Effects of suburban construction on runoff contributing zones in a small southern Ontario drainage basin / Les conséquences du développement suburbain pour les zones d'appel dans un petit bassin versant de sud Ontario

Abstract

The runoff response of a small drainage basin in southern Ontario has been monitored over a 5 year period, during which 25 per cent of its surface has been modified by suburban construction activity. Direct runoff response to summer and autumn rainstorms has not been noticeably affected by the development, but response to spring snowmelt has increased by three to four times. Summer and autumn storm runoff still appears to be generated mainly by direct precipitation on a natural, saturated, contributing zone alongside the channel, which has been little affected by the construction activity. The construction surfaces have had their infiltration capacities greatly reduced by devegetation and compaction, but runoff from them does not contribute to the storm hydrograph unless ephemeral channels and swales which link them to the main stream are saturated and capable of conducting flow. This happens rarely during rainstorms, but consistently during snowmelt, when ground conditions are extremely wet. The seasonal contrasts in the effect of partial suburban development on direct runoff response, are therefore caused by seasonal variations in the extent to which the construction surfaces are integrated into the active runoff contributing zone of the drainage basin.     

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

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.     

西秦岭温泉钼矿床成矿作用时限及其对斑岩型钼矿床系统分类制约

斑岩系统是一个涉及岩浆和热液作用的复杂系统,建立精细的斑岩系统成因模型对于寻找更为丰富的金属矿产尤为重要,成矿作用时限是建立成因模型和指导矿产勘查的关键。温泉钼矿床是西秦岭造山带内与晚三叠世花岗岩有关的斑岩型钼矿床,其在西秦岭造山带的独特发育蕴含印支期斑岩成矿作用、大陆地壳演化及矿产勘查关键科学问题。钼矿体主要赋存于温泉复式岩体Ⅱ单元和Ⅲ单元的黑云母二长花岗斑岩和似斑状二长花岗岩中,钼以细脉和浸染状矿化形式产出。赋矿岩石单元锆石U-Pb年龄为224.6±2.5Ma到216.2±1.7Ma,Ⅱ和Ⅲ单元分别侵位于~223Ma和~217Ma,持续约8Myr。辉钼矿Re-Os年龄为212.7±2.6Ma到215.1±2.6Ma,暗示晚三叠世钼成矿作用与花岗质岩浆作用密切时空关系,且成矿年龄稍晚,反映钼矿化主要发生在岩浆作用晚期阶段。成岩、成矿作用发生于华北板块与华南板块全面对接后秦岭造山带构造体制由碰撞到后碰撞的转折阶段,响应南秦岭变质变形、勉-略洋盆闭合及大别-苏鲁超高压岩石板片折返统一地质事件。黑云母K-Ar年龄为207~226Ma,可能反映~223Ma和~208Ma的岩体冷却事件和~216Ma的岩浆-热液成矿作用。锆石U-Pb、辉钼矿Re-Os和黑云母K-Ar多元同位素定年系统准确刻画岩体侵位、热液成矿与冷却事件上有所重叠,岩浆-热液分异演化充分,且具有较高的冷却速率,精确厘定温泉斑岩系统岩浆活动的"多期性"(复式岩体)、成矿事件的"瞬时性"(~214Ma)和成矿作用的"持续性"(~8Myr)。同时,系统对比全球典型斑岩钼(铜)矿床成矿动力学背景,细化分类方案,即产于挤压背景的大洋俯冲和大陆碰撞环境矿床及产于伸展背景的后碰撞、陆缘弧后和板内裂谷环境矿床。明确在大洋俯冲→大陆碰撞→后碰撞→板内裂谷旋回的四个阶段均可以产生规模的斑岩型钼(铜)矿床,且挤压向伸展过渡的构造体制转换尤其是大型矿床形成的有利环境。     

English Jurassic dasyclads: seaweed indicators of marine climate

Aragonitic chlorophyte (green) algae, typical of the warm seas of the Tethyan area, reached as far north as the present Cotswolds of Southern England in mid-Jurassic times, when conditions made colonisation possible. Few in numbers and species, they appear to show features similar to those of their living descendants found today in warm seas marginal to the tropics, so confirming the Jurassic palaeolatitude arrived at independently from palaeogeographical studies.     

Deep‐water foreland basin deposits of the Cerro Toro Formation,Magallanes basin,Chile: architectural elements of a sinuous basin axial channel belt

Coarse‐grained deep‐water strata of the Cerro Toro Formation in the Cordillera Manuel Señoret, southern Chile, represent the deposits of a major channel belt (4 to 8 km wide by >100 km long) that occupied the foredeep of the Magallanes basin during the Late Cretaceous. Channel belt deposits comprise a ca 400 m thick conglomeratic interval (informally named the ‘Lago Sofia Member’) encased in bathyal fine‐grained units. Facies of the Lago Sofia Member include sandy matrix conglomerate (that show evidence of traction‐dominated deposition and sedimentation from turbulent gravity flows), muddy matrix conglomerate (graded units interpreted as coarse‐grained slurry‐flow deposits) and massive sandstone beds (high‐density turbidity current deposits). Interbedded sandstone and mudstone intervals are present locally, interpreted as inner levée deposits. The channel belt was characterized by a low sinuousity planform architecture, as inferred from outcrop mapping and extensive palaeocurrent measurements. Laterally adjacent to the Lago Sofia Member are interbedded mudstone and sandstone facies derived from gravity flows that spilled over the channel belt margin. A levée interpretation for these fine‐grained units is based on several observations, which include: (i) palaeocurrent measurements that indicate flows diverged (50° to 100°) once they spilled over the confining channel margin; (ii) sandstone beds progressively thin, away from the channel belt margin; (iii) evidence that the eroded channel base was not very well indurated, including a stepped margin and injection of coarse‐grained channel material into surrounding fine‐grained units; and (iv) the presence of sedimentary features common to levées, including slumped units inferring depositional slopes dipping away from the channel margin, lenticular sandstone beds thinning distally from the channel margin, soft sediment deformation and climbing ripples. The tectonic setting and foredeep architecture influenced deposition in the axial channel belt. A significant downstream constriction of the channel belt is reflected by a transition from more tabular units to an internal architecture dominated by lenticular beds associated with a substantially increased degree of scour. Differential propagation of the fold‐thrust belt from the west is speculated to have had a major control on basin, and subsequently channel, width. The confining influence of the basin slopes that paralleled the channel belt, as well as the likelihood that numerous conduits fed into the basin along the length of the active fold‐thrust belt to the west, suggest that proximal–distal relationships observed from large channels in passive margin settings are not necessarily applicable to axial channels in elongate basins.     

AN E – ε – ℓ TURBULENCE CLOSURE SCHEME FOR PLANETARY BOUNDARY-LAYER MODELS: THE NEUTRALLY STRATIFIED CASE

The standard E – model generates aplanetary boundary layerthat appears to be much too deep. The cause of theproblem is traced to the equation for the dissipationrate () of turbulent kinetic energy (E), specifically theparameterization of dissipation production anddestruction. In the context of atmosphericboundary-layer modelling, we argue that a part of thedissipation production should be modelled as the inputto the spectral cascade from the energy-containingpart of the spectrum, with a characteristic length , while the equilibrium imbalancebetween local production and destruction ofdissipation is modelled as proportional toE2/E, as in the standard model. Wepropose an E – – turbulence closurescheme, in which both the mixing length, m, and are prescribed. The importance ofthe equation is diminished, though itstill determines the dissipation rate in the Eequation.     

IDENTIFICATION OF SEA-FLOOR SEDIMENTS USING UNDERWAY ACOUSTICS*

Laboratory measurements, and a few in situ observations, show that saturated marine sediments have interdependent mechanical and acoustical properties, Acoustically, of particular importance are the acoustic impedance, velocity of sound and the sound attenuation coefficient of the sediment. The first two properties can be measured relatively easily from a surface ship; the measurement of attenuation however, is more problematical. It is suggested that this can be achieved by a quantitative treatment of the acoustic data collected during routine sub-bottom profiling over a variable thickness of superficial sediments. In the assessment of four different sediment locations in the Irish Sea it was found that quantitative treatment of the acoustic signals yielded both a value of the attenuation coefficient as well as a measure of the frequency dependence of the attenuation. In addition a statistical analysis of the signal intensities seems to provide an indication of the relative roughness of the bottom and sub-bottom interfaces. From the wide range of information provided the mechanical properties of the sea-floor sediment may be estimated.     

The stability of sapphirine + quartz: calculated phase equilibria in FeO–MgO–Al2O3–SiO2–TiO2–O

The presence in rocks of coexisting sapphirine + quartz has been widely used to diagnose conditions of ultra‐high‐temperature (UHT) metamorphism (>900 °C), an inference based on the restriction of this assemblage to temperatures >980 °C in the conventionally considered FeO–MgO–Al₂O₃–SiO₂ (FMAS) chemical system. With a new thermodynamic model for sapphirine that includes Fe₂O₃, phase equilibra modelling using thermocalc software has been undertaken in the FeO–MgO–Al₂O₃–SiO₂–O (FMASO) and FeO–MgO–Al₂O₃–SiO₂– TiO₂–O (FMASTO) chemical systems. Using a variety of calculated phase diagrams for quartz‐saturated systems, the effects of Fe₂O₃ and TiO₂ on FMAS phase relations are shown to be considerable. Importantly, the stability field of sapphirine + quartz assemblages extends down temperature to 850 °C in oxidized systems and thus out of the UHT range.