1956-2011年黑龙江省龙卷风气候特征

利用富士达—皮尔森强度分类法对1956—2011年黑龙江省229个龙卷风样本进行分类,分析龙卷风事件的时空分布特征,探讨典型龙卷风个例的环流背景及形成机制。结果表明：1956—2011年黑龙江省龙卷风灾害具有明显的时空分布特征,20世纪60—80年代龙卷风活动频繁,90年代龙卷风发生频次最少,2001—2011年龙卷风发生频次略增加。龙卷风主要集中发生在夏季,以7月发生最多,且多出现在午后至傍晚。对龙卷风空间分析发现黑龙江省绥化地区是龙卷风多发区,与该地区的地理位置、气候条件和大气环流特征有关。不稳定的形势场是龙卷风产生的基础,暖湿气流的输送和冷暖空气的强对流运动为龙卷风的产生提供了有利条件。     

Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares

We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%.     

Multi-band optical variability of BL Lac object OQ 530

Historical optical data are combined on the BL Lac object OQ 530.Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investigate emission processes.To examine the possible existence of a lag between variations in different optical bands from this source,a statistical analysis is performed through the discrete correlation function(DCF)method and the z-transformed discrete correlation function(ZDCF)method.Monte Carlo simulations called"flux redistribution/random subset selection"(FR/RSS)are performed to obtain statistically meaningful values for the cross-correlation time lags and their related uncertainties.The analysis confirms that the variations in different optical light curves are strongly correlated,with zero-lag within the errors.Long term variability of color indexes is also analyzed.The result suggests a strong correlation between color index and brightness.A clear bluer-when-brighter chromatism is found,in the sense that the spectrum steepens as the brightness decreases.     

CCD photometry of five X-ray selected BL Lacertae objects

We present the results of the monitoring of a sample of 5 HBLs in the B, V and R bands during 2003–2008. All sources in our monitoring project show significant rapid optical variations, except 1ES 1959+650, however; for 1ES 1959+650, the gamma-ray variability on a timescale of ～7 hours has been observed by Holder et al. (Astrophys. J. 583:L9, 2003). Using these variability timescales, we estimate the black hole masses for each source with the Kerr black hole theory.     

A cyclical period variation detected in the updated orbital period analysis of TV Columbae

Two CCD photometries of the intermediate polar TV Columbae are made for obtaining two updated eclipse timings with high precision. There is an interval time ～17 yr since the last mid-eclipse time observed in 1991. Thus, the new mid-eclipse times might offer an opportunity to check the previous orbital ephemerides. A calculation indicates that the orbital ephemeris derived by Augusteijn et al. (Astron. Astrophys. Suppl. Ser. 107:219, 1994) should be corrected. Based on the proper linear ephemeris (Hellier in Mon. Not. R. Astron. Soc. 264:132, 1993), the new orbital period analysis suggests a cyclical period variation in the O–C diagram of TV Columbae. Using Applegate’s mechanism to explain the periodic oscillation in the O–C diagram, the required energy is larger than the energy that a M0-type star can afford over a complete variation period of ～31.0(±3.0) yr. Thus, the light travel-time effect indicates that the tertiary component in TV Columbae may be a dwarf with a low mass, which is near the lower mass limit of ～0.08M _⊙ as long as the inclination of the third body is high enough.     

大气干湿沉降样品处理及配套分析方法

本文介绍了干湿沉降样品处理方法及测定其各元素含量的配套分析方法。     

郯庐断裂带南段构造演化与邻区成矿作用——从年代学资料得到的启示

郯庐断裂带为我国东部北北东—北东向岩石圈深大断裂带。在其南段的邻区,分布有胶东金矿区、鲁西铁金矿区以及长江中下游的铁铜(金)成矿带和苏北油气田等矿产。从已获得大量测年资料分析,可将构造—岩浆—成矿事件分为3个阶段:1)早期(800～550 Ma):自元古宙泛古陆裂解和随之而来的加里东期古地震和局部海西期喷流作用,证实地壳运动早已拉开了它的"构造活动序幕",此阶段继承和构建了华北克拉通岩石圈先存的构造薄弱带,从成矿作用而论,此阶段可称为"成矿预备场地";2)主期(1 80～110 Ma):在三叠纪期间,扬子板块和华北板块陆—陆碰撞和中生代西太平洋板块向欧亚板块俯冲等,造就了现今郯庐断裂与分支断裂的构造格架。其中主峰形成时间为140～120 Ma±,在这个阶段广泛有钙碱性系列、富钾高锶钙碱系列、碱性系列岩浆和后期成矿热液,沿着有利构造空间剧烈活动和成矿就位。本区壳幔混熔型和壳源同熔型花岗岩,是地壳减薄和下地壳拆沉、底侵的产物,而不是单一的构造运动的结果。此阶段可称为断裂构造—岩浆活动—成矿作用的鼎盛期;3)晚期(60Ma～现代):沿东西向与北北东向(或北东向)断裂交汇处,存在橄榄玄武岩喷侵,为石油和天然气的形成提供了热源和物源,此期可称其为构造—岩浆活动的衰变期。     

东海陆架盆地伸展率和压缩率及构造跃迁

东海陆架盆地位于欧亚板块的东南缘和西太平洋活动大陆边缘,本文选取了东海陆架盆地主要凹陷的17条地震剖面,采用平衡剖面技术,计算了主要凹陷新生代不同演化阶段的伸展率和压缩率。分析表明,东海陆架盆地构造演化总体由西向东跃迁。晚白垩世至晚古新世东海陆架盆地裂陷中心在西部坳陷带,始新世东迁至东部坳陷带,上新世东迁至东海陆架盆地东侧的冲绳海槽盆地。古新世中后期东海陆架盆地西部坳陷带北侧昆山凹陷反转;中新世东部坳陷带的西湖凹陷反转。东海陆架盆地西部坳陷带与东部坳陷带构造演化不同,证明了东海陆架盆地的东西分带。西部坳陷带北部的长江坳陷和南部的台北坳陷构造演化不同,东部坳陷带北部的西湖凹陷和南部的钓北凹陷构造演化不同,证明了东海陆架盆地的南北分块。     

Some Fundamental Issues in Dynamic Compression and Tension Tests of Rocks Using Split Hopkinson Pressure Bar

Accurate characterizations of rock strengths under higher loading rates are crucial in many rock engineering applications. The split Hopkinson pressure bar (SHPB) system has been used to quantify the dynamic compressive strength of rocks using the short cylindrical specimen and the dynamic tensile strength of rocks using the Brazilian disc (BD) specimen. However, SHPB is a standard tool that is suitable for metal testing; there are some fundamental issues that need to be carefully visited in applying SHPB to rock dynamic tests. This paper addresses several such critical issues, including the choice of slenderness ratio of the compressive specimen, the effect of friction between the sample and bars on the measured results of compressive strength, the necessity of dynamic force balance on the dynamic BD test, and the validity of using the standard BD equation in the data reduction. We show that with proper experimental designs that address these issues, the dynamic compressive strength and dynamic tensile strength of rocks measured using SHPB are valid and reliable.