Analytical solutions of one‐dimensional infiltration before and after ponding

This paper is a continuation of previous research, which obtained a convenient solution for arbitrary surface fluxes before ponding. By means of Fourier Transformation this has been extended to derive analytical solutions of a linearized Richards' equation for arbitrary input fluxes after surface saturation. Copyright © 2003 John Wiley & Sons, Ltd.     

湖北黄土岭麻粒岩锆石拉曼光谱和等离子体质谱研究

对湖北黄土岭麻粒岩中锆石同时进行了激光拉曼探针、阴极发光 (CL)观察和U ,Th及Pb Pb年龄ICPMS测定 ,发现麻粒岩中部分锆石发生的不是固态重结晶作用 ,而是部分熔蚀 /沉淀再结晶过程。结合CL图像结构特征和2 0 7Pb/ 2 0 6Pb年龄初步推断 ,麻粒岩相事件发生在 2 0亿年之后。结构、化学和同位素组成的测定表明 ,大别地区广泛存在的燕山期热事件使锆石发生不同程度的变质重结晶作用 ,使锆石晶格愈合。     

扬子地台东南缘下寒武统清虚洞组风暴沉积特征及其重要意义

在扬子地台东南缘,下寒武统龙王庙阶清虚洞组主要由浅水碳酸盐岩组成。在野外露头剖面实测和室内镜下薄片观察的基础上,大量风暴沉积被发现于不同剖面清虚洞组的不同层位中,同时大量风暴诱发形成的沉积构造被识别出来,包括侵蚀基底、粗粒滞留沉积、粒序层理、平行层理、丘状交错层理(少见并且值得怀疑)以及沙纹层理,组成了多种类型的风暴沉积序列。结合更靠扬子东南缘的深水剖面中重力流沉积的缺乏,可以推断早寒武世龙王庙期扬子地台的沉积模式为碳酸盐缓坡。结合风暴的形成机制以及清虚洞组风暴沉积的发育特征(尤其是粗粒滞留砾屑的定向排列和典型丘状交错层理的缺乏),可以推断研究区风暴沉积形成于强烈的冬季风暴作用,并且早寒武世龙王庙期华南的古地理位置应当位于中纬度地区,这一结论对一些著名的全球古地理重建方案提出了质疑。同时中纬度地区大规模发育蒸发岩和碳酸盐岩还佐证了寒武纪地球处于热室(Hothouse)时期。     

Identification of Gleissberg Cycles and a Rising Trend in a 315-Year-Long Series of Sunspot Numbers

We show in this short note that the method of singular spectrum analysis (SSA) is able to clearly extract a strong, clean, and clear component from the longest available sunspot (International Sunspot Number, ISN) time series (1700?–?2015) that cannot be an artifact of the method and that can be safely identified as the Gleissberg cycle. This is not a small component, as it accounts for 13% of the total variance of the total original signal. Almost three and a half clear Gleissberg cycles are identified in the sunspot number series. Four extended solar minima (XSM) are determined by SSA, the latest around 2000 (Cycle 23/24 minimum). Several authors have argued in favor of a double-peaked structure for the Gleissberg cycle, with one peak between 55 and 59 years and another between 88 and 97 years. We find no evidence of the former: solar activity contains an important component that has undergone clear oscillations of \(\approx90\) years over the past three centuries, with some small but systematic longer-term evolution of “instantaneous” period and amplitude. Half of the variance of solar activity on these time scales can be satisfactorily reproduced as the sum of a monotonous multi-secular increase, a \(\approx90\)-year Gleissberg cycle, and a double-peaked (\(\approx10.0\) and 11.0 years) Schwabe cycle (the sum amounts to 46% of the total variance of the signal). The Gleissberg-cycle component definitely needs to be addressed when attempting to build dynamo models of solar activity. The first SSA component offers evidence of an increasing long-term trend in sunspot numbers, which is compatible with the existence of the modern grand maximum.     

北祁连西段肃南地区下志留统肮脏沟组河流相的发现及其大地构造意义

北祁连地区位于中国中央造山带中段,具有典型造山带的特征.区内志留系肮脏沟组沉积环境存在较大争议,以致对其沉积期古地理格局的认识就存在很大差异.本研究选取志留系肮脏沟组发育齐全的肃南地区老虎沟剖面为研究对象,通过野外剖面实测、室内薄片鉴定和碎屑岩粒度分析等方法对老虎沟剖面肮脏沟组沉积充填序列、沉积构造和沉积相类型进行了细...     

兰坪中新生代沉积盆地演化

兰坪中新生代沉积盆地形成和演化与金沙江洋的俯消减及洋陆转换过程密切相关,记录了其盆－山转换过程,早二叠世晚期－晚二叠世时期,由于金沙江洋的俯冲消减,形成了金沙江弧－盆系的空间配置,兰坪地区成为弧后盆地,早中三叠世,金沙江弧－盆系及东西两侧的昌都－兰坪陆块和中咱－中甸陆块的构造沉积式样发生大的转米,开始了兰坪中新生代盆－山转换历史,由于弧陆碰撞作用,使得兰坪分国地由弧后盆地转化成弧后前陆舅地,盆地中     

青藏高原北部温泉活动沉积盆地的沉积特征及其地质意义

晚新生代温泉沉积盆地，是青藏高原腹地在南北向挤压、东西向伸展的构造背景下，沿南北向边界走滑断层，经边界正断层和内部张剪断层的进一步发展而形成的近南北向单断单剪楔形半地堑活动沉积盆地。它可能代表了晚新生代青藏高原第三期强烈挤压隆升事件，是侧向向东剪切挤出的结果。笔者以盆地充填序列和TL、ESR测年资料为主要依据，推测唐古拉山在300～250ka前后全面进入冰冻圈；而以温泉活动沉积盆地为代表的中更新世晚期(224．0～150．2ka)的冰碛一冰水堆积则对应于青藏高原第三期隆升的断陷盆地发育阶段；中更新世晚期一晚更新世中期(144．0～56ka)为湖相沉积；晚更新世中期至今(35～0ka)对应于高原缓慢隆升与夷平发育阶段。长江溯源在35ka切割通天河盆地，形成通天河；而在16kat浸蚀切穿雁石坪一温泉兵站峡谷，形成布曲河。     

新疆伊犁盆地南缘中新生代以来构造演化与聚煤规律研究

新疆伊犁盆地以其丰富的煤碳和铀矿资源倍受专家与学者的高度关注,特别是伊犁盆地南缘。笔者从煤矿勘查角度,运用构造地质学、煤田地质学、沉积学的理论,从构造应力作用强度方面阐述伊犁盆地南缘现存的构造特征、构造格局以及含煤地层中下侏罗统水西沟群的沉积特征和赋煤性。笔者分析了古气候和沉积环境与聚煤关系,认为水西沟群是在温暖潮湿古气候条件下形成的冲积扇-扇三角洲体系的产物,有利于泥碳沼泽环境的形成,特别是西山窑组具备形成稳定而厚大煤层的基本条件。笔者重点分析中新生代以来的构造演化过程对煤矿的形成与保护作用,认为区域构造背景直接决定了盆地的形成与演化,从而影响着研究区成煤环境与赋煤潜力;构造格局或构造特征是成煤后构造演化的结果,即其活动影响着煤层成藏或保存程度;构造作用的差异性影响着煤层的保存状态和分布范围。     

Investigation of Arsenotrophic Microbiome in Arsenic‐Affected Bangladesh Groundwater

Arsenotrophic bacteria contribute to the nutrient cycling in arsenic (As) affected groundwater. This study employed a culture‐independent and ‐dependent investigation of arsenotrophic microbiomes in As affected groundwater samples collected from Madhabpur, Sonatengra, and Union Porishod in Singair Upazila, Manikganj, Bangladesh. Total As contents, detected by Atomic Absorption Spectrophotometry (AAS) of the samples, were 47 µg/L (Madhabpur, SNGW‐1), 53 µg/L (Sonatengra, SNGW‐2), and 12 µg/L (Union porishod, SNGW‐3), whereas the control well (SNGW‐4; depths >150 m) showed As content of 6 µg/L. Denaturing Gradient Gel Electrophoresis (DGGE) analysis of the amplified 16S rRNA gene from As‐affected groundwater samples revealed the dominance of aerobic bacteria Pseudomonas within heterogeneous bacterial populations. DGGE of heterotrophic enrichments supplemented with arsenite [As (III)] for 4 weeks showed the dominance of Chryseobacterium, Flavobacterium, and Aquabacterium, whereas the dominant genera in that of autotrophic enrichments were Aeromonas, Acinetobacter, and Pseudomonas. Cultured bacteria retrieved from both autotrophic and heterotrophic enrichments were distinguished into nine genotypes belonging to Chryseobacterium, Acinetobacter, Escherichia, Pseudomonas, Stenotrophomonas, Janibacter, Staphylococcus, and Bacillus. They exhibited varying range of As(III) tolerance from 4 to 27 mM. As(III) transformation potential was confirmed within the isolates with oxidation rate as high as 0.143 mM/h for Pseudomonas sp. Sn 28. The arsenotrophic microbiome specifies their potential role in groundwater As‐cycling and their genetic information provide the scientific basis for As‐bioremediation.     

Slow and Fast Rotating Coronal Holes from Geomagnetic Indices

The evolution of the 27-day recurrence in the series of two solar indices (Wolf number WN and 10.7 cm radio flux F) and two geomagnetic indices (Dst and ζ, variance of the geomagnetic field recorded at a magnetic observatory) have been studied over the 1957 – 2007 time span. Spectral energies contained in two period domains (25 – 27.3 and 27.3 – 31 days), designated as E ₁ and E ₂, have been computed. Whereas the evolution of E ₁ is the same for the four indices, that of E ₂ is essentially different for WN and F on the one hand, Dst and ζ on the other hand. Some general conclusions on the dynamics of the solar outer layers are inferred from these results. First the solar activity, as measured by WN, and when averaged over a few years, evolves in the same way whatever the latitude. Second, two families of coronal holes (CHs) are identified; the rapidly and the slowly rotating CHs evolve quite differently.