Physical conditions in the plasma tail of comet C/1987 P1 bradfield

Photometric measurements of photographic images of comet C/1987 P1 Bradfield have been carried out with a flat-bed scanner equipped with a slide module. Lengthwise and transverse photometric profiles of the cometary plasma tail have been obtained. Magnetic field induction and some other physical characteristics of the cometary plasma tail observed in November 1987 have been estimated with the use of the diffusion model for a cometary tail by Shul’man and Nazarchuk (1968). It has been shown that the scanned images of comets can be used for estimating the physical characteristics of cometary tails.     

Pulsational instability of yellow hypergiants

Instability of population I (X = 0.7, Z = 0.02) massive stars against radial oscillations during the post-main-sequence gravitational contraction of the helium core is investigated. Initial stellar masses are in the range 65M _⊙ ≤ M _ZAMS ≤ 90M _⊙. In hydrodynamic computations of self-exciting stellar oscillations we assumed that energy transfer in the envelope of the pulsating star is due to radiative heat conduction and convection. The convective heat transfer was treated in the framework of the theory of time-dependent turbulent convection. During evolutionary expansion of outer layers after hydrogen exhaustion in the stellar core the star is shown to be unstable against radial oscillations while its effective temperature is T _eff > 6700 K for M _ZAMS = 65M _⊙ and T _eff > 7200 K for M _ZAMS = 90M _⊙. Pulsational instability is due to the κ-mechanism in helium ionization zones and at lower effective temperature oscillations decay because of significantly increasing convection. The upper limit of the period of radial pulsations on this stage of evolution does not exceed ≈200 day. Radial oscillations of the hypergiant resume during evolutionary contraction of outer layers when the effective temperature is T _eff > 7300 K for M _ZAMS = 65M _⊙ and T _eff > 7600 K for M _ZAMS = 90M _⊙. Initially radial oscillations are due to instability of the first overtone and transition to fundamental mode pulsations takes place at higher effective temperatures (T _eff > 7700 K for M _ZAMS = 65M _⊙ and T _eff > 8200 K for M _ZAMS = 90M _⊙). The upper limit of the period of radial oscillations of evolving blueward yellow hypergiants does not exceed ≈130 day. Thus, yellow hypergiants are stable against radial stellar pulsations during the major part of their evolutionary stage.     

CONCEPTION OF ESTABLISHING THE SINO RUSSIAN BORDER FREE ECONOMIC REGION

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Pollution trend in the tumen river and its influence on regional development

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Geochemical characteristics of phosphorus near the Huanghe River estuary

INTRODUCTIONPhosphorus (P)isanimportantlimitingelementinglobaloceanicproductivity (Holland ,1 978) ,soknowledgeofPisakeytobetterunderstandingofthecyclingofcarbon ,nitrogen,sulfur,andothernu trientelements.Inasimplemassbalancemodel,thelevelofdissolvedPintheoceanisafunctionoftherateofinputviarivers,andtherateofoutputviadepositioninsediments.Inthepresentstudy,thefocusisontheriverinePinputbytheHuangheRiver (YellowRiver)totheBohaiSea,andespeciallyontheamountofPsolubilizedfromsolidphasesupo…     

新疆哈密地区天湖岩体岩石谱系单位划分及其岩浆演化

在１５万区域地质调查基础上,利用花岗岩等级体制填图方法对天湖花岗岩体进行解体,建立了三个填图单元,归并为一个超单元。对各单元岩石类型、矿物成分、组构及野外接触关系进行了论述。通过岩石化学和地球化学资料论证,该岩体是同一次岩浆熔融事件过程中曾经发生过三次岩浆侵入活动而形成的环状深成岩体。     

浅析四道沟金矿矿床成因及找矿方向

四道沟金矿是地质条件较为复杂的矿床,对其成因问题前人观点众说不一。比较典型的主要有岩浆热液成因和沉积变质成因,成因不同直接影响着找矿方向。根据矿床地质特征和工作实践认为：该矿床成因应为沉积变质－ 岩浆热液叠加改造型矿床。所以沉积变质和岩浆热液成矿的有利条件均应成为找矿的主要方向。据此开展的找矿工作已初步获得突破性进展。     

加氯水体有机浓集物对团头鲂血液指标的影响

本文对团头鲂 2项血液学指标 (红细胞数 RBC和血红蛋白量 Hb)的正常值进行了研究 ,同时检测了加氯水体中有机浓集物对这 2项指标的影响。结果表明 ,团头鲂血液中 RBC和 Hb的正常值受生长和水温等因素影响 ;在相同的试验条件下 ,加氯水体中的有机浓集物对团头鲂血液 RBC和 Hb有抑制作用 ,抑制率分别为 4 .3 %～ 2 6.0 %和 5.0 %～ 2 2 .5% ,表明此类物质对鱼类正常的生长代谢有一定的危害。     

羌塘盆地查郎拉地区中、新生代地质构造特征

本文系统研究了羌塘盆地查郎拉地区中、新生代的构造特征,将整个研究区划分为五个构造单元。即那日－ 破曲褶皱带、江达－ 杜日断褶带、塞仁那来－ 巴陇复式向斜断褶带、气相错－ 查巴断陷带、查曲公玛－ 日昂巴山间盆地。从晚三叠世以来,图幅内经历了印支期、燕山期、喜山期构造运动,印支期主要是在图幅北部上三叠统地层中形成北东向褶皱,燕山运动早期本区构造活动最为强烈,形成了全区范围内的东西向褶皱和断层,其中尤以南部塞仁那来－ 巴陇复式向斜断褶带最为强烈,构造最为紧密,燕山晚期,以断陷构造为主,形成中部的查曲公玛－ 日昂巴山间盆地和南部的气相错－ 查巴断陷带,喜山期主要是形成一些新构造活动。     

新疆尾亚韧性剪切带的基本特征及其意义

尾亚韧性剪切带形成于石炭纪晚期.根据其宏观变形构造、显微变形构造等变形特征,说明其经历了早期的推覆剪切和后期的右行推覆剪切两个主要演化阶段.对该区的构造演化及指导找矿增添了一点新的内容.