宁夏中卫县沙坡头地区黑色泥质页岩固沙性能研究

我国西北干旱半干旱地区，生态环境极为脆弱，土地沙漠化问题十分突出。防风固沙，恢复植被，遏制沙漠化，改善生态环境，是我国西部大开发战略和加快西部经济腾飞的主要任务之一。防风治沙首先要解决的问题是固沙保水。文章提出了利用宁夏腾格里沙漠东南缘中卫县沙坡头地区香山北麓的黑色泥质页岩在自然条件下天然胶结成壳作用于固沙的可能性。这类黑色泥质页岩具有遇水则吸水软化，风干则形成薄硬壳之特点。在斜坡坡面上或坡脚风化破碎或构造破碎或人工开挖的黑色泥质页岩碎块堆积的表面常形成1层1～5cm的硬壳。这类黑色泥质页岩在500℃时灼减量高达17．56％，说明具有很高的有机质含量，同时P2O5，和K2O含量也较高，有利于成壤和植物生长。黑色泥质页岩的天然胶结成壳作用与地表破碎的黑色泥质页岩堆积和特定的干旱半干旱气候以及本身成分、结构有关。这一硬壳层不但具有一定的强度和抗风蚀能力，而且还具有一定的吸水性和保水性。因此，借鉴草方格固沙方法，就地取材，充分利用黑色泥质页岩在自然条件下的天然胶结成壳性能，用于沙漠治理中的固沙。进一步对黑色泥质页岩天然胶结成壳的机理进行深入研究，并开展黑色泥质页岩固沙试验研究，有可能为腾格里沙漠治理开辟新的途径。     

黑色页岩风化过程中元素的活动性及参照系的选取初探--以湖南省麻田、桃花江剖面为例

系统考察了湖南省麻田和桃花江两个不同发育程度的下寒武统黑色页岩风化剖面,并提出了元素在理想剖面中的分布模式(概念模型);通过对比分析这两个剖面中元素的分布特征与理想分布模式的关系,并结合元素相关性研究、等质量图解的判别分析、微量元素的赋存状态及地球化学性质的探讨,认为在黑色页岩风化过程中,Ti为不活动元素,可作为参照系来计算其它元素的相对迁移性,Nb、Ta的活动性较小,Zr与Hf之间存在着共迁移现象;研究表明化学风化程度是影响元素活动性的重要因素.     

高碳黑色页岩型铂族元素矿床性探讨

简析了高碳黑色页岩型铂族元素矿床（PGED）的研究现状，并根据矿床的特征初步将该类矿床划分为中层状黑色页岩，薄层状黑色页岩和高碳构造岩型3类；并从形成环境，成因等方面对PGED形成进行了剖析，强调了源区供给，有机迁移和热液叠加作用的差异是导臻形成不同类型黑色含碳页岩型铂族元素矿床的根源，指出了我国贵州－湖南高碳黑色页岩型铂族元素成矿性较差与层薄和叠加温度低有关。     

Region of anomalous compression under Bondi-Hoyle accretion

We investigate the properties of an axisymmetric gas flow without angular momentum onto a small compact object, in particular, on a Schwarzschild black hole in the supersonic region; the velocity of the object itself is assumed to be low compared to the speed of sound at infinity. First of all, we show that the streamlines intersect (i.e., a caustic is formed) on the symmetry axis at a certain distance r _x from the center on the front side if the pressure is ignored. The characteristic radial size of the region in which the streamlines emerging from the sonic surface at an angle no larger than θ₀ to the axis intersect is Δr = r _x θ ₀ ² /3. To refine the flow structure in this region, we have numerically computed the system without ignoring the pressure in the adiabatic approximation. We have estimated the parameters of the inferred region with anomalously high matter temperature and density accompanied by anomalously high energy release.     

Stratigraphy, sedimentology and bulk organic geochemistry of black shales from the Proterozoic Vindhyan Supergroup (central India)

Four organic-rich shale units of the Proterozoic Vindhyan sedimentary succession have been scanned to reveal their origin and hydrocarbon potential. The wavy-crinkly nature of the carbonaceous laminae is suggestive of a microbial mat origin of the shales. These shales are thus different from Phanerozoic black shales which typically exhibit planar laminae. The hydrocarbon potential of the black shale units has been evaluated by Rock-Eval pyrolysis. Total organic carbon content of many of the shales exceeds 1%. The meanT _max for the black shales translate to a vitrinite reflectance range of 2.05-2.40% Rm based on standard conversion techniques. These shales have reached the catagenetic stage near the beginning of anthracite formation.     

中国东北全新世干湿状况的演变

通过综合分析植物花粉,沙土埋藏土壤,泥炭形成与发展,沙丘活动历史,黄土状土堆积和黑土发育等多种资料表明,我国东北地区的湿润程度或土壤水分含量在５ｋａ ＢＰ以前的早中全新世较低,中晚全新世不能增加,早中全新世最干燥时段出现的＾１４Ｃ年代９－８ｋａ ＢＰ,中晚全新世湿润时期可能是最近的２ｋａ,近现代气候比过去１０ｋａ平均状况湿润。     

Dissipative accretion flows around a rotating black hole

We study the dynamical structure of a cooling dominated rotating accretion flow around a spinning black hole. We show that non-linear phenomena such as shock waves can be studied in terms of only three flow parameters, namely the specific energy     , the specific angular momentum (λ) and the accretion rate     of the flow. We present all possible accretion solutions. We find that a significant region of the parameter space in the     plane allows global accretion shock solutions. The effective area of the parameter space for which the Rankine–Hugoniot shocks are possible is maximum when the flow is dissipation-free. It decreases with the increase of cooling effects and finally disappears when the cooling is high enough. We show that shock forms further away when the black hole is rotating compared to the solution around a Schwarzschild black hole with identical flow parameters at a large distance. However, in a normalized sense, the flow parameters for which the shocks form around the rotating black holes are produced shocks closer to the black hole. The location of the shock is also dictated by the cooling efficiency in that higher the accretion rate     , the closer is the shock location. We believe that some of the high-frequency quasi-periodic oscillations may be due to the flows with higher accretion rate around the rotating black holes.     

青藏高原黑碳气溶胶传输及沉降的季节特征模拟分析

根据全球气溶胶气候模式GEM-AQ/EC的1995~2004年模拟,分析了青藏高原大气黑碳气溶胶的来源、传输及沉降季节特征。研究表明:青藏高原黑碳气溶胶主要来自自由对流层和大气边界层的输送。相对于自由对流层的黑碳输送,紧邻青藏高原的南亚、东亚以及东南亚大气边界层的输送更有效,它形成了青藏高原由北向南、自西往东黑碳气溶胶浓度和沉降明显递增的基本分布形态。横跨欧亚大陆自由对流层的黑碳气溶胶由西向东向青藏高原的输送全年不变,夏季输送路径最北但强度最弱,冬季路径最南而强度最强。大气边界层黑碳气溶胶的输送受控于亚洲季风环流变化,来自南亚的黑碳气溶胶在春季越过孟加拉湾传输进入高原东南部,夏季则可翻越喜马拉雅山抵达青藏高原南部腹地;同时我国中部排放的黑碳气溶胶也在东亚夏季风向北扩展中驱动它从东向西往青藏高原东北部传输。从秋季到冬季,随着夏季风撤退,南亚黑碳源区向青藏高原传输衰退,东亚冬季风的反气旋性环流的南侧及西南侧的偏东风携带秋季我国东南部源区和冬季东南亚源区黑碳气溶胶向青藏高原东南部传输。受青藏高原明显的暖湿季和干冷季气候影响,干湿沉降分别主导了青藏高原冬季和夏季黑碳沉降,夏季青藏高原黑碳气溶胶沉降总量大多超过8~10 kg·km-2,在高原东北部的最高值超过40 kg·km-2。冬季青藏高原黑碳气溶胶沉降量最低,大部地区黑碳沉降低于5 kg·km-2。青藏高原黑碳沉降的冬夏季节相差约为2~8倍。