The internal structure of Jupiter family cometary nuclei from Deep Impact observations: The “talps” or “layered pile” model

We consider the hypothesis that the layering observed on the surface of Comet 9P/Tempel 1 from the Deep Impact spacecraft and identified on other comet nuclei imaged by spacecraft (i.e., 19P/Borrelly and 81P/Wild 2) is ubiquitous on Jupiter family cometary nuclei and is an essential element of their internal structure. The observational characteristics of the layers on 9P/Tempel 1 are detailed and considered in the context of current theories of the accumulation and dynamical evolution of cometary nuclei. The works of Donn [Donn, B.D., 1990. Astron. Astrophys. 235, 441-446], Sirono and Greenberg [Sirono, S.-I., Greenberg, J.M., 2000. Icarus 145, 230-238] and the experiments of Wurm et al. [Wurm, G., Paraskov, G., Krauss, O., 2005. Icarus 178, 253-263] on the collision physics of porous aggregate bodies are used as basis for a conceptual model of the formation of layers. Our hypothesis is found to have implications for the place of origin of the JFCs and their subsequent dynamical history. Models of fragmentation and rubble pile building in the Kuiper belt in a period of collisional activity (e.g., [Kenyon, S.J., Luu, J.X., 1998. Astron. J. 115, 2136-2160; 1999a. Astron. J. 118, 1101-1119; 1999b. Astrophys. J. 526, 465-470; Farinella, P., Davis, D.R., Stern, S.A., 2000. In: Mannings, V., Boss, A.P., Russell, S.S. (Eds.), Protostars and Planets IV. Univ. of Arizona Press, Tucson, pp. 1255-1282; Durda, D.D., Stern, S.J., 2000. Icarus 145, 220-229]) following the formation of Neptune appear to be in conflict with the observed properties of the layers and irreconcilable with the hypothesis. Long-term residence in the scattered disk [Duncan, M.J., Levison, H.F., 1997. Science 276, 1670-1672; Duncan, M., Levison, H., Dones, L., 2004. In: Festou, M., Keller, H.U., Weaver, H.A. (Eds.), Comets II. Univ. of Arizona Press, Tucson, pp. 193-204] and/or a change in fragmentation outcome modeling may explain the long-term persistence of primordial layers. In any event, the existence of layers places constraints on the environment seen by the population of objects from which the Jupiter family comets originated. If correct, our hypothesis implies that the nuclei of Jupiter family comets are primordial remnants of the early agglomeration phase and that the physical structure of their interiors, except for the possible effects of compositional phase changes, is largely as it was when they were formed. We propose a new model for the interiors of Jupiter family cometary nuclei, called the talps or “layered pile” model, in which the interior consists of a core overlain by a pile of randomly stacked layers. We discuss how several cometary characteristics—layers, surface texture, indications of flow, compositional inhomogeneity, low bulk density low strength, propensity to split, etc., might be explained in terms of this model. Finally, we make some observational predictions and suggest goals for future space observations of these objects.     

中国东部幔源流体的活动特征与成藏效应

中国东部进入地洼构造演化阶段后发生了一系列构造活化现象,形成了一系列伸展性断层和巨型深大断裂带,其中的一些超壳或岩石圈断裂成为壳幔物质与能量交换,特别是地幔流体上升的主要构造通道。在郯庐断裂带附近及两侧的松辽、辽河、黄骅、济阳、苏北和三水盆地(坳陷)中的许多气井中,He和CO2的含量很高,部分气井中He的浓度超过其工业品位(0.05%)CO2的含量在80%以上,甚至近于纯CO2气藏。这些气井中的He和CO2不仅显示幔源特征,而且CO2具有岩浆成因特征。此类幔源气体一般都和壳源气体组分复合,在储盖层及构造圈闭发育的地区聚集成藏。     

生物中碳氢化合物的结晶（英文）

文章专门讨论与特定成岩作用伴生的铬、铂和硫化物矿床形成的内生因素。该类成岩作用对矿石富集有显著影响。矿床的巨大规模起因于与广泛强烈的成岩过程有关的特殊的成矿作用。这些作用导致产在超基性杂岩中的特殊纯橄榄岩（铬矿石）、基性超基性层状侵入体中的低硫层和铁镁橄榄石纯橄榄岩（铂族金属矿床）的形成,以及富铁火成分异岩的透岩浆硫化作用（Ｃｕ Ｎｉ硫化物和Ｃｕ Ｚｎ Ｐｂ硫化物矿石）。还根据巨型矿床的成因模型提出了矿物学岩石学的找矿标志     

The AGNS and their host galaxies as seen in the mid-infrared

We present a new diagnostic diagram based on ISOCAMspectra (5-16 m) to distinguish the emission inducedby the active galactic nucleus (AGN) from that associated with thestar formation activity. This diagnostic based on the mid-IRcontinuum and the Unidentified Infrared Band (UIB) intensity allowsus to estimate the relative importance of the three components (HIIregions, diffuse/photo-dissociation regions (PDRs), and AGN) contained ingalaxy mid-infrared emission. In AGN spectra, we confirm the absenceof UIBs presumably photodissociated by the X-UV radiation field. Inaddition, a non-negligible continuum below 9 m commonlyassociated with emission from hot dust is present in AGNs. Adiagnostic diagram derived from these two results can be used fordetecting obscured AGNs embedded in a large concentration of dust.     

超大型矿床的探寻与研究的若干进展

本文主要讨论最近两年国内外探寻与研究超大型矿床所取得的若干进展。内容涉及：超大型矿床与类似名词定义、典型剖析、超大型矿床分类、矿化类型、全球背景研究等问题。在简要介绍国内外超大型矿床研究现状后，文中提出，结合我国矿产地质实际，宜以１９８７年国家储量委员会规定之大型矿床５倍储量为超大型矿床下限。超大型矿床可暂分三类：第一类之同类型大、中、小型矿分布甚广；第二类则反之，同类型矿床极罕见；第三类为过渡类型。笔者指出，不少有色金属在超大型矿床的矿化类型上有强烈选择性，即某一矿种虽可存在多种矿化类型，但一般仅一、二种类型可形成超大型矿床。提出这一点对寻找超大型矿床十分重要。文中举出若干实例，论证对某些超大型矿床进行全球背景研究之必要及超大型矿床研究可提高成矿理论水平。     

Concentrations of Trace Elements in Carbonate Reference Materials Coral JCp-1 and Giant Clam JCt-1 by Inductively Coupled Plasma-Mass Spectrometry

Trace elements in the Geological Survey of Japan carbonate reference materials Coral JCp-1 and Giant Clam JCt-1 were determined by inductively coupled plasma-mass spectrometry after digestion with 2% v/v HNO₃. A standard addition method was adopted in this determination in order to neutralise the Ca matrix effect. In addition, Sc, Y, In and Bi were used as internal standards to control the matrix effect and correct instrumental drift. Of the eighteen elements measured in JCp-1, precisions for fourteen elements, including Cu, Cd and Ba, were better than 10% RSD and concentrations ranged from 0.002 μg g^-1 (Cs) to 8.02 μg g^-1 (Ba). The concentrations of measured trace elements in JCt-1, except for Cu, were lower than those in JCp-1. Precisions for all elements with concentrations higher than 0.04 μg g^-1 in JCt-1 were also better than 10% RSD and concentrations were found to be between 0.001 μg g^-1 (Cs) and 4.84 μg g^-1 (Ba). The concentrations of more than fifteen trace elements in the aragonite reference materials are reported here for the first time. Both reference materials are suitable for use in geochemical studies of environmental reconstruction based upon biogenic carbonate materials.     

豆状核结构模糊对早期诊断大面积脑梗塞的价值

本文通过对２５例早期诊断的大面积脑梗塞的分析，论证了豆状核结构模糊在早期诊断大面积脑梗塞中的价值。     

Concentration and size variation of condensation nuclei at Mawson,Antarctica

Condensation nucleus (CN) concentrations have been measured at Mawson (67.6°S, 62.9°E) since mid 1981. Weekly median concentrations have an annual cycle with a maximum of around 300 to 400 cm^-3 in summer and a minimum of a few tens of particles per cm^-3 in winter. In this respect Mawson behaves very much like an Antarctic continental location. Preliminary measurements of the size distribution of CN particles taken over a nine month period suggest a seasonal change in typical particle radius from around 0.01 m in winter to around 0.04 m in summer. Diurnal variation in the CN concentration is generally very weak and does not show any systematic relation to the pronounced diurnal variation in wind-speed at Mawson.Department of Science, Antarctic Division     

外空扰动引力计算方法的内在联系

利用算子运算的方法，对求定外空扰动引力的Bjerhammar方法、虚拟点质量方法以及虚拟单层密度方法进行了系统地归纳；利用Possion核的再生特性及球谐函数的正交性质，给出了它们之间的换算关系；最后从两个方面分析了实用计算中各种方法的优劣。