华南、巽他和掸邦地块之间边界断裂的上新世—第四纪大规模构造反转

印度- 亚洲碰撞后，大陆板块沿着大型的左行走滑断裂挤出。规模最大的哀牢山- 红河剪切带(ASRR)将印支地块(巽他地块)与华南地块分隔开来。长约1000 km的红河活动断裂(RRF)沿哀牢山的北侧延伸，目前呈现出右行走滑兼正断的活动性质。本文在讨论了红河断裂系及其周缘的第三纪和现今变形特征(滑移性质反转、渐新世/第四纪位错、全新世滑动速率、GPS测量、地震机制等)基础之上，重点论述了其在上新世—第四纪从云南东南部到越南西北部、北部湾西部、再到更南的沙巴地区的断裂分布和运动学特征。新的数据证实，跨过三联点和越南西北部的奠边府断层之后，华南地块与巽他地块之间的现今大部分右行走滑主要沿着Da River断裂向Day Nui Con Voi(或称大象山)东南方向延伸。Da River断裂与RRF大致平行，是2020年M w 5. 0莫州地震的发震断层。进一步研究表明，Da River断裂很可能沿着渐新世—中新世莺歌海/宋红盆地西缘和越南东南海岸(归仁剪切带)向南延伸得更远，至少延伸到“Ile des Cendres”火山群，并可能继续延伸到沙巴- 文莱逆冲带的西端，靠近婆罗洲北部的近海活动边缘。最后，我们讨论了在菲律宾群岛、台湾岛和巽他群岛之间南海大部分地区大规模构造反转的运动学效应。     

九寨沟沟谷成因与演化

本文根据戴维斯流域理论及地史演化特征研究了九寨沟的成因，进而根据水均衡原理及Ｂｕｇｌｉ岩溶理论研究了九寨沟的演化。可以得出结论：九寨沟属流水成因，其演化发展主要受控于长海的断流、水动力条件的变迁及特殊的水化学环境。     

Variability of the Hα and Na I D line profiles in the spectrum of FU Ori

The variations of line profiles in the spectrum of FU Ori during several consecutive nights, from January 3 through January 8, 1999, have been traced for the first time in the entire history of studying this star. The variations of the Hα and Na I D line profiles are regular in pattern; at each time, the profiles of these lines were similar to a particular profile observed previously, suggesting that the phenomenon is periodic. We argue that the profile variations result from the axial rotation of the inner accretion-disk and disk-wind regions for which the temperature distribution and the wind-streamline orientation are not axisymmetric. The cause of the asymmetry could be the interaction of circumstellar matter with the stellar magnetic field if the magnetic axis is greatly inclined to the rotation axis. The possible binary nature of FU Ori seems a less likely cause of the asymmetry.     

Probing the close environment of young stellar objects with interferometry

The study of Young Stellar Objects (YSOs) is one of the most exciting topics that can be undertaken by long baseline optical interferometry. The magnitudes of these objects are at the edge of capabilities of current optical interferometers, limiting the studies to a few dozen, but are well within the capability of coming large aperture interferometers like the VLT Interferometer, the Keck Interferometer, the Large Binocular Telescope or 'OHANA. The milli-arcsecond spatial resolution reached by interferometry probes the very close environment of young stars, down to a tenth of an astronomical unit. In this paper, I review the different aspects of star formation that can be tackled by interferometry: circumstellar disks, multiplicity, jets. I present recent observations performed with operational infrared interferometers, IOTA, PTI and ISI, and I show why in the next future one will extend these studies with large aperture interferometers. This revised version was published online in July 2006 with corrections to the Cover Date.     

Gemini observations of disks and jets in young stellar objects and in active galaxies

We present first results from the Near-infrared Integral Field Spectrograph (NIFS) located at Gemini North. For the active galaxies Cygnus A and Perseus A we observe rotationally-supported accretion disks and adduce the existence of massive central black holes and estimate their masses. In Cygnus A we also see remarkable high-excitation ionization cones dominated by photoionization from the central engine. In the T-Tauri stars HV Tau C and DG Tau we see highly-collimated bipolar outflows in the [Fe II] λ 1.644 micron line, surrounded by a slower molecular bipolar outflow seen in the H₂ lines, in accordance with the model advocated by Pyo, T.-S., et al., Astrophys. J. 570, 724 (2002).     

Pitfalls in the AMS radiocarbon-dating of terrestrial macrofossils

The AMS ¹⁴C technique has the advantage that small samples of Late Quaternary age can be dated with high accuracy, and that errors due to reservoir effects can be avoided if specifically determined terrestrial micro- and macrofossils are measured. However, to obtain such high-accuracy measurements, it is important how small samples are handled prior to treatment in the radiocarbon laboratories. Here we present a set of 51 AMS ¹⁴C measurements, of which 31 dates gave expected ages and 20 dates resulted in anomalously young ages, despite the fact that all samples consisted of clearly identified Late Weichselian terrestrial plant macrofossils. To evaluate possible sources of error, we compared these samples in respect to preparation methods, sample storage and sample weight. Our results show that the long-term storage of wet macrofossil samples appears to have a significant effect on the radiocarbon age obtained, even when the samples are kept cool. Fungi or micro-organisms may easily be incorporated into a sample during preparation and identification, and can easily contribute to the contamination of a sample, if stored cool and wet for several months. © 1998 John Wiley & Sons, Ltd.     

线纹尖塘鳢仔幼鱼的生长发育与池塘育苗研究

线纹尖塘鳢的胚后发育大致分为仔鱼、稚鱼、幼鱼和成鱼期。初孵仔鱼仅2.875mm。前期仔鱼混合营养期短,仅2～3d。后期仔鱼为器官发育、奇鳍条基本形成期,历时10d,平均全长从4.31mm增至8.97mm。稚鱼为器官分化完毕,奇偶鳍条分节、鳞被形成期,历时27～29d,长至平均全长27.79mm。早期幼鱼鳞被等发育完善,进入生长时期。仔鱼开口饵料为150～200μm轮虫,其摄饵大小与口宽呈正相关。15mm后稚鱼可驯饵摄食人工混合料。对仔、稚、幼鱼的生长测定结果显示,全长与日龄呈线性关系L=0.5289t-0.7354(r2=0.9720),体重与日龄呈指数函数关系,W=0.8236e0.1267t(r2=0.9611),全长与体重呈幂函数关系,曲线回归方程W=0.0045L3.2527,b=3.2527,属匀速生长型。采用池塘培水,添加外源饵料生物系列,稚鱼全长15mm时开始驯饵。2002-2005年共培育全长2.2～3.4cm早期幼鱼523.7万尾,仔鱼培育成15mm稚鱼的成活率为26.8%,培育成早期幼鱼的成活率为75.7%。     

Angular velocity during the cycle deduced using the sunspot group age selection methodology

We have used the “age selection methodology” (ASM) (Zappalá and Zuccarello 1991) to study the variability of the sunspot groups angular velocity during the activity cycle. The ASM allows us to separate the contribution of Young Sunspot Groups (YSG) from that of Recurrent ones (RSG) in the Ω(θ) determination and therefore to evaluate whether the increase in angular velocity during minima (reported in literature using all sunspot groups as tracers), is due to a greater statistical weight of YSG on RSG or whether it reflects a global characteristic of the Sun. The results obtained from the analysis of sunspot groups data collected during the period 1874‐1981 (Greenwich Photoheliographic Results) indicate that during minima, besides the fact that the percentage of RSG drops to ≤ 5%, both YSG and RSG show the same increase in angular velocity, i.e. 0.16 degrees/day. Comparing our results with those reported in literature and taking into account the internal angular velocity as deduced by p‐mode oscillations, it is possible to conclude that the observed higher angular velocity of the Sun during minima concerns several layers of the Sun.     

广东罗定龙塘碱性花岗岩锆石SHRIMP定年及地质意义

龙塘碱性花岗岩位于广东云开大山地区,属罗定泗纶混合岩田区,其中的锆石均为具有老核新壳的变质复合型锆石。SHRIMP定年结果,新壳6个测点加权平均年龄为265±1.8Ma,反映该岩体的成岩年龄,相当于中二叠世,属于海西晚期。老核获得最大的U-Pb年龄为1098Ma,相当于中元古代;457Ma和414Ma可能是新壳和老核的混合年龄。根据锆石的成因类型,结合微观所见的岩石结构(反映沉积变质成因的粒状变晶结构和花岗变晶结构等),表明该碱性花岗岩的成因可能是砂泥质沉积物经变质而成。