基于J2EE和ArcGIS平台的分布式WebGIS设计与实现

J2EE提供了一个跨平台、可移植、多用户、标准的企业级Java服务器端部署平台;组件化的ArcGIS产品ArcIMS和ArcSDE实现了基于Internet的GIS,两者的结合确保了架构的可维护性和可扩展性。本文介绍了该架构下的系统结构和实现过程。     

渤海J油田储量不确定性分析及优选

地质建模的最终目的是建立反映地质认识的地质模型,并对储量不确定性进行定量表征。储量是油田开发方案编制的基础,一个油田科学合理的开发往往需设计乐观、推荐、悲观三个方案,分别对应着乐观、推荐、悲观三个储量,即储量的P10,P50,P90。渤海J油田正处于开发的前期研究阶段,井点资料少,储层的纵横向变化快,储量不确定性强,而如何优选储量的P10,P50,P90成为决定油田开发方案编制的关键一环。该文通过构造、储层及油藏特征的分析首先确定了影响该油田储量的5个不确定性因素,即:构造幅度、油水界面深度、孔隙度下限、泥岩主变程、泥岩次变程,并分析了它们的分布范围,通过地质模型的建立对各个不确定性因素开展敏感性分析,确定油水界面深度、孔隙度下限、泥岩主变程是影响储量最大的3个因素,并以此为基础对J油田的储量进行了不确定性分析,优选了储量的P10,P50,P90。     

中国碱蓬属植物修订

本文对《中国植物志》藜科(Chenopodiaceae)碱蓬属(Suaeda Forsk. ex Scop.)长期存在的分类错误进行了纠正。将其中的高碱蓬S. altissima (L.) Pall.合并入碱蓬S. glauca (Bunge) Bunge,纵翅碱蓬S. pterantha (Kar. et Kir.) Bunge合并入刺毛碱蓬S. acuminata (C.A. Mey.) Moq.,同时增加了垦利碱蓬(新种)S. kenliensis J. W. Xing sp. nov。由此将中国碱蓬属(Suaeda)植物从原来的20种,变更为19种。并重新修订了中国碱蓬属(Suaeda)植物的分种检索表,使中国碱蓬属(Suaeda)植物的系统分类更趋于完善,为《中国植物志》的修订和碱蓬属(Suaeda)植物分类及其深入研究与开发利用提供了依据。     

部分遮蔽类星体SDSS J151653.22+190048.2的紫外波段中等宽度发射线起源

类星体SDSS J151653.22+190048.2 (简称J1516+1900)在紫外-光学-近红外波段展现出奇特的光谱性质:其光学Hα、Hβ和近红外的Paα、Paβ等发射线的半高全宽(full width at half maximum intensity, FWHM)均超过5000 km/s,等值宽度接近类星体平均值;而紫外波段光谱的常见发射线Lyβ、OVI、Lyα、NV、Si IV和CIV等,由FWHM1700 km/s的中等宽度成分主导.这种现象很可能是由于紫外发射线的宽线成分经尘埃消光,强度严重削弱,从而使得中等宽度成分凸显出来;在光学和近红外波段,尘埃消光减弱,发射线由宽线成分主导,潜在的中等宽度成分不容易被看到.根据中等宽度成分的线宽和J1516+1900中央超大质量黑洞的质量MBH5.75×108M⊙,在维里化假设下,估计中等宽度发射区到中央黑洞的距离约为1.6 pc.另一方面,利用J1516+1900丰富的观测谱线,结合光致电离模型计算,可以限定J1516+1900的中等宽度发射线区气体密度1012cm-3、电离参数10-0.65.据此估计该发射线区到中心黑洞距离0.016 pc,只有维里化距离的1%.这一矛盾结果预示着中等宽度发射区可能具有较为复杂的物理结构,未来需要观测更多类似J1516+1900的部分遮蔽类星体并进行系统的分类和研究.     

Polycyclic aromatic hydrocarbons in water,mussels (Brachidontes sp., Tagelus sp.) and fish (Odontesthes sp.) from Bahía Blanca Estuary,Argentina

Polycyclic aromatic hydrocarbons (PAHs), one of the major groups of anthropogenic environmental pollutants, were firstly identified and measured in coastal waters, native mussels and fish of an industrialized South American estuary.     

基于J2ME手机的工程测量软件中的乘幂算法

使用J2ME手机开发工程测量软件过程中,由于CLDC1.1的局限,提供的数值计算函数并不充分,特别是缺少关键的乘幂计算函数。推导乘幂计算的数学算法,给出按此方法计算的实例。在J2ME手机开发中通过建立roadMath类,完成乘幂计算的JAVA编程实现,同时扩充CLDC1.1的数学计算函数。     

基于网格的地图服务研究

在分析目前地图服务存在问题的基础上,将网格技术应用到移动空间信息服务领域,研究了基于网格的位置服务原理和特点.针对地图服务存在的问题,提出了基于网格的地图服务,并通过与J2ME技术的结合实现了一个Java手机地图服务系统,可以改善地图服务的性能,提高位置服务的效率.     

Magnetic hydrogen atmosphere models and the neutron star RX J1856.5–3754

RX J1856.5−3754 is one of the brightest nearby isolated neutron stars (INSs), and considerable observational resources have been devoted to it. However, current models are unable to satisfactorily explain the data. We show that our latest models of a thin, magnetic, partially ionized hydrogen atmosphere on top of a condensed surface can fit the entire spectrum, from X-rays to optical, of RX J1856.5−3754, within the uncertainties. In our simplest model, the best-fitting parameters are an interstellar column density   N _H≈ 1 × 10²⁰ cm⁻²  and an emitting area with   R ^∞≈ 17 km  (assuming a distance to RX J1856.5−3754 of 140 pc), temperature   T ^∞≈ 4.3 × 10⁵ K  , gravitational redshift   z _g ∼ 0.22  , atmospheric hydrogen column   y _H≈ 1 g cm⁻²  , and magnetic field   B ≈ (3–4) × 10¹² G  ; the values for the temperature and magnetic field indicate an effective average over the surface. We also calculate a more realistic model, which accounts for magnetic field and temperature variations over the NS surface as well as general relativistic effects, to determine pulsations; we find that there exist viewing geometries that produce pulsations near the currently observed limits. The origin of the thin atmospheres required to fit the data is an important question, and we briefly discuss mechanisms for producing these atmospheres. Our model thus represents the most self-consistent picture to date for explaining all the observations of RX J1856.5−3754.     

Study of the fast X-ray transient XTE J1901+014 based on INTEGRAL,RXTE, and ROSAT data

The source XTE J1901+014 discovered by the RXTE observatory during an intense outburst of hard radiation and classified as a fast X-ray transient is studied. The source’s spectral characteristics in the quiescent state have been investigated for the first time both in the soft X-ray energy range (3–20 keV) based on ROSAT and RXTE data and in the hard energy range (>20 keV) based on INTEGRAL data. A timing analysis of the source’s properties has revealed weak nonperiodic bursts of activity on time scales of several tens of seconds and two intense (～0.5–1 Crab) outbursts more than several hundred seconds in duration. Certain assumptions about the nature of the object under study are made.