Isolating quartz-dominated OSL signal of rock slice by using pulsed stimulation: Implications for dating burial age of cobbles     

《Quaternary Geochronology》2022

Although the OSL signal sourced from quartz is expected to be more stable and bleached more rapidly than the IRSL signal sourced from feldspar in a general sense, the former is much less investigated than the latter for rock surface related luminescence dating. It is mainly due to the difficulty in isolating quartz-dominated OSL signals from rock slices, and the low sensitivity and non-fast component dominated OSL signals for quartz in most of rocks. In merit of the sub-conduction band transition of trapped electrons of feldspar under both green light stimulation and IR stimulation at elevated temperature (Jain and Ankjӕrgaard, 2011), it is expected that the contribution of feldspars to the green light stimulated luminescence could be substantially reduced by a prior IR stimulation at elevated temperature. Meanwhile, more fast-component dominated quartz OSL signal (if there is any) could be obtained by green light stimulation (Bailey et al., 2011). Therefore, in this study, we investigated the feasibility of using the post-IR pulsed green stimulation, which is performed at 25 °C (PGLSL₂₅) following two IR stimulations (IR₅₀IR₂₂₅), to isolate the quartz-dominated OSL signals from rock slices of granite cobbles for burial dating. The decay characteristics of stimulation curve, characteristic saturation dose and thermal stability of the pIR₅₀IR₂₂₅ PGLSL₂₅ signal suggest that this signal is quartz-dominated, but still not fast-component dominated. We tentatively validated the equivalent dose (D_e) measurement protocol by dose recovery experiment. The luminescence-depth profiles show that the bleaching depths of pIR₅₀IR₂₂₅ PGLSL₂₅ signals are slightly smaller than or close to that of the IR₅₀ signals, while they are much shallower for the pIR₅₀IR₂₂₅ signals. The pIR₅₀IR₂₂₅ PGLSL₂₅ procedure enables multiple D_e values determined from luminescence signals, with different bleachabilities and stabilities, from both feldspars and quartz in one measurement, which is of potential for buried age dating of cobbles.  相似文献   

冻融作用下污泥固化轻质土动力特性及结构演化          下载免费PDF全文

杨爱武  王斌彬  钟晓凯 《水文地质工程地质》2022,49(1):57-65

冻融作用会影响污泥固化轻质土动力特性和结构特性。为研究不同冻融循环次数和冻结温度下的污泥固化轻质土动力特性及结构演化,对冻融循环作用后的污泥固化轻质土进行动三轴试验和固结试验。试验结果表明:在冻融循环作用下,污泥固化轻质土动应力-应变曲线呈弱应变硬化型。污泥固化轻质土动强度和变形随着冻融次数（n）的增加和冻结温度（T）的降低而减小。经历前4次冻融作用后,对固化土变形和动强度影响较大,经历8次冻融循环后基本趋于稳定。冻融循环对土体动力特性的影响本质上是对土体结构性的影响。固化土冻融结构势（m_dσn）的变化规律与动强度类似,随冻融次数的增加和冻结温度的降低而下降。冻融循环次数是影响污泥固化轻质土动力特性和结构性的主要因素,冻结温度为次要因素。  相似文献   

XDQ-120型钻机动力头的优化设计          下载免费PDF全文

白祖卫  王顺平  黄军航 《探矿工程》2015,42(7):42-44

XDQ-1200型钻机是专门针对山区丘陵地带设计的钻机,对其质量的大小提出了很严格的要求。为此对动力头的结构件进行了有限元静力学分析,对其箱体的强度和刚度进行分析、优化,在满足受力的情况下,尽量减轻箱体质量,以达减重目标。介绍了XDQ-1200型钻机动力头的设计背景、理念以及设计优化过程。  相似文献   

XDQ-1200型全液压轻型岩心钻机电液控制系统设计与应用          下载免费PDF全文

刘旭光  盛海星  王敏 《探矿工程》2015,42(9):49-52

XDQ-1200型全液压轻型岩心钻机采用了电液比例控制技术,具有自动化水平高、效率高、易操作、可靠性高等优点。简要介绍了该钻机的性能特点,重点阐述了动力头回转、给进系统的液压控制原理和钻机的整体电气原理设计。生产试验表明,钻机运行良好,工作稳定,进尺速度快,操作简单,功能先进,自动化程度高。  相似文献   

中国大陆降水时空变异规律——I.气候学特征   总被引：2，自引：0，他引：2       下载免费PDF全文

任国玉  战云健  任玉玉  陈峪  王涛  柳艳菊  孙秀宝 《水科学进展》2015,26(3):299-310

为系统了解大尺度降水气候特征,利用2 300多个国家级气象站逐日观测资料,分析了中国大陆1956—2013年多年平均降水的空间分布和季节性变化规律。主要新认识有:① 暴雨量、暴雨日数和暴雨强度最高的站点在华南沿海,而小雨量、小雨日数最多的站点主要在江南内陆山区、丘陵;东部季风区山地、丘陵多出现低强度降水,平原和沿海易出现高强度降水;② 四季降水量均由西北内陆向东南沿海递增,南方秋季降水量明显小于春季,但华西和江南沿海秋季降水量较多,冬季降水在东南丘陵出现高值中心;③ 珠江和东南诸河流域降水量年内存在2个峰值,其中珠江流域有6月主峰值和8月次峰值,东南诸河流域主峰在6月中下旬,次峰在8月末,长江流域总体表现为单峰型,出现在6月下旬和7月初,西南诸河流域和北方所有流域降水均表现为夏季单峰型;④ 南方各大河流域从2月末到6月中下旬陆续进入雨季,北方各大河流域进入雨季时间集中在6月末、7月初;南、北方雨季结束时间比雨季开始时间集中,从南到北进入雨季时间持续120 d以上,而从北到南退出雨季时间则仅持续不到45 d;⑤ 丰雨期的持续时间,珠江流域从5月初到9月上旬后期,东南诸河从5月上旬到7月上旬,8月末到9月初再度短暂出现,长江流域从6月中下旬到7月中旬,西南诸河从7月中旬到 8月下旬,淮河流域从7月上旬至7月底、8月初,辽河流域在8月初出现极短丰雨期;⑥ 降水年际变异性最高的站点在青藏高原西南、塔里木盆地、阿拉善高原、华北平原北部和汾河谷地,海河流域年降水具有最大的变异系数。  相似文献   

准噶尔盆地玛湖凹陷深层油气流体相态研究   总被引：1，自引：0，他引：1  

张鸾沣  雷德文  唐勇  阿布力米提  陈刚强  胡文瑄  曹剑 《地质学报》2015,89(5):957-969

准噶尔盆地玛湖凹陷深层(5000m)是我国深层油气勘探当前的一个热点风险领域。为给区域下步油气勘探提供参考,通过对区内烃源岩和油气进行系统的地质地球化学正演、反演对比综合研究,重点分析了油气流体相态。结果表明,研究区深层稳定发育石炭系—二叠系四套烃源岩,有机质丰度高,普遍达到中等—好质量,类型多种多样,既可生油亦可生气,加之所有烃源岩均已基本进入高—过成熟演化,因此深层油气流体相态总体应高熟轻质,可能包括高熟轻质油、干酪根裂解气、油裂解气等。原油地球化学研究表明,原油随埋藏深度增加、层位变老,油质有逐渐变轻的趋势,成熟度有逐渐增大的趋势,保存条件亦逐渐变好,因此预测深层原油油质更轻、成熟度更高、保存条件更好。天然气地球化学研究表明,中浅层天然气可能属于混合来源,包括干酪根裂解气和油裂解气,规模性的高过成熟天然气可能在深层。因此,研究区深层油气资源丰富,相态轻质,成藏有利,值得勘探。这些认识还可供具有相似油气地质背景地区在研究和勘探时类比参考。  相似文献   

阶段性干旱胁迫对小麦光合生理特性及产量结构的影响          下载免费PDF全文

严韬  朱国良  葛非凡  蒋跃林  李威  吴文革 《气象与减灾研究》2019,42(1):46-53

在人工遮雨的条件下,采用盆栽的种植方式探究"皖麦68"营养生长期(返青期—开花期)及生殖生长期(开花期—成熟期)轻度干旱胁迫(土壤相对含水量为55%±5%)及复水(土壤相对含水量为70%±5%)对其光合生理特性及产量结构的影响。结果表明:返青期至成熟期充分供水(CK)的小麦旗叶光合参数和产量最高。开花至成熟期复水(DN)的小麦叶片在复水后光合能力迅速恢复,表现出了超补偿效应:光合速率(16.43μmol/(m~2·s))甚至超过了CK(15.01μmol/(m~2·s));采用非直角双曲线模型拟合小麦旗叶的光响应曲线,其中DN的曲角θ最大;DN产量较CK略有降低但千粒重为34.51 g,高于CK(34.44 g)。开花至成熟期轻度干旱(ND)及全生育期轻度干旱(DD)的小麦光合特征参数与产量均显著降低。DD产量最低、品质最差,但其收获指数I_H高于CK、仅次于DN。在小麦返青期—开花期进行水分管理适量减少灌溉,开花期—成熟期复水能够提升籽粒的干物质积累量,获得较高的产量及品质。  相似文献   

共线SPDC下剩余脉冲泵浦光滤光特性研究     

白云  权润爱  张羽  侯飞雁  刘涛  张首刚  董瑞芳 《时间频率学报》2014,(1):1-9

从宽带脉冲泵浦光的光谱及滤光片的滤光特性参数出发,分析了自发参量下转换（SPDC）产生纠缠光源的系统中各类滤光片对剩余脉冲泵浦光的滤除效率。分析结果表明,适当组合不同类型的滤光片可以有效地滤除剩余脉冲泵浦光,并从实验上验证了分析结果的正确性。该研究为脉冲泵浦光条件下SPDC过程产生的纠缠光源的有效测量提供了理论指导和实验验证。  相似文献   

Brief history of ground-based very high energy gamma-ray astrophysics with atmospheric air Cherenkov telescopes     

《Astroparticle Physics》2014

The discovery of the Crab Nebula as the first source of TeV gamma rays in 1989, using the technique of ground-based imaging air Cherenkov telescope, has marked the birthday of observational gamma astronomy in very high energy range. The team led by Trevor Weekes, after twenty years of trial and error, success and misfortune, step-by-step improvements in both the technique and understanding of gamma shower discrimination methods, used the 10 m diameter telescope on Mount Hopkins in Arizona, and succeeded measuring a 9σ signal from the direction of Crab Nebula. As of today over 160 sources of gamma rays of very different types, of both galactic and extra-galactic origin, have been discovered due to this technique. This is a really fast evolving branch in science, rapidly improving our understanding of the most violent and energetic sources and processes in the sky.The study of these sources provides clues to many basic questions in astrophysics, astro-particle physics, physics of cosmic rays and cosmology. Today’s telescopes, despite the young age of the technique, offer a solid performance. The technique is still maturing, leading to the next generation large instrument. This article is devoted to outlining the milestones in a long history that step-by-step have made this technique emerge and have brought about today’s successful source hunting.  相似文献   

Sputtering and high altitude meteors     

K. A. Hill  L. A. Rogers  R. L. Hawkes 《Earth, Moon, and Planets》2004,95(1-4):403-412

Conventional ablation theory assumes that a meteoroid undergoes intensive heating during atmospheric flight and surface atoms are liberated through thermal processes. Our research has indicated that physical sputtering could play a significant role in meteoroid mass loss. Using a 4th order Runge-Kutta numerical integration technique, we tabulated the mass loss due to the two ablation mechanisms and computed the fraction of total mass lost due to sputtering. We modeled cometary structure meteoroids with masses ranging from 10⁻¹³ to 10⁻³ kg and velocities ranging from 11.2 to 71 km s⁻¹. Our results indicate that a significant fraction of the mass loss for small, fast meteors is due to sputtering, particularly in the early portion of the light curve. In the past 6 years evidence has emerged for meteor luminosity at heights greater than can be explained by conventional ablation theory. We have applied our sputtering model and find excellent agreement with these observations, and therefore suggest that sputtered material accounts for the new type of radiation found at great heights.  相似文献