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51.
X射线衍射数据分析系统评价   总被引:3,自引:1,他引:3  
以贵州省高灰、高污染组分煤中矿物质的分析为例,应用Bruker AXS D8 Advance衍射仪测得煤中矿物相的X射线衍射图谱,分别应用数据分析系统EVA 12.0、X’Pert HighScore 2.0和MDI Jade 5.0对矿物物相组成的原始测试数据进行定性分析,通过对比分析过程和结果的差异比较了三款软件系统之间的异同和优劣。  相似文献   
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53.
介绍了河南省气象台与地市局、国家基本站之间依托于邮电部门的X.25分组交换网组建的全省X.25分组交换网的设计思想和具体实现。  相似文献   
54.
有棘无棘两种表型栉江珧28S和COI基因序列差异的比较   总被引:1,自引:0,他引:1  
在形态学分析的基础上,对有棘和无棘两种不同表型栉江珧(Atrina pectinata)的28S rDNA和COI基因片段进行序列分析比较.结果显示这两种表型的DNA序列差异很小,28S rDNA(1 075 bp)无差异,而COI(659 bp)碱基差异最大为1.5%,不能提供这两种表型的栉江珧划分为两个种的证据.  相似文献   
55.
In organic soils, hydraulic conductivity is related to the degree of decomposition and soil compression, which reduce the effective pore diameter and consequently restrict water flow. This study investigates how the size distribution and geometry of air‐filled pores control the unsaturated hydraulic conductivity of peat soils using high‐resolution (45 µm) three‐dimensional (3D) X‐ray computed tomography (CT) and digital image processing of four peat sub‐samples from varying depths under a constant soil water pressure head. Pore structure and configuration in peat were found to be irregular, with volume and cross‐sectional area showing fractal behaviour that suggests pores having smaller values of the fractal dimension in deeper, more decomposed peat, have higher tortuosity and lower connectivity, which influences hydraulic conductivity. The image analysis showed that the large reduction of unsaturated hydraulic conductivity with depth is essentially controlled by air‐filled pore hydraulic radius, tortuosity, air‐filled pore density and the fractal dimension due to degree of decomposition and compression of the organic matter. The comparisons between unsaturated hydraulic conductivity computed from the air‐filled pore size and geometric distribution showed satisfactory agreement with direct measurements using the permeameter method. This understanding is important in characterizing peat properties and its heterogeneity for monitoring the progress of complex flow processes at the field scale in peatlands. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   
56.
从黔南、桂北的航天遥感图像上可以清楚地看出,地表的宏观岩溶地貌明显地受控于区域性大型“X”共轭节理系统,此类节理构成一幅巨型的渗滤网,成为大气降水下渗的主要通道,从而导致被其穿透的岩石遭受溶蚀,形成以线性岩溶谷地为主体的岩溶景观。即水平地层分布区,呈片状“X”形网络结构;直立地层分布区,呈羽状条带结构。水体下渗至潜水面后,将主要沿“X”节理走向向当地最低侵蚀基准面排泄,从而形成复杂的地下管道网络系统。首次利用网上Google Earth影像研究喀斯特环境,解决了只能依赖航片和卫星照片才能研究地球地貌的瓶颈,这对地貌研究和喀斯特石漠化的研究和治理提供了廉价便利的影像材料。  相似文献   
57.
主要介绍在CorelDRAW X5中通过VBA的程序开发环境下实现线渐变的方法,通过开发出河流渐变工具,以单线河流渐变为例,解决了通过CorelDRAW X5进行地图制图过程中遇到的单线河流渐变的问题。  相似文献   
58.
We present archival Rossi X-ray Timing Explorer ( RXTE ) and simultaneous Advanced Satellite for Cosmology and Astrophysics ( ASCA ) data of the eclipsing low mass X-ray binary (LMXB) X 1822−371. Our spectral analysis shows that a variety of simple models can fit the spectra relatively well. Of these models, we explore two in detail through phase-resolved fits. These two models represent the case of a very optically thick and a very optically thin corona. While systematic residuals remain at high energies, the overall spectral shape is well approximated. The same two basic models are fitted to the X-ray light curve, which shows sinusoidal modulations interpreted as absorption by an opaque disc rim of varying height. The geometry we infer from these fits is consistent with previous studies: the disc rim reaches out to the tidal truncation radius, while the radius of the corona (approximated as spherical) is very close to the circularization radius. Timing analysis of the RXTE data shows a time-lag from hard to soft consistent with the coronal size inferred from the fits. Neither the spectra nor the light curve fits allow us to rule out either model, leaving a key ingredient of the X 1822−371 puzzle unsolved. Furthermore, while previous studies were consistent with the central object being a 1.4 M neutron star, which has been adopted as the best guess scenario for this system, our light curve fits show that a white dwarf or black hole primary can work just as well. Based on previously published estimates of the orbital evolution of X 1822−371, however, we suggest that this system contains either a neutron star or a low mass (≲2.5 M) black hole and is in a transitional state of duration shortward of 107 yr.  相似文献   
59.
为探讨高原牌70kN和进口120,210kN瓷绝缘子的成分和结构性能,中采用原子吸收光谱(AAS)和X射线衍射(XRD)方法,对三类产品进行了检测。结果表明,有效成分除K2O外,70kN和210kN的SiO2,Al2O3,Fe2O3含量接近,主晶相基本相同,有刚玉,莫来石、石英和长石等;结晶相总量:70kN35%,120kN40%,210kN48%,这表明机械强度愈大,结晶相含量愈高,只需调整70kN原样的部分成分,粒度和工艺,即生产出高等级(如210kN)瓷绝缘子。  相似文献   
60.
The strong spectral interference between Br‐ and Al‐induced X‐ray lines hampers the utilisation of electron probe microanalysis (EPMA) for measuring Br mass fractions in Al‐bearing minerals and glasses. Through measuring Br‐free Al‐bearing materials, we established an EPMA method to quantify the overlap from AlKα on BrLβ, which can be expressed as a linear function of the Al2O3 content. The count rate of the BrLβ peak signal was enhanced by high beam currents and long measurement times. Application of this EPMA method to Al‐ and Br‐bearing materials, such as sodalite and scapolite, and to five experimental glasses yielded Br mass fractions (in the range of 250–4000 μg g?1) that are consistent with those measured by microbeam synchrotron X‐ray fluorescence (μ‐SXRF) spectrometry. The EPMA method has an estimated detection limit of ~ 100–300 μg g?1. We propose that this method is useful for measuring Br mass fractions (hundreds to thousands of μg g?1) in Al‐bearing minerals and glasses, including those produced in Br‐doped experiments. In addition, the natural marialitic scapolite (ON70) from Mpwapwa (Tanzania) containing homogeneously distributed high mass fractions of Br (2058 ± 56 μg g?1) and Cl (1.98 ± 0.03% m/m) is an ideal reference material for future in situ analyses.  相似文献   
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