测绘工程专业人才培养模式的研究与实践

本文从学校定位及专业实际出发,探讨了测绘工程专业目前存在的问题,研究测绘工程专业人才培养模式和培养计划的基本思路及课程结构体系.从专业设置管理体制的建立、测绘工程专业专项建设经费的设立、实训基地的建设、现代化教学手段等方面对人才培养模式及培养计划实施的保障体系进行了探讨.     

Case study of a giant debris flow in the Wenjia Gully, Sichuan Province, China

The debris flow, which was triggered in the Wenjia Gully on August 13, 2010, is an extreme example of mass movement events, which occurred after the Wenchuan earthquake of May 12, 2008. This Earthquake triggered in the Wenjia Gully the second largest co-seismic landslide, which can be classified as a rockslide-debris avalanche. A lot of loose sediments was deposited in the basin. In the main so called Deposition Area II of this landslide, with a volume of 30?×?10⁶?m³, flash floods can easily trigger debris flows because of the steep bottom slope and the relative small grain sizes of the sediments. The largest debris flow of August 13, 2010 destroyed the most downstream dam in the catchment during a heavy rain storm. The debris flow with a peak discharge of 1,530?m³/s and a total volume of 3.1?×?10⁶?m³ caused the death of 7 persons, 5 persons were missing, 39 persons were injured and 479 houses buried. After three rainy seasons, only 16?% of the landslide-debris deposition was taken away by 5 large-scale debris flow events. Since the threshold for rainfall triggered debris flows in the Wenjia Gully and other catchments drastically decreased after the Wenchuan Earthquake, new catastrophic events are expected in the future during the rainy season.     

Crustal structure beneath the Songpan—Garze orogenic belt

The Benzilan-Tangke deepseismic sounding profile in the western Sichuan region passes through the Song-pan-Garze orogenic belt with trend of NNE.Based on the travel times and the related amplitudes of phases in the record sections,the 2-D P-wave crustal structure was ascertained in this paper.The velocity structure has quite strong lateral variation along the profile.The crust is divided into 5layers,where the first,second and third layer belong to the upper crust,the forth and fifth layer belong to the lower crust.The low velocity anomaly zone gener-ally exists in the central part of the upper crust on the profile,and it integrates into the overlying low velocity basement in the area to the north of Ma‘erkang.The crustal structure in the section can be divided into 4parts:in the south of Garze-litang fault,between Garze-Litang fault and Xianshuihe fault,between Xianshuihe fault and Longriba fault and in the north of Longriba fault,which are basically coincided with the regional tectonics division.The crustal thickness decreases from southwest to northeast along the profile,that is ,from62km in the region of the Jinshajiang River to 52km in the region of the Yellow River.The Moho discontinuity does not obviously change across the Xianshuihe fault basesd on the PmP phase analysis.The crustal average velocity along the profile is lower,about 6.30 km/s.The Benzilan-Tangke profile reveals that the crust in the study area is orogenic.The Xianshuihe fault belt is located in the central part of the profile,and the velocity is positive anomaly on the upper crust,and negative anomaly on the lower crust and upper mantle.It is considered as a deep tectonhic setting in favor of strong earthquake‘s accumulation and occurrence.     

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斜方蓝辉铜矿在我国的发现及其微结构

作者在我国福建省上杭紫金山铜矿中发现了一种具有页片构造的Ｃｕ－Ｓ矿物。其基质相的化学式可表示为Ｃｕ１．７５６Ｓ,与１９６９年在日本发现的斜方蓝辉铜矿的化学式一致,这是该矿物在我国的首次发现;该矿物页片相的化学式可表示为Ｃｕ１．６８４Ｓ,是笔者未曾描述过的一种新的Ｃｕ－Ｓ矿物相,该矿物基质相和页片相混合的Ｘ射线衍射图谱上的绝大多数峰与合成斜方蓝辉铜矿的衍射峰可对应。由此,笔者认为上述成分略有差异的连     

\"西气东输\"工程沿线煤层气资源开发潜力评价

“西气东输”工程经过多个大型煤层气田,总资源量近１０万亿ｍ＾３,相当于塔里木盆地的天然气资源量,工程沿线的沁水,鄂尔多斯盆地是我国煤层气勘探开发的重点区域,已经取得了煤层气产气量的突破。“西气东输”工程的实施,为勘探开发煤层气创造了管网条件。     

长输管道抗震研究的新进展

本文主要从以下4个方面:地震对长输管道的危害、长输管道震害的研究方法、管道抗震分析和管道抗震的措施,介绍了近几年长输管道抗震方面的研究进展,指出了今后长输管道的研究方向。     

地震观测仪器自动监控软件设计与实现

结合地震地球物理观测台网台站监测工作实际,研制一款地震观测仪器自动监控软件。该软件适用于不同网络环境下IP类仪器设备的网络实时或定时自动监控,地球物理观测类仪器时钟、状态和观测数据的定时自动监控,能自动识别当日观测数据中的无效数据、变幅异常、干扰、地震和限幅等信息,无需借助其他硬件和软件即可将告警信息以短信方式发送给值班人员和管理人员,可实现对仪器原始观测数据的自动备份和手动恢复,及对仪器的一键重启和校正时钟等控制类操作,无需跨平台操作即可查看当日观测数据曲线及分析数据的完整性和有效性,从而实现对仪器的统一高效管理。     

Generation and evolution of interplanetary slow shocks

It is well known that most MHD shocks observed within 1 AU are MHD fast shocks. Only a very limited number of MHD slow shocks are observed within 1 AU. In order to understand why there are only a few MHD slow shocks observed within 1 AU, we use a one-dimensional, time-dependent MHD code with an adaptive grid to study the generation and evolution of interplanetary slow shocks (ISS) in the solar wind. Results show that a negative, nearly square-wave perturbation will generate a pair of slow shocks (a forward and a reverse slow shock). In addition, the forward and the reverse slow shocks can pass through each other without destroying their characteristics, but the propagating speeds for both shocks are decreased. A positive, square-wave perturbation will generate both slow and fast shocks. When a forward slow shock (FSS) propagates behind a forward fast shock (FFS), the former experiences a decreasing Mach number. In addition, the FSS always disappears within a distance of 150R_⊙ (where R_⊙ is one solar radius) from the Sun when there is a forward fast shock (with Mach number \geq1.7) propagating in front of the FSS. In all tests that we have performed, we have not discovered that the FSS (or reverse slow shock) evolves into a FFS (or reverse fast shock). Thus, we do not confirm the FSS-FFS evolution as suggested by Whang (1987).