武汉市油气库雷电预警服务系统设计与应用

依托湖北省气象局科技发展基金项目,湖北省防雷中心于2013年开发出武汉市油气库雷电预警服务系统。在介绍该系统设计思路、主要功能、运行流程的基础上,以2013年7月5—6日武汉市一次强降水过程为例,选取湖北省气象局所在地周边两家加油站作为服务对象进行系统应用测试,跟踪检测系统运行情况及服务效果。结果表明,雷电预警系统闪电监测准确,预警及闪电信息发布及时,服务对象对此反馈良好。     

Rhomboidal versus triangular spherical harmonic truncation: Some verification statistics

Abstract

In the construction of global primitive equation models, based on the spherical harmonic method, two forms of truncation are in general use. Theoretical considerations suggest the triangular truncation method is superior, but the easily coded rhomboidal truncation is more commonly used. A verification experiment employing the Canadian Operational Spectral Model has been performed to determine if the theoretical superiority of the triangular truncation can be realized in practice. It was found that at least in the restricted case of extra‐tropical forecasts of less than 48 h, that the two truncation methods produced forecasts of equivalent accuracy.     

初夏至盛夏东亚副热带西风急流变化与江淮出梅的关系

利用1961—2005年逐候资料对东亚副热带西风急流初夏至盛夏变化与江淮出梅的关系进行了分析。结果表明,多年平均7月初夏至盛夏急流中心由西太平洋地区西跳至青藏高原的同时我国东部地区急流北跳至37.5°N以北,比梅雨结束早1候;急流北跳使得我国东部高空强辐散中心北移至华北地区,江淮地区上空辐散显著减弱,上升运动减弱,从而使得江淮梅雨结束,雨带北移;而急流中心的西跳仅使得我国东部地区高空辐散中心减弱,降水减弱,有利于雨带北移。我国东部急流北跳与江淮地区梅雨结束时间显著正相关,在北跳偏早(晚)年份梅雨结束早(晚),长江中下游地区降水偏少(多),而急流中心西跳早晚对我国华北北部地区和淮河附近地区降水有较大影响。可见,我国东部急流北跳与梅雨结束关系密切,可作为梅雨结束的先期信号。     

Distribution of early-type stars and dusty matter in the direction of the stellar cluster NGC 1893

The distribution of 255 O-B9-A2, K-G stars and interstellar dust in the direction of the stellar cluster NGC 1893 is studied using V, B-V, and U-B photometric data. Sixteen groups of stars (associations) are discovered at various distances. The first group includes 9 stars of different spectral classes of later types in the sun’s neighborhood lying at a distance of 110 pc. The next 3 groups, at distances of 420, 890, and 14300 pc, are type B associations and the remaining twelve groups are OB associations. They are designated as Aur 0.11, Aur B 0.43, Aur B 0.89, Aur OB 1.4, Aur OB 2.6, AurOB 3.8, Aur OB 4.6, Aur OB 5.4, Aur OB 6.1, Aur OB 7.4, Aur OB 9.3, Aur OB11.6, Aur OB14.3, Aur OB 17.9, Aur OB 25.9, and Aur OB 31.3. For most of these stars the absorption lies within the range from 0m.45 to 5m.41. Such high absorption may be caused by circumstellar absorption as well as by the diffuse nebula IC 410. The dusty matter is distributed nonuniformly in the Aur 0.11, Aur B 0.43, and Aur B 0.89 associations. There is no dust in the space between the associations. There is essentially no dust within the groups (associations) at distances greater than 0.9 kpc. (See Table 2.) __________ Translated from Astrofizika, Vol. 50, No. 2, pp. 243–251 (May 2007).     

CMB recombination lines of hydrogen: The differential spectrum

We have calculated the distortions of the cosmic microwave background (CMB) spectrum in the wavelength range 2–50 cm due to the superposition of the CMB hydrogen recombination radiation in subordinate lines. The level populations were determined by numerically solving the equation of recombination kinetics together with the statistical equilibrium equations for a 60-level model hydrogen atom. The relative distortions are ≈10^?7–10^?6, with their wavelength dependence having a low-contrast, wavy pattern. However, the contrast increases severalfold and becomes pronounced when passing to the differential distortion spectrum. We study the dependence of the distortions on cosmological parameters.     

辽宁省大石桥－吉洞峪一带辽河岩群变质地层的对比研究

辽宁省大石桥－吉洞峪一带出露的主要为古元古代的变质层状岩系，由云母片岩、长英质粒岩和大理类组成。区域上形成一大型北东向的复式向斜构造。复向斜南北两翼变质地层对比问题是辽吉东部辽河岩群研究的主要内容之一。作者根据五年来在大石桥－吉洞峪一带进行１∶５万区调所获得的新资料，从标志层及组合标志层、岩相学特征、主要标志层的岩石化学和稀土地球化学特征、变质作用演化等方面的研究入手，讨论了复向斜两翼变质地层对比的问题。结果表明，辽河岩群构成复向斜南北两翼的变质地层是完全可以对比的，从而进一步证实辽河岩群是一个不可分割的整体     

Space-Time Geometry of Quark and Strange Quark Matter

We study quarkand strangequarkmatter in the contextof generalrelativity.For this purpose,we solve Einstein's field equations for quark and strange quark matter in spherical symmetric space-times. We analyze strange quark matter for the different equations of state (EOS) in the spherical symmetric space-times,thus we are able to obtain the space-time geometries of quark and strange quark matter. Also,we discuss the features of the obtained solutions. The obtained solutions are consistent with the results of Brookhaven Laboratory,i.e. the quark-gluon plasma has a vanishing shear (i.e. quark-gluon plasma is perfect).     

桂北376铀矿床烃气地球化学研究

烃气测量法在锡、金、铜、铅锌等金属矿床找矿中得到了广泛应用,而该技术在花岗岩型铀矿找矿中的应用鲜有报道。本文对桂北376铀矿床已知矿体开展了烃气测量试验,结果显示：相较于其他金属矿,该铀矿区花岗岩和土壤中总烃含量极低,而且花岗岩总烃含量(平均19.42μL/kg)高于上覆土壤(平均6.32μL/kg)。花岗岩中U与多数烃气组分呈负相关,与重烃呈正相关,重烃在U迁移过程中作用强于轻烃;花岗岩烃气标准化配分模式以C₁、iC₄和C₂^-正异常为特征;铀矿化程度与iC₄/nC₄、(C₁+iC₄+C₂^-)/(C₂+C₃+nC₄)及C₂^-/C₃^-比值呈正相关,与C₂₊/∑C比值呈负相关等可为寻找铀矿提供依据。3...     

Relationship between garnet skarn and W mineralization: A case study from the Tongshankou Cu-Mo-W deposit,Daye, Hubei.SCIEI北大核心CSCD

石榴子石是矽卡岩型矿床的标志性矿物之一,其结构和成分特征被广泛用来示踪早期成矿流体性质的变化,但其生长过程与金属元素富集过程的关系还不清楚。本文对长江中下游成矿带最西端鄂东矿集区内的铜山口铜钼钨矿床中的石榴子石开展了显微结构和电子探针主量元素、LA-ICP-MS微量元素点分析和面扫描分析。结果显示,铜山口矿床中的石榴子石端元成分以钙铁榴石-钙铝榴石为主,普遍含有一定量的W,特别是在钙铁榴石端元比例高的石榴子石中(可达3898×10-6),且W与Mo、As、Sn存在明显的正相关关系、与Ti存在一定的负相关关系,指示W以类质同象的方式进入石榴子石晶格。石榴子石可包裹结构简单的白钨矿或被具复杂结构的白钨矿交代,指示石榴子石记录了白钨矿形成前和形成过程中流体性质(氧逸度和W含量等)的变化。铜山口矿床中钙铁榴石的大量结晶,导致成矿早期W的大量分散,不利于高品位和大规模钨矿的形成,仅在这些钙铁榴石遭受强烈的退化蚀变时,释放的W在一定程度能够提高矿石的品位,这可能是氧化性矽卡岩型钨矿通常比还原性矽卡岩型钨矿品位低、规模小的重要原因。石榴子石的成分特征(如W、Sn等元素含量和W/Sn、W/Mo和W/As等比值)可以作为判断矽卡岩的氧化还原性和钨矿床的品位及规模的依据,并具有成为W、Mo和Sn等矿床的找矿勘查指示矿物的潜力。