Investigation of the linear polarization in infrared absorption bands

We consider the effects of the grain size, shape, structure, and chemical composition as well as the angle between the grain rotation axis and the incident ray on the full widths at half maximum (FWHM) of the polarization bands in the two deepest infrared absorption bands observed in the spectra of protostars, the water-ice band centered at 3.1 μm and the silicate band centered at 9.7 μm, using a core—mantle confocal spheroid model with various axial ratios a/b and relative volumes of the core material. We have found that the observed polarization bands with FWHM_p < 0.3 μm in the water-ice absorption band can be explained only by oblate and prolate particles with r _v ≤ 0.35 μm and the polarization bands with FWHM_p ≈ 0.3 μm can be explained only by particles with r _v ≈ 0.35 μm. Broad silicate absorption bands (FWHM ≈ 3 μm) with broad polarization bands (FWHM_p ≈ 2.7 μm) can be explained by particles with r _v ≈ 0.35 μm. Narrow silicate absorption bands (FWHM ≤ 3 μm) with any FWHM of the polarization bands can be explained by a mixture of particles of two types of olivine. Narrow polarization bands (FWHM_p ≈ 2 μm) with broad absorption bands can be explained only by very small particles, r _v ≤ 0.1 μm. We have found the relationships between the effective polarization and extinction cross sections and estimated the ranges of observed polarizabilities that can be explained by particles of given shape and orientation in each of the bands independently. Independent studies of the observational data for each of the bands are shown to give a wider choice of particle model parameters.     

On the magnitude and direction of the anisotropy of galactic cosmic rays

The results of measuring the diurnal cosmic-ray intensity variations in the energy range 1–100 TeV are discussed. Whereas the phase of the first harmonic of the sidereal daily wave directly determines the phase (right ascension) of the cosmic-ray anisotropy vector, the amplitude and declination of the true anisotropy cannot be reconstructed directly from the amplitude of the first harmonic. However, they can be determined by invoking data on the zero harmonic. The results of some recent experiments purporting to measure the cosmic-ray anisotropy with a particularly high accuracy are shown to be interpreted erroneously.     

Static pressure of hot gas: Its effect on the gas disks of galaxies

The static pressure of the hot gas that fills clusters and groups of galaxies can affect significantly the volume density and thickness of the gas disks in galaxies. In combination with the dynamic pressure, the static pressure allows several observed peculiarities of spiral galaxies surrounded by a hot medium to be explained.     

碎石桩复合地基的抗液化特性探讨

饱和砂土地震液化问题是岩土地震工程中一个重要的研究课题。在多种可行的防治液化措施中 ,最普遍的方法是采用碎石桩复合地基。本文结合目前国内外碎石桩复合地基的抗液化研究的最新进展 ,对碎石桩的密实、排水减压和减震作用做了较详细的评述 ,最后还提出碎石桩复合地基抗液化特性需要进一步研究的问题     

天山南坡科其卡尔巴契冰川消融期气候特征分析

通过分析天山南坡科其卡尔巴契冰川区的气候变化特征及其对冰川消融变化过程的影响, 研究了冰川对气候变化的响应机理及其对塔里木河水资源的影响规律.科其卡尔巴契冰川区夏季气温比较高, 基本处于正温, 日较差较小; 气温直减率较小, 平均值为0.60·℃\5(100m)-1, 冰川冷效应不明显; 对流性降水较多, 降水量的75%发生在白天; 冰川区局地环流--山谷风发育, 海拔3 900 m以上冰川受西风环流影响显著; 净辐射在7月和8月中上旬均较大, 在8月下旬后净辐射开始逐渐减小, 与冰川消融是一致的. 7月初至7月下旬是消融较强的两个时段, 冰川平均消融速率为38.66 mm·5d-1, 到8月中旬消融速率略有降低, 平均为34.79 mm·d-1, 至9月中旬降至28.83 mm·d-1.     

Geochemistry of Ore Fluids and Rb-Sr Isotopic Dating for the Wulong Gold Deposit in Liaoning, China

On the basis of detailed geological studies of the Wulong gold deposit, three metallogenic stages can be identified. With quartz fluid inclusions as an object of study, the authors investigated phase characteristics, compositional variations, temperature and pressure changes, fluid evolution, Pb isotope tracing and Rb-Sr isotopic dating of fluid inclusions entrapped in the above three metallogenic stages. The results show that Na+ is decreased obviously with metallogenic evolution, while K+ and other cations and gas compositions (H2, CO, CH4 and CO2) are increased slightly, and that the temperature and salinity vary in a pulsating manner along with the metallogenic evolution. Inverse calculation of hydrogen and oxygen isotopes indicate that at the first metallogenic stage the fluids were magmatic water, at the second stage they were dominated by magmatic water with a minor amount of meteoric water involved, and at the third stage, i.e., the final stage of metallogenesis, the fluids were composed complete     

山东招远金岭金矿埠南矿区1#脉流体特征及成矿物理化学条件研究

金岭金矿埠南矿区成矿流体成分特征显示流体为有幔源流体参与的岩浆水与大气水的混合流体。均一法测温表明成矿温度在 10 3～ 35 2℃ ,变化较大 ;通过Shenberger等和Hayashi等LogfO2 - pH图解 ,温度较低的成矿中期阶段 (2 5 0℃± )流体系统中的金明显比早期阶段 (30 0℃± )富集。成矿流体中金主要以Au(HS) -2 形式存在。根据含CO2 三相包体估算 ,流体压力在 5 1～ 70MPa之间。根据Sibson等断裂带流体垂直分带曲线 ,在流体压力为4 0～ 370MPa时 ,断裂带流体压力和深度之间为非线性关系 ,成矿深度既不能用静水压力梯度也不能用静岩压力梯度来计算 ,应该用特定的流体压力和深度关系式计算。通过分段拟合深度和压力之间的关系式计算出金岭金矿成矿深度在 5 .7～ 6 .78km之间 ;按照Gebre Mariam等提出太古代后生金矿深度分类 ,属典型中成脉型金矿。     

新疆雅满苏铁矿床地空高光谱异常特征及应用

正雅满苏铁矿床位处东天山成矿带,成矿地质条件优越。前人在矿床的成矿规律、地球化学、矿床类型、流体来源等方面,开展了较多科研工作(李厚民等,2014;王兴保,2005)。但在遥感地质方面的研究和应用工作还未开展。铁矿床及外围区域属准平原状丘陵地貌,基岩出露,地表蚀变信息丰富,可获取高质量的地空高光谱遥感数据,有利于发挥高光谱遥感的技术优势。     

青藏高原东部春季感热通量与我国东部气温的年际关系

利用ERA-Interim提供的地表感热、环流场资料和1979-2013年753站中国春季气温观测资料探讨了青藏高原（以下简称高原）东部春季感热通量与我国东部气温的关系。春季高原东部感热与我国东部气温在年际变化上存在密切的相关关系。去除9年滑动平均以后的SVD第一模态结果表明,当高原东部感热出现南弱（强）北强（弱）时,对应我国东北和华南地区的气温异常偏低（高）。当春季高原感热呈现南负北正的分布时,高层200 hPa上,高纬东风异常减弱背景西风有利于冷空气的南下,加之副热带西风急流显著增强,有利于东北地区形成气旋性环流。中低层环流场上,我国北方地区上空为一深厚的东北冷涡所控制,从对流层低层到高层,均呈现较强的气旋式环流分布。一方面,它引导西伯利亚冷空气南下,造成我国东北地区气压异常减弱,气温异常偏低;另一方面,其西侧北风异常阻滞了华南地区上空的背景西南风,不利于暖气流的输送。进一步分析得出,与PC1相关的南北温度差值场上,东亚地区上空从低纬到高纬呈现“负-正-负”的分布形势,有利于副热带西风急流在我国上空的显著增强。气旋中心上暖下冷的结构,导致位涡显著发展并向低层伸展、侵入,增强了对流层中低层的气旋性环流。气旋中心整个对流层为深厚的异常干空气,湿度负值中心与冷中心相对应,表明干冷空气异常下传发展。干侵入使得冷涡加强发展,维持了异常气旋性环流,导致春季东北、华南地区的异常降温。虽然前冬Nino3.4区海温与春季感热相关较好,但其对我国东部春季气温影响并不显著。     

葡萄石的热膨胀性与压缩性及其地质意义

利用同步辐射X射线衍射及拉曼光谱技术对葡萄石分别进行了原位高温及原位高压实验。原位高温实验结果表明葡萄石的热膨胀系数为K=1. 77(3)×10~(-5)K~(-1),轴向热膨胀系数具有各向异性(α_aα_bα_c),葡萄石在1073K时开始发生脱水反应,分解为钙长石及硅灰石。原位高压X射线衍射实验结果表明,在大于12. 4GPa时,葡萄石的晶胞参数发生不连续变化,可能发生了相变;在24. 0GPa左右,葡萄石发生不可逆的非晶化转变。原位高压拉曼光谱表明,葡萄石在12. 6GPa左右发生相变,这一相变很可能与其[(Si,Al)O_4]四面体中的Si发生有序排列有关。结合葡萄石的热膨胀性及压缩性,我们确定了葡萄石在高温高压下的稳定范围,这一结果对认识上地幔中含水矿物的状态以及地幔中水的来源有重要意义。