有线电视网络安全监控系统

在有线电视台前端采用数字信标插入器在视频插入标志,在有线电视网中对此标志进行检查,即可判断有线网络中播出的信号是否合法,若不符合设定,则通过电话网络向前端发出报警信号,前端收到报警信号后,向值班人员发出声光报警,从而达到对有线电视网络进行实时监控的目的。较详细地说明了该系统及各主要部分的原理及具体实现。     

Appearance of neutron stars in the state of subsonic propeller

The state of subsonic propeller is intermediate between the states of supersonic propeller and accretor in the evolutionary tracks of magnetized compact stars. The rotational rate of a star at this stage decelerates due to the interaction between its magnetosphere and the surrounding hot, quasi-static plasma envelope. The magnetospheric radius is smaller than the corotation radius and the boundary of the magnetosphere is stable with respect to interchange instabilities. The rate of the mass flux from the inner radius of the envelope to the stellar surface is limited by the rate of plasma diffusion into the magnetic field of the star. As a result, the subsonic propeller would appear as a low-luminosity accretion-powered pulsar with a soft X-ray spectrum.     

Inside and outside of supernovae

A newly formed neutron star in a supernova finds itself in a dense environment, in which the gravitational energy of accreting matter can be lost to neutrinos. For the conditions in SN 1987A, 0.1M may have fallen back onto the central neutron star on a timescale of hours after the explosion, after which the accretion rate is expected to drop sharply. Radiation is trapped in the flow until the mass accretion rate drops to 2×10^–4 M yr^–1 at which point radiation can begin to escape from the shocked envelope at an Eddington limit luminosity. Between this neutrino limit and the Eddington limit, 3×10^–8 M yr^–1, there are no steady, spherical solutions for neutron star accretion. SN 1987A should have reached the neutrino limit within a year of the explosion; the current lack of an Eddington luminosity can be attributed to black hole formation or to a clearing of the neutron star envelope. There is no evidence for newly formed neutron stars in supernovae. Radio supernovae, which were initially interpreted as pulsar activity, probably involve circumstellar interaction; SN 1993J shows especially good evidence for outer shock phenomena.     

Two magnetars: SGR 1627–41 and 1E 1547–5408

We describe the results obtained with Target of Opportunity observations of the galactic sources SGR 1627–41 and 1E 1547–5408. These two transients show several similarities supporting the interpretation of Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters as a single class of strongly magnetized neutron stars.     

Contamination of short GRBs by giant magnetar flares: Significance of downward revision in distance to SGR 1806–20

We highlight how the downward revision in the distance to the star cluster associated with SGR 1806–20 by Bibby et al. (2008) reconciles the apparent low contamination of BATSE short GRBs by intense flares from extragalactic magnetars without recourse to modifying the frequency of one such flare per 30 years per Milky Way galaxy. We also discuss the variety in progenitor initial masses of magnetars based upon cluster ages, ranging from ∼50 M_⊙ for SGR 1806–20 and AXP CXOU J164710.2–455216 in Westerlund 1 to ∼17 M_⊙ for SGR 1900+14 according to Davies et al. (2009) and presumably also 1E 1841–045 if it originated from one of the massive RSG clusters #2 or #3.     

线性令牌总线仿真监控软件的设计与实现

线性令牌总线(LTPB)是一种先进的机载互连技术,它具有高带宽、实时性强和高可靠性等特点。本文主要从系统角度给出了LTPB测试系统中仿真监控软件的设计与实现。本仿真监控软件的开发对于验证总线接口单元(BIU)是否能够准确实现LTPB协议功能与性能,以及总线网络整体运行情况的监控有着重要的意义,为LTPB能够尽早在我国的航空电子系统中得以应用起到了一定的作用。     

GNSS双频导航信号用户完好性监测机制研究

用户完好性监测指标通常被用于衡量导航信息的可信度,针对单个卫星导航系统用户完好性监测指标过高、可用性较差的问题,提出一种全球导航卫星系统(GNSS)多系统双频信号联合完好性监测机制,该监测机制使用一定完好性风险分配值下的保护门限作为联合观测下的监测指标;另外,为了确保各种监测假设下的用户完好性,分别讨论了无故障及一颗卫星故障假设下的伪距观测误差获取、保护门限计算以及完好性风险指标分配等问题。仿真结果表明该用户监测机制可有效降低保护门限、提高可用性,在用于I类精密进近时全球大部分区域用户的可用性水平大于95%。     

某型发动机地面信息管理系统设计与实现

针对某型发动机地面监控缺乏信息管理的现状,本文围绕实际需求,构建了信息管理系统功能模型,设计了包括信息管理模块、数据分析模块、故障诊断模块、报告生成模块的管理系统,并采用C/S结构设计方式集成多种软件予以实现.     

基于单片机和CdS涂层老化探头的装备腐蚀监测系统设计

针对装备对腐蚀状态监测需求,以 MSP320单片机为核心控制器、CdS涂层老化探头为腐蚀状态传感器,设计了一款 4路腐蚀状态监测系统,并用于某型车辆腐蚀状态监测。实验结果表明,该系统能真实监控该型车辆的腐蚀状态,为该车辆的预防性维修提供了重要技术和数据支持。同时,该系统具有安装灵活方便、工作可靠、体积小等优点,具有较高的推广应用价值。     

煤矿安全生产微型机监控系统

用微型计算机监测与控制煤碳生产,可以大大提高煤矿的安全生产和自动化水平,进一步改善煤矿的生产管理和增加企业效益。本文具体介绍了一个适用于中、小型煤矿的安全生产微型机监测与控制系统的功能、结构和软、硬件配置,并着重讨论了系统主站的几个关键技术问题是怎样解决的。该系统现已投入运行。实践证明,设计合理,性能稳定,工作可靠,它是一个特别适用于中、小型煤矿的廉价安全生产监控系统。