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51.
某港口堆场地基上部5.0m系吹填而成,地表下18m范围均属软土,经真空预压初级加固后地基承载力仅在80—90kPa,局部区域上部淤泥土层土性指标较差,含水量大于50%,地基承载力不足60kPa。为了使地基达到230kPa的承载要求,设计采用深层搅拌法加固超软弱地基。通过现场成桩工艺试验和检测表明,桩身水泥土强度在90d龄期时大于1.80MPa,单桩承载力标准值大于150kN,以φ600桩径、桩长13.5m、置换率为0.308和φ500桩径、桩长13.5m、置换率为0.267两种方案布置的复合地基承载力标准值均超过了230kPa的设计要求。试验结果表明,深层搅拌法在港口超软弱地基土应用只要施工工艺适当,完全可以使地基承载力提高2—3.5倍以土,从而节省大量的工程投资。 相似文献
52.
融冰季节北极破碎冰区热通量的初步研究 总被引:5,自引:1,他引:5
利用航空遥感数字影像的解析结果和实测气象,海洋和海冰资料,定量研究了夏季融冰期北极破碎冰区的热通量,计算了海洋对大气的热贡献,结果表明,在北极夏季海冰融化时,短波辐射远远大于感热和潜热通量,是表面热通量的决定因素,海洋对大气的热贡献主要由长波辐射决定,在观测期间,海洋对大气的热贡献为38~104Wm^-2,这部分热量的大小与海冰的密集度有关,当海冰密集度小于0.8时,海洋对大气的热贡献随海冰密度度的增大而减小,而当海冰密集度超过0.8以后,该热通量将随海冰密集度的增大而增大。 相似文献
53.
Impact of Montmorillonite and Calcite on Release and Adsorption of Cyanobacterial Fatty Acids at Ambient Temperature 总被引:1,自引:0,他引:1
Minerals might act as important sorbents of sedimentary organic matter and reduce biodegradation, which favors the formation of hydrocarbon source rocks in the earth's history. Since most organic matter is degraded during the sinking process, at ambient temperature, it is important to investigate the adsorption capacity of different minerals during this process, to assess the organic loss from primary productivity to sedimentary organic matter. In this study, montmorillonite and calcite have been selected to study the impact of different minerals on the release, adsorption, and deposition of cyanobacterial (Synechococcus elonpata) fatty acids (FAs) at ambient temperature. Gas chromatography (GC), gas chromatography-mass spectrometry (GC-MS) have been utilized to detect the variation in fatty acids. Primary results suggest that minerals have a different impact on dissolved organic matter. Montmorillonite can specifically enhance the release of fatty acids from cyanobacterial cells by lowering the pH values of the solution. The adsorption of the dissolved organic matter by montmorillonite will also be enhanced under a lower pH value. Conjunction of fatty acids with montmorillonite to form a complex will favor the sinking and preservation of these organics. Selective adsorption is observed among fatty acids with different carbon numbers. In contrast, calcite does not show any impact on the release and adsorption of organic matter even though it is reportedly capable of acting as a catalyst during the transformation of organic matter at high temperature. The primary data bridge a link between primary productivity and sedimentary organic matter, suggesting the relative importance of claystones in the formation of hydrocarbon source rocks in the earth's history. 相似文献
54.
特种罐在能源的储备和运输中具有重要意义,在研究特种罐现有容量计量技术的基础上,自主创新提出了基于放样原理和测量机器人实现特种罐容量快速和精密计量的原理和方法。将特种罐容量计量转化为点位放样问题,较好地克服了全站仪现有测量技术的缺点,并利用软件实现了特种罐容量计量的数据采集、数据计算、数据修正和报表输出的一体化。通过实际测量数据,分析了该方法的测量精度和测量效率。 相似文献
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Based on the theory of thermal conductivity, in this paper we derived a formula to estimate the prolongation period (AtL) of cooling-crystallization process of a granitic melt caused by latent heat of crystallization as follows:△tL=QL×△tcol/(TM-TC)×CP where TM is initial temperature of the granite melt, Tc crystallization temperature of the granite melt, Cp specific heat, △tcol cooling period of a granite melt from its initial temperature (TM) to its crystallization temperature (Tc), QL latent heat of the granite melt.
The cooling period of the melt for the Fanshan granodiorite from its initial temperature (900℃) to crystallization temperature (600℃) could be estimated -210,000 years if latent heat was not considered. Calculation for the Fanshan melt using the above formula yields a AtL value of -190,000 years, which implies that the actual cooling period within the temperature range of 900°-600℃ should be 400,000 years. This demonstrates that the latent heat produced from crystallization of the granitic melt is a key factor influencing the cooling-crystallization process of a granitic melt, prolongating the period of crystallization and resulting in the large emplacement-crystallization time difference (ECTD) in granite batholith. 相似文献
The cooling period of the melt for the Fanshan granodiorite from its initial temperature (900℃) to crystallization temperature (600℃) could be estimated -210,000 years if latent heat was not considered. Calculation for the Fanshan melt using the above formula yields a AtL value of -190,000 years, which implies that the actual cooling period within the temperature range of 900°-600℃ should be 400,000 years. This demonstrates that the latent heat produced from crystallization of the granitic melt is a key factor influencing the cooling-crystallization process of a granitic melt, prolongating the period of crystallization and resulting in the large emplacement-crystallization time difference (ECTD) in granite batholith. 相似文献
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Sukanta Roy Labani Ray Anurup Bhattacharya R. Srinivasan 《International Journal of Earth Sciences》2008,97(2):245-256
The Late Archaean Closepet Granite batholith in south India is exposed at different crustal levels grading from greenschist
facies in the north through amphibolite and granulite facies in the south along a ∼400 km long segment in the Dharwar craton.
Two areas, Pavagada and Magadi, located in the Main Mass of the batholith, best represent the granitoid of the greenschist
and amphibolite facies crustal levels respectively. Heat flow estimates of 38 mW m−2 from Pavagada and 25 mW m−2 from Magadi have been obtained through measurements in deep (430 and 445 m) and carefully sited boreholes. Measurements made
in four boreholes of opportunity in Pavagada area yield a mean heat flow of 39 ± 4 (s.d.) mW m−2, which is in good agreement with the estimate from deep borehole. The study, therefore, demonstrates a clear-cut heat flow
variation concomitant with the crustal levels exposed in the two areas. The mean heat production estimates for the greenschist
facies and amphibolite facies layers constituting the Main Mass of the batholith are 2.9 and 1.8 μW m−3, respectively. The enhanced heat flow in the Pavagada area is consistent with the occurrence of a radioelement-enriched 2-km-thick
greenschist facies layer granitoid overlying the granitoid of the amphibolite facies layer which is twice as thick as represented
in the Magadi area. The crustal heat production models indicate similar mantle heat flow estimates in the range 12–14 mW m−2, consistent with the other parts of the greenstone-granite-gneiss terrain of the Dharwar craton. 相似文献