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1.
介绍一种以89C51为核心,通过AD和LED,实现光电经纬仪摄影机目标距离显示的方法。该方法提出了一些新的设计方案,从而使整个系统结构简单,运行可靠。 相似文献
2.
Ashley Gerard Davies Dennis L. Matson Glenn J. Veeder Torrence V. Johnson Diana L. Blaney 《Icarus》2005,176(1):123-137
The modeling of thermal emission from active lava flows must account for the cooling of the lava after solidification. Models of lava cooling applied to data collected by the Galileo spacecraft have, until now, not taken this into consideration. This is a flaw as lava flows on Io are thought to be relatively thin with a range in thickness from ∼1 to 13 m. Once a flow is completely solidified (a rapid process on a geological time scale), the surface cools faster than the surface of a partially molten flow. Cooling via the base of the lava flow is also important and accelerates the solidification of the flow compared to the rate for the ‘semi-infinite’ approximation (which is only valid for very deep lava bodies). We introduce a new model which incorporates the solidification and basal cooling features. This model gives a superior reproduction of the cooling of the 1997 Pillan lava flows on Io observed by the Galileo spacecraft. We also use the new model to determine what observations are necessary to constrain lava emplacement style at Loki Patera. Flows exhibit different cooling profiles from that expected from a lava lake. We model cooling with a finite-element code and make quantitative predictions for the behavior of lava flows and other lava bodies that can be tested against observations both on Io and Earth. For example, a 10-m-thick ultramafic flow, like those emplaced at Pillan Patera in 1997, solidifies in ∼450 days (at which point the surface temperature has cooled to ∼280 K) and takes another 390 days to cool to 249 K. Observations over a sufficient period of time reveal divergent cooling trends for different lava bodies [examples: lava flows and lava lakes have different cooling trends after the flow has solidified (flows cool faster)]. Thin flows solidify and cool faster than flows of greater thickness. The model can therefore be used as a diagnostic tool for constraining possible emplacement mechanisms and compositions of bodies of lava in remote-sensing data. 相似文献
3.
Statistical analysis of sand grain/bed collision process recorded by high-speed digital camera 总被引:1,自引:0,他引:1
A high‐speed digital camera was employed to record the sand grain/bed collision process. With image processing and a statistical method, a series of parameters of the collision process were obtained. The results show that the collision process of a grain with rebounding can be represented by two parameters: the kinetic energy restitution coefficient and the collision angle. Both parameters satisfy a normal distribution, and they are dependent on one another. With an increase of the collision angle, the distribution of the kinetic energy restitution gradually reduces from a broad to a narrow range with low values. The percentage of vertical velocity restitution coefficients greater than 1 can reach 70% or more, which ensures that the settling time of the sand grains in the air increases and that they receive more energy from the air to progress the saltation movement. 相似文献
4.
Zhou Haiyan Zhou Xun Chai Rui Yu Lan Liu Chunhui Li Liangping 《Environmental Geology》2008,53(7):1483-1489
Thermal groundwater occurs in bedrock aquifers consisting of the dolomite of the Wumishan Group of the Jixianin System and
the Cambrian carbonate in the Xiaotangshan geothermal field near the northern margin of the North China Plain, China. The
hot water in the geothermal field of basin-type discharges partly in the form of the Xiaotangshan hot spring under natural
conditions. The hot water has TDS of less than 600 mg/L and is of Na·Ca-HCO3 type. The geothermal water receives recharge from precipitation in the mountain area with elevation of about 500 m above
sea level to the north of the spring. Thermal groundwater flows slowly south and southeast through a deep circulation with
a residence time of 224 years estimated with the Ra–Rn method. The Xiaotangshan hot spring dried up in the middle of the 1980s
owing to the increasing withdrawal of the hot water in the geothermal field in the past decades. The water level of the geothermal
system still falls continually at an annual average rate of about 2 m, although water temperature changes very little, indicating
that the recharge of such a geothermal system of basin-type is limited. Over-exploitation has a dramatic impact on the geothermal
system, and reduction in exploitation and reinjection are required for the sustainable usage of the hot water. 相似文献
5.
锌、铝及其合金涂层对钢铁的防护,不仅对阴极起保护作用(Gartland,1987), 对涂层本身也具有良好的抗腐蚀性能。此外,涂层中金属微粒表面形成的致密氧化膜,也起到了防腐蚀的作用。在不同大气环境下,锌、铝有良好的耐蚀性,其腐蚀速率比钢铁要低得多(李言涛,1998)。采用热喷涂锌、铝及其合金涂层对钢铁构件和构筑物进行长效防护早在20世纪20年代就已开始应用,至今仍是普遍采用的防护措施,并在继续发展(李守本等,1989)。20年代初,法国首先用于海水闸门的防腐;40年代美国用于墨西哥湾的海上井架和海上输油管以及舰船的防腐;60年代英、法、德等国海军将这一技术扩大应用到舰船的上部结构和船壳。而金属热喷涂技术在海洋工程中使用非常有限,第一次使用热喷铝涂层防护近海平台的实例是Conoco公司在北海的Murchison结构上的锥形塔,并且已获得了4a良好的使用效能(Fisher et al.,1987;Shaw et al.,1985)。1984年6月,Hutton张力支柱平台(TLP)在北海下水(水深148 m)安装。系链、升降机和锥形塔均采用火焰热喷涂技术喷涂铝涂层进行防护(Tyson,1985)。1992年6月,Hotton平台使用8a后,对升降机绳索进行观察,在飞溅区没有发现腐蚀现象,也没有检测到褐色渗漏效应(Fisher et al.,1995)。 相似文献
6.
7.
简要分析了非量测数码相机哈苏H1D在南极中山站及拉斯曼丘陵地区所获取的影像数据的几何精度,阐明了利用该影像数据进行空中三角测量,DLG,DOM制作的技术流程及作业过程中出现问题的处理方法。 相似文献
8.
东北大兴安岭多年冻土区工程地质特征及评价 总被引:4,自引:1,他引:3
土体在冻结状态具有极高的压缩模量, 具有弹性体的工程地质特征。但是在冻土地温升高过程中, 这种特征急剧衰减, 产生蠕变和流变, 建筑物地基强度降低, 导致建筑物基础破坏。同时土体在冻结过程中产生的冻胀作用也将导致建筑物基础的破坏。东北大兴安岭地区多年冻土为高纬度低海拔多年冻土, 其分布具有明显纬度地带性特点。本文在分析该区多年冻土分布特征及冻土工程地质特点的基础上, 对由于土体的冻胀和融沉导致的建筑物基础的危害进行分类研究, 针对性的提出了用热棒降低土体温度以保证多年冻土稳定及用排水的方法减少水对建筑物地基多年冻土影响的工程病害处理措施。 相似文献
9.
10.
An updated analysis of geothermal data from the highland area of eastern Brazil has been carried out and the characteristics of regional variations in geothermal gradients and heat flow examined. The database employed includes results of geothermal measurements at 45 localities. The results indicate that the Salvador craton and the adjacent metamorphic fold belts northeastern parts of the study area are characterized by geothermal gradients in the range of 6–17°C/km. The estimated heat flow values fall in the range of 28–53 mW/m2, with low values in the cratonic area relative to the fold belts. On the other hand, the São Francisco craton and the intracratonic São Francisco sedimentary basin in the southwestern parts are characterized by relatively higher gradient values, in the range of 14–42°C/km, with the corresponding heat flow values falling in the range of 36–89 mW/m2. Maps of regional variations indicate that high heat flow anomaly in the São Francisco craton is limited to areas of sedimentary cover, to the west of the Espinhaço mountain belt. Crustal thermal models have been developed to examine the implications of the observed intracratonic variations in heat flow. The thermal models take into consideration variation of thermal conductivity with temperature as well as change of radiogenic heat generation with depth. Vertical distributions of seismic velocities were used in obtaining estimates of radiogenic heat production in crustal layers. Crustal temperatures are calculated based on a procedure that makes simultaneous use of the Kirchoff and Generalized Integral Transforms, providing thereby analytical solutions in 2D and 3D geometry. The results point to temperature variations of up to 300°C at the Moho depth, between the northern Salvador and southern São Francisco cratons. There are indications that differences in rheological properties, related to thermal field, are responsible for the contrasting styles of deformation patterns in the adjacent metamorphic fold belts. 相似文献