Broad-band spectral properties of accreting X-ray binary pulsars

Broad-band spectra of accreting X-ray binary pulsars can be fitted by a phenomenological model composed of a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently, a qualitative picture able to explain the overall broad-band spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review of these recent theoretical developments, I will present a case study of how different modeling of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.     

基于小波变换的非平稳信号趋势项剔除方法

分析了空间飞行器遥测信号处理传统趋势项剔除方法的优势和不足,提出了基于小波变换的非平稳信号趋势项剔除方法。这种方法通过滤波器组将信号分解与重构,实现趋向性信号与零均值平稳随机信号的分离。仿真实验表明,该方法简单、高效,适用于非平稳随机信号的处理,是一种实用的趋势项剔除方法。     

Balloon altitude studies of southern hemisphere hard X-ray sources by the Imperial College-University of Tasmania-INPE collaboration

Hard X-ray balloon altitude measurements with a 1600 cm² phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

基于反馈补偿K-means的救援物资需求预测

针对低空应急救援过程中救援物资需求的多样性与不确定性,提出基于反馈补偿K-means相似搜索的物资需求预测算法。通过比较非平稳数据处理方法,采用差分自回归平均移动模型（ ARIMA）对历史灾情数据进行平滑处理;将预处理后的灾情数据运用基于反馈补偿的K-means方法进行聚类分析;再对比夹角余弦,杰卡德相似系数以及相关系数这3种方法,搜索出相似度最大历史灾情案例,并线性求解当前低空应急救援所需物资量。实验结果表明,在基于反馈补偿K-means相似搜索的物资需求预测过程中,运用相关系数搜索的误差是最小的,方法不仅提高了大数据处理能力,而且在一定程度上提高了预测精度。     

类X-37B升力体再入飞行通信特性中断研究

针对再入非平衡等离子流场的数值仿真方法及等离子体鞘套对不同波段电磁波传输特性的预测开展研究。首先,利用某工程钝头体飞行器再入实测通信飞行测量数据,初步校验数值仿真等离子体特性和通信特性方法的正确性;其次,在典型弹道下针对升力体再入飞行器开展等离子体鞘套数值仿真,分别给出S波段、Ka波段与K波段电磁波衰减特性,研究指出结合当前国内中继星体制情况采用高频段电磁波Ka波段或K波段中继通信方式是解决通信黑障的技术途径之一;最后,研究了电磁波数衰减受传播方向角和攻角的影响规律。研究结果可为发展解决我国再入飞行器通信黑障的设计方案提供参考。     

基于ARIMA模型的拉萨降水量时间序列分析与预测

应用差分自回归滑动平均模型（ARIMA）模型对西藏拉萨地区1969年至2009年的年降水量资料进行建模分析。建立的模型通过了参数的显著性检验和模型的显著性检验。模型的实证分析表明在短期内模型具有较高的预测精度,ARIMA模型可以较好的应用于降水量的预测,对相关部门采取措施应对自然灾害提供了理论支持。     

航空业务量的季节性预测方法及其评价

通过对中国航空运输业务总周转量、客运量、货邮运量的月度和季度数据的预测分析，评价了Holt-Winters法和ARIMA方法在航空业务量季节性预测中的预测效果。研究结果表明，两种方法都有较高的预测精度，但季节性ARIMA方法要优于Holt-Winters法．使用季度数据和ARIMA方法的预测效果最好。     

Multiband echo tomography of Sco X-1

We present preliminary results of a simultaneous X-ray/optical campaign of the prototypical LMXB Sco X-1 at 1–10 Hz time resolution. Lightcurves of the high excitation Bowen/HeII emission lines and a red continuum at λ_c  6000 Å were obtained through narrow interference filters with ULTRACAM, and these were cross-correlated with simultaneous RXTE X-ray lightcurves. We find evidence for correlated variability, in particular when Sco X-1 enters the Flaring branch. The Bowen/HeII lightcurves lag the X-ray lightcurves with a light travel time which is consistent with reprocessing in the companion star while the continuum lightcurves have shorter delays consistent with reprocessing in the accretion disc.     

X-47B无人空战系统及其对抗途径分析

X-47B型无人空战系统是当今最先进的无人机系统之一,势必给现有电子对抗技术及装备带来严重冲击.从其任务使命、系统功能、特色技术入手,分析对其实施电子对抗的技术难点和可能的薄弱环节,探讨对X-47B进行侦察探测和电子对抗的技术途径.