土壤、大气尘中晶体的组成及其物源指示意义——以长沙、株洲和湘潭地区为例     

张广平吴堑虹  戴塔根方建武张建新  徐海珍苏调红 《地质通报》2007,26(11):1459-1462

基于长沙、株洲和湘潭地区大气尘(可吸入颗粒和近地表积尘)和表层土壤的X-射线衍射(XRD)分析数据,采用微量相鉴定方法获得的结果显示,大气尘和表层土壤中包含石英、石膏、方解石、白云石、硫酸镉等自然矿物及SiS_2、NiTi、Cd_3As_2、FeOCl等非自然源晶体。比较了长沙、株洲、湘潭地区大气尘与表层土壤的晶体组成,分析了大气尘矿物及非自然源晶体的空间分布,探讨了其环境指示意义。  相似文献   

Solubility of FeO in (Mg,Fe)SiO₃ perovskite and the post-perovskite phase transition     

Shigehiko Tateno  Kei Hirose  Nagayoshi Sata  Yasuo Ohishi 《Physics of the Earth and Planetary Interiors》2007,160(3-4):319-325

Phase relations in Mg_0.5Fe_0.5SiO₃ and Mg_0.25Fe_0.75SiO₃ were investigated in a pressure range from 72 to 123 GPa on the basis of synchrotron X-ray diffraction measurements in situ at high-pressure and -temperature in a laser-heated diamond-anvil cell (LHDAC). Results demonstrate that Mg_0.5Fe_0.5SiO₃ perovskite is formed as a single phase at 85–108 GPa and 1800–2330 K, indicating a high solubility of FeO in (Mg,Fe)SiO₃ perovskite at high pressures. Post-perovskite appears coexisting with perovskite in Mg_0.5Fe_0.5SiO₃ above 106 GPa at 1410 K, the condition very close to the post-perovskite phase transition boundary in pure MgSiO₃. The coexistence of perovskite and post-perovskite was observed to 123 GPa. In addition, post-perovskite was formed coexisting with perovskite also in Mg_0.25Fe_0.75SiO₃ bulk composition at 106–123 GPa. In contrast to earlier experimental and theoretical studies, these results show that incorporation of FeO stabilizes perovskite at higher pressures. This could be due to a larger ionic radius of Fe²⁺ ion, which is incompatible with a small Mg²⁺ site in the post-perovskite phase.  相似文献   

肺炎性假瘤的CT诊断与鉴别诊断     

毕纯龙  万霞  杨立国  张慰 《CT理论与应用研究》2007,16(1):77-80

目的: 分析肺炎性假瘤的CT表现.方法: 对32例经手术病理证实的肺炎性假瘤的CT及临床资料进行回顾性分析.结果: 病灶多位于肺胸膜下,广基地与胸膜相连;多呈圆形或类圆形,边缘光滑,直径2-5cm,密度均匀;边缘可见粗长毛刺,棘状突起或浅分叶;可有淋巴结肿大.结论: 全面综合地分析肺炎性假瘤的CT表现特征,结合肺内感染病史,肺炎性假瘤的正确诊断与鉴别诊断是很有帮助.  相似文献   

Thermal alteration of coal in the Khasyn coalfield, Magadan region, Russia     

I.E. Stukalova  O.V. Rusinova 《International Journal of Coal Geology》2007,71(4):462

The Early Cretaceous coal deposits of the Khasyn coalfield are intruded by Palaeogene diabase dikes. The coal has vitrinite reflectance values of 2.0–2.5% R_o, and characteristics of normal anthracite at some distance from the dikes, but at direct contact with the dike two morphological coal varieties occur: coal inclusions in the diabase dike and dispersed carbonaceous matter within the dike rock. Both types of coaly matter have properties typical of anthracites: strong anisotropy, altered internal structure and high vitrinite reflectance values ranging from 3.8 to 5.5% R_o. The X-ray diffraction measurements of the interplanar spacing d(002) and the crystallite sizes Lc and La show rather similar values for coal inclusions in the dike and dispersed carbonaceous matter. The additional reflection at 3.37 Å, corresponding to semi-graphite admixture, occurs in the coal and carbonaceous matter inside the dike and is absent in the natural coal outside the dike.  相似文献   

Simulating coseismic deformation of quartz in the middle crust and fabric evolution during postseismic stress relaxation — An experimental study   总被引：3，自引：0，他引：3  

Claudia A. Trepmann  Bernhard Stckhert  Dorothe Dorner  Rasoul Hamidzadeh Moghadam  Martina Küster  Klaus Rller 《Tectonophysics》2007,442(1-4):83-104

Non-steady state deformation and annealing experiments on vein quartz are designed to simulate earthquake-driven episodic deformation in the middle crust. Three types of experiments were carried out using a modified Griggs-type solid medium deformation apparatus. All three start with high stress deformation at a temperature of 400 °C and a constant strain rate of 10^− 4 s^− 1 (type A), some are followed by annealing in the stability field of α-quartz for 14–15 h at zero nominal differential stress and temperatures of 800–1000 °C (type A + B), or by annealing for 15 h at 900 °C and at a residual stress (type A + C).The quartz samples reveal a very high strength > 2 GPa at a few percent of permanent strain. The microstructures after short-term high stress deformation (type A) record localized brittle and plastic deformation. Statisc annealing (type A + B) results in recrystallisation restricted to the highly damaged zones. The new grains aligned in strings and without crystallographic preferred orientation, indicate nucleation and growth. Annealing at non-hydrostatic conditions (type A + C) results in shear zones that also develop from deformation bands or cracks that formed during the preceding high stress deformation. In this case, however, the recrystallised zone is several grain diameters wide, the grains are elongate, and a marked crystallographic preferred orientation indicates flow by dislocation creep with dynamic recrystallisation. Quartz microstructures identical to those produced in type A + B experiments are observed in cores recovered from Long Valley Exploratory Well in the Quaternary Long Valley Caldera, California, with considerable seismic activity.The experiments demonstrate the behaviour of quartz at coseismic loading (type A) and subsequent static annealing (type A + B) or creep at decaying stress (type A + C) in the middle crust. The experimentally produced microfabrics allow to identify similar processes and conditions in exhumed rocks.  相似文献   

铝硅酸盐矿物和玻璃中Al的配位与局部结构   总被引：3，自引：2，他引：1  

彭明生  李迪恩 《矿物学报》1998,18(4):425-430

利用同步辐射的AlK边X射线吸收近进结构（XANES）谱研究了刚玉和铝硅酸盐矿物（蓝晶石,红柱石,夕线石和钠长石）中Al的配位与局部结构,证明该方法可以作为新的结构探针研究结构未知体系中Al的配位与局部结构。例如,Al的K边XANES谱证明在室温压条件,钠长石玻璃中的Al保持为四面体配位（AlIV）,局部结构与钠长石晶体中的Al相似;尽管硬玉晶体中的Al为八面体配位,但硬玉玻璃中的Al变为四面体配位（AlIV）。而在相同的高温压条件（4．4GPa,1575C）下制备的硬玉-钠长石玻璃系列中,压力引起四面体配位的Al变成五次（Alv）和六次配位（AlVl）,且五次和六次配位Al的比例随玻璃中硬玉含量的增加而增大。  相似文献   

新矿物(19931～199312)     

黄蕴慧  蔡剑辉  曹亚文 《岩石矿物学杂志》1998,(2)

本文以表格形式列举了１９９３年１月至１９９３年１２月经《国际矿物学协会（ＩＭＡ）新矿物与矿物命名委员会（ＣＮＭＭＮ）》批准并在各国矿物学杂志上发表的４２个新矿物的中文英文名称、化学式及其他数据。数据依次为：矿物的晶系、空间群、晶胞参数、主要粉晶数据（Ｉ、ｈｋｌ）、物理性质（晶形、颜色、条痕、光泽、解理、发光、硬度、密度等）、光学性质（一、二轴晶,正、负光性,折光率,反射率,双反射,２Ｖ,色散,吸收性,多色性等）、产状、共生矿物等。  相似文献   

Recent progress on anomalous X-ray pulsars     

Victoria M. Kaspi 《Astrophysics and Space Science》2007,308(1-4):1-11

I review recent observational progress on Anomalous X-ray Pulsars, with an emphasis on timing, variability, and spectra. Highlighted results include the recent timing and flux stabilization of the notoriously unstable AXP 1E 1048.1–5937, the remarkable glitches seen in two AXPs, and the newly recognized variety of AXP variability types, including outbursts, bursts, flares, and pulse profile changes. I also discuss recent discoveries regarding AXP spectra, including their surprising hard X-ray and far-infrared emission, as well as the pulsed radio emission seen in one source. Much has been learned about these enigmatic objects over the past few years, with the pace of discoveries remaining steady. However additional work on both observational and theoretical fronts is needed before we have a comprehensive understanding of AXPs and their place in the zoo of manifestations of young neutron stars.   相似文献   

Chandra observations of neutron stars: an overview     

M. C. Weisskopf  M. Karovska  G. G. Pavlov  V. E. Zavlin  T. Clarke 《Astrophysics and Space Science》2007,308(1-4):151-160

We present an overview of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for observations of unprecedented clarity and accuracy. Many of these observations have provided new insights into neutron star physics. We present an admittedly biased and overly brief review of these observations, highlighting some new discoveries made possible by the Observatory’s unique capabilities. This includes our analysis of recent multiwavelength observations of the putative pulsar and its pulsar-wind nebula in the IC443 SNR.   相似文献   

Morphologies of AGN host galaxies using HST/ACS in the CDFS-GOODS field     

Priya Hasan 《Astrophysics and Space Science》2007,312(1-2):63-77

Using HST/ACS images in four bands F435W, F606W, F775W and F850LP, we identify optical counterparts to the X-ray sources in the Chandra Deep Field South in the GOODS South field. A detailed study has been made of these sources to study their morphological types. We use methods like decomposition of galaxy luminosity profiles, color maps and visual inspection of 192 galaxies which are identified as possible optical counterparts of Chandra X-ray sources in the CDFS-GOODS field. We find that most moderate luminosity AGN hosts are bulge dominated in the redshift range (z≈0.4–1.3), but not merging/interacting galaxies. This implies probable fueling of the moderate luminosity AGN by mechanisms other than those merger driven.  相似文献