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.     

Silver Film Growth on Glass Ceramic by Radio Frequency Magnetron Sputtering

Thin silver films are deposited by radio frequency magnetron sputtering on glass ceramic at room temperature.Variations of sputtering power,bios voltage and power density are carried out for each deposition,then parts of as-deposited samples are subjected to annealing at 600 ℃ within a vacuum chamber.Structural properties are studied by X-ray diffraction(XRD),scanning electron microscope(SEM)and laser scanning confocal microscope(LSCM).It is shown that structural properties have a strong dependency on sputtering power and annealing temperature.Electrical contact resistance measured by a four point probe instrument is directly affected by the thickness of films.It is also found that the film conductivity,especially in thinner films,is improved by the increasing grain size.Finally,the film adhesion is observed by scratch tests.And the adhesive ability deposited by radio frequency magnetron sputtering shows a better performance than that produced by traditional methods.     

环刷刷丝接触压力检测系统设计

环刷是导电滑环的重要组成部件,其接触压力是滑环使刷丝变形后产生的刷丝对滑环的作用力。环刷刷丝接触压力值微小,影响因素较多,但环刷刷丝接触压力的大小将直接关系着导电滑环的技术性能和使用寿命。本文针对环刷的特点详细研究了环刷刷丝接触压力的测量方法和技术,并设计了一套环刷刷丝接触压力检测系统,实现了对环刷刷丝接触压力的自动精密测量。     

ABPSK原理及实现

从理论到实践，比较详细地说明了ABPSK调制的原理及与普通DBPSK调制的关系，给出了具体的实现过程框图，通过计算机模拟给出了若干调制的例子，并给出了相应的图表。     

Robustness of multiple-limb manipulation systems

Ｄｕｒｉｎｇｒｅｃｅｎｔｙｅａｒｓ，ｃｏｎｓｉｄｅｒａｂｌｅｒｅｓｅａｒｃｈｅｆｏｒｔｈａｓｂｅｅｎｄｅｖｏｔｅｄｔｏｔｈｅｓｔｕｄｙｏｆｔｈｅｍｕｌｔｉ－ｐｌｅ－ｌｉｍｂｍａｎｉｐｕｌａｔｉｏｎｓｙｓｔｅｍｓｗｉｔｈｔｈｅａｂｉｌｉｔｙｔｏｕｓｅａ...     

Be／X射线双星LSI＋61°303的光谱研究

给出了１９９２－１９９５年Ｂｅ／Ｘ射线双星ＬＳＩ＋６１°３０３每年的光谱观测结果，分析了光谱发射线轮廓及其变化，观测显示Ｈβ发射线轮廓具有典型的气壳吸收，表明观测视线与Ｂｅ星赤道平面平行，同时发现Ｈα发射线参数发等值宽度和双峰强度之比也具有类似射电流量的周期性变化，但其变化与射电玫光学光度的变化不同，因此认为此变化可能与中子星周期的吸积盘及其轨道交食有关。     

Cr12V与Cr12MoV钢的接触疲劳性能研究

对Cr12V与Cr12MoV钢的接触疲劳性能进行了对比试验研究。结果表明,Cr12V钢比Cr12MoV钢有较高的接触疲劳寿命,额定寿命L10是Cr12MoV钢的2.11倍,中值寿命L50是Cr12MoV钢的1.62倍。分析认为,Cr12V钢与Cr12MoV钢相比,具有较高的硬度、较小的碳化物尺寸以及较高的V含量,这是Cr12V钢接触疲劳寿命高的原因。     

压力角螺旋角等对弧齿锥齿轮强度的影响

讨论了压力角，螺旋角对弧齿锥齿轮齿面接触强主工，齿根弯曲强度的影响，及齿轮工作齿面为凸面或凹面时齿根弯曲强度的变化，建立了菱形接触的名义接触应力公式并探讨了这类接触区对接触强度的影响。     

考虑铰链间隙的投放机构动力学特性分析

为了分析铰链间隙对机构运动特性的影响,针对一种投放机构,通过对模型进行分析,将其简化为一个四连杆机构,建立投放机构的非线性弹簧阻尼模型,同时采用库仑摩擦描述机构间隙处的摩擦作用,并将建立好的模型导入到Adams仿真分析软件中,进行动力学特性分析。仿真分析结果表明：利用Adams软件可以有效地建立含铰链间隙的投放机构动力学模型,分析间隙对机构在开启过程的影响,仿真结果能够预测铰链间隙对机构运动特性的影响,为机构的设计和优化提供依据,并有利于在工程方面的应用。     

角接触球轴承生热预测方法与灵敏度分析

通过拉丁超立方实验设计法获取角接触球轴承NSK-7015C的结构参数样本数据,采用Newton-Raphson法求解轴承变形几何协调方程、滚动体平衡方程和内圈平衡方程所构成的非线性方程组。应用Kriging和Monte Carlo相结合的方法(AK-MCS)构建样本数据与轴承生热的函数关系,在此基础之上使用全局灵敏度计算方法计算轴承结构参数对轴承生热的影响。研究结果表明:在相同轴承结构参数下,采用AK-MCS法预测的轴承生热与轴承拟静力学分析模型求得的结果差值均小于0.003 W,说明AK-MCS算法的预测结果具有较高的准确性;轴承生热对轴承滚动体直径变化反应最灵敏,轴承内、外圈沟道直径影响次之,轴承内、外圈沟道曲率半径影响最小,该研究能够为轴承结构参数的设计优化和加工精度的选择提供理论依据。