Spectroscopic diagnostics for CDS and SUMER

The CDS and SUMER instruments will make extensive use of spectroscopic diagnostics to determine the physical parameters of the solar transition region and corona. A great deal of effort is going into the development of these techniques to ensure that they are accurate. This requires interfacing solar analysis programs with the best available atomic data calculations. Recent developments in this work will be presented, with specific examples of useful spectral line ratios.     

飞机起落架故障数据库模型与实现方法研究

讨论了民用飞机起落架故障数据库的结构模型，基于关系模型故障数据库故障树存储结构的表示及实现，详述了Treeview的基本功能和使用方法等内容。文章最后介绍了采用VFP建立Boeing737起落架故障数据库的部分功能。     

EUV spectroscopy as a plasma diagnostic

The EUV wavelength regions is rich in emission lines from the transition region and the corona. Spectroscopic techniques have been used extensively to determine the physical conditions in the solar atmosphere for such diverse phenomena as coronal holes, active regions, sunspots, flares, etc. The diagnostics and dynamics of plasmas, both homogeneous and inhomogeneous plasmas, are reviewed. The future projects such as the CDS and SUMER instruments on SOHO have been discussed as they cover EUV wavelength region and will provide a wealth of observational data with excellent spatial, spectral, and temporal resolution.     

基于仿射变换的飞机图像的识别

 先基于细胞神经网络提取飞机图像轮廓,再用基于仿射变换方法对多种飞机的轮廓图像做不变特征的提取,把多种飞机的不变特征放在数据库中。进行飞机类型识别时先计算实时图像中飞机(目标) 的不变特征,然后与数据库中的每个不变特征做相关运算,即可识别飞机的型号。     

SUMER Observations of Coronal-Hole Temperatures

Observations of emission lines in the vacuum-ultraviolet spectral range with calibrated instrumentation provide crucial information on the prevailing plasma temperatures in the solar atmosphere. Coronal-hole temperatures measured by the SUMER spectrometer on SOHO will be presented in this contribution. Electron temperatures can be estimated from the formation temperatures of the observed emission lines. Line-ratio and emission-measure analyses, however, offer higher accuracies. Typical electron temperatures at altitudes of H<200?Mm in coronal holes are below 1?MK in bright structures—the coronal plumes—with higher values in darker areas—the inter-plume regions. Line-width measurements yield effective ion temperatures, which are much higher than the electron temperatures. Observations of line profiles emitted from species with different masses allow a separation of the effective temperatures into ion temperatures and unresolved non-thermal motions along the line of sight.     

Outflow Velocities at the Base of a Polar Coronal Hole During the 1998 Total Eclipse

Polar coronal holes represent the most convincing site from which the high-speed solar wind originates. Here we report high-accuracy Doppler shifts measured in the O VI (1037.6 Å) line obtained by SUMER on SOHO inside an interplume region within the south polar coronal hole. We infer limits on the outflow velocity and draw hints about the flow geometry.     

数据库在飞机连接技术系统上的应用

飞机连接是飞机制造技术中的一项重要的关键技术.利用Oracle数据库管理系统,在收集整理相关资料的基础上,建构了飞机连接数据库.描述和存储了飞机连接中的技术条件数据、连接件的工艺数据和连接件的关联数据等,并建立了数据的相互关联.说明利用PowerBuilder应用开发工具进行数据库应用程序开发的全过程和相关的原理.最后,对所设计的＂飞机连接信息技术系统＂做了简要的经济性分析.     

Signatures of Coronal Hole Spectra Between 660 Å and 1460 Å Measured with Sumer on Soho

Spectra of the northern polar coronal hole measured with the SUMER spectrometer on SOHO on 25 October 1996 are analyzed. We present spectra taken at locations on the solar disk where part of the spectrometer slit intersects a polar coronal hole region and an area of brighter emission from outside of the coronal hole area. By comparing the line intensities between the parts of the spectrum taken inside the "dark" area of the coronal holes and the brighter regions, we work out the signatures of the specific coronal hole in the chromosphere, transition region and lower corona. We find that emissions of neutral atom lines, of which there are many in the spectrum of SUMER, show no difference between the coronal hole and the bright boundary areas, whereas all ionized species show strong intensity enhancements, including the continuum emissions of carbon and hydrogen. These enhancements are larger than in normal quiet Sun areas. This revised version was published online in June 2006 with corrections to the Cover Date.     

Heating Diagnostics with MHD Waves

The heating of the solar atmosphere is a fundamental problem of modern solar and astrophysics. A review of the seismological aspects of magnetohydrodynamic (MHD) waves with an emphasis on standing longitudinal waves in the context of coronal heating is presented. Efforts made recently may be split into two categories: forward modelling and data inversion. Forward modelling can be applied to predict the observational footprints of various heating scenarios. A new diagnostic method based on the analysis of Doppler shift time series is outlined with specific application to solar coronal conditions. The power of the method is demonstrated and tested using synthetic data and comparing them with actual high-resolution (e.g. SoHO/SUMER) observations. Further, related recent examples of standing longitudinal oscillations in coronal loop structures observed with the new Hinode/EIS instrument are also presented. These latter observations provide an advanced ground for MHD seismology as a tool for plasma heating diagnostics in the atmosphere of the Sun.     

Fine structure and the emission filling factor

There is observational evidence for an extreme fine structure in the solar transition region, much smaller than 1 in size (Dereet al., 1987, 1988) Corresponding to this extreme fine structure there appear to be an equally complex dynamical structure. We review the evidence for such dynamical extreme fine structure as demonstrated by the frequent appearance of multiple velocities, i.e. distinctly different velocities in the transition region occurring within the angular resolution element. Multiple velocities are prominent in active regions and particularly near sunspots, where velocity components may be supersonic. However, multiple velocities are frequent also in quiet regions. The consequences of such fine structure for modeling the transition region will be outlined. Finally the appropriate CDS and SUMER observations needed to extend our knowledge of a finely structured transition region and corona, spatially or in time, are discussed.     

AutoCAD ARX数据库编程方法

本文介绍了一种在AutoCAD ARX程序中使用外部数据库的方法。由于采用了ODBC技术，该方法可以适用于Visual FoxPro,Access,SQL Server等多种数据库。为开发在AutoCAD环境下工作的数据库管理系统提供了有益的研究成果。     

固体火箭发动机CAD系统实现

介绍了一种系统固体火箭发动机CAD(SRMCAD)的组成和实现。系统集成多个功能子模块,功能较全。利用本系统可快速构造固体火箭发动机,进行全面的性能计算。系统是一种有效的发动机设计辅助工具。     

基于B/S的民用飞机结构修理方案平台的设计与实现

民用飞机结构修理过程中有时会遇到超出手册范围的情况,在制定超手册结构修理方案的过程中,为了给维修工程人员提供相关的参考方案,本文开发一种基于Browser/Service（B/S）的民用飞机结构修理方案平台。首先从业务流程和平台功能角度对平台需求进行分析;然后基于平台开发所使用的各项技术,从平台架构、数据库、平台功能模块三方面对平台设计进行详细分析;最后通过实际操作演示,对平台的主要功能模块进行测试。结果表明：该平台人机界面友好、扩展性良好、操作简单方便,实现了民用飞机结构飞机损伤信息和修理方案电子化,能够根据损伤信息自动推荐出数据库中存储的若干修理方案,为维修工程部门更快制定超手册修理方案提供支持。     

Observation of Transition Region Fine Structures with Soho/Sumer

We present a preliminary analysis of two quiet Sun transition region areas observed with the SOHO/SUMER spectrometer, using lines from oxygen, nitrogen and silicon. The average quiet Sun physical parameters are studied as a function of line intensity. Systematic variations of line position and width with increasing intensity are found. A large number of small-scale active points have been observed, and preliminary analysis of the physical properties and dynamics of these active features is presented. A jet-like structure, found in an active point, is also investigated and its velocity along the line of sight determined. This revised version was published online in June 2006 with corrections to the Cover Date.     

大数据高性能排序算法的设计与实现

针对大数据排序算法的需求,提出了基于任务驱动的并行排序算法。该算法采用任务驱动、AIO(Asynchronous Input/Output,异步输入/输出)和双缓冲区机制等技术充分利用系统资源;通过构造等价排序键,优化快速排序算法;并在算法实现上,采用多线程处理任务,通过控制线程个数控制并行度。综合利用这些技术,该算法使得大数据的排序性能接近理论极限值,在CPU(Central Processing Unit,中央处理器)资源充裕的情况下,利用异步压缩技术,还可以突破这一极限,最终实现的系统2 000s就可以对超过500Gbyte的磁盘数据做一次完整的排序。在数据库设计中充分利用此思想,将会实现连接和线程的分离,数据库将可以支持更大的连接数,从而提高数据库支持的并发度。     

Statistical Analysis of EUV and UV Lines Inside and Outside of Solar Coronal Holes

Two studies performed with SUMER (the Solar Ultraviolet Measurements of Emitted Radiation spectrometer on SOHO) in September 1996 are presented. Spatial scans, a long exposure time and a broad spectral window provide reliable line profiles for various regions of the Sun (off-limb corona, coronal hole, quiet Sun, bright and dark regions on disk) and for different formation temperatures (Si II, 14 000 K; C IV, 100 000 K; Ne VIII, 630 000 K). Line intensity, position and width distributions are presented together with the line positions relative to the wavelength seen above the limb. This revised version was published online in June 2006 with corrections to the Cover Date.     

The extension of explosive events from the transition region to the corona

We describe the properties of high velocity events in the corona and upper transition region and propose that they are the same phenomenon as the well studied explosive events seen in the lower transition region around T=10⁵ K. Furthermore, we discuss how the SOHO spectrometers, CDS and SUMER, may be used to check this conjecture. Magnetic reconnection has been considered a strong candidate for the physical mechanism causing explosive events. We present a phenomenological model showing how some of the observed properties of explosive events may be explained by reconnection occurring in small magnetic loops.     

The Morphology of the Solar Upper Atmosphere During the Sunspot Minimum

The solar upper atmosphere (SUA) is defined as the volume above the photosphere occupied by plasmas with electron temperatures, T _e, above 2×10⁴ K. Until the Skylab era, only little was known about the morphology of the SUA, while the quality of the spectroscopic observations was continually improving. A spherically symmetric atmosphere was assumed at that time, in which the temperature increased with height. With advances in the observational techniques, it became apparent that the morphology of the SUA was very complex even during the minimum of the magnetic activity cycle. In particular, spectroscopic measurements with high spectral and spatial resolution, which were made in the light of ultraviolet emission lines representing a variety of temperatures, led to the conclusion that most of the radiation from the solar transition region could not be explained by assuming a continuous chromosphere-corona interface, but rather by a region of unresolved fine structures. Recent observational results obtained by modern instruments, such as the Extreme-ultraviolet Imaging Telescope (EIT), the Large Angle Spectroscopic Coronagraph (LASCO), and the Solar Ultraviolet Measurements of (SUMER) spectrograph on the Solar and Heliospheric Observatory (SOHO), as well as the Transition Region and Coronal Explorer (TRACE), and their interpretations will be presented in this review of our understanding of the morphology of the SUA.     

计算机辅助机用铰刀设计

介绍了基于VB环境的铰刀CAD系统的构成与主要模块功能。本设计是以Visual Basic 6．0为开发工具，以Auto CAD2002为图形输出环境，来开发机用铰刀计算机辅助设计软件。该系统对输入的铰刀数据加以分析计算，然后调用数据库中存储的相关参数，自动驱动CAD完成零件图绘制。     

计算机辅助计划管理和决策总体设计

 介绍一种新机研制计划管理和决策支持系统的总体设计方案及其实现的具体措施。详细介绍了几个主要模块的设计思想。