塔中地区志留系碎屑锆石测年及其地质意义

志留系是塔里木盆地第一套砂岩储层广泛分布的沉积盖层,其沉积来源与成因对志留纪构造演化及周边造山带的研究具有重要意义。塔中地区3个志留系样品的碎屑锆石LA?ICP?MS U?Pb定年研究表明,志留系具有比较集中的二期物源年龄：南华纪中期、古元古代中期。碎屑锆石测定的年龄表明塔中志留系物源均来自前寒武纪,塔中东部源区方向的塔南隆起基底在奥陶纪已隆升成为蚀源区。大量的新元古代中期锆石年龄表明塔里木板块在新元古代时期可能与Rodinia超大陆具有相似的聚合与裂解演化史。     

A preliminary study of early agriculture practices at the Haojiatai site in Luohe city,Henan Province

As the most fundamental economic sector of human societies,farming has played a significant role in interactions between humans and the environment.The study of crop patterns in various regions could not only clarify the economic foundations of early societies,but also greatly improve our understanding of interactions among human beings,the environment,and other creatures.In this regard,this study focuses on early agriculture practices at the Haojiatai site,situated in the cultural and natural transitional region between North and South China.Macro plant remains from this site reveal that foxtail millet was the most important staple crop here during the Longshan and Xinzhai periods(4300–3800 cal.yr BP),along with common millet and a small amount of rice and soybean.This crop pattern is in contrast to the ancient environmental conditions of this region,and cultural factors such as agriculture traditions and food preferences may have been more important in the formation process of this crop pattern.     

A model of Titan's aerosols based on measurements made inside the atmosphere

The descent imager/spectral radiometer (DISR) instrument aboard the Huygens probe into the atmosphere of Titan measured the brightness of sunlight using a complement of spectrometers, photometers, and cameras that covered the spectral range from 350 to 1600 nm, looked both upward and downward, and made measurements at altitudes from 150 km to the surface. Measurements from the upward-looking visible and infrared spectrometers are described in Tomasko et al. [2008a. Measurements of methane absorption by the descent imager/spectral radiometer (DISR) during its descent through Titan's atmosphere. Planet. Space Sci., this volume]. Here, we very briefly review the measurements by the violet photometers, the downward-looking visible and infrared spectrometers, and the upward-looking solar aureole (SA) camera. Taken together, the DISR measurements constrain the vertical distribution and wavelength dependence of opacity, single-scattering albedo, and phase function of the aerosols in Titan's atmosphere.Comparison of the inferred aerosol properties with computations of scattering from fractal aggregate particles indicates the size and shape of the aerosols. We find that the aggregates require monomers of radius 0.05 μm or smaller and that the number of monomers in the loose aggregates is roughly 3000 above 60 km. The single-scattering albedo of the aerosols above 140 km altitude is similar to that predicted for some tholins measured in laboratory experiments, although we find that the single-scattering albedo of the aerosols increases with depth into the atmosphere between 140 and 80 km altitude, possibly due to condensation of other gases on the haze particles. The number density of aerosols is about 5/cm³ at 80 km altitude, and decreases with a scale height of 65 km to higher altitudes. The aerosol opacity above 80 km varies as the wavelength to the −2.34 power between 350 and 1600 nm.Between 80 and 30 km the cumulative aerosol opacity increases linearly with increasing depth in the atmosphere. The total aerosol opacity in this altitude range varies as the wavelength to the −1.41 power. The single-scattering phase function of the aerosols in this region is also consistent with the fractal particles found above 60 km.In the lower 30 km of the atmosphere, the wavelength dependence of the aerosol opacity varies as the wavelength to the −0.97 power, much less than at higher altitudes. This suggests that the aerosols here grow to still larger sizes, possibly by incorporation of methane into the aerosols. Here the cumulative opacity also increases linearly with depth, but at some wavelengths the rate is slightly different than above 30 km altitude.For purely fractal particles in the lowest few km, the intensity looking upward opposite to the azimuth of the sun decreases with increasing zenith angle faster than the observations in red light if the single-scattering albedo is assumed constant with altitude at these low altitudes. This discrepancy can be decreased if the single-scattering albedo decreases with altitude in this region. A possible explanation is that the brightest aerosols near 30 km altitude contain significant amounts of methane, and that the decreasing albedo at lower altitudes may reflect the evaporation of some of the methane as the aerosols fall into dryer layers of the atmosphere. An alternative explanation is that there may be spherical particles in the bottom few kilometers of the atmosphere.     

湘中邵阳凹陷二叠系龙潭组页岩含气性特征与气体成因

针对湘中地区邵阳凹陷二叠系龙潭组页岩气资源评价,部署了页岩气调查井2015H-D3井,通过现场解析气等相关样品测试定量分析了页岩含气性特征及其影响因素,并借助气体稳定碳、氢同位素对气体成因进行了初步探讨.结果显示:钻深从150m处开始出现气显,随深度增加,解析气含量呈现先逐渐增大后减小的趋势,300～425m为最高含气层段,累计厚度达125m,现场解析气含量全部大于0.5m^3/t,最高为2.35m^3/t,平均1m^3/t,证实龙潭组具良好页岩气资源潜力.当埋深大于300m时,解析气含量受有机碳含量控制,而埋深小于300m时,解析气含量并不简单受控于有机碳含量,而是受到保存条件的严重制约.气体碳、氢同位素测试显示δ13C1介于-29.87‰～-36.82‰,平均为-34.52‰,δ¹³C_2介于-29.45‰～-31.02‰,平均为-30.09‰,δD1介于-131.20‰～-178.40‰,平均为-167.40‰.气体成因分析揭示龙潭组页岩气属热成因中的油型气类型.基于沉积现象判断龙潭组为海陆过渡相环境,与氢同位素判断结果基本吻合,但目前还无法确定具体判定区间.     

Hydrocarbons in the Basement of the South China Sea (Vietnam) Shelf and Structural–Tectonic Model of their Formation

Geotectonics - The paper considers the origin of hydrocarbon accumulations within the Pre-Cenozoic basement of the Vietnam shelf. It is shown that the formation of hydrocarbon deposits is...     

过去千年中国东部持续性严重干旱事件的模拟研究

文章利用CESM1.1(公共地球系统模式)模式过去千年集合试验结果,对模拟的过去千年中国东部持续性严重干旱事件的时空特征及发生机制进行了初步分析。模式模拟出过去千年中国东部发生了7次持续性严重干旱事件,分别为883~910年、951~977年、1253~1305年、1327~1346年、1471~1488年、1587~1610年和1688~1699年干旱事件,其中仅1471~1488年干旱事件与中国东部旱涝指数对应较好,表明模式对中国东部干旱事件的模拟能力较低。这7次干旱事件均与模拟的ENSO(厄尔尼诺-南方涛动)负位相状态相对应,揭示ENSO可能对中国东部干旱事件的发生起了非常重要的作用。模拟分析结果显示,1253~1305年干旱事件前期可能主要受火山活动驱动,后期则可能受到太阳活动和自然内部变率的影响。另外,1587~1610年干旱事件后期可能也受到火山活动的影响;883~910年和951~977年干旱事件则完全受自然内部变率的影响。对1327~1346年、1471~1488年和1688~1699年这3次干旱事件,无法分辨外强迫和内部变率ENSO的各自贡献。     

新疆伊犁河谷黄土滑坡冻融失稳机理研究

伊犁河谷地处中国天山山脉西段,属于典型的季节性冻土区,季节性冻融作用对斜坡稳定性影响强烈。本文以皮里青河"3.24"滑坡为例,通过现场详细调查、多期遥感影像动态比对、数值模拟等方法,研究了黄土滑坡冻融失稳机理与滑坡运动特征,得到以下几点认识:(1)滑坡失稳与水密切相关,一方面是地表水侵蚀作用,另一方面是地下水的冻融作用;(2)根据变形特征,将滑坡失稳过程分为坡脚侵蚀、冻结滞水和冻融循环破坏三个阶段,模拟结果表明,地下水水位上升导致孔隙水压力增大是滑坡冻融失稳的主要原因;(3)DAN-W数值模拟软件的Voellmy模型和Frictional模型可较好地模拟滑坡的运动堆积过程,模拟结果显示,滑坡历时12.8 s,最大运动速度17.7 m/s,平均堆积厚度4.9 m,运动距离139 m。本研究为伊犁河谷地区黄土冻融滑坡的早期识别与风险评估提供了重要的技术支撑。     

一次双台风影响下暴雨过程的中尺度涡旋模拟分析

本文对上海地区一次双台风环境影响的暴雨过程进行数值模拟及分析,探讨了强降水过程中大气中低层的涡旋特征及发展机理。结果表明:(1)暴雨过程处于双台风、大陆高压的共同影响下,中低层伴随有较明显的中尺度低涡发展。(2)与涡旋相关的局地垂直涡度由低层开始发展,先期涡度发展集中于850 hPa以下,之后向大气中上层发展增强,涡旋尺度强度也随之发展,最终形成在对流层下半部具有闭合式气旋性环流的深厚涡旋。(3)影响局地涡度变化的水平平流项、垂直平流项、散度制造项和倾斜项对不同时间、不同高度的涡度作用各不相同,其中散度制造项是中低层涡度的主要来源,垂直平流项的输送作用对中上层的涡度发展有重要作用,倾斜项对涡旋发展移动也有部分贡献。(4)通过敏感性试验考察了对流潜热反馈的贡献,发现潜热释放过程通过加热改变大气温压场结构,从而维持并改变局地涡度倾向的中低层辐合及对流上升运动,对涡旋的发展和移动起了重要影响。     

环境场对边界层低空急流形成的影响

本文利用两层流的浅水波模式,讨论了环境场对边界层低空急流形成的影响,并得到了边界层低空急流的特征宽度为L₀=(ρ₂-ρ₁)/(ν₂ρ₂-ρ₁ν₁)L₀*C₀*,式中C₀*=√gh₂, L₀*=C₀*/f为Rossby变形半径,ρ₁,p₂和v₁,v₂分别为上下两层大气的密度和大尺度经向地转风,H₂为低层大气的厚度,g为重力加速度,f为柯氏参数,当高低层大气中的大尺度经向地转风的垂直切变越强时,所形成的中尺度边界层低空急流就越强;当低层大气中的温度增高和湿度增大、并且低层大气中的大尺度经向地转风越强、高度越低时,越有利于形成边界层低空急流。