云南羊拉铜矿矽卡岩形成时代与矿床成因：来自石榴子石和磁铁矿组分的约束

羊拉铜矿是金沙江缝合带中部已发现的规模最大的印支期铜矿床,矿体以层状—似层状产出于花岗闪长岩外围、变质砂岩与碳酸盐岩地层的层间破碎带中。该矿床在成因类型上存在喷流-沉积成因、复合成因、矽卡岩成因等多种观点。本文以矽卡岩矿石中石榴子石、磁铁矿为研究对象,利用LA-ICP-MS原位微区分析技术开展了石榴子石U-Pb年代学和石榴子石、磁铁矿成分测试分析,以进一步限定该矿床成矿时代和成因类型。分析结果显示,石榴子石中U、Th、Pb的含量分别为1.18×10^-6～6.69×10^-6、0.04×10^-6～1.43×10^-6、0.11×10^-6～1.16×10^-6,获得Tera-Wasserburg下交点年龄为231.0±5.3 Ma(2σ,n=32,MSWD=2.1),与矿区花岗闪长岩形成时代高度一致。结合磁铁矿微量元素组成与全球矽卡岩型矿床可类比等特征,明确羊拉铜矿床属于典型矽卡岩型铜矿床。石榴子石以钙铁榴石组分为主,具轻稀土富集、重稀土亏损的配分模式,这可能受晶体...     

丽水市旅游气候舒适度分析

采用人体舒适度气象指数（BCMI）、寒冷指数（CI）、温湿指数（THI）和度假气候指数（HCI）等4个综合性的气候指标,对丽水市的旅游气候舒适度进行了分析评价,并着重对比分析了BCMI和HCI对旅游气候适宜性的表征能力。结果表明：丽水市全年有8个月BCMI处在4～6级之间,属一类气候适宜区;冬季CI值较低,无严寒现象,夏季低海拔地区THI值偏高,但海拔600 m以上地区（约占市域面积6成）THI值较低,适宜“避暑纳凉”;HCI比传统的BCMI表现的更客观、更全面,它不仅考虑了气候的热舒适性影响,还考虑了降水和云量对旅游出行及观光的影响,且就时间尺度而言,HCI更适合旅游舒适度逐日预报的开展。     

2007/2008和2008/2009冬季平流层强、弱极涡事件对应的行星波活动的对比分析

在对逐日气象资料进行纬向谐波分析的基础上, 对比和讨论了2007/2008年冬季强极涡期间和2008/2009冬季弱极涡期间平流层和对流层不同波数的行星波的变化特征, 特别关注强极涡或弱极涡发生之后, 500 hPa 沿60°N和30°N行星波1波和2波振幅和位相的差异, 以及相应的500 hPa位势场的差异, 进而讨论为什么不同的平流层极涡异常会对东亚有不同的影响, 特别讨论为什么同一种极涡异常, 对我国南北方近地面气温的影响会不同。结果表明:平流层极涡发生异常时, 平流层行星波活动有明显的异常。随着极涡异常的下传, 对流层行星波的振幅和位相也有明显的变化, 而且, 对于不同的纬度带, 其变化又有不同, 表现为:2008年1月强极涡发生之后, 500 hPa行星波1波和2波的扰动都向南伸, 而2009年1月的弱极涡(SSW)期间和之后, 1波和2波的扰动都偏北; 在对流层, 强极涡和弱极涡发生之后不但行星波1波和2波的振幅有所差异, 其位相也有明显的不同。特别是, 其位相的差异还随纬度而变化。就同一年(或者说对于同是强极涡或者同是弱极涡)而言, 无论是1波还是2波, 在60°N和30°N附近的扰动相比, 几乎反位相。这样就使得它们的500 hPa 位势场也有明显不同:在东半球, 主要表现为乌拉尔高压和东亚大槽的强度和位置不同。2008年1月强极涡发生之后, 乌拉尔高压和东亚大槽东移, 不利于冷空气向欧亚大陆北部(包括我国北方)的输送, 使这些地区的温度偏高;而2009年1月弱极涡之后, 东亚大槽西退, 利于冷空气向欧亚大陆北部输送, 导致这些地区较冷。对于同一种极涡异常(如2008强极涡或者2009弱极涡)由于南方和北方行星波扰动的位相不同, 对南方和北方冷暖空气的输送也就不一样。所以同一种极涡异常对(我国)南北地区的温度影响是不同的。     

分块DPCM与5/3整数小波变换结合的天文图像无损压缩

针对海量的天文图像数据与有限的存储空间和带宽资源之间矛盾日益突出这一问题,提出一种无损压缩方法,首先将超大天文图像分块,再使用差分脉冲编码调制和5/3整数小波变换,最后使用霍夫曼算法编码。对该方法的原理和具体实现做了详细的分析与介绍,通过实验验证该方法比天文中常用的tar、PKZip、WinZip、WinRar软件在压缩比上分别提高了30%、29%、26%、2%,压缩速度远大于WinZip和WinRar;且该算法实现简单,适合硬件实现和利于并行处理。     

Dependence of the holmberg effect on separations between paired galaxies

To investigate the dependence of the Holmberg effect of paired galaxies on three-dimensional separations, we have constructed four subsamples characterized by three-dimensional separations s ≤ 50 kpc, 50 kpc < s ≤ 100 kpc , 100kpc < s ≤150kpc , and 150 kpc < s ≤ 200 kpc , respectively. In this study, linear correlation coefficients and surplus standard deviations of color indices, luminosity, and size between two components of paired galaxies are calculated. It is found that there is a weak tendency for correlation coefficients of color indices to increase with decreasing three-dimensional separations, but such a tendency does not exist for ones of luminosity and size. We also note that there is no tendency for surplus standard deviations to decrease with decreasing three-dimensional separations. This suggests that it is still very difficult to clearly affirm the dependence of the Holmberg Effect of paired galaxies on three-dimensional separations.     

Secular period decreasing of detached chromospherically active binaries

The long-term orbital period changes of a large sample of detached chromospherically active binaries (CABs) were studied. Eleven such systems were found to be undergoing secular period decreases with the rates of ?6.3×10^?9 to ?1.1×10^?6 days per year. The period decreasing rates are found to vary depending on the orbital period. The longer the orbital period is, the more rapidly the period decreases. Following Stepien (Mon. Not. R. Astron. Soc. 274:1019, 1995), the period decreasing rate predicted by angular momentum loss (AML) caused by magnetic wind is computed for each system. A comparison between the observed and calculated period decreasing rates shows that the former values are obviously larger than the latter by 1–3 orders of magnitude. It suggests that the magnetic wind is not likely the determinant mechanism driving the AML in these systems. Finally, the orbital angular momentum (AM) and the rate of AML, $\dot{J}$ , are computed for each system. It shows that the AM have a similar change with the orbital period like dP/dt does, but $\log\dot{J}/J$ presents no strict changing with the kinematical ages.     

REE and Sr-Nd Isotope Geochemistry for Yixian Fluorite Deposit,Western Liaoning Province,China,and Its Geological Implications

Up to now,there were no systematic studies of geochemistry and isotopic age for the Yixian(义县) fluorite deposit,western Liaoning(辽宁) Province,China.Based on the analysis of metallogenic geological setting,we studied the REE,Rb-Sr and Sm-Nd isotopes.The chondrite-normalized REE patterns of fluorite are characterized by moderate LREE depletion(LREE/HREE=0.95-3.57,(La/Yb)N=0.08-2.84) and enrichment of Sr(146×10-6-596×10-6) and moderately positive Eu anomalies(δEu=1.10-1.34),which are similar to those of the ho...     

青藏高原昆仑—汶川地震系列与巴颜喀喇断块的最新活动

青藏高原是中国最主要的地震活动区之一。最近十多年来,在青藏高原中部连续发生了1997年西藏玛尼Ms7.5级地震、2001年青海昆仑山Ms8.1级地震、2008年3月新疆于田Ms7.3级地震和5月四川汶川Ms8.0级地震及2010年青海玉树Ms7.1级地震,它们相继发生于青藏断块区巴颜喀喇断块四周边界活动断裂带上,是该断块最新活动的结果。发生于断块南北边界断裂上的3次地震都是走滑断裂错动的结果,发生在断块东南端的汶川地震则是挤压逆冲断裂的产物,而西北端的于田地震则呈现出张性特征,它们共同反映青藏断块区巴颜喀喇条状断块向东南方向滑动的最新活动。自1900年以来,青藏断块区和巴颜喀喇断块的强震活动表现出多期活动和区域性转移的特征,20世纪早期Ms7.0级以上强地震活动的主体地区在青藏断块区北部边界构造带,中期转移到高原南部喜马拉雅板块边界构造带和断块区南部断块,最近十多年来则在巴颜喀喇断块及周缘边界断裂上活动。青藏高原这种块体活动和地震活动与澳大利亚-印度板块对亚洲大陆的推挤作用相关,因而,青藏高原和巴颜喀喇断块的强震活动与澳-印板块边界苏门答腊强震活动相对应。目前苏门答腊地区强震活动仍在继续,因此,近期对巴颜喀喇断块及青藏高原南部地区的强震活动和强震危险性仍需加以注意。     

Mineralogical and geochemical investigations of the Dajia Salento-type bauxite deposits,western Guangxi,China

The Dajia Salento-type bauxite deposit in western Guangxi is hosted within the Quaternary ferrallitic soil profile, and it formed via breaking up, weathering and oxidizing of Permian bauxite orebodies occurring as a semi-continuous layer in the upper Permian. Mineralogical analyses reveal that diaspore, hematite and kaolinite are the major minerals in bauxite ores with small amounts of anatase, chamosite, gibbsite, goethite, illite, zircon, quartz and pyrite. The ore texture and mineral assemblage reveal that the depositional/diagenetic environment of the Dajia bauxite was much close to phreatic environment. Both the ore texture and the morphology of zircon grains also indicate that most of the bauxitic soils were transported a short distance. Diaspore is suggested to be non-metamorphic in origin and mainly formed in a reducing condition of diagenetic environment, while kaolinite is the product of the in situ epigenetic replacement of alumina in diaspore by dissolved silica. Geochemical analyses indicate that Al₂O₃, Fe₂O₃, SiO₂ and TiO₂ are the main components of the bauxite ores and trace elements such as Zr, Hf, Nb, Ta, Th and U were enriched during the bauxitization process. Simultaneously, Zr vs. Hf and Nb vs. Ta show a high correlation. Geochemical indices such as Zr/Hf, Nb/Ta and Eu/Eu* (among others) denote that the magmatic rocks related to the Emeishan plume in western Guangxi and the carbonates in the underlying Maokou Formation provided the main sources of material for the bauxite ores.