地磁暴期间中国中低纬电离层的CIT研究

利用电离层层析成像技术(Computerized Ionospheric Tomography, CIT)处理115°E子午圈附近6个台站的GPS观测数据, 分析了2004年11月地磁暴期间中国中低纬电离层的响应情况. 结果表明, 电离层呈正相扰动, 且不同高度上的响应不同, 800 km以下电子密度有不同程度的增加, 且在峰值高度附近增幅最大, 800 km以上地磁暴的影响并不显著; 伴随地磁能量的注入, 赤道异常峰极向扩展; 随磁扰强度的降低, 电子密度也逐渐恢复至平静水平. 这些结果与以往的理论和观测结果一致, 初步估计扰动是由热层暴环流引起的, 并受到赤道异常峰移动的影响.     

Control and utilization of range-dependent beampattern with waveform diverse array radars

The transmit antenna beampattern of the phased array radar is only a function of angle, limiting its ability to discriminate the targets from the same direction. Recently, the waveform diverse array radars expand the angle-dependent beampattern to an angle-time-range-dependent three-dimensional function by modulating the frequencies/time delays/phases across different transmit antenna elements. In this respect, extra Degrees-of-Freedom (DOFs) in the range domain are achieved, which opens up an innovative way to fulfil the tasks with enhanced system performance by jointly using the angle and range information. This paper summaries the developments of waveform diverse radars, including the Frequency Diverse Array (FDA), the Space-Time-Circulating-Array (STCA), and the Element-Pulse-Coding (EPC) frameworks, with emphasis on the analysis of the range-dependent beampattern from the basic properties upon how it is controlled. Moreover, the most recent advances of utilizing such a range-dependent beampattern in target detection, parameter estimation and identifiability, clutter suppression, jammer suppression and Synthetic Aperture Radar (SAR) imaging are discussed.     

高能(450kV)X射线参考辐射场附加过滤研究

利用MCNP程序对450kV X光机建立模型,计算各参考辐射质下的原级谱、平均光子能量。对ISO4037-1中已有范围的管电压与附加过滤片厚度关系曲线进行二次拟合,确定模拟厚度范围。利用MCNP计算各附加过滤组合下的平均光子能量值,并与外推法得出的平均光子能量值进行对比,将相对偏差最小时的附加过滤作为最终确定值。从部分能量点的模拟与测量结果的对比可看出,模拟得出的平均光子能量在2%以内与PTB及中国计量院测量结果保持一致,附加过滤最大相对偏差为18%。     

柔性印制膜在太阳电池阵的应用及热适应性试验研究

针对微小卫星太阳电池阵高体积比的功率需求,设计了带柔性印制电路（FPC）的太阳电池阵。该太阳电池阵将太阳电池、FPC与基板集成为一体,具有厚度薄、质量小等优点。通过热循环试验对其环境适应性进行考核,X射线检测结果表明,太阳电池阵上锡焊焊盘与覆铜层连接部位受热应力的影响较大,在长期高低温循环条件下存在锡焊焊盘与覆铜层断裂的风险。为此,给出提升太阳电池阵上FPC抗热形变能力的设计建议,以期为后续太阳电池阵设计提供参考。     

一种用于深空探测的Chirp变换频谱分析仪设计与实现

根据深空探测对频谱分析仪抗辐射、高分辨率、低功耗的需求,研究一种基于Chirp变换的高分辨率频谱分析仪设计及其实现.利用中心频率为1GHz、带宽为400MHz、色散时间为10μs的声表面波滤波器,提出了一种模拟和数字相结合的高分辨率频谱分析仪设计方案,并搭建原理实验系统完成了实测验证,其分析带宽为400MHz,频率分辨率达到152kHz,功耗约为3.6W.分析了压缩线器件非理想特性对频率分辨率的影响,利用实测压缩线频率响应特性获得幅度和相位补偿曲线,对展宽线信号进行幅相失配补偿.仿真结果表明,该补偿方法可将频率分辨率提高至108kHz.     

"海洋一号"卫星的检漏技术

文章介绍了"海洋一号"卫星检漏所采用的两种方法,特别指出采用加压真空检漏方法更能真实地测得卫星的实际漏率,并可提高工作效率.     

太阳微波爆发动态频谱仪

介绍了北京天文台已投入观测的1.0—20GHz,2.6—3.8GHz太阳射电频谱仪及1999年投入观测的5.2—76GHz太阳射电频谱仪。它们是第23周太阳活动峰年我国太阳物理界的重要观测设备已投入观测的频谱仪获得不同类型的太阳射电爆发资料分别为171个和146个,这些事件在时间和频率上有丰富的幅度和结构的变化。不同太阳射电爆发反映太阳大气不同高度上耀斑的时间和空间的演化过程,为研究不同大气高度中耀斑物理动力学过程、能量释放、粒子加速提供了更多的依据。     

Structure and development of quiet loops in the solar corona

X-ray emission from solar coronal loops changes on two different timescales: a) flare loops and transient active region brightenings show a rapid variability, b) quiet region loops are quasi-steady and change only slowly with time. This different time behavior has been analyzed on the basis of Yohkoh SXT observations and we report here on the results from our analysis, mainly focussing on quiet loop variability.     

彩色计算干涉技术及应用

在对高速气流进行干涉法测量时 ,由于激波的作用或者光的散射、斑点等现象 ,干涉图的干涉条纹可能会出现不连续。笔者通过仿真M Z干涉仪或全息干涉仪光学模型 ,并且采用对多块不规则网格的计算流体力学结果进行重构的直接体视化图形算法 ,得到了高分辨率的彩色数值干涉图 ,克服了干涉条纹的不连续性并给出了一个弹道靶中超高声速钝锥流场的例子     

On the optical variability of a be star,HDE 245770, — the optical counterpart of the transient X-ray pulsar A0535+26

Photoelectric WBVR observations of Be star HDE 245770=V 725 Tau, the optical counterpart of the transient X-ray pulsar A0535+26, having a pulse period of about 104 s, were conducted for more than 10 years. An irregular long-term optical variability of the star with amplitudes of the order of a few tenths of magnitude was found to be a usual phenomenon. In some cases rapid changes of the star's optical luminosity with a characteristic period of a few tens of minutes or a few hours, and an amplitude of several hundredths of magnitude in all the spectral bands used, which have practically coincided or correlated with the X-ray pulsar outbursts detected by X-ray satellites, were observed.Photoelectric recording of the optical flux from HDE 245770 were made in 1981–1982 with a time resolution of 1 second and 10 s, respectively, in theR spectral band (₀ 7000 Å) and in the narrowH -emission-line band (_1/2 75 Å) using a 48-cm reflector of High-Mountain Tien-Shan observatory of the Sternberg Astronomical Institute near Alma-Ata. An analysis of autocorrelation functions of the flux changes from object under study and a comparison with the star BD+26° 876 indicated the variability of luminosity of V 725 Tau in theR spectral band on a time scale of a few tens of second; this variability resembles shot noise with a characteristic time of stochastic bursts of about 15–20 s and their amplitudes of about a few tenths of a percent. InH -emission-line radiation autocorrelation functions and power spectra show quasiperiodic variability of luminosity of HDE 245770 with a characteristic period of about 100–150 s and an amplitude in the neighbour-hood of 0.5%. The latter result is not quite reliable because of not quite fine weather conditions during the observations; independent observations and check-up are required.