Geology, Geochemistry and Genesis of the Hongshijing Gold Deposit in Ruoqiang,Xinjiang

1IntroductionTheHongshijinggolddepositislocatedinthenorthofLuobupouLakeofRuoqiang ,about 30 0kmsouthwestofHamiCity ,Xinjiang .ItwasdiscoveredbytheSixthGeologicalTeamofXinjiangduringgeo chemicalexploration .TheHongshijinggolddeposit,whichoccursinthegold bearingformationcomposedofMiddleandLateCarboniferousvolcanicandpyroclasticrocks ,isabrittle ductileshearzonetypegolddepositcontrolledbyariftbelt.TheHongshijinggolddepositislocatedinthesouthwestoftheHongshi jing -Maotoushanmineralizationb…     

遥感用于地震预报的途径

本文提出了遥感用于地震预报的思路、途径及步骤,并从理论上进行了阐述。     

中国重要金属矿产资源现状、供需、进出口数据集

金属矿产是经济社会发展的物质基础。本数据集采集了16种对国民经济发展有重要影响的大宗紧缺矿产（铁、锰、铜、铝、金、铅、锌、镍、铬）、优势矿产（钨、钼、锡、锑）及战略新兴矿产（锂、钴、钛）2006—2017年的世界及中国资源储量、原矿产量、消费量、贸易量及贸易金额等数据。数据集为Excel表格型数据,包含6个sheet表（世界资源量、中国查明资源储量、中国基础储量、中国原矿产量、中国原矿消费量、中国进出口量）,旨在分析研究我国在工业化进程中后期阶段所需重要金属矿产的资源现状和供需趋势。数据集显示：①我国大宗紧缺矿产如铁、锰、铜、金等查明资源储量虽稳步增长,但开采消耗量大,使得基础储量增速缓慢;未来需求总量仍将维持高位,国内保障程度不足,进口量持续攀升。优势矿产资源钨、锑储采比低,后备资源接替不足,优势程度下降;②战略新兴矿产锂、钴、钛资源量、基础储量增长缓慢或呈下降态势,国内资源品质较差,难利用资源多;产量、消费量近十年快速增长,且未来将持续高增长,国内资源储量增长缓慢,供需矛盾凸显。该数据集对已有金属矿产供需数据的收集和总结,为今后金属矿产勘查及战略部署提供参考。     

山东重力场季节性变化特征

利用山东地区2010—2012年6期流动重力测量资料,研究了鲁南网重力场的变化特征。结果表明重力场呈明显的季节性变化,即每年的3月与8月,重力场存在反向变化,变化幅值相近;季节性变化与降水有关。     

Puzzling Origin of CEMP-r/s Stars: An Interpretation of Abundance and Enrichment of s- and r-Process Elements from Asymptotic Giant Branch Supernovae

CEMP-r/s stars at low metallicity are known as double-enhanced stars that show enhancements of both r-process and s-process elements. The chemical abundances of these very metal-poor stars provide us a lot of information for putting new restraints on models of neutron-capture processes. In this article, we put forward an accreted scenario in which the double enrichment of r-process and s-process elements is caused by a former intermediate-mass Asymptotic Giant Branch (AGB) companion in a detached binary system. As the AGB superwind is only present at the ultimate phase of AGB stars, there is thus a lot of potential that the degenerate-core mass of an intermediate-mass AGB star reaches the Chandrasekhar limit before the AGB superwind. In these circumstances, both s-process elements produced in the AGB shell and r-process elements synthesized in the subsequent explosion would be sprayed contemporaneously and accreted by its companion. Despite similarity to physical conditions of a core-collapse supernova, a major focus in this scenario is the degenerate C–O core surrounded by an envelope of a former intermediate-mass AGB donor that may collapse and explode. Due to the existence of an outer envelope, r-process nucleosynthesis is expected to occur. Hypothesizing the material-rich europium (Eu) accreted by the secondary via the wind from the supernova to be in proportion to the geometric fraction of the companion with respect to the exploding donor star, we find that the estimated yield of Eu (as representative of r-process elements) per AGB supernova event is about 1 × 10^?9 M _⊙ ～ 5 × 10^?9 M _⊙. Using the yields of Eu, the overabundance of r-process elements in CEMP-r/s stars can be accounted for. The calculated results show that the value of parameter f , standing for efficiency of wind pollution from the AGB supernova, will reach about 10⁴, which means that the enhanced factor is much larger than unity due to the impact of gravity of the donor and the result of the gravitational focusing effect of the companion.     

Molecular phylogenetic analysis of attached Ulvaceae species and free-floating <Emphasis Type="Italic">Enteromorpha</Emphasis> from Qingdao coasts in 2007

Based on the sequence data of the nuclear ribosomal DNA internal transcribed spacer (ITS) 1, 5.8 S, and ITS 2, the molecular phylogeny was analyzed on Ulvaceae species collected from Qingdao coasts in summer of 2007, including 15 attached Ulva and Enteromorpha samples from 10 locations and 10 free-floating Enteromorpha samples from seven locations. The result supported the monophyly of all free-floating Enteromorpha samples, implying the unialgal composition of the free-floating Enteromorpha, and the attached Ulvaceae species from Qingdao coasts were grouped into other five clades, suggesting that they were not the biogeographic origin of the free-floating Enteromorpha in that season. Supported by NSFC (40506030); the Innovative Key Project of the Chinese Academy of Sciences (KZCX2-YW-209); Science & Technology Project of Qingdao City (06-2-2-12-JCH)     

小叶锦鸡儿(Caragana microphylla)群落蒸散发模拟

基于2016、2017年生长季原位气象监测数据,利用Shuttleworth-Wallace(S-W)模型模拟了科尔沁沙地主要固沙植物小叶锦鸡儿(Caragana microphylla)群落的蒸散发,对蒸散组分进行了拆分,并利用涡度相关系统对模拟蒸散发值进行了验证。结果表明:2016、2017年生长季小叶锦鸡儿群落蒸散发量分别为345.4、325.2 mm,土壤蒸发量分别为93.8、83.8 mm,植被蒸腾量分别为251.6、241.4 mm,土壤蒸发占总蒸散发分别为27.2%、25.8%。30 min尺度上模拟值与实测值一致性较高,模拟精度大体表现为晴天>阴天>雨天。持续干旱和降水后,小叶锦鸡儿蒸腾耗水规律明显不同,持续干旱时期小叶锦鸡儿保持较低的蒸腾耗水,且具有明显的"午休"现象,连续降水后小叶锦鸡儿"午休"消失,蒸腾耗水增强。饱和水汽压差是影响小叶锦鸡儿蒸散发的主要因子。     

基于均衡伪多道匹配滤波的海底电缆多次波压制方法研究（英文）

由于自由表面、海底等强反射界面的影响,海底电缆采集资料中鸣震等干扰往往非常严重且与有效波耦合在一起,降低了资料品质。海底电缆双检合成技术利用速度检波器和压电检波器对于下行波场的不同极性响应可以有效压制检波点端多次波,突出有效反射,提高地震资料的分辨率。本文在深入研究双检合成理论及匹配滤波技术的基础上,提出了基于均衡伪多道自适应匹配滤波方法的双检匹配合成方法压制检波点端多次波,不依赖于传统的求取反射系数的匹配合成方法,完全数据驱动,并在合成记录和实际资料的处理过程中均取得了良好的效果,证明了方法的有效性。     

基于AHP的地质遗迹旅游资源评价:以汉中天坑群为例

汉中天坑群是在中国32°~33°N湿润热带—亚热带岩溶地貌区北界首次发现的岩溶地质遗迹。为了科学地评价汉中天坑群地质遗迹旅游资源,为下一步旅游规划与开发提供科学依据,本文从生态旅游资源条件、生态环境条件、生态旅游开发条件等3个方面选取资源景观价值、资源科学与文化价值、生态环境质量、环境安全条件、区位与交通条件和社会经济条件等作为主要评价指标,建立多层层次结构模型,运用层次分析法对其进行地质遗迹旅游资源综合评价,得出汉中天坑群地质遗迹旅游资源综合评价得分为90.67分。本文研究表明,汉中天坑群具有五级生态旅游资源的禀赋,具有较高的开发利用价值。      

云南鹤庆盆地近1Ma来的气候序列重建初探

云南鹤庆盆地近1Ma来的孢粉植物群很好地揭示了本区的环境演化过程。本文利用植物生态位知识,通过模糊数学方法对鹤庆(QH)孔孢粉序列所记录的古气候信息进行重塑,建立了近1Ma来的年均温、年降水量及年较差序列,并将本区气候演化分为4个气候旋回,32个气候期。该序列可与黄土-古土壤序列及海洋δ18O阶段对比,但冷暖波动的幅度及降温时段持续的长短有其特色,表明本区气候既受全球气候变化的控制,又受青藏高原阶段隆升的制约;近1Ma来气温的波动幅度呈递增趋势,0.30MaB.P.尤其显著;冷、暖段间年均温的变化幅度由第一气候旋回的7℃增大到第三气候旋回的9℃(按4次平滑值计算),而样点的实际最大差值由8℃增至16℃;最强烈的降温发生在第二气候旋回中的0.45～0.14MaB.P.时间段,这与玉龙雪山冰川活动规模最大相一致;降温时年降水量及年较差值增大,证实近1Ma来,西南季风区的气候组构与东南季风区不同。