A Test of the In Situ Permeable Flow Sensor at Savannah River, SC     

Sanford Ballard  Glenn T. Barker  Ralph L. Nichols 《Ground water》1996,34(3):389-396

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测井资料在碳酸盐岩储层评价中的应用   总被引：4，自引：0，他引：4  

魏历灵  农社卿  胡国山 《新疆地质》2005,23(1):73-78

以塔河油田碳酸盐岩储集层基本特征为依据，利用常规和能谱测井资料信息比值法和重叠法等技术．致力于储集层缝、孔、洞测井响应特征敏感性评价研究，从中提取8项储层敏感性参数，并对其进行综合评判，确定出划分储层类别的标准，经过50口井的测试资料验证，采用多参数综合评判来划分储层类别是可行的，对储层的评价效果较好，使常规测井资料得到了更深入、广泛的应用。  相似文献   

Low-pressure granulite facies metamorphism in the Larsemann Hills area, East Antarctica; petrology and tectonic implications for the evolution of the Prydz Bay area   总被引：4，自引：0，他引：4  

K. STÜWE  R. POWELL 《Journal of Metamorphic Geology》1989,7(4):465-483

ABSTRACT Thermobarometric studies on various granulite facies areas along the Prydz Bay coast, East Antarctica (73°-79°E, 68°-70°S), show that, at around 1100 Ma, during a late Proterozoic orogeny, the rocks of the Larsemann Hills suffered a lower pressure metamorphic peak than the surrounding areas. Along the Prydz Bay coast, the rocks affected by this event include parts of the Vestfold Hills block plus all of the Rauer Group, the Larsemann Hills and the Munro Kerr Mountains. The dykes in the south-west corner of the Vestfold Hills were recrystallized during this event with little deformation at temperatures not quite as high as in the areas further south-west (650°C, 6.5 kbar) (Collerson et al., 1983), the Rauer Group was metamorphosed at 800°C and 7.5 kbar (Harley, 1987a), the Larsemann Hills at 750°C and 4.5 kbar, and the Munro Kerr Mountains probably at around 850°C and 5 kbar. Retrograde equilibration in the different areas occurred during decompression to about 10 km depth in all areas, followed by isobaric cooling at this depth. This paper shows that the peak metamorphism in the Larsemann Hills occurred at a pressure which is too low to have been the consequence of thermal relaxation of overthickened crust with normal mantle heat flow. Although other areas in Prydz Bay were metamorphosed at sufficiently high pressures so that their decompression paths are not inconsistent with a continental collision model, the inferred pre-metamorphic peak histories and the requirement of consistency with the Larsemann Hills, make it unlikely that collision followed by erosion-driven decompression is an appropriate model. We suggest that the thermal regime of the crust in the Larsemann Hills region was controlled by a perturbation in the asthenosphere, with magma invasion of the crust. We suggest that the 500 Ma event, represented in Prydz Bay by granitic outcrops at Landing Bluff and by several K/Ar ages from the Larsemann Hills area, was responsible for the final excavation of the terrane.  相似文献   

Modern and ancient geotherms beneath southern Africa     

Sanford Ballard  Henry N. Pollack 《Earth and Planetary Science Letters》1988,88(1-2)

Estimates of subsurface temperatures in the Archean craton of southern Africa during the Archean derived from diamond thermobarometry studies are remarkably similar to temperatures estimated for the same depths today, even though heat production in the earth and the mean global heat flow were probably substantially higher in the Archean. We present multi-dimensional numerical models for the thermal environment of the Archean craton in southern Africa during the Archean in which deep mantle heat is diverted away from the craton toward the surrounding oceanic lithosphere by a lithospheric root beneath the craton. Extrapolation of present-day models to thermal conditions appropriate for the Archean is inadequate to explain the similarity of present-day and Archean temperatures in the cratonic root. Reconciliation of the modern and ancient temperature estimates requires either relaxation of the constraints that the cratonic crustal heat production and/or the earth's mean mantle temperature were higher in the Archean than they are today, or that substantial “erosion” of the lithosphere comprising the cratonic root has occurred since the Archean. The latter possibility could perhaps result from revolatilization of the cratonic root in association with thermal perturbations in the mantle, for which there is evidence in southern Africa in the form of post-Archean tectonic and igneous activity.  相似文献   

Coastal Massachusetts pond development: edaphic,climatic, and sea level impacts since deglaciation     

Marjorie Green Winkler  Patricia R. Sanford 《Journal of Paleolimnology》1995,14(3):311-336

Kettle ponds in the Cape Cod National Seashore in southeastern Massachusetts differ in their evolution due to depth of the original ice block, the clay content of outwash in their drainage basins, and their siting in relation to geomorphic changes caused by sea-level rise, barrier beach formation, and saltmarsh development. Stratigraphic records of microfossil, carbon isotope, and sediment changes also document late-glacial and Holocene climatic changes.The ponds are separated into 3 groups, each of which follow different development scenarios. Group I ponds date from the late-glacial. They formed in clay-rich outwash, have perched aquifers and continuous lake sediment deposition. The earliest pollen and macrofossil assemblages in Group I pond sediments suggest tundra and spruce-willow parklands before 12 000 yr B.P., boreal forest between 12 000 and 10 500 yr B.P., bog/heath initiation and expansion during the Younger Dryas between 11 000 and 10 000 yr B.P., northern conifer forest between 10 500 and 9500 yr B.P., and establishment of the Cape oak and pitch pine barrens vegetation after 9500 yr B.P. Sedimentation rate changes suggest lowered freshwater levels between 9000 and 5000 yr B.P. caused by decreased precipitation on the Atlantic Coastal Plain. Lake sediment deposition began in the middle Holocene in Group II ponds which formed in clay-poor outwash. These ponds date from about 6000-5000 yr B.P. In these ponds sediment deposition began as sea level rose and the freshwater lens intersected the dry basins. The basal radiocarbon dates of these ponds and stable carbon isotope analyses of the pond sediments suggest a sea-level curve for Cape Cod Bay. Holocene topographic changes in upland and the landscape surrounding the ponds is reconstructed for this coastal area.Group III ponds in the late Holocene landscape of the Provincelands dunes originated as interdunal bogs about 1000 yr B.P. and became ponds more recently as water-levels increased. Peat formation in the Provincelands reflects climatic changes evident on both sides of the Atlantic region.This is the 8th in a series of papers published in this special AMQUA issue. These papers were presented at the 1994 meeting of the American Quaternary Association held 19–22 June, 1994, at the University of Minnesota, Minneapolis, Minnesota, USA. Dr Linda C. K. Shane served as guest editor for these papers.  相似文献   

The In Situ Permeable Flow Sensor: A Ground-Water Flow Velocity Meter   总被引：2，自引：0，他引：2  

Sanford Ballard 《Ground water》1996,34(2):231-240

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Stable and radio-isotope analysis to determine recharge timing and paleoclimate of sandstone aquifers in central and southeast Libya     

Mohamed Al Faitouri  William E. Sanford 《Hydrogeology Journal》2015,23(4):707-717

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2011年11月苏州一次灰霾天气过程分析          下载免费PDF全文

吴珂  汪婷  曾山佰  何娜 《气象与环境学报》2013,29(6):31-36

2011年11月10-14日苏州地区发生了一次严重灰霾天气过程,利用气象观测资料、探空资料及大气成分站监测资料对苏州三个站点的受污染情况进行了综合分析。结果表明：灰霾期间地面受弱气压场控制,风力较小,且有接地逆温的持续存在,大气水平和垂直输送都很弱,导致大量污染物在近地面堆积,能见度恶化;三站中昆山站灰霾持续时间最长,共计104时次,影响程度最重,重度灰霾占总数的39 %,中度和重度灰霾超过灰霾总数的一半;灰霾时各粒径颗粒物浓度均维持在较高水平,细粒子在可吸入颗粒物中占有较大比重,说明细粒子对灰霾贡献作用大,14日凌晨昆山及太仓出现大雾天气时细粒子比重甚至超过了灰霾时,而相对湿度峰值只有94 %,因此将该段天气定性为雾霾共存或者湿性霾更妥;秸秆焚烧污染期间,BC浓度明显上升,其绝对浓度要高出正常情况的3倍左右;通过CO/SO₂及PM₁₀/SO₂对比发现昆山站受秸秆焚烧污染程度要严重的多,因此推测昆山本地郊区可能也存在零星秸秆露天焚烧点。  相似文献   

Some Characteristics of a Propagating Brittle Tensile Crack     

Merle E. Hanson  Allan R. Sanford 《Geophysical Journal International》1971,24(3):231-244

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Soft X-ray diagnostics of the kinematics of high-velocity clouds     

D. A. Bone  T. W. Hartquist  P. Sanford 《Astrophysics and Space Science》1983,92(1):173-176

We have made near-infrared photometric observations of nine β-Cephei and eight δ-Scuti stars inJ, H, andK bands. The observed fluxes are in good agreement with those expected according to their spectral types. We conclude that these stars do not have any anomalous emission in these near-infrared bands.  相似文献