Lithosphere mapping beneath the North American plate   总被引：2，自引：0，他引：2  

W.L. Griffin  Suzanne Y. O''Reilly  B.J. Doyle  N.J. Pearson  H. Coopersmith  K. Kivi  V. Malkovets  N. Pokhilenko 《Lithos》2004,77(1-4):873-922

Major- and trace-element analyses of garnets from heavy-mineral concentrates have been used to derive the compositional and thermal structure of the subcontinental lithospheric mantle (SCLM) beneath 16 areas within the core of the ancient Laurentian continent and 11 areas in the craton margin and fringing mobile belts. Results are presented as stratigraphic sections showing variations in the relative proportions of different rock types and metasomatic styles, and the mean Fo content of olivine, with depth. Detailed comparisons with data from mantle xenoliths demonstrate the reliability of the sections.

In the Slave Province, the SCLM in most areas shows a two-layer structure with a boundary at 140–160 km depth. The upper layer shows pronounced lateral variations, whereas the lower layer, after accounting for different degrees of melt-related metasomatism, shows marked uniformity. The lower layer is interpreted as a subcreted plume head, added at ca. 3.2 Ga; this boundary between the layers rises to <100 km depth toward the northern and southern edges of the craton. Strongly layered SCLM suggests that plume subcretion may also have played a role in the construction of the lithosphere beneath Michigan and Saskatchewan.

Outside the Slave Province, most North American Archon SCLM sections are less depleted than similar sections in southern Africa and Siberia; this may reflect extensive metasomatic modification. In E. Canada, the degree of modification increases toward the craton margin, and the SCLM beneath the Kapuskasing Structural Zone is typical of that beneath Proterozoic to Phanerozoic mobile belts.

SCLM sections from several Proterozoic areas around the margin of the Laurentian continental core (W. Greenland, Colorado–Wyoming district, Arkansas) show discontinuities and gaps that are interpreted as the effects of lithosphere stacking during collisional orogeny. Some areas affected by Proterozoic orogenesis (Wyoming Craton, Alberta, W. Greenland) appear to retain buoyant, modified Archean SCLM. Possible juvenile Proterozoic SCLM beneath the Colorado Plateau is significantly less refractory. The SCLM beneath the Kansas kimberlite field is highly melt-metasomatised, reflecting its proximity to the Mid-Continent Rift System.

A traverse across the continent shows that the upper part of the cratonic SCLM is highly magnesian; the decrease in mg# with depth is interpreted as the cumulative effect of metasomatic modification through time. The relatively small variations in seismic velocity within the continental core largely reflect the thickness of this depleted layer. The larger drop in seismic velocity in the surrounding Proton and Tecton belts reflects the closely coupled changes in SCLM composition and geotherm.  相似文献   

Subsea-floor replacement in volcanic-hosted massive sulfide deposits   总被引：1，自引：0，他引：1  

Mark G. Doyle  Rodney L. Allen   《Ore Geology Reviews》2003,23(3-4):183-222

Recent research on volcanic-hosted massive sulfide (VMS) deposits indicates that syngenetic subsea-floor replacement ores form an important component of many deposits. In the context of VMS deposits, subsea-floor replacement can be defined as the syn-volcanic formation of sulfide minerals within pre-existing volcanic or sedimentary deposits by infiltration and precipitation in open spaces (fractures, inter- and intra-granular porosity) as well as replacement of solid materials.There are five criteria for distinguishing subsea-floor replacement in massive sulfide deposits: (1) mineralized intervals are enclosed within rapidly emplaced volcanic or sedimentary facies (lavas, intrusions, subaqueous mass-flow deposits, pyroclastic fallout); (2) relics of the host facies occur within the mineral deposit; (3) replacement fronts occur between the mineral deposit and the host lithofacies; (4) the mineral deposit is discordant to bedding; and (5) strong hydrothermal alteration continues into the hanging wall without an abrupt break in intensity. Criteria 1–3 are diagnostic of replacement, whereas criteria 4 and 5 may suggest replacement but are not alone diagnostic. Because clastic sulfide ores contain accessory rock fragments collected by the parent sediment gravity flow(s) during transport, criteria 2 can only be applied to massive, semi-massive, disseminated or vein style deposits, and not clastic ores.The spectrum of VMS deposit types includes deposits that have accumulated largely subsea-floor, and others in which sedimentation and volcanism were synchronous with hydrothermal activity, and precipitation of sulfides occurred at and below the sea floor over the life of the hydrothermal system. Deposits that formed largely subsea-floor are mainly hosted by syn-eruptive or post-eruptive volcaniclastic facies (gravity flow deposits, water-settled fall, autoclastic breccia). However, some subsea-floor replacement VMS deposits are hosted by lavas and syn-volcanic intrusions (sills, domes, cryptodomes). Burial of sea-floor massive sulfide by lavas or sediment gravity flow deposits can interrupt sea-floor mineralization and promote subsea-floor replacement and zone-refining.The distance below the sea floor at which infiltration and replacement took place is rarely well constrained, with published estimates ranging from less than 1 to more than 500 m, but mainly in the range 10–200 m. The upper few tens to hundreds of metres in the volcano-sedimentary pile are the favoured position for replacement, as clastic facies are wet, porous and poorly consolidated in this zone, and at greater depths become progressively more compacted, dewatered, altered, and less amenable to large scale infiltration and replacement by hydrothermal fluids. Furthermore, sustained mixing between the upwelling hydrothermal fluid and cold seawater is regarded as a major cause of sulfide precipitation in VMS systems, and this mixing process generally becomes less effective with increasing depth in the volcanic pile.The relative importance of subsea-floor replacement in VMS systems is related principally to four factors: the permeability and porosity patterns of host lithofacies, sedimentation rate, the relative ease of replacement of host lithofacies (especially glassy materials) and early formed alteration minerals during hydrothermal attack, and physiochemical characteristics of the hydrothermal fluid.  相似文献   

Turbulent flow over a wavy boundary     

Doyle Knight 《Boundary-Layer Meteorology》1977,11(2):205-222

The linearized, two-dimensional flow of an incompressible fully turbulent fluid over a sinusoidal boundary is solved using the method of matched asymptotic expansions in the limit of vanishing skin-friction.A phenomenological turbulence model due to Saffman (1970, 1974) is utilized to incorporate the effects of the wavy boundary on the turbulence structure.Arbitrary lowest-order wave speed is allowed in order to consider both the stationary wavy wall, and the water wave moving with arbitrary positive or negative velocity.Good agreement is found with measured tangential velocity profiles and surface normal stress coefficients. The phase shift of the surface normal stress exhibits correct qualitative behavior with both positive and negative wave speeds, although predicted values are low.  相似文献   

Verification of an ENSO-Based Long-Range Prediction of Anomalous Weather Conditions During the Vancouver 2010 Olympics and Paralympics     

Ruping Mo  Paul I. Joe  Chris Doyle  Paul H. Whitfield 《Pure and Applied Geophysics》2014,171(1-2):323-336

A brief review of the anomalous weather conditions during the Vancouver 2010 Winter Olympic and Paralympic Games and the efforts to predict these anomalies based on some preceding El Niño–Southern Oscillation (ENSO) signals are presented. It is shown that the Olympic Games were held under extraordinarily warm conditions in February 2010, with monthly mean temperature anomalies of +2.2 °C in Vancouver and +2.8 °C in Whistler, ranking respectively as the highest and the second highest in the past 30 years (1981–2010). The warm conditions continued, but became less anomalous, in March 2010 for the Paralympic Games. While the precipitation amounts in the area remained near normal through this winter, the lack of snow due to warm conditions created numerous media headlines and practical problems for the alpine competitions. A statistical model was developed on the premise that February and March temperatures in the Vancouver area could be predicted using an ENSO signal with considerable lead time. This model successfully predicted the warmer-than-normal, lower-snowfall conditions for the Vancouver 2010 Winter Olympics and Paralympics.  相似文献   

Herschel out-of-field stray-light characterization     

U. Klaas  K. Okumura  M. Ferlet  T. Müller  M. Sanchez-Portal  B. Altieri  D. Doyle  G. L. Pilbratt 《Experimental Astronomy》2014,37(2):331-345

Out-of-field stray-light spots of the Herschel telescope optics relative to the PACS and SPIRE instrument apertures were modeled by ray tracing simulations with the Advanced Systems Analysis Program (ASAP, by Breault Research Organization) prior to launch. The predicted stray-light behaviour was verified by dedicated stray-light calibration observations in-flight. This resulted in a special feature of the Herschel Science Mission Planning Software, marking the sky positions of stray-light spots by the very bright infrared planetary sources Venus, Mars, Jupiter, and Saturn, as well as the Moon, thus avoiding contamination of scientific photometric observations by out-of-field stray-light of these sources.  相似文献   

Heterogeneous andesite–dacite ejecta in 26–16.6 ka pyroclastic deposits of Tongariro Volcano,New Zealand: the product of multiple magma-mixing events     

Phil Shane  Louise R. Doyle  Ian A. Nairn 《Bulletin of Volcanology》2008,70(4):517-536

The previously poorly documented 26–16.6 ka interval of pyroclastic volcanism from Tongariro Volcano is marked by three distal lapilli fall units (Rt1-3) exposed in ring-plain deposits. The distal Rt1-3 units are tentatively correlated to proximal scoria deposits on the upper slopes of North Crater based on their dispersal patterns, petrography and geochemistry. Lapilli in each of the Rt1-3 deposits are characterised by variable groundmass crystallinity, vesicularity and colour within individual clasts. Matrix glasses are mostly microlite-free, and compositionally diverse across the deposits (SiO₂ = 62–75 wt%), with wide composition ranges occurring within single clasts. The glasses represent different melts that were mingled and mixed shortly before eruption; a finding supported by widely variable Fe–Ti oxide equilibrium temperature estimates (∼830–1,200°C). Ranges of 30–160°C (typically 70°C) occur within individual clasts. Some clinopyroxene crystals display Mg-rich (∼Mg #88) rim zones around homogeneous low-Mg (∼Mg #68) cores, with abrupt transition zones. This zoning is interpreted as resulting from the injection of a more mafic melt into a stagnating, resident magma. Crystal-melt equilibria indicate that several episodes of mafic intrusion occurred, to produce hybrid melts with zoned crystals forming isolated ponds within the resident magma. Variable mixing from the percolation of melts and the coalescence of melt ponds would explain the wide range of melt compositions and equilibrium temperatures observed in the ejecta. The magma heterogeneity was preserved by quenching on prompt eruption, with much of the short-duration chaotic mixing of melts and crystals occurring in the conduit. The Rt1-3 eruptions were from an open magmatic system consisting of one or more long-lived stagnant crystal mush zones, from which eruptions were rapidly triggered by new injections of mafic magmas from greater depths. A similar pattern of magmatic dynamics was observed in the much smaller 1995 eruptions of the neighbouring Ruapehu Volcano.  相似文献   

An alternative measure of discharge effectiveness     

Martin W. Doyle  Catherine A. Shields 《地球表面变化过程与地形》2008,33(2):308-316

Since 1960, geomorphic effectiveness has been quantified by analytically combining measures of the frequency and the magnitude of geomorphic processes, most often for the case of sediment yield in rivers via the calculation of effective discharge, Q_eff. Here we leverage the Q_eff analysis approach to develop an alternative metric, the functional‐equivalent discharge Q_fed, which is the discharge that will reproduce the magnitude of the sediment load generated by the full hydrologic distribution. Q_fed is intended to be a more representative metric of hydrologic variability than Q_eff: whereas Q_eff provides a measure of the effectiveness of individual flow rates, Q_fed incorporates a measure of the average effectiveness of the entire flow distribution. We develop an analytical approximation of Q_fed based on relatively few parameters, apply the approach to a set of suspended sediment load data and describe how Q_fed varies broadly with sediment and hydrologic conditions. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

Multidisciplinary investigations at Stalag Luft III allied prisoner‐of‐war camp: The site of the 1944 “great escape,” Zagan,Western Poland     

J.K. Pringle  P. Doyle  L.E. Babits 《Geoarchaeology》2007,22(7):729-746

Stalag Luft III, situated in Zagan, Poland (formerly eastern Germany), was the site of a World War II Allied aviator prisoner of war (POW) camp famous for repeat escape attempts—notably the mass escape of 76 POWs in March 1944, shown in the 1963 film “The Great Escape.” The site has had little attention to date because it was within restricted military training grounds until 1992. This paper reports on attempts to locate the undiscovered “Dick” escape tunnel (the “Tom” and “Harry” tunnels from the same escape attempt were discovered and destroyed by camp authorities). Geological and geophysical surveys located hut 122, which contained the “Dick” entrance shaft. Subsequent archaeological investigations included surface artifact collection and inspection of the rubble‐filled, tunnel entrance shaft. Excavations to a depth of 10 m through yellow glacio‐fluvial sand resulted in the discovery of the refilled “Dick” tunnel with intact bed‐board shoring and ventilation system. Our investigation provides valuable insights into POW escape efforts. © 2007 Wiley Periodicals, Inc.  相似文献   

Long-Period Oscillations in Polar Plumes as Observed by cds on Soho     

D. Banerjee  E. O'Shea  J.G. Doyle 《Solar physics》2000,196(1):63-78

We examine spectral time series of the transition region line Ov 629Å, observed with the Coronal Diagnostic Spectrometer (CDS) on the SOHO spacecraft in July 1997. Both Fourier and wavelet transforms have been applied independently to the analysis of plume oscillations in order to find the most reliable periods. The wavelet analysis allows us to derive the duration as well as the periods of the oscillations. Our observations indicate the presence of compressional waves with periods of 10–25 min. We have also detected a 11±1 min periodicity in the network regions of the north polar coronal hole. The waves are produced in short bursts with coherence times of about 30 min. We interpret these oscillations as outward propagating slow magneto-acoustic waves, which may contribute significantly to the heating of the lower corona by compressive dissipation and which may also provide enough energy flux for the acceleration of the fast solar wind. The data support the idea that the same driver is responsible for the network and plume oscillations with the network providing the magnetic channel through which the waves propagate upwards from the lower atmosphere to the plumes.  相似文献   

Polar Plumes and Inter-plume regions as observed by SUMER on SOHO     

Banerjee  D.  Teriaca  L.  Doyle  J.G.  Lemaire  P. 《Solar physics》2000,194(1):43-58

We present observations of Ovi 1032 Å line profiles obtained with the SUMER instrument on SOHO extending from the solar disk to 1.5 R above the limb in the north polar coronal hole. Variations of the intensity and linewidth in the polar plume and inter-plume regions are investigated. We find an anti-correlation between the intensity and the linewidth in the plume and inter-plume regions with detailed plume structures been seen out to 1.5 R . Possible implications regarding the magnetic topologies of these two regions and related heating mechanisms are discussed. The Ovi linewidth measurements are combined with UVCS output to provide an overview of its variations with height extending up to 3.5 R . We find a linear increase of the linewidth from 1 to 1.2 R , then a plateau followed by a sharp increase around 1.5 R .  相似文献