夏季两次低槽冷锋型暴雨成因对比分析

利用常规观测资料和NCEP 1°×1°再分析资料,对对流层低层无低涡、无低空急流配置的低槽和冷锋影响下2004年7月29—30日后倾槽和2004年8月3—4日前倾槽两次暴雨过程的成因进行了对比分析,结果表明: 虽然两次过程对流层中低层形势非常相近,但在空间结构上却存在显著差异。后倾槽锋区向冷空气倾斜且成3段锋,其中,第1段锋在850 hPa以下,冷空气虽较弱,但对整个降水过程起抬升触发作用,暴雨区出现在该段锋移动方向的前沿,即地面辐合线呈气旋性弯曲的流线密集处;前倾槽锋区完整,湿斜压锋区向暖区倾斜,暴雨区出现在锋前1～2个纬距处,即地面辐合线右侧偏南气流密集带中。两次过程低层均有强的水汽输送,存在高温高湿区,925 hPa比湿均达15 g〖DK〗·kg-1以上,所不同的是,后倾槽暴雨区位于水汽通量大值区、等〖WTBX〗θe〖WTBZ〗密集线前沿及风场辐合明显的水汽辐合区内,而前倾槽暴雨区则位于水汽通量等值线密集带中的水汽辐合区、〖WTBX〗θe〖WTBZ〗暖舌的舌尖和风场辐合处,但更偏向暖空气一侧。此外,暴雨易发生在山区或海岸线等特殊地形抬升的区域。     

冲绳海槽中段表层沉积物物源判识及定量估算

海洋沉积物的物质来源的定量、半定量研究,是海洋沉积学的重要课题之一,也是难题之一。本文是从沉积物不同成因组分的含量入手,研究冲绳海中段表层沉积物物质来源的一种尝试。首先介绍了常规法（即镜下鉴定和统计）和碳稳定同位素示踪法的基本途径和计算模式,并对两种方法进行了对比和评价。其次,根据沉积物的具体情况,选择比较合适的方法,定量估算了各站各成因组分的含量。最后根据估算结果,编绘了主要成因组分含量的分布图。     

基于浮标资料的中国东部海域最大波高特征分析

利用原国家海洋局2010—2015年的浮标资料,计算渤、黄、东海有效波高和最大波高的线性关系,并通过1992—2011年共20 a的数值模拟有效波高资料计算中国东部海域各月的2.5 m、4 m、6 m以上最大波高频率和最大波高月极值分布。结果发现:中国东部海域由北至南,最大波高与有效波高的比值逐渐增大;最大波高频率和最大波高月极值空间分布均由渤海、黄海至东海逐渐增大,最大波高频率的极值12月最大,4或5月最小,最大波高月极值9月最大,4月最小。其时空分布表明:受不同天气系统影响,夏秋季台风较多,容易出现极值较大的最大波高;秋冬季冷空气较强,虽然最大波高极值相对较小,但大浪持续时间长、频率大、影响范围广。     

A BRIEF INTRODUCTION TO THE NEW METHOD FOR RIVER PROFILE ANALYSIS: Integral Approach

The topography and geomorphology of active orogens result from the interaction of tectonics and climate. In most orogens, a fluvial channel is most sensitive to the coupling between tectonics, lithology, and climate. Meanwhile, the related signals have been recorded by both the drainage geometry and channel longitudinal profile. Thus, how to extract tectonic information from fluvial channels has been a focused issue in geologic and geomorphologic studies. The well known stream-power river incision model bridges the gap between tectonic uplift, river incision and channel profile change, making it possible to retrieve rock uplift pattern from river profiles. In this model, the river incision rate depends on the rock erodibility, contributing drainage area and river gradient. The steady-state form of the river incision model predicts a power-law scaling between the drainage area and channel gradient. Via a linear regression to the log-transformed slope-area data, the slope and intercept are channel concavity and steepness indices, respectively. The concavity relates to lithology, climatic setting and incision process while the channel steepness can be used to map the spatial pattern of rock uplift. For its simple calculation process, the slope-area analysis has been widely used in the study of tectonic geomorphology during past decades. However, to calculate river slope, the coarse channel elevation data must be smoothed, re-sampled, and differentiated without any reasonable smooth window or rigid mathematical fundamentals. One may lose important information and derive stream-power parameters with high uncertainties. In this paper, we introduce the integral approach, a procedure that has been widely used in the latest four years and demonstrated to be a better method for river profile analysis than the traditional slope-area analysis. Via the integration to the steady-state form of the stream-power river incision equation, the river longitudinal profile can be converted into a straight line of which the independent variable is the integral quantity χ with the unit of distance and the dependent variable is the relative channel elevation. We can calculate the linear correlation coefficient between elevation and χ based on a series of concavity values and find the best linear fit to be the reasonable channel concavity index. The slope of the linear fit to the χ value and elevation is simply related to the ratio of the uplift rate to the erodibility. Without calculating channel slope, the integral approach makes up for the drawback of the slope-area analysis. Meanwhile, via the integral approach, a steady-state river profile can be expressed as a continuous function, which can provide theoretical principle for some geomorphic parameters (e.g., slope-length index, hypsometric integral). In addition, we can determine the drainage network migration direction using this method. Therefore, the integral approach can be used as a better method for tectonogeomorphic research.     

The Sloan Digital Sky Survey monitor telescope pipeline

The photometric calibration of the Sloan Digital Sky Survey (SDSS) is a multi‐step process which involves data from three different telescopes: the 1.0‐m telescope at the US Naval Observatory (USNO), Flagstaff Station, Arizona (which was used to establish the SDSS standard star network); the SDSS 0.5‐m Photometric Telescope (PT) at the Apache Point Observatory (APO), NewMexico (which calculates nightly extinctions and calibrates secondary patch transfer fields); and the SDSS 2.5‐m telescope at APO (which obtains the imaging data for the SDSS proper). In this paper, we describe the Monitor Telescope Pipeline, MTPIPE, the software pipeline used in processing the data from the single‐CCD telescopes used in the photometric calibration of the SDSS (i.e., the USNO 1.0‐m and the PT). We also describe transformation equations that convert photometry on the USNO‐1.0m u ′g ′r ′i ′z ′ system to photometry the SDSS 2.5m ugriz system and the results of various validation tests of the MTPIPE software. Further, we discuss the semi‐automated PT factory, which runs MTPIPE in the day‐to‐day standard SDSS operations at Fermilab. Finally, we discuss the use of MTPIPE in current SDSS‐related projects, including the Southern u ′g ′r ′i ′z ′ Standard Star project, the u ′g ′r ′i ′z ′ Open Star Clusters project, and the SDSS extension (SDSS‐II). (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

氮钾配施对生姜产量和砂姜黑土肥力的效应

研究了淮北平原砂姜黑土地区生姜氮钾配施的增产效应和对土壤养分的影响。结果表 明:氮钾配施可以大幅度提高生姜的产量,施钾的增产幅度,柴姜为15.3%～58.4%,平均增产率 为35.8%;狮子头姜产量提高18.2%～46.9%,平均增产28.7%。增施氮钾肥可有效提高土壤有 机质、全N、有效P、速效K、缓效K、有效Ca和有效Mg含量,降低NO3-盐含量,促使土壤pH趋于 中性,对全P和碱解N含量影响较小。土壤N素和P素大量盈余,不施钾时土壤K亏损严重,施钾 处理土壤钾基本上处于盈余状态,有利于维持和提高土壤肥力。     

Evidence for high‐temperature fractionation of lithium isotopes during differentiation of the Moon

Lithium isotope and abundance data are reported for Apollo 15 and 17 mare basalts and the LaPaz low‐Ti mare basalt meteorites, along with lithium isotope data for carbonaceous, ordinary, and enstatite chondrites, and chondrules from the Allende CV3 meteorite. Apollo 15 low‐Ti mare basalts have lower Li contents and lower δ⁷Li (3.8 ± 1.2‰; all uncertainties are 2 standard deviations) than Apollo 17 high‐Ti mare basalts (δ⁷Li = 5.2 ± 1.2‰), with evolved LaPaz mare basalts having high Li contents, but similar low δ⁷Li (3.7 ± 0.5‰) to Apollo 15 mare basalts. In low‐Ti mare basalt 15555, the highest concentrations of Li occur in late‐stage tridymite (>20 ppm) and plagioclase (11 ± 3 ppm), with olivine (6.1 ± 3.8 ppm), pyroxene (4.2 ± 1.6 ppm), and ilmenite (0.8 ± 0.7 ppm) having lower Li concentrations. Values of δ⁷Li in low‐ and high‐Ti mare basalt sources broadly correlate negatively with ¹⁸O/¹⁶O and positively with ⁵⁶Fe/⁵⁴Fe (low‐Ti: δ⁷Li ≤4‰; δ⁵⁶Fe ≤0.04‰; δ¹⁸O ≥5.7‰; high‐Ti: δ⁷Li >6‰; δ⁵⁶Fe >0.18‰; δ¹⁸O <5.4‰). Lithium does not appear to have acted as a volatile element during planetary formation, with subequal Li contents in mare basalts compared with terrestrial, martian, or vestan basaltic rocks. Observed Li isotopic fractionations in mare basalts can potentially be explained through large‐degree, high‐temperature igneous differentiation of their source regions. Progressive magma ocean crystallization led to enrichment in Li and δ⁷Li in late‐stage liquids, probably as a consequence of preferential retention of ⁷Li and Li in the melt relative to crystallizing solids. Lithium isotopic fractionation has not been observed during extensive differentiation in terrestrial magmatic systems and may only be recognizable during extensive planetary magmatic differentiation under volatile‐poor conditions, as expected for the lunar magma ocean. Our new analyses of chondrites show that they have δ⁷Li ranging between ?2.5‰ and 4‰. The higher δ⁷Li in planetary basalts than in the compilation of chondrites (2.1 ± 1.3‰) demonstrates that differentiated planetary basalts are, on average, isotopically heavier than most chondrites.     

面向异构空间区域分片的3RM缝隙处理模型

针对分布式环境下区域分片片段间的各种原始缝隙,提出一种3RM(Three Relational Matrix)缝隙处理模型。该模型采用两阶段流程,第1步划分空间计算单元,对区域分片边界处的要素进行聚类分组;第2步对各个空间计算单元进行缝隙处理。模型研究区域分片边界处缝隙的描述和区分方法,依据要素拓扑关系、属性关系以及精度3种关系建立了3RM缝隙处理矩阵,发现线状和面状要素在分片数据边界处的38种潜在的缝隙,并建立了相应的缝隙处理方法。运用3RM模型对异构的土地利用分片数据进行缝隙处理试验,试验结果表明,本文提出的缝隙处理模型能够有效处理实际分片数据当中的各种缝隙。     

中祁连东段什川杂岩基的岩石化学特征及年代学研究

祁连造山带被托莱南山-了高山构造带及宗务隆山-贵得构造带分为北祁连、中祁连及南祁连构造带.什川岩基位于中祁连构造带东部,由闪长岩、斜长花岗岩、二长花岗岩组成;对二长花岗岩进行U-Pb单颗粒锆石微区LA-ICP-MS同位素测定,获得444.6Ma及414.3Ma两组加权平均年龄,前者代表岩石的形成年龄,后者代表构造热事件年龄.二长花岗岩主量元素w(SiO2)=68.66%～80.77%,w(K2O)/w(Na2O)>1和A/CNK介于0.95～1.21间,总体为钾质钙碱性过铝质花岗岩.岩石富集LILE元素(K、Th、Rb、Ba等),亏损HFSE元素(Ta、Nb、Y等);稀土元素总量较高(∑REE多介于109.05×10-6～322.66×10-6),轻重稀土强烈分馏(∑LREE/∑HREE介于7.92～31.68),稀土元素分配模式为轻稀土富集型,具中等-强Eu负异常(δEu=0.26～0.58).岩石矿物组合及岩石地球化学特征共同表明,什川岩基为中上地壳泥砂质岩石部分熔融而成,形成温度较低,为加厚地壳拆沉熔融成因.这为祁连造山带构造演化及其深部动力学机制研究提供了新的资料.     

青藏高原多年冻土区土壤需氧可培养细菌多样性及群落功能研究

以青藏高原腹地不同植被类型多年冻土区土壤细菌为研究对象, 分析了可培养菌群数量、 多样性和生理代谢功能的变化及其与环境因子间的关系. 结果显示: 从沼泽草甸到高寒荒漠, 土壤水分、 总碳、 总氮含量逐渐降低, pH值升高, 可培养细菌数量在2.97×10⁶~2.88×10⁷ CFU·g^-1, 与含水量、 总碳、 总氮显著正相关; Actinobacteria(51.4%)和γ-Proteobacteria(31.7%)为优势菌群, α-protebacteria仅在沼泽草甸中有分布, β-protebacteria、 Bacterioidetes丰度与含水量、 总碳、 总氮间显著正相关; 自沼泽到荒漠, 菌群代谢活性和Shannon功能多样性指数降低, pH与Shannon指数显著负相关, 继氨基酸类碳源之后, 多聚物逐渐成为被细菌群落主要利用的碳源种类. 研究表明, 伴随冻土退化地上植被逆向演替的过程, 青藏高原多年冻土地下土壤微生物群落丰度、 遗传和代谢功能多样性均发生了不同程度的响应.