Quaternary glaciations of the Rongbuk Valley,Tibet     

DANIEL H. MANN  RONALD S. SLETTEN  RICHARD E. REANIER 《第四纪科学杂志》1996,11(4):267-280

Randomisation tests on boulder weathering data distinguish moraines of four different ages in the Rongbuk Valley, all deposited by valley glaciers flowing northward into Tibet from the Himalaya. Lichenometry utilising subgenus Rhizocarpon distinguishes two groups of moraines, those <100 yr old and those older than several thousand years. The degree of soil development has a similar, limited utility in relative-age dating these moraines. The radiocarbon ages of calcium carbonate coatings in the lower horizons of moraine soils provide minimum-limiting ages of 1900 yr BP for the penultimate advance of the Rongbuk glacier (Samdopo moraine) and 9500 yr BP for the Rongbuk moraine, the moraine suggested by previous workers to represent the last glacial maximum. Equilibrium-line depression associated with the Rongbuk moraine probably was slight, <200 m. The small magnitude of this depression relative to glaciers in other mountain ranges could relate to a weakening of the monsoon in full glacial times, recent tectonic uplift, and/or to the insensitivity of these high-altitude glaciers to lowering temperatures in the rain shadow of Mount Everest.  相似文献   

Finite difference approximations to the advection-diffusion equation     

DANIEL G. WRIGHT 《地球，A辑:动力气象学与海洋学》1992,44(3):261-269

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INTRODUCTION     

DANIEL Z. SUI 《Geographical review》2007,97(3):iii-vi

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Microstructures of sediment flow deposits and subglacial sediments: a comparison     

MATTHEW S. LACHNIET  GRAHAME J. LARSON  DANIEL E. LAWSON  EDWARD B. EVENSON  RICHARD B. ALLEY 《Boreas: An International Journal of Quaternary Research》2001,30(3):254-264

Microstructural analysis of glacial deposits has recently been used as a research tool to determine sediment genesis. However, the occurrence of microstructures in deposits of known origin has not been sufficiently documented, hindering our ability to confidently interpret microstructures in sediments of unknown origin. Our objective is to present a calibration study of microstructures of recent sediment flow deposits and associated sediments from the Matanuska Glacier, Alaska, and to evaluate the degree of commonality with microstructures found in subglacially deformed sediments. Microstructures in sediment flow deposits can be formed as a result of sediment transport, deposition, and/or post-depositional processes, and are related to the viscosity regime of the source flow. Characteristic microstructures formed during brittle deformation include shears, faults, and brecciation; microstructures formed during ductile deformation include folds, pressure shadows, re-orientation of clasts around a 'core' stone, fine laminations, basal shear zones, imbrication, and flow fabrics. Other microstructures include fluid escape and injection structures, clast haloes, and fissility. The results of our comparison suggest that sediment flow deposits share many microstructures in common with subglacially deformed sediments.  相似文献   

Diagnosing cyclogenesis by partitioning energy and potential enstrophy in a linear quasi‐geostrophic model     

DANIEL HODYSS  RICHARD GROTJAHN 《地球，A辑:动力气象学与海洋学》2001,53(5):567-577

Baroclinic development is studied with 2 linear, quasi‐geostrophic models. One model is the Eady model, the other uses more realistic wind, density, Coriolis, and static stability. Initial‐value solutions are diagnosed using time series of potential enstrophy ( H ), total energy ( E ), the components of H and E , and the amplitude norm. Two vertical structures for the initial condition are used for both models. One initial condition is representative of a class of initial conditions studied previously having enhanced nonmodal growth (NG). The other initial condition approximates observed conditions prior to cyclogenesis. Results are shown for the most unstable normal mode wavelength of each model. The growth rates of the components of H and E evolve quite differently for different initial states and models tested. NG in H is shown to be sensitive to the contribution of the boundary potential vorticity (BPV) of the initial state; small adjustments in eddy structure at the boundary significantly alter BPV and H growth rates. The amount of NG is related to how far BPV present initially differs from the asymptotic normal mode. The effect upon NG of each approximation present in the Eady model (but not in the other model) are considered. Using realistic mean flow shear, static stability, or compressibility can significantly reduce NG but including linearly varying Coriolis parameter did not. Two conceptual models of NG are considered. Growth by increasingly favorable superposition remains relevant. Growth by "tilting into the vertical" is shown to be incorrect.  相似文献   

Seismic evidence of up to 200 m lake‐level change in Southern Patagonia since Marine Isotope Stage 4     

ANDREA CATALINA GEBHARDT  CHRISTIAN OHLENDORF  FRANK NIESSEN  MARC DE BATIST  FLAVIO S. ANSELMETTI  DANIEL ARIZTEGUI  PIERRE KLIEM  STEFAN WASTEGÅRD  BERND ZOLITSCHKA 《Sedimentology》2012,59(3):1087-1100

Maar lake Laguna Potrok Aike is located north of the Strait of Magellan (south‐eastern Patagonia). Seismic reflection profiles revealed a highly dynamic palaeoclimate history. Dunes were identified in the eastern part of the lake at approximately 30 to 80 m below the lake floor, overlying older lacustrine strata, and suggest that the region experienced dry conditions probably combined with strong westerly winds. It is quite likely that this can be linked to a major dust event recorded in the Antarctic ice cores during Marine Isotope Stage 4. The dunes are overlain by a series of palaeo‐shorelines indicating a stepwise water‐level evolution of a new lake established after this dry period, and thus a change towards wetter conditions. After the initial, rapid and stepwise lake‐level rise, the basin became deeper and wider, and sediments deposited on the lake shoulder at approximately 33 m below present‐day lake level point towards a long period of lake‐level highstand between roughly 53·5 ka cal. bp and 30 ka cal. bp with a maximum lake level some 200 m higher than the desiccation horizon. This highstand was then followed by a regressional phase of uncertain age, although it must have happened some time between approximately 30 ka cal. bp and 6750 yrs cal. bp . Dryer conditions during the Mid‐Holocene are evidenced by a dropping lake level, resulting in a basin‐wide erosional unconformity on the lake shoulder. A second stepwise transgression between ca 5·8 to 5·4 ka cal. bp and ca 4·7 to 4 ka cal. bp with palaeo‐shorelines deposited on the lake shoulder unconformity again indicates a change towards wetter conditions.  相似文献   

Environmental history of southern Patagonia unravelled by the seismic stratigraphy of Laguna Potrok Aike     

FLAVIO S. ANSELMETTI  DANIEL ARIZTEGUI†  MARC DE BATIST‡  A. CATALINA GEBHARDT§  TORSTEN HABERZETTL¶  FRANK NIESSEN§  CHRISTIAN OHLENDORF  BERND ZOLITSCHKA 《Sedimentology》2009,56(4):873-892

Laguna Potrok Aike, located in southernmost Patagonia (Argentina, 52°S) is a 100 m deep hydrologically closed lake that probably provides the only continental southern Patagonian archive covering a long and continuous interval of several glacial to interglacial cycles. In the context of the planned ‘International Continental Scientific Drilling Program’ initiative ‘Potrok Aike Maar Lake Sediment Archive Drilling Project’, several seismic site surveys that characterize in detail the sedimentary subsurface of the lake have been undertaken. Long sediment cores recovered the material to date and calibrate these seismic data. Laguna Potrok Aike is rimmed steeply, circular in shape with a diameter of ∼3·5 km and is surrounded by a series of subaerial palaeoshorelines, reflecting varying lake-level highstands and lowstands. Seismic data indicate a basinwide erosional unconformity that occurs consistently on the shoulder of the lake down to a depth of −33 m (below 2003 ad lake level), marking the lowest lake level during Late Glacial to Holocene times. Cores that penetrate this unconformity comprise Marine Isotope Stage 3-dated sediments (45 kyr bp ) ∼3·5 m below, and post-6800 cal yr bp transgressional sediments above the unconformity. This Middle Holocene transgression following an unprecedented lake-level lowstand marks the onset of a stepwise change in moisture, as shown by a series of up to 11 buried palaeoshorelines that were formed during lake-level stillstands at depths between −30 and −12 m. Two series of regressive shorelines between ∼5800 to 5400 and ∼4700 to 4000 cal yr bp interrupt the overall transgressional trend. In the basin, mound-like drift sediments occur after ∼6000 cal yr bp, documenting the onset of lake currents triggered by a latitudinal shift or an increase in wind intensity of the Southern Hemispheric Westerlies over Laguna Potrok Aike at that time. Furthermore, several well-defined lateral slides can be recognized. The majority of these slides occurred during the mid-Holocene lake-level lowering when the slopes became rapidly sediment-charged because of erosion from the exposed shoulder sediments. Around 7800 and 4900 cal yr bp , several slides went down simultaneously, probably triggered by seismic shaking.  相似文献   

MEXICAN URBAN COLONIAS IN THE SALT RIVER VALLEY OF ARIZONA     

CHRIS LUKINBEAL  DANIEL D. ARREOLA  D. DREW LUCIO 《Geographical review》2010,100(1):12-34

The history of the Salt River Valley is often characterized as a boomtown narrative that highlights the exploding Anglo population and rapid suburban sprawl that followed World War II. Frequently overlooked is the fundamental role that Mexicans played in the early suburbanization process through the formation of urban colonias, or suburban Mexican settlements. Early Mexican suburbs, despite their rural atmosphere, were connected to the pre–World War II urbanization process in the Salt River Valley. Our research seeks to amend and clarify the urban historical record by documenting the diverse and dispersed array of Mexican suburban settlements, a process generated by industrial agriculture, decentralization, and residential segregation.  相似文献   

Isotopic composition of trapped and cosmogenic noble gases in several Martian meteorites     

DANIEL H. GARRISON  DONALD D. BOGARD 《Meteoritics & planetary science》1998,33(4):721-736

Abstract— Isotopic abundances of the noble gases were measured in the following Martian meteorites: two shock glass inclusions from Elephant Moraine (EET) 79001, shock vein glass from Shergotty and Yamato (Y) 793605, and whole-rock samples of Allan Hills (ALH) 84001 and Queen Alexandra Range (QUE) 94201. These glass samples, when combined with literature data on a separate single glass inclusion from EET 79001 and a glass vein from Zagami, permit examination in greater detail of the isotopic composition of Ne, Ar, Kr, and Xe trapped from the Martian atmosphere. The isotopic composition of Martian Ne, if actually present in these glasses, remains poorly defined. The ⁴⁰Ar/³⁶Ar ratio of trapped Martian atmospheric Ar is probably considerably lower than the nominal ratio of 3000 measured by Viking, and data on impact glasses suggest a value of ～1900. The atmospheric ³⁶Ar/³⁸Ar ratio is ≤4.0. Martian atmospheric Kr may be enriched in lighter isotopes by ～0.5%/amu compared to both solar-wind Kr and to the Martian composition previously reported. The isotopic composition of Xe in these glasses agrees with that previously reported in the literature. The Martian atmospheric ³⁶Ar/¹³²Xe and ⁸⁴Kr/¹³²Xe elemental ratios are higher than those reported by Viking by factors of ～2.5–1.6 (depending on the ⁴⁰Ar/³⁶Ar ratio adopted) and ～1.8, respectively, and are discussed in a separate paper. Cosmogenic gases indicate space exposure ages of 2.7 ± 0.6 Ma for QUE 94201 and Shergotty and 14 ± 1 Ma for ALH 84001. Small amounts of ²¹Ne produced by energetic solar protons may be present in QUE 94201 but are not present in ALH 84001 or Y-793605. The space exposure age for Y-793605 is 4.9 ± 0.6 Ma and appears to be distinctly older than the ages for basaltic shergottites. However, uncertainties in cosmogenic production rates still makes somewhat uncertain the number of Martian impact events required to produce the exposure ages of Martian meteorites.  相似文献   

Sediment trend models fail to reproduce small-scale sediment transport patterns on an intertidal beach   总被引：2，自引：0，他引：2  

GERHARD MASSELINK  DANIEL BUSCOMBE  MARTIN AUSTIN†  TIM O'HARE†  PAUL RUSSELL† 《Sedimentology》2008,55(3):667-687

A rigorous test is presented of the application of sediment trend models to an intertidal beach environment characterized by bar morphology. Sediment samples were collected during low tide from a regular grid and their sediment fall velocity distributions, obtained using a settling tube, were analysed using moment analysis. The net sediment transport direction determined from beach surveys, hydrodynamic measurements, wave ripple observations and sediment transport modelling was compared with predictions by sediment trend models based on the spatial distribution of sediment parameters. It was found that the sediment transport pathways and patterns of sedimentation predicted using sediment trend models were at odds with field observations, and varied significantly depending on whether surface or sub‐surface sediment samples were used. The sediment trend models are thought to fail because, in energetic and morphologically variable beach environments, spatial patterns in sediment characteristics are mainly attributed to the presence of different hydrodynamic regions and associated morphology, rather than sediment pathways. The use of sediment trend models cannot replace the collection of morphological, hydrodynamic and sediment transport data in the field to define relationships between flows, forms and sedimentation patterns on a dynamic intertidal beach.  相似文献