混气电解加工中两相流音速及阻塞机理研究

着重分析研究气液两相流音速特性及其阻塞机理。通过测量由小药量电雷管爆炸而产生的压力波传播速度，然后修正到音速。试验结果表明，气液两相流音速与气泡率、当地压力及其流型有关。由于气液混合物强烈的压缩性，混气电解加工间隙中易于出现类似可压缩气体的阻塞现象。     

基于建构主义理论抛锚式教学模型的ESP教学设计——以《客舱乘务英语》为例

基于建构主义理论指导下的抛锚式教学,强调以真实事件或真实问题作为教学活动的基础。本文针对当前高校ESP课堂教学的现状,简要分析了存在的问题及原因,由此引入建构主义学习理论的观点,并对将抛锚式教学方法融入到客舱乘务英语课的教学进行例析,以期改变传统ESP课堂教学的弊端,实现ESP以学习为中心的教学原则。     

一种新型的基于预测的卫星资源分配方法

针对传统的按需分配方式所造成的长时延问题,提出了一种新型的基于业务预测的按需分配方法。该方法通过预测业务在等待队列中的长度,将预测信息发送给网络资源控制中心,再由控制中心动态地分配带宽资源,达到服务质量的要求。在阐述了按需分配和业务预测的基本算法后,通过仿真分析了不同的业务类型采用不同的预测信息发送间隔时间的时延性能,分析中考虑了实时业务比非实时业务享有更高的优先权,并且比较了常规按需分配与基于业务预测的按需系统分配方法的时延性能。仿真结果表明利用业务预测,选择合适的预测信息发送间隔时间,能够有效地改善带宽资源分配的时延性能,相比一般的按需分配方式服务质量有了明显的提高。     

基于开路电压法的电池荷电状态估计误差校正

本文提出分别研究电池开路电压在充电结束后停置过程和放电结束后停置过程的不同变化规律,并考虑了不同停置时间在两个过程中的作用和影响,从而达到提高开路电压法估算荷电状态精度的效果。实验验证表明,此方法的精度比传统开路电压法更加准确。     

Separation of the Galactic Cosmic Rays and Inner Earth Radiation Belt Contributions to the Daily Dose Onboard the International Space Station in 2005–2011

The DB-8 detectors of the ISS radiation monitoring system (RMS) have operated almost continuously onboard the ISS service module since August 2001 till December 2014. The RMS data obtained were used for the daily monitoring of the radiation environment aboard the station. This paper considers the technique of RMS data analysis that allows one to distinguish the contributions of galactic cosmic rays and the Earth’s inner radiation belt to the daily dose based on the dosimetry data obtained as a result of the station’s passage in areas of the highest geomagnetic latitudes. The paper presents the results of an analysis of the dosimetry data based on this technique for 2005–2011, as well as a comparison with similar results the authors obtained previously using the technique based on an analysis of the dosimetry data obtained during station passages in the area of the South Atlantic Anomaly.     

Modes of uncontrolled rotational motion of the <Emphasis Type="Italic">Progress M-29M</Emphasis> spacecraft

We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3–7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft’s angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft’s motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth–Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1–0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angularvelocity measurements. The measurements of the electric current from solar arrays were used for verification.     

Control of the Onboard Microgravity Environment and Extension of the Service Life of the Long-Term Space Station

The problem of control of the on-board microgravity environment in order to extend the service life of the long-term space station has been discussed. Software developed for the ISS and the results of identifying dynamic models and external impacts based on telemetry data have been presented. Proposals for controlling the onboard microgravity environment for future long-term space stations have been formulated.