Possibilities of GPS kinematic measurements for geological survey in East Slovakia

This paper deals with transformation procedures for observed GPS data from the world geodetic system WGS-84 into the national geodetic grid datum S-UTCN (system of united trigonometric cadaster network) and Baa (the Baltic Sea after adjustment). Transformation from WGS-84 into SUTCN is performed most frequently by means of the 7-element Helmert transformation with three identical points. Geodetic network was adjusted by two ways.     

Chandra observations of the X-ray jet in 3C 66B

Our Chandra observation of the FR I radio galaxy 3C 66B has resulted in the first detection of an X-ray counterpart to the previously known radio, infrared and optical jet. The X-ray jet is detected up to 7 arcsec from the core and has a steep X-ray spectrum, α ≈1.3±0.1 . The overall X-ray flux density and spectrum of the jet are consistent with a synchrotron origin for the X-ray emission. However, the inner knot in the jet has a higher ratio of X-ray to radio emission than the others. This suggests that either two distinct emission processes are present or differences in the acceleration mechanism are required; there may be a contribution to the emission from the inner knot from an inverse Compton process or it may be the site of an early strong shock in the jet. The peak of the brightest radio and X-ray knot is significantly closer to the nucleus in the X-ray than in the radio, which may suggest that the knots are privileged sites for high-energy particle acceleration. 3C 66B's jet is similar both in overall spectral shape and in structural detail to those in more nearby sources such as M87 and Centaurus A.     

Cygnus X-3 with ISO: investigating the wind

We have observed the energetic binary Cygnus X-3 in both quiescent and flaring states between 4 and 16 μm using the ISO satellite. We find that the quiescent source shows the thermal free–free spectrum typical of a hot, fast stellar wind, such as from a massive helium star. The quiescent mass-loss rate arising from a spherically symmetric, non-accelerating wind is found to be in the range (0.4–2.9)×10⁻⁴ M_⊙ yr⁻¹, consistent with other infrared and radio observations, but considerably larger than the 10⁻⁵ M_⊙ yr⁻¹ deduced from both the orbital change and the X-ray column density. There is rapid, large-amplitude flaring at 4.5 and 11.5 μm at the same time as enhanced radio and X-ray activity, with the infrared spectrum apparently becoming flatter in the flaring state. We believe that non-thermal processes are operating, perhaps along with enhanced thermal emission.     

A Chandra detection of the radio hotspot of 3C 123

Chandra X-ray Observatory observations of the powerful, peculiar radio galaxy 3C 123 have resulted in an X-ray detection of the bright eastern hotspot, with a 1-keV flux density of ∼5 nJy. The X-ray flux and spectrum of the hotspot are consistent with the X-rays being inverse-Compton scattering of radio synchrotron photons by the population of electrons responsible for the radio emission ('synchrotron self-Compton emission') if the magnetic fields in the hotspot are close to their equipartition values. 3C 123 is thus the third radio galaxy to show X-ray emission from a hotspot which is consistent with being in equipartition. Chandra also detects emission from a moderately rich cluster surrounding 3C 123, with L _X(2–10 keV)=2×10⁴⁴ erg s⁻¹ and kT ∼5 keV, and absorbed emission from the active nucleus, with an inferred intrinsic column density of 1.7×10²² cm⁻² and an intrinsic 2–10 keV luminosity of 10⁴⁴ erg s⁻¹.     

面向对象和DEM的ZY-1 02C影像湿地提取研究

本文运用面向对象分类与DEM数据相结合的方法,对资源卫星一号02C卫星遥感影像进行湿地提取。探索了基于对象与DEM信息的提取技术,在02C影像湿地的提取应用,对研究我国国产卫星在湿地监测和保护方面有重要的意义。研究结果表明：（1）面向对象的遥感影像信息提取方法,可同时兼顾影像光谱信息及空间信息,适用于02C影像的湿地提取,精度得到明显提高;（2）基于对象与DEM信息的提取方法,使沼泽地与草地相混淆的现象明显减轻,湿地分类精度进一步提高,该方法适用于高分辨率遥感影像的湿地提取研究;（3）基于对象与DEM信息提取的水田、水体、沼泽地及河滩的精度,分别为88.46%、97.44%、86.96%和83.33%,满足资源卫星一号02C遥感影像对湿地进行监测和保护的需要。     

89C51实现光电经纬仪摄影机目标距离的显示

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。     

黄河一级支流水土保持“3S”分析应用

改善黄河流域生态环境是推动西部大开发的有力保证。本文以黄河一级支流为单元,以秃尾河、皇甫川和窟野河为重点研究对象,介绍了如何利用GPS、RS和GIS相结合的技术,动态监测黄河流域水土流失情况,为黄河流域环境治理提供科学依据。     

基于FLAC3D数值模拟的老采空区剩余沉降量分析计算—以山东枣庄安博化工项目为例

空区的剩余沉降值计算是采空区地质灾害危险程度一种定量分析的方法,利用FLAC3D直接模拟早期采煤形成的老采空区塌陷状态,计算出老采空区的剩余沉降量。以山东枣庄安博化工项目为例,首先采用物探、钻探手段探测老采空区深度、顶板塌落与破碎状况以及地质地层信息,其次结合岩心试验地质材料参数结果进行FLAC3D模拟,计算自重作用下采空区剩余沉降量,以及加载建筑后老采空区剩余沉降值,对比了传统概率积分法计算沉降值,结果基本一致,说明计算方法是可靠的。最后分析加载应力与破碎带剩余沉降值的数量关系。为老采空区土地稳定性评估以及剩余沉降量的计算方法提供科学依据与借鉴。     

面向山地地区的区域地质三维模型构建

针对山地地区地质构造复杂的特点,研究现有三维地质模型构建方法。结合已有地质资料,设计从构建剖面框架、绘制剖面到构建地质模型等流程,构建山地地区的区域地质三维模型,实现区域地质三维模型在三维数字城市平台的可视化集成模拟,以及三维场景中对区域地质的管理查询。