基于J2EE架构的企业卡资源管理系统的设计与实现

介绍了J2EE架构和多层体系结构的发展，在B／S三层架构的基础上给出了包含应用服务器中间件的多层分布式应用体系结构，并把此体系结构应用于电信氽业的有价卡管理系统项目中。分析了此项同的功能结构和体系结构，采用J2EE开发平台和技术设计实现了由浏览器、Web服务器、应用服务器、数据库服务器组成的多层体系架构。     

Some thoughts on pulsation and binarity

Intensive monitoring of main-sequence stars for pulsational studies continuously reveals new binaries and multiple systems. The resulting extensive data sets lead to exact orbital parameters, and to accurate masses of the components. This is also the case higher up the main sequence, though less frequently. We discuss a few examples where intensive observational efforts are necessary in order to improve our knowledge of the pulsational behaviour in the upper main-sequence instability domains, but we emphasize that observational efforts alone that turn out more and more of the same type of data, are by far insufficient, and that there is urgent need for theoretical developments. Determination of highly accurate stellar parameters is of paramount importance and is much more needed than time-series observations.     

政府办公自动化系统建设和应用浅谈

本文简要地介绍了办公自动化的发展过程,分析了其常用的功能、特点,以及内容分类,论述了目前办公自动化系统的技术支撑和实现,并指出政府办公自动化系统在开发和应用中存在的问题和解决思路。对系统的推广使用具有一定的参考意义。     

基于J2EE的分布式WebGIS研究

在对比分析传统的WebGIS各种实现模式优缺点的基础上，探讨了利用企业级J2EE技术实现分布式WebGIS的解决方案，使WebGIS更好地满足企业级应用的需要。     

基于ArcIMS与J2EE城市信息发布系统的设计与应用

介绍了基于ArcIMS和J2EE体系结构集成开发城市信息发布系统的总体框架设计、数据库设计和系统功能设计,并采用此设计方案实现了一个具体实例。     

基于J2EE和ArcIMS的地质灾害危险性评估项目备案系统

本文对J2EE和ArcIMS的地质灾害危险性评估项目备案系统的总体框架结构、系统三层体系结构、模块化思想设计要点和实现的技术路线及关键技术。系统应用Struts技术、数据库技术、ArcIMS的WebGIS技术和网络技术,建立了通用地理信息功能与地质灾害危险性评估项目备案自动审批的分布式软件系统,实现了地质灾害危险性评估项目备案的自动审批、管理、分析、决策、发布的一体化平台。该系统为有关部门提供辅助决策支持和信息发布服务。     

Struts+EJB构架在B/S开发中的应用与改进

讲述了Struts＋EJB构架在B/S开发中的集成使用,介绍了EJB技术、Struts原理及其使用技巧;并总结技术优势.最后通过一个实例,讲述了使用EJB和Struts的方法并对其进行改进.     

Long-term infrared variability of the UX Ori-type star SV Cep

We investigate the long-term optical–infrared variability of SV Cep and explain it in the context of an existing UX Ori (UXOR) model. A 25-month monitoring programme was completed with the Infrared Space Observatory in the 3.3–100 μm wavelength range. Following a careful data reduction, the infrared light curves were correlated with the variations of SV Cep in the V band. A remarkable correlation was found between the optical and the far-infrared light curves. In the mid-infrared regime, the amplitude of variations is lower, with a hint for a weak anti-correlation with the optical changes. In order to interpret the observations, we modelled the spectral energy distribution of SV Cep assuming a self-shadowed disc with a puffed-up inner rim, using a two-dimensional radiative transfer code. We found that modifying the height of the inner rim, the wavelength dependence of the long-term optical–infrared variations is well reproduced, except the mid-infrared domain. The origin of variation of the rim height might be fluctuation in the accretion rate in the outer disc. In order to model the mid-infrared behaviour, we tested adding an optically thin envelope to the system, but this model failed to explain the far-infrared variability. Infrared variability is a powerful tool to discriminate between models of the circumstellar environment. The proposed mechanism of variable rim height may not be restricted to UXOR stars, but might be a general characteristic of intermediate-mass young stars.     

Synchronous <Emphasis Type="Italic">UBVR</Emphasis> photometry and spectroscopy of DI Cephei

We present our synchronous spectroscopy and photometry of DI Cep, a classical T Tauri star. The equivalent widths and radial velocities of the individual components and Hα, Hβ, D1 and D2 Na I, and HeI λ5876 Å emission line profiles exhibit variability. We have found a clear positive correlation between the brightness and equivalent width for the Hα and Hβ emission lines. The photometric and spectroscopic data are satisfactorily described in phases of a 9-day period. The expected magnetic field of the star has been estimated using existing magnetospheric models to be 655–1000 G. The star is suspected to be a binary.