) to Holocene ages were determined for the core from three optically stimulated luminescence (OSL) measurements on fine sands (13, 23 and 29 m BG). Detailed examination has failed to detect any evidence of a boundary between Narrabri and Gunnedah formations revealing rather a gradual change in dominance of clays and silts over sands and gravels embedded in a clay-rich matrix. This result challenges the conceptualisation used to conduct groundwater modelling on the Liverpool Plains.  相似文献   

Numbers,types, and compositions of an unbiased collection of cosmic spherules     

Susan TAYLOR  James H. LEVER  Ralph P. HARVEY 《Meteoritics & planetary science》2000,35(4):651-666

Abstract— Micrometeorites collected from the bottom of the South Pole water well (SPWW) may represent a complete, well‐preserved sample of the cosmic dust that accreted on Earth from 1100–1500 A.D. We classified 1588 cosmic spherules in the size range 50–800 μm. The collection has 41% barred olivine spherules, 17% glass spheres, 12% cryptocrystalline spherules, 11% porphyritic olivine spherules, 12% relicgrain‐bearing spherules, 3% scoriaceous spherules, 2% I‐type spherules, 1% Ca‐AI‐Ti‐rich (CAT) spherules, and 1% G‐type spherules. We also found bubbly glass spherules, spherules with glass caps, and ones with sulfide coatings—particles that are absent from other collections. A classification sequence of the stony spherules (scoriaceous, relic‐grain‐bearing, porphyritic, barred olivine, cryptocrystalline, glass, and CAT) is consistent with progressive heating and evaporation of Fe from chondritic materials. The modern‐day accretion rate and size distribution measured at the SPWW can account for the stony spherules present in deep‐sea collection through preferential dissolution of glass and small stony spherules. However, weathering alone cannot account for the high accretion rate of I‐type spherules determined for two deep‐sea collections. The SPWW collection provides data to constrain models of atmospheric‐entry heating and to assess the effects of terrestrial weathering.  相似文献   

Caffeine and Pharmaceuticals as Indicators of Waste Water Contamination in Wells   总被引：6，自引：0，他引：6  

Ralph L. Seiler  Steven D. Zaugg  James M. Thomas  Darcy L. Howcroft 《Ground water》1999,37(3):405-410

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Planetary waves in the mesosphere lower thermosphere during stratospheric sudden warming: observations using a network of meteor radars from high to equatorial latitudes     

Koushik  N.  Kumar  K. Kishore  Ramkumar  Geetha  Subrahmanyam  K. V.  Kishore Kumar  G.  Hocking  W. K.  He  Maosheng  Latteck  Ralph 《Climate Dynamics》2020,54(9):4059-4074

Climate Dynamics - In the present communication, characteristics of mean winds and planetary waves in the mesosphere lower thermosphere (MLT) region during sudden stratospheric warming (SSW) events...  相似文献   

Properties of hot stars in the Wolf--Rayet galaxy NGC 5253 from ISO-SWS spectroscopy     

Paul A. Crowther  S. C. Beck  Allan J. Willis  Peter S. Conti  Patrick W. Morris  Ralph S. Sutherland 《Monthly notices of the Royal Astronomical Society》1999,304(3):654-668

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Morphodynamic assessment of side channel systems using a simple one‐dimensional bifurcation model and a comparison with aerial images          下载免费PDF全文

R. Pepijn van Denderen  Ralph M. J. Schielen  Astrid Blom  Suzanne J. M. H. Hulscher  Maarten G. Kleinhans 《地球表面变化过程与地形》2018,43(6):1169-1182

Side channel construction is a common intervention applied to increase a river's conveyance capacity and to increase its ecological value. Past modelling efforts suggest two mechanisms affecting the morphodynamic change of a side channel: (1) a difference in channel slope between the side channel and the main channel and (2) bend flow just upstream of the bifurcation. The objective of this paper was to assess the conditions under which side channels generally aggrade or degrade and to assess the characteristic timescales of the associated morphological change. We use a one‐dimensional bifurcation model to predict the development of side channel systems and the characteristic timescale for a wide range of conditions. We then compare these results to multitemporal aerial images of four side channel systems. We consider the following mechanisms at the bifurcation to be important for side channel development: sediment diversion due to the bifurcation angle, sediment diversion due to the transverse bed slope, partitioning of suspended load, mixed sediment processes such as sorting at the bifurcation, bank erosion, deposition due to vegetation, and floodplain sedimentation. There are limitations to using a one‐dimensional numerical model as it can only account for these mechanisms in a parametrized manner, but the model reproduces general behaviour of the natural side channels until floodplain‐forming processes become important. The main result is a set of stability diagrams with key model parameters that can be used to assess the development of a side channel system and the associated timescale, which will aid in the future design and maintenance of side channel systems. © 2017 The Authors. Earth Surface Processes and Landforms published by John Wiley & Sons Ltd.  相似文献   

Harmonic analysis of tides and tidal currents in South San Francisco Bay,California     

Ralph T. Cheng  Jeffrey W. Gartner 《Estuarine, Coastal and Shelf Science》1985,21(1):57-74

Water level observations from tide stations and current observations from current-meter moorings in South San Francisco Bay (South Bay), California have been harmonically analysed. At each tide station, 13 harmonic constituents have been computed by a least-squares regression without inference. Tides in South Bay are typically mixed; there is a phase lag of approximately 1 h and an amplification of 1·5 from north to south for a mean semi-diurnal tide. Because most of the current-meter records are between 14 and 29 days, only the five most important harmonics have been solved for east-west and north-south velocity components. The eccentricity of tidal-current ellipse is generally very small, which indicates that the tidal current in South Bay is strongly bidirectional. The analyses further show that the principal direction and the magnitude of tidal current are well correlated with the basin bathymetry. Patterns of Eulerian residual circulation deduced from the current-meter data show an anticlockwise gyre to the west and a clockwise gyre to the east of the main channel in the summer months due to the prevailing westerly wind. Opposite trends have been observed during winter when the wind was variable.  相似文献   

Sea-surface wave growth under extraterrestrial atmospheres: Preliminary wind tunnel experiments with application to Mars and Titan     

Ralph D. Lorenz  Erin R. Kraal  Jered Cheney  Ronald Greeley 《Icarus》2005,175(2):556-560

We describe for the first time the generation and measurement of capillary waves in a water surface in a wind tunnel running with air at pressures of 15-1000 mbar. These experiments suggest a stronger dependence of wave generation on atmospheric density than the simple proportionality that might be expected from energy transfer arguments. Additionally, airflow over a nonaqueous fluid (kerosene) was found to produce waves of higher amplitude than for water under the same conditions. These preliminary results may indicate different efficiencies of wave generation on other planets, for which empirical terrestrial relations therefore do not apply, and thus may have a bearing on the lack of strong shoreline features on Mars and the possibility of specular glints from hydrocarbon lakes on Titan.  相似文献   

The effect of neutrinos on the initial fireballs in gamma-ray bursts     

Hylke B. J. Koers  Ralph A. M. J. Wijers 《Monthly notices of the Royal Astronomical Society》2005,364(3):934-942

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