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.     

The effect of neglecting VLBI reference station clock offsets on UT1 estimates

Very Long Baseline Interferometry (VLBI) allows to monitor universal time (UT1) by conducting regular international experiments. Such dedicated observation networks are equipped with different hardware components, which require different processing strategies when the data are correlated. As the timing units at each stations are usually offset with respect to universal time (UTC) this effect should be considered during correlation processing. Thus, it is investigated how neglecting of these offsets theoretically impacts the estimation of UT1. Three different strategies for the proper handling of the timing offset will be discussed and their advantages/drawbacks will be pointed out. Moreover, it is studied how neglecting of these timing offsets affects UT1 time-series and how such a missing correction can be applied a posteriori. Although the discussed effect is for most of the UT1 experiments smaller than the formal error of the estimates, it is important to consider station clock offsets properly in next-generation VLBI systems, which are expected to improve accuracy of results by about one order of magnitude.     

Introduction to the Payloads and the Initial Observation Results of Chang＇E-1

Chang'E-1,the orbiter circling the moon 200km above the moon surface,is the first Chinese Lunar exploration satellite.The satellite was successfully launched on 24th October 2007.There are 8 kinds of scientific payloads onboard,including the stereo camera,the laser altimeter,the Sagnac-based interferometer image spectrometer,the Gamma ray spectrometer,the X-ray spectrom-eter,the microwave radiometer,the high energy particle detector,the solar wind plasma detector and a supporting payload data management system.Chang'E-1 opened her eyes to look at the moon and took the first batch of lunar pictures after her stereo camera was switched on in 20th November 2007.Henceforth all the instruments are successfully switched on one by one.After a period of parameter adjustment and initial check out,all scientific instruments are now in their normal operating phase.In this paper,the payloads and the initial observation results are introduced.     

LALR(1)分析器快速生成

根据LR(0)自动机的构造理论及Deremer和Pennello的LALR(1)向前看符号集计算公式,提出求解公式中的lookback关系和includes关系的高效算法. 研究过程表明,LR(0)项目集闭包计算和项目集的查找是LR(0)分析器构造过程中的主要性能瓶颈.对这两个计算过程给出了高效的数据结构和算法设计,实现了LALR(1)分析器的快速生成.系统实现及实验数据表明,LALR(1)分析器的生成速度超过了自由软件基金会的LALR(1)分析器生成器Bison.      

SiO2f/SiO2复合材料自身及其与铜、不锈钢的钎焊

采用AgCuTi活性钎料,在880℃/10min规范下成功实现了SiO2f/SiO2自身、SiO2f/SiO2与Cu和SiO2f/SiO2与1Cr18Ni9Ti三种接头的连接。实验结果表明,三种接头中靠近SiO2f/SiO2母材的界面处均形成了一层薄薄的扩散反应层组织,反应层中出现了Ti和O的富集,根据两者的原子比例推断生成了TiO2相;另外,三种接头中心区都形成了由灰色相和白色相共同组成的Ag-Cu共晶组织,其中灰色相为Cu基固溶体,白色相为Ag基固溶体。接头剪切强度结果显示,SiO2f/SiO2/Cu接头剪切强度为12.4MPa,SiO2f/SiO2/1Cr18Ni9Ti接头剪切强度为18.4MPa,接头中的残余应力是决定接头强度大小的重要因素之一。     

1-3型压电纤维主动叠层板扭转特性的研究

对4类典型铺层的1-3型压电纤维复合材料主动板的变形模式进行了理论分析。在此基础上对具有扭转变形模式的主动叠层板进行了振动特性分析,得到了该类型主动叠层板在外界电场激励下的稳态解。最后对该类主动叠层板的扭转振动特性进行了深入的研究,包括作用电场强度的大小、频率对扭转特性的影响、压电纤维铺层角和压电纤维体积比对主动叠层板扭转特性的影响等。算例表明本文计算模型和有限元得到的结果符合良好,同时算例结果表明含1-3型压电纤维复合材料主动叠层板具有良好的主动扭转特性。     

螺旋桨桨叶1P气动载荷研究

介绍了一种１Ｐ载荷实验研究方法－桨叶应变测试法,首先通过桨叶剖面速度三角形及气动力分析给出了１Ｐ载荷与测量应变的关系,然后通过地面试验和飞行试验进行了验证。试验结果表明,螺旋桨１Ｐ载荷主要由于非对称气流流过桨盘面改变了桨叶剖面速度三角形而引起,迎角,侧滑角的增加,会产生较大的１Ｐ载荷;机动飞行,如快速拉杆,荷兰滚等也会产生较大的１Ｐ载荷。     

猎鹰9号火箭发射及箭体复用的分析

猎鹰9号火箭截至2023年年底已完成286次发射。对猎鹰9号火箭特别是Block5版本火箭的发射情况进行了完整梳理统计,重点分析了一级箭体的复用情况以及发射、回收的相关能力保障,对火箭的经济性和未来前景作了预测。     

实验室条件下IRMSS遥感器MTF与遥感图像参数的相关分析设计与性能评估

调制传递函数MTF(ModuleTransferFunction)在物理光学理论中 ,是光学系统成像性能的综合评价指标。遥感器MTF的性能变化会导致遥感图像的质量变化 ,遥感图像质量的变化则导致描述遥感图像的参数的变化。文章以CBERS - 1的 0 2星IRMSS遥感器为例 ,在实验室条件下模拟遥感器在轨运行的成像过程并获得图像数据 ,MTF可通过专业仪器直接测量 ,然后再进行MTF与遥感图像参数的相关分析 ,从而确定出与MTF相关性最强的图像参数。文章的相关分析采用SPSS统计分析软件完成     

1,5-二氨基四唑含能配合物的制备、表征及其催化性能研究

合成出2种以1,5-二氨基四唑(DAT)为配体,苦味酸根为外界,钴和铜为中心离子的含能配合物,并对其结构进行了表征.运用示差扫描热分析(DSC)方法,就目标化合物对高氯酸铵(AP)、奥克托金(HMX)和六硝基六氮杂异伍兹烷(HNIW)热分解的影响进行了研究.利用电荷耦合器件(CCD)燃速测定系统,研究了目标化合物对缩水...