网页中矢量地图显示的解决方案

在地理信息系统的Web站点开发中,我们遇到了很多棘手的问题,最直接的是矢量显示的问题,因为浏览器作为容器不具有处理矢量的能力,要达到这个目的,它需要嵌入其他有处理矢量能力的容器。目前,解决这个问题有两个方案:一是ActiveX控件技术;二是Java Applet技术。本文简单介绍一下两种技术,并主要讨论JavaApplet技术怎样实现矢量数据的显示。     

An Improved Ekman Layer Approximation for Smooth Eddy Diffusivity Profiles

The Ekman boundary-layer model is extended analytically for a gradually varying eddy diffusivity K(z) ≥ 0, z ≥ 0. A solution for the Ekman layer is provided having similar structure to the constant-K case; that is, exponentially decaying sine functions for the two horizontal wind components. The analytical asymptotic solution compares well with its numerical counterpart for various K(z). The result can be useful in theoretical studies such as Ekman pumping, for efficient estimation of the Ekman layer profiles in various analyses with near-neutral stratifications, or for a rapid initialization of mesoscale models.     

高频电磁波测井同时求解视电导率和视介电常数

利用 Ｌａｍｂｅｒｔ Ｗ函数的性质,针对单发单收和单发双收两种电磁波测井仪器,给出 了一种求解视介电常数和视电导率的方法．理论分析和数值实验表明,该方法在计算速度和 精度方面,明显优于传统的求解复杂非线性方程组的方法．与查表方法相比,该方法不需要 预先计算大量图版,且精度较高．     

W3(OH)区域H2O脉泽的快速时变

通过对 Ｗ３（ＯＨ）区域 ２２ ＧＨz Ｈ_(２)Ｏ脉泽源的短时间跟踪观测,探测到速度为-５２．８ ｋｍ／ｓ子谱的流量密度呈线性下降趋势,变化时标约为 １９天．同时也观测到了整个脉 泽源的谱线宽度与该子谱的强度之间的相关变化．这些现象可能是由脉泽云之间的相 互碰撞导致脉泽抽运率的变化所引起的。     

W Crv: the shortest-period Algol with non-degenerate components?

Radial velocity data for both components of W Crv are presented. In spite of providing full radial-velocity information, the new data are not sufficient to establish the configuration of this important system because of large seasonal light curve perturbations, which prevent a combined light curve/radial-velocity solution. It is noted that the primary minimum is free of photometric perturbations, and this property may help to explain the elusive source of these perturbations. Photometrically, the system appears to be a contact binary with poor or absent energy exchange, but such an explanation – in view of the presence of light curve perturbations – is no more plausible than any one of the semi-detached configurations, with either the more-massive or less-massive components filling the associated Roche lobes. Lengthening of the orbital period and the size of the less-massive component above its main-sequence value, both suggest that the system is the shortest-period (0.388 d) known Algol with non-degenerate components.     

湖南沃溪金锑钨矿床的金矿化作用研究:基于元素地球化学特征和自然金的热力学模拟分析

湖南沃溪金锑钨矿床是江南造山带中金、锑、钨、均达到大型规模的典型矿床,其自然金的金成色值极高(＞998)。本文聚焦湖南沃溪金锑钨矿床中金矿化作用,通过ICP- MS测试和包裹体显微测温实验查明不同矿物与围岩的元素地球化学特征和成矿流体特征,并通过热力学模拟分析自然金的成矿条件,探讨金成色值及金银比值对金矿化的指示作用和研究价值。ICP- MS测试结果显示,金银比值在白钨矿(103~520)和黄铁矿(69~673)中相对较高,在辉锑矿(6~65)和围岩(0. 3~35)中相对较低,在石英(6~199)中则变化较大。基于包裹体显微测温结果(200~350℃),本文建立了自然金成矿流体的热力学模型,分析并查明在黄铁矿与绢云母共生的自然金成矿流体中,硫离子浓度比温度更容易影响金溶解度,且金成色值主要与温度呈正相关,与硫离子浓度呈负相关。通过对比研究和讨论,认为沃溪矿床大量金矿化可能形成于温度较高和硫离子浓度较低的白钨矿成矿流体中,而极高成色值的自然金可能与高金银比值的白钨矿和黄铁矿共生。上述方法和结论可为其他金矿床的研究提供新思路。     

桂北苗儿山- 越城岭印支期（含电气石）白云母花岗岩及相关的Nb- Ta- W成矿作用

桂北苗儿山-越城岭岩基是一个多时代复式岩体,出露有新元古代、加里东期、印支期和燕山期花岗岩,与花岗岩相关有多个加里东期和印支期的大型W矿床,如牛塘界钨(锡)、界牌钨铜、云头界钨钼矿床等,另外越城岭的戈洞坪地区还发现了燕山期铌钽成矿作用。豆乍山岩体位于苗儿山岩体中部,主要由二云母花岗岩组成,本次研究在豆乍山钻孔样品中发现富含Nb-Ta-W氧化物的(含电气石)白云母花岗岩,为进一步全面认识苗儿山-越城岭地区的多时代成矿信息,查明不同类型成矿过程,对钻孔内花岗岩及其成矿作用开展了详细的研究。钻孔样品主要包含二云母花岗岩和细粒的(含电气石)白云母花岗岩,其中细粒的(含电气石)白云母花岗岩穿插了主岩体。详细的矿物学工作显示(含电气石)白云母花岗岩中含有多样的稀有金属副矿物,其中白云母花岗岩中有铌铁矿族矿物、铌铁金红石、锡石等氧化物,而含电气石白云母花岗岩则包含了复杂的Nb-Ta-W的氧化物矿物集合体,主要为铌铁矿族矿物、钨铌铁矿、骑田岭矿和黑钨矿等;另外还在白云母花岗岩中发现一些富含白钨矿的电气石细脉。白云母花岗岩中岩浆锡石U-Pb定年结果为219±4 Ma,属于印支期成矿作用。结合岩相学观察结...     

Photometric study of the newly discovered short period eclipsing binary 1SWASP J133105.91 + 121538.0

A total of 311 BVRI observations were carried out on 4 May 2013 for the new short period W UMa system 1SWASP J133105.91 + 121538.0 using the 1.88 m reflector telescope of Kottamia Astronomical Observatory (KAO) at NRIAG. A photometric solution of these light curves was obtained by means of Wilson–Devinney (WD) code. A spotted model was applied to treat the asymmetry of the light curve. The results show that the more massive component is hotter than the less massive one with about ΔT ∼ 300 K. The system is at a distance of 89 ± 3.6 pc. Based on the physical parameters of the system, we investigate the evolutionary state of the components. Both components are above the zero age main sequence (ZAMS) track by about 0.2 magnitudes.     

Discovery of large-scale methanol and hydroxyl maser filaments in W3(OH)

Images of the 6.7-GHz methanol maser emission from W3(OH) made at 50- and 100-mas angular resolution with the Multi-Element Radio-Linked Interferometer Network (MERLIN) are presented. The masers lie across the western face of the ultracompact H  ii region in extended filaments which may trace large-scale shocks. There is a complex interrelation between the 6.7-GHz methanol masers and hydroxyl (OH) masers at 1.7 and 4.7 GHz. Together the two species trace an extended filamentary structure that stretches at least 3100 au across the face of the ultracompact H  ii region. The dominant 6.7-GHz methanol emission coincides with the radio continuum peak and is populated by masers with broad spectral lines. The 6.7-GHz methanol emission is elongated at position angle 50° with a strong velocity gradient, and bears many similarities to the methanol maser disc structure reported in NGC 7538. It is surrounded by arcs of ground state OH masers at 1.7 GHz and highly excited OH masers at 13.44 GHz, some of which have the brightest methanol masers at their focus. We suggest that this region hosts the excitation centre for the ultracompact H  ii region.