基于WiMAX的地质灾害应急无线通信系统探索     

达格  张丽君 《国土资源信息化》2008,(4):15-19

基于OFDM核心技术的WiMAX(全球微波接入互操作性)具有4G技术的特点。与3G和WiFi无线通讯技术相比具有明显的高速率、大容量数据传输优势。本文就基于WiMAX的地质灾害应急通讯系统的几种技术方案加以详细论述,说明WiMAX在地质灾害应急指挥中具有广阔前景。  相似文献   

Early Cretaceous Climate Changes Recorded in Magnetic Susceptibility and Color Index Variations of the Lower Liupanshan Group, Central China     

DAI Shuang  ZHU Qiang  HUANG Yongbo  DA SILVA A. Christine  ZHAO Jie  LIU Junwei  KONG Li  PENG Dongxiang  LUO Lingling  YAN Ningyun  WANG Wenjie  ZHANG Xiang 《《地质学报》英文版》2016,90(3):1011-1023

This study carried out comprehensive analysis on sedimentology, magnetic susceptibility(χlf) and color data of the continental sediments of the Liupanshan Group in Central China so as to obtain climatic change information during the 129.14–122.98 Ma interval. Based on the results of the ?lf and of the redness(a*), the section can be divided into two segments:(1) 129.14–126.3 Ma, with the lowest ?lf values and strongly variable relatively high values of redness and(2) 126.3–122.98 Ma, with high ?lf values and relatively low redness. Analysis of the lithology and facies as well as the magnetic minerals and their contents points to a detrital origin of the magnetic minerals and this allow us to interpret the relationship between magnetic susceptibility variations and climate changes. Our study shows that the climate was significantly dry and hot during the whole studied interval although the interval between 126.3 Ma and 122.98 was a little bit cooler with increased humidity.  相似文献   

全珊瑚骨料海水混凝土力学性能试验研究   总被引：3，自引：1，他引：2  

糜人杰  余红发  麻海燕  达波  袁银峰  张小平  朱海威  窦雪梅 《海洋工程》2016,34(4):47-54

为了探讨全珊瑚骨料海水混凝土的基本力学性能,并比较其与普通混凝土和轻集料混凝土的差异,通过实验系统测定了珊瑚混凝土的基本力学性能,建立了其轴心抗压强度(f_(c,m))、劈裂抗拉强度(f_(sp,m))、抗折强度(f_(t,m))与立方体抗压强度(f_(cu,m))之间的线性关系与计算公式。结果表明:在强度等级C20~C50的范围内,珊瑚混凝土的f_(c,m)和f_(sp,m)分别比普通混凝土的f_(c,m)和f_(sp,m)高出10%~48%和9%~33%,随着强度等级的提高,两种混凝土之间的差距在减小。珊瑚混凝土的f_(t,m)与普通混凝土的ft,m之间的差异规律与强度等级有关,较低强度等级的C30珊瑚混凝土ft,m比普通混凝土的f_(t,m)要高4%,而较高强度等级的C55珊瑚混凝土f_(t,m)比普通混凝土的f_(t,m)低13%。较高强度等级的C50珊瑚混凝土f_(c,m)、f_(sp,m)和f_(t,m)分别比页岩陶粒轻集料混凝土的f_(c,m)、f_(sp,m)和f_(t,m)低11%、0.9%和4%。  相似文献   

长庆中部气田奥陶纪马家沟组储层成岩模式与孔隙系统   总被引：1，自引：2，他引：1  

吴亚生何顺利  卢涛达世攀  李跃刚戴永定 《岩石学报》2006,22(8):2171-2181

长庆中部气田奥陶纪马家沟组马五～马五储层的主要成岩作用包括:(Ⅰ)准同生白云石化作用;(Ⅱ)白云石对小球状硬石膏结核(简称"膏球")和板状硬石膏晶体的交代;(Ⅲ)石膏的溶解;(Ⅳ)自生石英、自生粘土矿物在白云石晶间生长;(Ⅴ)早期方解石的充填作用;(Ⅵ)晚期方解石的充填作用;(Ⅶ)钾石盐的充填作用;(Ⅷ)去白云石化作用。其中造成孔隙的是(Ⅰ)、(Ⅱ)、(Ⅲ),破坏孔隙的主要是(Ⅴ)、(Ⅵ)、(Ⅶ)、(Ⅷ)。最重要的成岩作用是(Ⅰ)、(Ⅱ)、(Ⅲ)。主要的成岩模式有:云化-溶蚀型、云化-溶蚀-充填型、云化-溶解型、云化-交代-溶解型、云化-交代-溶解-早充填型、云化-交代-溶解-早充填-晚充填型、云化-交代-溶解-早充填-晚充填-钾石盐充填型。其中云化-溶解型、云化-交代-溶解型以及云化-溶蚀型是形成孔隙的主要成岩方式。主要的孔隙系统类型有5种:密球型、"球 胀裂缝型"、"球 晶间溶孔型"、晶模孔型、晶间溶孔型。其中,密球型、"球 胀裂缝型"、"球 晶间溶孔型"是最主要的孔隙系统类型。长庆中部气田马五段储层的发育首先受沉积微相控制,即膏球的发育;在此基础上还受成岩方式控制。膏球发育于马五、马五、马五、马五,尤其是马五。白云石对硬石膏球的交代作用和石膏的溶解作用广泛发育于马五、马五、马五、马五、马五、马五、马五、马五地层中。早期方解石、晚期方解石和钾石盐的充填作用主要发育在马五、马五、马五和马五地层中,而在马五、马五地层中不发育。膏球在马五、马五、马五不发育。所以,马五、马五、马五是最好的储集层段马五、马五是其次的储集层段。马五、马五、马五是最差的储集层段。  相似文献   

塔里木盆地喀什凹陷北缘烃源岩潜力探讨   总被引：1，自引：0，他引：1  

达江  宋岩  赵孟军  傅国友  杨芝林 《新疆地质》2007,25(1):77-80

对喀什凹陷北缘烃源岩进行了综合评价分析,通过对喀什凹陷北缘3套潜在烃源岩的分布、有机质丰度、类型、成熟度的对比分析,认为喀什凹陷北缘石炭系海相碳酸盐岩分布有限,综合评价指标较差,为非烃源岩;二叠系海陆过渡相泥岩分布较广,为差烃源岩;侏罗系煤系源岩分布虽然局限,但是厚度大,评价指标好,是喀什凹陷主要的烃源岩.石炭系碳酸盐岩和二叠系泥岩不具备为大中型气田提供烃源的潜质.  相似文献   

PRÉSENTATION DES RÉSULTATS DE L'ENQUÊTE UNESCO—AIHS SUR LES BASSINS REPRÉSENTATIFS ET EXPéRIMENTAUX DANS LE MONDE     

J. A. DA COSTA  J. JACQUET 《水文科学杂志》2013,58(4):107-119

  相似文献   

INTERMODAL TRANSPORTATION IN NORTH AMERICA AND THE DEVELOPMENT OF INLAND LOAD CENTERS*   总被引：1，自引：0，他引：1  

Brain Slack 《The Professional geographer》1990,42(1):72-83

This paper analyzes the changes that are transforming intermodal transportation in the United States and Canada. Traffic is being concentrated at a relatively small number of inland load centers that serve as regional truck distribution points, and are linked by high volume dedicated train services. Both theoretical and practical implications of the changes are examined, and a range of research questions are presented.  相似文献   

基于GIS的徐州市火灾应急救援系统设计与实现     

仲旸  李保杰  笪柳炎 《测绘与空间地理信息》2021,44(5):45-48

为了提高城市火灾应急救援效率,最大限度降低人民群众生命财产损失,以ArcGIS Engine和ArcGIS Object SDK for.Net为桌面GIS应用程序的二次开发框架,构建PC桌面端徐州市火灾应急救援系统.该系统充分利用GIS强大的海量数据存储、查询及分析的特色功能,实现数据管理、信息查询、应急救援、风险评估及案件记录等功能,可解决目前消防指挥部门中诸如人工查询低效导致火场信息不清、救援方案不明确,救援路线不佳导致救援效率低下、人工记录不全面等问题,为徐州城市火灾高效救援提供技术支持.  相似文献   

Search for Phobos and Deimos gas/dust tori using in situ observations from Mars Global Surveyor MAG/ER     

Marit Øieroset  David A. Brain  David L. Mitchell  Jasper S. Halekas  Mario H. Acuña 《Icarus》2010,206(1):189-198

More than 490 elliptical aerobraking and science phasing orbits made by Mars Global Surveyor (MGS) in 1997 and 1998 provide unprecedented coverage of the solar wind in the vicinity of the orbits of the martian moons Phobos and Deimos. We have performed a comprehensive survey of magnetic field perturbations in the solar wind to search for possible signatures of solar wind interaction with dust or gas escaping from the moons. A total of 1246 solar wind disturbance events were identified and their distribution was examined relative to Phobos, the Phobos orbit, and the Deimos orbit. We find that the spatial distribution of solar wind perturbations does not increase near or downstream of Phobos, Phobos’ orbit, or Deimos’ orbit, which would have been expected if there is significant outgassing or dust escape from the martian moons. Of the 1246 magnetic field perturbation events found in the MGS data set, 11 events were found within 2000 km of the Phobos orbit, while three events were found within 2000 km of the Deimos orbit. These events were analyzed in detail and found to likely have other causes than outgassing/dust escape from the martian moons. Thus we conclude that the amount of gas/dust escaping the martian moons is not significant enough to induce detectable magnetic field perturbations in the solar wind. In essence we have not found any clear evidence in the MGS magnetic field data for outgassing or dust escape from the martian moons.  相似文献   

Day-side ionospheric conductivities at Mars     

H.J. Opgenoorth  R.S. Dhillon  M. Lester  S.E. Milan  D. Brain 《Planetary and Space Science》2010,58(10):1139-1151

We present estimates of the day-side ionospheric conductivities at Mars based on magnetic field measurements by Mars Global Surveyor (MGS) at altitudes down to ∼100 km during aerobraking orbits early in the mission. At Mars, the so-called ionospheric dynamo region, where plasma/neutral collisions permit electric currents perpendicular to the magnetic field, lies between 100 and 250 km altitude. We find that the ionosphere is highly conductive in this region, as expected, with peak Pedersen and Hall conductivities of 0.1-1.5 S/m depending on the solar illumination and induced magnetospheric conditions. Furthermore, we find a consistent double peak pattern in the altitude profile of the day-side Pedersen conductivity, similar to that on Titan found by Rosenqvist et al. (2009). A high altitude peak, located between 180 and 200 km, is equivalent to the terrestrial peak in the lower F-layer. A second and typically much stronger layer of Pedersen conductivity is observed between 120 and 130 km, which is below the Hall conductivity peak at about 130-140 km. In this altitude region, MGS finds a sharp decrease in induced magnetic field strength at the inner magnetospheric boundary, while the day-side electron density is known to remain high as far down as 100 km. We find that such Titan-like behaviour of the Pedersen conductivity is only observed under regions of strongly draped magnetospheric field-lines, and negligible crustal magnetic anomalies below the spacecraft. Above regions of strong crustal magnetic anomalies, the Pedersen conductivity profile becomes more Earth-like with one strong Pedersen peak above the Hall conductivity peak. Here, both conductivities are 1-2 orders of magnitude smaller than the above only weakly magnetised crustal regions, depending on the strength of the crustal anomaly field at ionospheric altitudes. This nature of the Pedersen conductivity together with the structured distribution of crustal anomalies all over the planet should give rise to strong conductivity gradients around such anomalies. Day-side ionospheric conductivities on Mars (in regions away from the crustal magnetic anomalies) and Titan seem to behave in a very similar manner when horizontally draped magnetic field-lines partially magnetise a sunlit ionosphere. Therefore, it appears that a similar double peak structure of strong Pedersen conductivity could be a more general feature of non-magnetised bodies with ionised upper atmospheres, and thus should be expected to occur also at other non-magnetised terrestrial planets like Venus or other planetary bodies within the host planet magnetospheres.  相似文献