基于PLC的烟机产量控制系统

采用FP1PLC以及PWS－1711图形操作终端，实现了对卷烟产量的实时监控。文中介绍了系统硬件组成与软件设计以及运行结果。     

Challenges in X-ray binary timing: current and future

Millisecond X-ray time variability studies of accreting low-magnetic-field neutron stars and stellar-mass black holes in X-ray binaries probe the motion of matter in regions of strong gravity. In these regions, general relativity (GR) is no longer a small correction to the classical laws of motion, but instead dominates the dynamics: we are studying motion in strongly curved spacetime. Such millisecond X-ray variability studies can therefore provide unique tests of GR in the strong-field regime. The same studies also constrain neutron-star parameters such as stellar mass and radius, and thereby the equation of state (EOS) of ultradense matter. I briefly review the status, and discuss the prospects for mapping out space-time near accreting stellar-mass compact objects, and measuring the EOS of dense matter, through millisecond timing, particularly with an eye towards future missions. The overwhelming consideration for timing sensitivity is collecting area: contrary to most applications, the signal-to-noise ratio for the aperiodic timing phenomena produced by accretion flows increases proportionally with count rate rather than as the square root of it. A 10 times larger instrument turns 1σ effects into 10σ effects (or does as well in 1% of the time). With the Rossi X-ray Timing Explorer (RXTE), using 0.6 m² collecting area, we have found several timing diagnostics from the accretion flow in the strong field region around neutron stars and black holes, as well as signals from neutron star surface hot spots. Combined work between RXTE and the new sensitive X-ray spectrographs onboard Chandra and XMM can already begin to clinch the geometry and physical mechanisms underlying these signals. Future instruments, larger in area by an order of magnitude and in some cases with enhanced spectral capabilities, are expected to turn these diagnostics of GR into true tests of GR. They are also expected to put strong constraints on neutron-star structure, and thereby on the EOS of supranuclear density matter.     

极限条件下的大角度扩散段优化设计数值模拟

为提升某低速风洞大角度扩散段静压恢复性能,降低总压损失至分流隔板的水平,采用计算流体动力学(CFD)方法对该扩散段不同设计方案进行了模拟.采用阻尼网能有效抑制分离,阻尼网布置位置和开孔率对大角度扩散段内的流动状态和总压损失有很大影响.使用直线壁面扩散时,由于扩散角过大,第1层阻尼网对抑制大角度扩散段入口分离效果很弱,总压损失无法达到预期设定指标.采用三次曲线壁面扩散时,总压损失明显降低,小于预期指标,但存在小范围的分离.分级扩散能有效降低总压损失,按照最大静压恢复设计的分级扩散段,避免了入口的气流分离,能大幅度降低总压损失.对分级扩散的进一步研究表明,按照最大静压恢复设计的第1级扩散段扩散角已达到上限,为抑制第3级扩散段的分离,缩短第2级扩散段,减小第3级扩散段扩散角的方法是合理的.通过对不同方案流态的比较得出了最佳的参数匹配,总压损失指标达到了设计要求.因此采用数值模拟能够获得最佳的大角度扩散段设计结果.      

Polarization effects in radiation from compact X-ray sources

The theory of polarization effects in radiation from compact X-ray sources is presented. The following four problems are considered: 1) the polarization of X-rays from the magnetized neutron stars; 2) the polarization of X-rays from the accretion disk around a black hole; 3) the optical polarization from X-ray binaries, and 4) the results of X-ray polarimetric observations.     

泡沫型干扰幕对电磁波传播的能量耗散机理研究

在研究特种泡沫新型长效无污染、多波段干扰技术的过程中,通过泡沫型干扰幕的多界面特征、特种组份微粒的散射作用、气泡的湮灭效应以及媒质的能量吸收作用等方面的实验,总结出了电磁波通过泡沫型干扰幕时的能量耗散机理,为泡沫型干扰幕的实用性研究提供了理论依据。     

炭／陶复合材料电热性能的研究

通过在陶瓷基体原料(高岭土)中添加炭系导电原料(石墨、炭黑),经球磨混合、模压成形和烧结工艺制得炭/陶复合材料.采用X射线衍射(XRD)、扫描电镜(SEM)、数字测温仪等分析和测试了所研制试样的相组成、显微结构以及电热性能.结果表明,本实验的烧结条件下,炭系导电原料不会和陶瓷基体发生反应,其导电性不会受到影响.单一石墨和炭黑含量超过30和25wt%或石墨加炭黑混合(m石墨: m炭黑=1: 1)导电原料含量超过30wt%时,可在炭/陶复合材料内部形成良好的连续导电通道,且该材料具有优良的电发热性能.     

The iron Kα-line diagnostics of the rotating black hole metric in Seyfert galaxies

Observations of Seyfert galaxies in X-ray region reveal the wide emissive lines in their spectra, which can arise in inner parts of accretion disks, where the effects of General Relativity (GR) must be taken into account. A spectrum of a solitary emission line of a hot spot in Kerr accretion disk is simulated depending on the radial coordinate r and the angular momentum a = J/M of a black hole, under the assumption of equatorial circular motion of a hot spot. It is shown that the characteristic two-peak line profile with the sharp edges arises at a large distance (about r ≈ (3–10) r_g). The inner regions emit the line, which is observed with one maximum and extremely wide red wing. We present results of simulations for the isothermal and Shakura–Sunayev disks.     

FY-2C星辐射致冷器太阳屏研制

在风云二号(FY-2)01批气象卫星的基础上,为提高辐射致冷器(以下简称辐冷器)的性能,对C星辐冷器太阳屏进行了改进.根据太阳屏保护膜厚度和翻边白漆等表面特性对辐冷器性能的影响,通过控制保护膜厚度和改用耐紫外光的KS-Z无机漆等以改善C星太阳屏表面特性.地面试验和在轨测试结果表明,C星辐冷器温度和制冷量均在理论计算范围内,太阳屏技术改进有效.     

双头容积式自动灌装控制系统的设计

双头容积式自动灌装控制系统采用西门子S7-300系列PLC和西门子的MP277触摸屏,利用伺服电机精确控制灌装桶的位置和速度,下位机采用Step7 5.4编程软件实现自动灌装生产线PLC控制,上位机采用WinCC Flexible 2008组态软件设计自动灌装生产线的HMI,并通过MPI协议,触摸屏与PLC精通准确可靠,实时监视和控制灌装生产线。该自动灌装生产线已投入使用,不仅运行稳定可靠,而且控制精度高。     

放电电压和屏栅电压对离子推力器性能的影响

利用试验和数值模拟相结合的方法研究6 cm Kaufman离子推力器放电电压和屏栅电压的变化对其工作性能的影响。试验中,离子推力器使用氩气作为推进剂,测量了多组不同工况下的性能参数。此外,基于Goebel的理论模型模拟了放电电压对束流电流和推进剂利用率的影响;采用单元内粒子 蒙特卡罗碰撞（PIC-MCC方法模拟屏栅电压对束流电流、推进剂利用率和加速栅极电流的影响。试验和数值模拟结果一致,发现当放电电压逐渐增大时,引出的束流电流和推进剂利用率先增加然后趋于稳定;当屏栅电压逐渐增大时,引出的束流电流和推进剂利用率先增加然后趋于稳定,加速栅极电流先减小后趋于稳定。研究可以为提高多模式离子推力器的性能提供参考。