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Instruments, Detectors and the Future of Astronomy with Large Ground Based Telescopes

Results of a survey of instrumentation and detector systems, either currently deployed or planned for use at telescopes larger than 3.5 m, in ground based observatories world-wide, are presented. This survey revealed a number of instrumentation design trends at optical, near, and mid-infrared wavelengths. Some of the most prominent trends include the development of vastly larger optical detector systems (> 10⁹ pixels) than anything built to date, and the frequent use of mosaics of near-infrared detectors – something that was quite rare only a decade ago in astronomy. Some future science applications for detectors are then explored, in an attempt to build a bridge between current detectors and what will be needed to support the research ambitions of astronomers in the future.     

Effect of chemical fertilizers on the fractionation of Cu,Cr and Ni in contaminated soil

Effect of chemical fertilizers (urea, NH₄Cl, Ca(NO₃)₂, KCl and KH₂PO₄) on the fractionation of Cu, Cr and Ni was studied by a 4-month incubation experiment. Using sequential extraction procedure, it was found that the application of fertilizers could change the distribution of Cu, Cr and Ni in the fractions of soil. Applying urea (CO(NH₂)₂) significantly decreased the concentrations of Cu, Cr and Ni in water soluble plus exchangeable (WE) fraction, but increased those in Fe–Mn oxides bound (FM) fraction (p < 0.01). However, application of NH₄Cl caused an increase in the WE fraction by 27.7% for Cu, 111.5% for Cr and 20.4% for Ni. The CO(NH₂)₂ raised the soil pH from 4.51 to 4.96, whereas NH₄Cl lowered the pH of soil by 0.44 units. The WE fraction of the three heavy metals was significantly increased, while the FM fraction was significantly decreased by adding KCl (p < 0.01). Moreover, the supply of KH₂PO₄ reduced the WE and carbonate bound (CB) fractions of Cu, Cr and Ni in the soil, however, it raised Cu and Ni in the residual (RS) fraction and Cr in the FM fraction. In addition, the mobility index indicated that KCl and NH₄Cl increased the mobility of Cu, Cr and Ni in the soil, whereas urea and KH₂PO₄ decreased the mobility of the three metals in the soil. These results suggest that applying chemical fertilizers does not only provide plant nutrients, but may also change the speciation and mobility of heavy metals in the soil.     

金活动态提取剂提取-电感耦合等离子体质谱法测定深穿透地球化学样品中的金

金的地球化学勘查基于金的准确测定,地球化学样品中金含量通常处于ng/g水平,需先进行分离富集,再采用电感耦合等离子体质谱法(ICP-MS)或石墨炉原子吸收光谱法(GFAAS)进行测定。当前,隐伏矿床勘查是地球化学探测技术的发展前沿,金活动态提取技术是寻找隐伏金矿的有效手段之一。相比于全量分析,金的活动态含量更低,需要解决选择性提取、高效预富集与准确测定等一系列难题。本文采用柠檬酸铵与土壤中黏土矿物及次生矿物作用促使吸附和可交换组分的金进入提取液,以硫脲和硫代硫酸钠络合金使活动态金向提取液中扩散,达到选择性提取的目的,建立了提取液中金的预富集及ICP-MS测定方法。实验确定的分析条件为:采用5g/L柠檬酸铵-2g/L硫脲-5g/L硫代硫酸钠为提取剂,提取时间24h,在酸性硫脲介质下用活性炭富集金,金吸附率可达89.6%～109.2%,灰化解吸温度为650～700℃。本方法检出限为0.05ng/g,相对标准偏差(RSD)为9.4%～10.2%,加标回收率为91.2%～93.4%。与已报道的硫酸铁-硫脲-硫代硫酸钠溶液提取再GFAAS测定的方法相比,本方法具有检出限低、测试线性范围宽、测试速度快的优势;应用于森林覆盖区黑龙江东安金矿区地球化学探测试验,金活动态异常与隐伏金矿位置一致。     

基于PS-InSAR技术的武威市地面沉降时空变化特征

武威市位于甘肃省中部,是一座典型的农业城市,分布有大量农业耕地。由于土壤疏松,地面容易受到降水和地下水的影响,易发生地面沉降地质灾害对居民的生产、生活造成不利影响。本文利用2017年2月至2022年12月的Sentinel-1A数据,通过PS-InSAR技术提取了武威市的地面沉降监测数据,包括视线向形变速率和累积形变量。对形变场的时空分布特征进行了详细分析,并引入Mogi模型反演地下深部变形范围。最后,结合研究区的降水数据和GRACE重力卫星获取到由陆地水负荷引起的地表形变数据,并对研究区的沉降成因进行了初步分析。结果表明,研究区存在两个主要沉降区,其中主沉降区A的最大累积沉降量达到-290.9 mm,视线向形变速率为-52.0 mm/a;主沉降区B的沉降量达到-178.1 mm,视线向形变速率为-43.8 mm/a。地表沉降呈现周期性变化,且向东南方向逐步扩展,与降水和地下水变化特征相似。通过Mogi模型反演,得出了主沉降区的地下影响范围（半径）和深度,其中主沉降区A为40.96 m和133.67 m,主沉降区B为38.60 m和140.78 m。按季节划分统计形变数据,结果表明,由于研究区所属干旱区,自然降水无法对地面沉降产生显著影响,而农耕时大量地下水的抽取才是导致区域地面沉降的主要原因。

     

新疆东天山地区星星峡群的解体及地质意义

新疆东天山地区星星峡一带的原星星峡群为一套岩性复杂、变质程度差异很大的变质岩系, 在该区进行的1:50000区调工作中, 通过详细的地表调查和地层剖面测量, 并参考了相关变质侵入体的同位素年龄后认为, 根据岩石组合、变质程度、同位素年龄等地质标志, 可将其初步解体为大致形成于晚太古代—古元古代的天湖岩群(Ar₃—Pt₁T.)和长城纪星星峡岩群(ChX.)两套时代不同的岩群。该岩群的解体和区域对比表明, 中天山星星峡一带和塔里木北缘库鲁克塔格一带的前南华系基底应该是一致的, 属于统一的塔里木北缘隆起带。      

进积型三角洲交汇区沉积模式--以东营凹陷沙三中亚段为例

作为碎屑岩储层发育的最主要沉积相类型之一,进积型三角洲在油气勘探领域具有举足轻重的地位;加强对进积型三角洲沉积模式的研究,对于油气储层预测具有重要现实意义。渤海湾盆地东营凹陷古近纪湖盆内发育的东营三角洲和永安三角洲在沙河街组三段中亚段沉积期发生了交汇,而有关两个三角洲的交汇方式、沉积特征及交汇区储层的预测尚未引起足够的重视。以岩芯观测、录井和地震资料为基础,分析了东营凹陷古近系沙三段中亚段三角洲交汇区沉积特征,探讨了沉积期次、交汇过程,建立了三角洲交汇区沉积模式。研究表明,东营凹陷沙河街组三段中亚段主要发育湖泊、进积型三角洲沉积;储集砂体主要形成于三角洲前缘水下分流河道,河口坝微相次之,浊积岩主要分布于深湖区。认为此前界定的东营三角洲的分布范围可能被夸大,而永安三角洲的沉积规模可能被低估。东营凹陷古近系沙三中亚段可划分为9个期次,其作用过程可分为局部交汇阶段和完全交汇阶段。三角洲水下交汇区是水流汇聚和沉积物卸载的有利场所,叠置砂体可成为有利的油气储层,因而具有重要的油气勘探价值。     

太行山地形对“96.8”暴雨影响的数值试验研究

利用ＭＭ４模型,设计了４种模式地形方案,讨论了太行山地形对“９６．８”暴雨降水量的贡献;并利用垂直运动和水汽通量等物理量,探讨了太行山地形对本次暴雨过程增幅作用的机制。结果显示,太行山地形对本次暴雨过程的降水中心强度及位置有显著影响,具有６０％增幅作用。太行山地形对垂直运动及水汽辐合也都具有增幅作用。模式地形越真实,预报结果越好,地形越高,降水增幅作用越明显。     

基于高频GNSS的2014年于田MS7.3级地震的同震位移研究

After the Yutian M_S7.3 earthquake,the authors instantly collected 1Hz high frequency data of the 4 reference stations within 350 km around the epicenter,and calculated the GNSS data with the TRACK module. The results showed that:( 1) The co-seismic displacement of Yutian station,about 54 km from the epicenter,is the most obvious,particularly in the EW component,with a change of about 52.5 ± 11mm,which is more than three times the mean-square error of calculating precision.( 2) In the Yutian reference station,the biggest variation in the EW component appeared within 1 minute after the earthquake.( 3) The change in the NS component is not great.     

应用样条插值提高GRAPES模式物理过程反馈精度

GRAPES (Global/Regional Assimilation and PrEdiction System) 模式动力框架中垂直方向变量的跳层设置采用Charney-Phillips分布,在整层上进行位温、水物质的计算,物理过程中在半层上对其进行处理。这样在GRAPES模式中,进入物理过程之前和物理过程计算完毕之后,都要采用线性插值进行整层和半层之间物理量的转换。由于线性插值精度欠佳,为提高上述反馈过程的精度,并保证水物质的正定性,该研究引入样条插值,并在水物质的插值过程中进行保单调处理,有效减小了位温场、水物质场的预报偏差,并提升了模式的综合预报性能。