The eastern continuation of the Cadomian orogen: U–Pb zircon evidence from Saxo-Thuringian granitoids in south-western Poland and the northern Czech Republic

We report U–Pb single zircon ages from three pre-Variscan granitoids in the NE part of the Bohemian Massif. The Platerówka granodiorite from the Lausitz-Izera Unit, the Polish Sudetes, has been dated at 533±9 Ma. The Bitouchov granite form the SW part of the South Krkonoe Unit, the Czech Sudetes, gave an age of 540+11/–10 Ma, and the Wdroe granodiorite in the Fore-Sudetic Block yielded 548±9 Ma. All these latest Vendian/Early Cambrian granitoids represent the post-tectonic expression of a late Proterozoic Cadomian orogenic cycle and demonstrate the eastward extent of the Cadomian basement into the Variscan orogen. Granodiorites of similar age have so far been reported from Brittany and especially from the Saxo-Thuringian Terrane to the NE and SW of the Elbe Fault Zone. We conclude that the Saxo-Thuringian Terrane extends across the Elbe and Sudetic Marginal Fault Zones into the Fore-Sudetic Block.     

Effects of the number of stations and time resolution on derivation

For at least 30 years now it has been well known that the Dst index can be modelled using the solar wind as input. Since then, many attempts have been made to improve the predictability of Dst using different approaches. These attempts are useful, for instance, to understand which features of the solar wind–magnetosphere interactions are most important in producing magnetospheric activity and how the Dst index would improve the space weather forecast. The Dst index is by far the most reliable and simple indication that a magnetic storm is in progress. In this work, the effect of using more than four magnetic stations and shorter time intervals than the hourly averages used in Sugiura's procedures is evaluated. The discussion is based on the results presented by Burton in 1975 and Feldstein in 1984 considering 4 or 12 magnetic stations and time averages of 2.5 min for a magnetic disturbed period that occurred from February 7–28, 1967, including two geomagnetic storms. The analysis has shown that the global representation of a magnetic storm by the standard Dst (Sugiura) is well preserved either using 4, 6, 12 magnetic stations or using 1 h, 2.5 min 1 min averages. A brief review of the current understanding of Dst has been included to support the discussions. The analysis performed has shown that a more refined Dst index (time and number of stations>4) would be useful to investigate the intrinsic processes and the different current systems involved in the ring current development during magnetic storms; the standard Dst, as it is conceived, is quite adequate to monitor geomagnetic storms and identify their overall features; concerning the magnetic stations normally considered, the inclusion of higher magnetic latitude stations (>35) may underestimate the observed Dst.     

3mm多普勒云雷达测量反演云内空气垂直速度的研究

垂直指向的W-波段大气云雷达(WACR)不仅测量云粒子的反射率因子Z, 而且测量多普勒速度谱。本文利用寿县气象站WACR在2008年11月1日一个时段的测量, 进行云内空气垂直速度反演试验。首先讨论个例中反射率、 Doppler平均速度及谱宽的分布特征及原因, 然后利用小粒子示踪法和改进的以小粒子示踪法为基础的粒子下降速度w0—反射率因子 (w0－Z) 关系法反演了云内空气垂直速度, 进而结合Doppler谱数据分析反演结果。结果显示: 小粒子示踪法在湍流较弱时能比较精确地反演空气垂直速度, 而湍流较强时, 湍流造成的误差不可忽略; 改进算法在湍流较强时能够减少湍流对反演结果的影响。     

ADS 80数码航摄仪L0级影像后处理试验

介绍了三线阵数码航摄仪ADS 80,探讨了其Level 0级影像的后处理技术,分析了不同软件在相同地面分辨率下不同地面控制条件下的后处理精度。得出的结论是控制点分布、数量、位置和航摄影像地面分辨率对ADS 80相机L0级影像空三解算和生成的L1级影像精度影响较大;在充分考虑以上因素的情况下,ADS 80相机在获取的航摄影像地面分辨率低于成图比例尺要求时仍能得到较高的校正精度。     

1951—2007年辽宁省农业界限温度变化及其成因探讨

对1951-2007年辽宁省稳定通过0℃、10℃积温和持续日数变化进行了分析.结果表明:(1)近57年来辽宁省稳定通过0℃和10℃积温和持续日数呈递增趋势,其中稳定通过10℃积温和持续日数递增趋势更明显;(2)各标准气候期稳定通过0℃和10℃积温变化趋势不同,第1个和第2个30年标准气候期呈现递增趋势较弱,最近30年标准气候期呈显著递增趋势;各标准气候期稳定通过0℃和10℃持续日数均为递增趋势,而且后期递增较前期更为显著;(3)中部和沿海城市稳定通过0℃、10℃积温和持续日数递增趋势强于北部和西部;(4)城市化引起的热岛效应是观测到的稳定通过0℃、10℃积温和持续日数递增的重要原因,而区域气候变暖则进一步加强了递增趋势.     

Photometric observations and orbital period variations of HS 0705 + 6700 and NY Vir

We present photometric observations of two post-common-envelope stars, NY Vir (=PG 1336-018) and HS 0705 + 6700. The V band CCD observation of NY Vir was performed by a 40 cm telescope at Ege University Observatory and the R band observations of HS 0705 + 6700 were performed by 100 cm telescope at TÜB?TAK National Observatory. The new light curves were analyzed by the WD code and the physical parameters of stars were determined. We obtained new mid-eclipse timings for HS 0705 + 6700 and combined them with those previously published data. The analysis of the O-C residuals yields a period of about 8.06 ± 0.28 yr and an amplitude of 98.5 s for the system HS 0705 + 6700, which is attributed to the third star physically bounded to the evolved eclipsing pair. A mass function of 1.2 × 10⁻⁴ M_⊙ for the third star is obtained. The existence of a third star is also confirmed by the light curve analysis, indicating light contribution of about 0.043 at phase 0.25 in R-bandpass of the eclipsing pair. Using mass-luminosity relationship of the low mass stars we estimate a mass of 0.12 M_⊙ with an orbital inclination of about 20°. The O-C residuals obtained for the system NY Vir were represented by a downward parabola which indicates orbital period decrease in the system. Using the coefficient of quadratic term we calculate a rate of orbital period decrease of about dP/dt = −4.09 × 10⁻⁸days yr⁻¹. The period decrease we have measured in NY Vir may be explained by angular momentum loss from the binary system.     

贵州梵净山前寒武系甚低级变质作用研究

本文运用伊利石结晶度、绿泥石结晶度、云母b0值和绿泥石地质温度计研究了梵净山前寒武系甚低级变质作用。结果表明经Kisch伊利石结晶度标样校正的伊利石结晶度Kübler指数为0.20~0.99°Δ2θ,绿泥石结晶度árkai指数为0.22~0.63°Δ2θ。由此阐明梵净山前寒武系经历了成岩作用到浅变质作用的影响,迄今依然保留了成岩带、近变质带和浅变质带的岩石记录。成岩岩石具有伊蒙混层特征成岩指示矿物,浅变质带具有钠云母特征变质指示矿物。钾云母(伊利石)b0值范围为:0.9000~0.9045nm;平均0.9018nm,b0值累积频率曲线分布介于典型中压—中低压系列之间,估算的压力为366MPa。峰期变质温度为293~364℃,平均342℃,古变质温压梯度为27℃/km。近变质带界线穿越地层和梵净山背斜轴线,表明甚低级变质作用为成岩-构造运动同期或后期构造增厚引起下部和底部岩石随温压的升高而产生的。     

A LIMITED-LENGTH-SCALE k-ε MODEL FOR THE NEUTRAL AND STABLY-STRATIFIED ATMOSPHERIC BOUNDARY LAYER

Analytical and numerical models of the neutral and stably-stratifiedatmospheric boundary layer are reviewed. Theoretical arguments andcomputational models suggest that a quasi-steady state is attainable in aboundary layer cooled from below and it is shown how this may be incorporatedwithin a time-steady, one-dimensional model. A new length-scale-limitedk- model is proposed for flows where a global maximum mixing length isimposed by the finite boundary-layer depth or, in stably-stratifiedconditions, by the Obukhov length, whilst still reducing to a form consistentwith the logarithmic law in the surface layer. Simulations compare favourablywith data from the Leipzig experiment and from Cardington airfield inEngland.     

低浓度磷酸一酯的膜富集和气相色谱测定

磷酸一酯（ＲＯ）Ｐ（Ｏ）（ＯＨ）２是一种强极性的有机磷化合物。研究了水体中磷酸一（１－萘）酯的富集和上色谱分析,建立了一个简便快速、高灵敏度、实用的分析方法。富集是采用固相萃取方法,选用载有十八烷基硅烷的尼龙滤膜吸附,甲醇洗脱,回收率达７２％￣７％。它的气相色谱分析选用ＢＳＴＦＡ为衍生剂,反应条件为温度６５℃,反应时间３０ｍｉｎ,获得了满意的结果。方法的最低检测限为０。０６ｎｇ。     

海洋沉积物中烃类化合物预处理条件优化及应用

运用分辨率高、稳定性好的ＨＰ６８９０ 毛细管气相色谱仪定性、定量测定海洋沉积物中的正构烷烃和多环芳烃。对沉积物样品的预处理中抽提、蒸发、柱层析、萃取等步骤条件进行优化。优化方法中,正构烷烃系列化合物回收率为６５ ％ ～７６ ％ ,多环芳烃系列化合物为８８ ％ ～９５％ ,标准偏差是２．７％ ～２０．２％ （ｎ＝ ３）