Single electron loss in the collisions of C3 + and atomic hydrogen

This paper studies the projectile electron loss cross sections of C^{3 +} colliding with atomic hydrogen in the frame work of extended over-barrier model at intermediate velocities (25 keV/u--600 keV/u). The electron loss is calculated in terms of the interaction between the screened target nucleus and the active projectile electron and of the interaction between projectile electron and target electron. Compared with the convergent close-coupling calculations, screening and anti-screening calculations, this model satisfactorily reproduces the experimentally obtained energy dependence of the electron-impact ionisation cross sections and the single electron loss cross sections over the energy range investigated here.     

Effect of superstrong magnetic field on electron screening at the crusts of neutron stars

The influences of electron screening (ES) and electron energy correction (EEC) are investigated by superstrong magnetic field (SMF). We also discuss in detail the discrepant factor between our results and those of Fushiki, Gudmundsson and Pethick (FGP) in SMF. The results show that SMF has only a slight effect on ES when B < 10⁹ T on the surfaces of most neutron stars. Whereas for some magnetars, SMF influence ES greatly when B > 10⁹ T . For instance, due to SMF the ES potential may be increased about 23.6% and the EEC may be increased about 4 orders of magnitude at ρ/μ_e = 1.0×10⁶ mol/cm³ and T₉ = 1. On the other hand, the discrepant factor shows that our results are in good agreement with FGP's when B < 10⁹ T . But the difference will be increased with increasing SMF.     

Effect of strong magnetic field on chemical potential and electron capture in magnetar

The chemical potential of electrons in a strong magnetic field is investigated. It is shown that the magnetic field has only a slight effect on electron chemical potential when B<10¹¹ T, but electron chemical potential will decrease greatly when B>10¹¹ T. The effects of a strong magnetic field on electron capture rates for ⁶⁰Fe are discussed, and the result shows that the electron capture sharply decreases because of the strong magnetic field.     

行星际等离子区对火星探测器距离观测量的影响

根据Muhleman和Anderson在1981年给出的行星际空间等离子体密度模型,模拟计算了行星际等离子区对8GHz电波的距离延迟与太阳-地球-航天器夹角(SEP)和光路径长度(L)的关系。结果显示,在本文的模拟条件下,距离延迟随SEP和L从几毫米变化到几十米。最后,分别仿真了一条地火转移轨道和环火星轨道,计算了两种情况下行星际等离子区延迟对测站到航天器距离观测量的影响。     

扬子板块西缘攀西地区白草矿区黄铁矿标型元素特征及其指示意义

黄铁矿是重要的金属硫化物矿物,在多种矿床中均有产出,其标型特征对矿床成因、矿体空间分布等具有重要的指示意义.以扬子板块西缘攀西地区白草矿区黄铁矿为研究对象,利用矿相学、电子探针等分析方法来对比研究浸染状、致密块状、斑杂状、网脉状矿石中黄铁矿的标型元素特征.结果表明:白草矿区黄铁矿Fe、S平均含量(质量分数,下同)分别为...     

SporadicE ionization associated with meteor events

Two meteor events which were sighted in the Gujarat skies of India, were accompained by the visibility of sporadicE ionization on the ionograms recorded at Ahmedabad (Geog. Lat. 23·2°N, long. 72·30°E). The first event was the Dhajala fireball which flashed into the geoatmosphere along an E-N to W-S trail at about 20·40 h IST on 28 January 1976; the closest distance of the ground projection of meteor trail from Ahmedabad was 50km. The other event was a possible meteor group sighted over Ahmedabad on 28 May 1978, at about 21·10 h IST. This work describes the nature of the sporadicE ionization observed on Ahmedabad ionograms during the two events. Features of theEs echo during the Dhajala event which indicate that it could be of meteoric origin are discussed. Meteor theory is used to relate the observed ionization with the physical dimensions of the Dhajala meteorite as obtained by other workers.     

长江口地区绿色颗粒的矿物学研究

本文对长江下游河道、长江口现代沉积区、口外残留砂沉积区及大陆架现代沉积区表层沉积物中的绿色颗粒进行了系统的矿物学研究。特别运用透射间和能谱分析对其内部超微结构、单晶结构和单晶化学组成进行了研究。长江口地区的绿色颗粒从宏观形态上可分为三类：颗粒状、书页状和生物状，不同的形态者，其形成机制基本相同，只是微晶聚集的微空间环境不同。绿色颗粒的颜色和成熟度有较密切的关系，颜色愈深，K和Fe含量愈高。其成熟度也愈高，K2O含量为3－7％，仅少数可达8.5％。绿色颗粒主要矿物成分为海绿石、鲕绿泥石、磁绿泥石和蒙4皂石。其中以海绿石为主，因此是一种复合型绿色颗粒。不同形态及不同沉积亚环境中绿色颗粒的矿物成分并无太大差别。     

黑硼锡镁矿孪晶的电子衍射分析

黑硼锡镁矿是1985年在我国发现的一种新矿物,微孪晶特别发育,其电子衍射斑点往往具规律的分裂现像。用选区电子衍射获得[010]、[141]和[121]定向带轴电子衍射斑点分裂图,经矩阵分析,确定两套斑点分裂是由其呈挛晶结构关系所致,孪晶面为(101),属于面律孪晶,这种孪晶的微形貌由明场像(BF)得到证实。根据不同取向的电子衍射图,确定该矿物属单斜晶系,a_0=10.7,b_0=3.01,c_0=5.39,β=94.5°。上述挛晶结构特征及其晶体学数据与X射线单晶研究结果有很好的可比性。     

钙稀土氟碳酸盐矿物中新多型体的HREM研究

利用高分辨电子显微术（ＨＲＥＭ）研究了钙稀土氟碳酸盐矿物系列中氟碳铈矿（Ｂ）／直氟碳钙铈矿（Ｓ）的混层结构。发现并确定了Ｂ＿５Ｓ＿２（ＩＨ，３Ｒ）、Ｂ＿５Ｓ＿４（３Ｒ，６Ｒ）和Ｂ＿（１８）Ｓ＿（１０）（ＩＨ）规则混层矿物中５种新多型的晶体结构类型、晶胞参数以及理论晶体化学式等。ＨＲＥＭ研究揭示出，在Ｂ＿ｍＳ＿ｎ（ｍ＞ｎ）型规则混层矿物新多型体的结晶过程中，成矿地质环境是复杂的。阐明了这些多型体是由该系列矿物中的氟碳铈矿（Ｂ）和直氟碳钙铈矿（Ｓ）结构单元层以不同比例沿ｃ轴方向的有序堆垛构成。