我国某地工业白云母成因类型、控制矿化因素及其矿物学的研究     

許殿琇  黄典豪 《地质学报》1965,44(4)

工业白云母的成因类型、控制矿化因素及其矿物学特征的研究,有助于白云母矿床的工业评价。作者根据三年的室內外工作所获实际资料对本区上述问题作一探讨。不当之处,敬希指正。在野外工作期间,得到张克安、刘人俊工程师和队上领导及其他同志的帮助;本文完  相似文献   

Impact-generated atmospheres over Titan, Ganymede, and Callisto     

Zahnle K  Pollack JB  Grinspoon D  Dones L 《Icarus》1992,95(1):1-23

The competition between impact erosion and impact supply of volatiles to planetary atmospheres can determine whether a planet or satellite accumulates an atmosphere. In the absence of other processes (e.g., outgassing), we find either that a planetary atmosphere should be thick, or that there should be no atmosphere at all. The boundary between the two extreme cases is set by the mass and velocity distributions and intrinsic volatile content of the impactors. We apply our model specifically to Titan, Callisto, and Ganymede. The impacting population is identified with comets, either in the form of stray Uranus-Neptune planetesimals or as dislodged Kuiper belt comets. Systematically lower impact velocities on Titan allow it to retain a thick atmosphere, while Callisto and Ganymede get nothing. Titan's atmosphere may therefore be an expression of a late-accreting, volatile-rich veneer. An impact origin for Titan's atmosphere naturally accounts for the high D/H ratio it shares with Earth, the carbonaceous meteorites, and Halley. It also accounts for the general similarity of Titan's atmosphere to those of Triton and Pluto, which is otherwise puzzling in view of the radically different histories and bulk compositions of these objects.  相似文献   

Will the Russians return from the near abroad?     

Dunlop JB 《Post-Soviet geography》1994,35(4):204-215

The author "examines a range of issues surrounding the involuntary migration of Russian populations from the non-Russian republics of the former USSR. Among the questions addressed are possible magnitudes of in-migration into Russia (with special attention paid to conditions in one of the major source regions, Central Asia), attitudes in Russia regarding appropriate policy with respect to treatment of co-nationals in the near abroad and whether their return to Russia would have a positive or negative impact, and conditions in areas of Russia that presently are absorbing the greatest numbers of migrants. The assertion that Russian policy should seek aggressively to prevent the out-migration of Russian populations [from] the near abroad is assessed critically."  相似文献   

Coupled atmosphere-ocean models of Titan's past     

McKay CP  Pollack JB  Lunine JI  Courtin R 《Icarus》1993,102(1):88-98

We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time. The partial pressures of N2 and CH4 in the atmosphere are dependent on the ocean temperature and composition. We find that the resulting system is stable against a runaway greenhouse. Accounting for the decreased solar luminosity, we find that Titan's surface temperature was about 20 K colder 4 Gyr ago. Without an ocean, but only small CH4 lakes, the temperature change is 12 K. In both cases we find that the surface of Titan may have been ice covered about 3 Gyr ago. In the lakes case condensation of N2 provides the ice, whereas in the ocean case the ocean freezes. The dominant factor influencing the evolution of Titan's surface temperature is the change in the solar constant--amplified, if an ocean is present, by the temperature dependence of the solubility of N2. Accretional heating can dramatically alter the surface temperature; a surface thermal flux of 500 erg cm-2 sec-1, representative of small levels of accretional heating, results in a approximately 20 K change in surface temperatures.  相似文献   

第四系沉积地层内剪切波分裂：新马德里地震带中部的新构造含意     

Harr.  JB 徐明才 《物探化探译丛》1997,(2):26-35

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陕西金堆城钼矿床中铁钼华的矿物学特征及其意义   总被引：1，自引：0，他引：1  

黄典豪 《岩石矿物学杂志》1989,8(4):352-360

铁钼华产于陕西金堆城斑岩钼矿床的氧化带内,该矿物以往被认为是钼华。笔者对该矿物进行了物理光学性质、化学成分、X射线衍射、穆斯堡尔谱、红外光谱以及失重和差热分析的研究,定名为铁钼华,其分子式为Fe_2(MoO_4)_3·6.8H_2O。同时,将其与国外天然和人工合成的铁钼华作了对比,确定其是在酸性氧化环境中形成的次生矿物。它是原生钼矿床的直接找矿标志。  相似文献   

一种用于探测和修补砾石充填缺陷的独特的机械和测井系统     

Toney  JB 潘葆芝 《物探化探译丛》1991,(6):69-70

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东秦岭地区钼矿床的铼-锇同位素年龄及其意义   总被引：28，自引：11，他引：28  

黄典豪  吴澄宇  杜安道  何红蓼 《矿床地质》1994,13(3):221-230

金属矿床的成矿年龄多年来一直是矿床地质工作者关注的问题之一。中国地质科学院岩矿测试技术研究所建立的铼－锇同位素定年实验室，为研究钼矿床的形成时代提供了新的手段。因辉钼矿是最主要的含铼矿物之一，且基本上不含普通锇，其中所含＾１８７Ｏｓ是由＾１８７Ｒｅ衰变而来，故放射成因＾１８７Ｏｓ的积累是矿物年龄及铼含量的函数。本文采用同位素稀释－等离子体质谱法，测定了东秦岭钼矿带中几个不同类型的大型钼矿床的Ｒｅ－  相似文献   

对比安大略阿伯蒂比带曼罗镇太古代科马提岩流的Re—Os,Sm—Nd和Rb—Sr…     

Walk.  RJ 黄典豪 《国外矿床地质》1994,(1):33-43

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黄龙铺钡天青石的矿物学研究及其意义   总被引：1，自引：0，他引：1  

黄典豪  刘金定  王义昌  江秀杰 《岩矿测试》1983,(2):118-124

黄龙铺钼矿床中脉石矿物“天青石”以其颜色、粗大晶体和形态引人瞩目。该矿床的辉钼矿—方铅矿—黄铁矿—“天青石”—石英—方解石脉,呈大脉和网脉状产于熊耳群细碧岩内。“天青石”除在黄龙铺产出外,在邻近地区构成矿床(点),因此,确定其确切种属不仅有矿物学意义,而且对其矿床(点)进行合理评价也有实际价值。我们根据该矿物的物理性质和化学成分并与国外钡天青石资料对比,将其定名为钡天青石。  相似文献