JYZ11A钻孔记录的居延泽演化历史

我国内陆干旱区在末次冰期(含深海氧同位素第3阶段)是否存在古大湖近年来持续存在争论。居延泽是黑河的尾闾湖之一, 位于我国典型干旱区, 是开展这项研究的理想区域。依据居延泽盆地最低处的JYZ11A钻孔(全孔长61.13m, 本文侧重上部27m岩芯), 使用石英光释光测年获得3个可靠释光年龄并据此建立年代框架。全孔10cm间距测量沉积物粒度, 钻孔上部16.7m以2cm间距测量低频磁化率, 本文侧重分析JYZ11A钻孔上部10m的指标记录。综合岩性地层、沉积物粒度分布特征和粒度、磁化率指标记录, 并与前人已有研究进行对比, 本研究发现末次冰期时居延泽盆地主要堆积棕色冲洪积物和风沙沉积物, 早全新世为风沙沉积, 中全新世出现浅灰色湖相沉积与风沙交替沉积, 而稳定湖泊只在约3ka时才逐渐形成, 可能存在多次湖面波动并留下古湖岸堤。因此, 居延泽盆地在末次冰期包括深海氧同位素第3阶段晚期并不存在稳定大湖。居延泽早全新世干涸、中晚全新世湖泊较稳定发育的全新世成湖模式与季风区湖泊演化模式明显不同, 而与许多中亚干旱区的湖泊、风成沉积等古环境记录相似, 它们可能共同指示了一种有别于中国季风区的全新世区域湿度演化模式。     

苏北平原MIS 3阶段海侵事件的沉积记录

MIS 3阶段的气候与环境是古气候与古环境研究的热点,该阶段中国沿海地区的海侵过程是沿海平原环境演化的重要事件。根据苏北平原宝应By1钻孔的 14 C年代结果和沉积特征、微体生物组合特点,确认苏北平原MIS 3阶段存在明显的海侵事件,潮滩与泻湖相沉积层的厚度约7m,深度在By1孔19~26m,海相层位于长江三角洲地区的典型末次冰盛期的硬粘土层之下,14 C年代在距今26~39ka之间,属于MIS 3阶段的沉积,岩芯沉积物的沉积构造以水平的薄层砂质粉砂沉积为主。沉积物中大量的海相有孔虫壳体在研究的岩芯段中是最丰富的; 此外,还发现咸水环境下的Sinocytheridea impressa (Brady),Spinileberis pulchra与Spinileberis furuyaensis,Neomonoceratina chenae Zhao,Keijella bisanensis (Okubo)等形类壳体; 该段岩芯中的植物残体、碳屑也很丰富,有机质含量丰富,显示比较封闭的弱动力环境,指示了潮滩、泻湖沉积环境。     

Preface to the special issue “Tectonics and depositional infilling of western Pacific marginal sea”

Marine Geophysical Research -     

Estimates of AGN Black Hole Mass and Minimum Variability Timescale

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.     

澜沧—耿马地震震源动力学参数研究

本文使用沧澜—耿马地震主震后在震区建立的数字地震仪记录,用波谱法测算澜沧—耿马余震的震源动力学参数。就这些参数的统计特征,对该双主震型两主震区的地下介质不同状态予以讨论。     

粘土矿物对海水中主要营养盐的吸附研究

对海水中磷盐和硝酸盐在粘土矿物上的吸附行为的研究发现，海水体系中高岭土对磷酸盐的吸附能力大于蒙脱土，其原因为，粘土颗粒的表层铝／硅结构比是控制磷酸盐吸附的主要因素，其中铝含量越高，肿附能力越大。考察ＰＨ、粘土酸改性处理等因素对吸附作用的影响，结果表明，ＰＨ＜８．５的磷酸盐吸附ＰＨ曲线呈峰形，其吸附作用以阴离子交换为主；ＰＨ＞８．５时磷酸盐的吸附作用以沉淀吸附为主。酸改性蒙脱土可提高吸附磷酸盐的能力     

池沼公鱼耳石日轮的观察研究

于1989年3－8月，从辽阳汤河水库捕取成熟的池沼公鱼，获得人工授精卵。用压片法光镜下连续观察胚胎发育后期和前仔鱼期耳石轮纹的形成，并采集已知月龄的幼、成鱼耳石，制片镜检轮纹数量和排列。结果表明，仔鱼在印黄接近吸收完并开始摄食外界食物时，即孵出后第6d至第7d形成第1个轮纹，之后每天一轮，这些轮纹就是日轮；日轮间距呈规律性变化，这些变化与鱼体生长发育及生态条件密切相关。     

The influence of magnetic fields on neutrino-dominated accretion disc

We consider the influence of magnetic fields on the model of neutrino-dominated accretion flows (NDAFs) for gamma-ray bursts (GRBs) via the assumption that the accretion rate of the disc is totally caused by the torque of the Lorentz force, i.e. the magnetic braking of large-scale magnetic fields and magnetic viscosity of small-scale magnetic fields. We calculate the structure, composition, luminosity of neutrino emission and the Poynting flux, and the rate of mass loss driven by neutrino heating or launched centrifugally by large-scale magnetic fields, based on the physical condition of the magnetized NDAFs. It is shown that the magnetized disc is favourable to interpret the diverse prompt emissions as well as the X-ray flares observed in the early afterglow of GRBs.     

Self-similar solution of hot accretion flows with ordered magnetic field and outflow

Observations and numerical magnetohydrodynamic (MHD) simulations indicate the existence of outflows and ordered large-scale magnetic fields in the inner region of hot accretion flows. In this paper, we present the self-similar solutions for advection-dominated accretion flows (ADAFs) with outflows and ordered magnetic fields. Stimulated by numerical simulations, we assume that the magnetic field has a strong toroidal component and a vertical component in addition to a stochastic component. We obtain the self-similar solutions to the equations describing the magnetized ADAFs, taking into account the dynamical effects of the outflow. We compare the results with the canonical ADAFs and find that the dynamical properties of ADAFs such as radial velocity, angular velocity and temperature can be significantly changed in the presence of ordered magnetic fields and outflows. The stronger the magnetic field is, the lower the temperature of the accretion flow will be and the faster the flow rotates. The relevance to observations is briefly discussed.     

Quasi-Periodic Long-Term Solar Radio Pulsations During A Decimetric Type IV Burst

Long-periodic pulsations with a period of tens of seconds associated with a Type IV solar radio emission are found at 1420 and 2000 MHz. Some features (such as the bandwidth, periodicity, frequency drift, amplitude, and relative amplitude) of the pulsations are introduced and discussed in this paper.