涡喷发动机外场监测分析仪的设计

针对发动机试车测试仪表精度低、测试参数少的问题，利用计算机自动测量技术，对某型发动机的试车性能进行了监控设计。这不仅提高了测试精度、拓宽了测量检查范围，而且为地勤人员分析、判断发动机故障提供了更加全面、精确、可靠的技术数据。     

Advanced data acquisition system for SEVAN

Huge magnetic clouds of plasma emitted by the Sun dominate intense geomagnetic storm occurrences and simultaneously they are correlated with variations of spectra of particles and nuclei in the interplanetary space, ranging from subtermal solar wind ions till GeV energy galactic cosmic rays. For a reliable and fast forecast of Space Weather world-wide networks of particle detectors are operated at different latitudes, longitudes, and altitudes. Based on a new type of hybrid particle detector developed in the context of the International Heliophysical Year (IHY 2007) at Aragats Space Environmental Center (ASEC) we start to prepare hardware and software for the first sites of Space Environmental Viewing and Analysis Network (SEVAN). In the paper the architecture of the newly developed data acquisition system for SEVAN is presented. We plan to run the SEVAN network under one-and-the-same data acquisition system, enabling fast integration of data for on-line analysis of Solar Flare Events. An Advanced Data Acquisition System (ADAS) is designed as a distributed network of uniform components connected by Web Services. Its main component is Unified Readout and Control Server (URCS) which controls the underlying electronics by means of detector specific drivers and makes a preliminary analysis of the on-line data. The lower level components of URCS are implemented in C and a fast binary representation is used for the data exchange with electronics. However, after preprocessing, the data are converted to a self-describing hybrid XML/Binary format. To achieve better reliability all URCS are running on embedded computers without disk and fans to avoid the limited lifetime of moving mechanical parts. The data storage is carried out by means of high performance servers working in parallel to provide data security. These servers are periodically inquiring the data from all URCS and storing it in a MySQL database. The implementation of the control interface is based on high level web standards and, therefore, all properties of the system can be remotely managed and monitored by the operators using web browsers. The advanced data acquisition system at ASEC in Armenia was started in November, 2006. The reliability of the multi-client service was proven by continuously monitoring neutral and charged cosmic ray particles. Seven particle monitors are located at 2000 and 3200 m above sea level at a distance of 40 and 60 km from the main data server.     

Research by the Tasmanian cosmic ray group during the International Geophysical Year

Systematic recording of the cosmic radiation commenced in Hobart in 1946 and at Mawson in Antarctica in 1955, making these two of the longest running cosmic ray observatories in the world. For the IGY, observations were also made at a sub-Antarctic island and near the equator, and an airborne survey of the nucleonic component was made from Geomagnetic Latitude −60°, south of Australia, to Japan and back. At Hobart there were neutron monitors, vertical and inclined muon telescopes, an ionization chamber, and two muon telescopes at ∼40 m of water equivalent underground. The research based on these and other observations determined the energy dependence of the Forbush and 11-year variations and concentrated, in particular, on understanding the anisotropic nature of galactic cosmic rays up to 150 GeV; the anisotropies in the onset phase of Forbush decreases; and the anisotropies in solar cosmic ray events. An investigation was initiated to calculate the trajectories and cutoff rigidities of cosmic rays in a high order simulation of the geomagnetic field. This was completed in 1959–60.     

实现SMP机群虚拟化的方法

机群是一类重要的并行计算机体系结构,成本低廉,可扩展性强,但编程复杂,管理难度大.利用虚拟化技术可以将机群抽象成具有共享内存特征的虚拟机,支持共享内存的编程模式,从而克服机群的不足.当前,在该领域有少量探索性的研究成果,但都不能支持对称多处理机(SMP,Symmetric Multiprocessor)机群虚拟化.本文提出一种新颖的虚拟化SMP机群的方法,即利用硬件虚拟化技术,在操作系统(OS,Operating System)之下构建分布式虚拟机监视器(DVMM,Distributed Virtual Machine Monitor),通过DVMM对机群的资源进行感知、整合、虚拟化和呈现,使SMP机群对OS呈现为一台具有共享内存特征的虚拟机;通过DVMM与OS配合,实现在虚拟机上透明地运行并行应用软件.     

军用飞机外场可靠性监控方法及实现

军用飞机可靠性监控的目的在于对现役的军用飞机、机群的可靠性状况及飞机维修大纲的实施情况进行连续的监督与控制,以提高军机的系统效能,充分保证军机的战斗力。结合中国国情论述了军用飞机,监控指标的选取、计算、控制界限的确定及具体实现。     

1553B总线监视器系统软件设计

1553B总线是一种集中式控制的串行总线型网络，其组成包括一个总线控制器、若干远置终端，还可以包括总线监视器。本文详细介绍了1553B总线监视器系统软件的设计，探讨了设计中需要注意的几个问题。     

基于Inmarsat D+的车辆监控系统研究

Inmarsat D 在全球范围内为用户提供了高质量、高可靠性的双向短信息通信服务。基于Inmarsat D 相关技术，研究了基于Inmarsat D 的车辆监控系统的设计。详细阐述了系统的设计思想和相关实现技术的可行性。系统的开发与应用，必将对车辆调度管理的高效性、车辆运行状态统计分析的准确性以及车辆交通意外责任判定的公正性等，提供可靠保障。     

Athens Neutron Monitor Data Processing Center – ANMODAP Center

Cosmic ray measurements in Athens were initiated in November 2000 with a standard 6NM-64 neutron monitor. Within the last years an effort has been made in order to construct an effective database of neutron monitor (NM) and satellite data in real-time, regarding the necessities of space weather monitoring (Athens Neutron Monitor Data Processing Center – ANMODAP Center). The prospective goal of this network is to make possible the receiving of all data in real-time in close sequence from all servers around the globe. The graphical representation of all these data in real-time is available through the website of the station (http://cosray.phys.uoa.gr). Moreover, a second database that collects data with 1-min resolution operates in a parallel mode. The online services as a special ‘Alert’ algorithm for Ground Level Enhancements (GLEs) and some models created to analyze aspects of GLEs as the neutron monitor Basic Anisotropic Neutron Ground Level Enhancement (BANGLE) model and the Forbush Decreases (FORD) model as well, are presented. Moreover, a short account on work performed on the possible relationship between the geomagnetic activity level and the biological effects is given.     

Cosmic ray measurements in High Tatra mountains: 1957–2007

Lomnický Štít (LS, situated at High Tatra mountain, 2634 m above sea level, in the direction of 49.40°N, 20.22°E; geomagnetic vertical cut-off rigidity for cosmic rays ∼4 GV) is a relevant place for cosmic ray studies. After a brief review of the LS research history we present a selection of the results based on the measurements performed by the neutron monitor located at that site. In particular, the characteristics of quasi-periodicities and the diurnal variability amplitude and phase obtained from those data are discussed.     

New He neutron monitor for Chilean Cosmic-Ray Observatories from the Altiplanic zone to the Antarctic zone

We present the results of three years of continuous operations and the principal characteristics of our new ³He neutron monitors installed in the Chilean Network of Cosmic-Ray Observatories. During the years 2004 and 2005, we began the construction of this International Geophysical Year (IGY)-type ³He neutron monitor, with the intention of replacing the older proportional tubes of the BF₃. These new monitors are installed in stations at locations ranging from the near-equatorial zone to the Antarctic zone. As a reference system, we used our own BF₃ neutron monitors and previously complemented the collected data with a Monte Carlo simulation for the proton-yield function response of the Putre neutron monitor. Herein, we present for the first time the data obtained from our new high-mountain observatory located in the Altiplanic zone.