固体火箭发动机点火过程内流场的二维预示

本文对固体火箭发动机点火过程的内场流进行了二维无粘非定常分析，计算得到了该阶段燃烧室中压强，温度和速度的分布。本文还提出了以近似预示复杂三维装药发动机内流场的有效积法。     

考虑二次流影响的压缩系统稳定性模型

利用Ａｄｋｉｎｓ－Ｓｍｉｔｈ二次流模型计算得到转子出口截面落后角沿叶高的变化。在压缩系统稳定性模型中考虑叶尖流面落后的角影响，并提出一个新的时滞参数计算公式，计算结果表明，落后角的大小对压缩系统的稳定性影响很大，同时揭示了叶尖间隙对压缩系统稳定性的影响。     

Optical search for gamma-ray bursts

The preliminary results from optical search for light pulses associated with gamma ray bursts by means of the Czechoslovak Fireball Network plate collection at the Ondřejov observatory are given. Optical monitoring represents more than 7700 hours, but no real optical counterpart was found. Problems associated with the optical search for gamma ray bursts are discussed.     

Research Advances of Solar Corona and Interplanetary Physics in China: 2012–2014

Solar transients and their related interplanetary counterparts have severe effects on the space environments of the Earth. Therefore, the research of solar corona and interplanetary physics has become the focus of study for both solar and space scientists. Considerable progress has been achieved in these aspects by the solar and space physics community of China during 2012–2014, which will be given in this report. The brief report summarizes the research advances of solar corona and interplanetary physics into the following parts: solar wind origin and turbulence, coronal waves and seismology, solar eruptions, solar energetic particle and galactic cosmic ray, magnetic reconnection,Magnetohydrodynamic(MHD) models and their applications, waves and structures in solar wind,propagation of ICMEs/shocks and their arrival time predictions. These research achievements have been achieved by Chinese solar and space scientists independently or via international collaborations.     

相域输电线路模型中的频率相关转换矩阵

首先针对使用传统算法得到的频率相关转换矩阵元素存在突变点的问题,提出一种新算法用于消除频率相关转换矩阵元素的突变点.新算法先使用传统算法计算出每个频率点的转换矩阵,再通过一个基于最优化原理的平滑过程消除转换矩阵中元素的突变点.通过不换位双回三相输电线路算例,验证了新算法的有效性.在此基础上,利用消除突变点的频率相关转换矩阵分别计算特征导纳矩阵和传播矩阵,通过对比分析,近一步阐明了频率相关转换矩阵中元素的突变点对特征导纳矩阵连续性具有较大影响,而对传播矩阵连续性的影响很小.      

Advance of interplanetary physics study in China: 2008—2010

Interplanetary physics study is an important ingredient in space weather research. Considerable progress this aspect has been achieved by the space physics community of China in recent years. This brief report summarizes the latest advances of the interplanetary physics research in China during the period of 2008--2010. This report includes solar corona and solar wind, interplanetary transients, energetic particles, MHD simulation, space plasma, and prediction methods for physical phenomena originating from both solar corona and interplanetary space.      

Effects of UV-B radiation on photosynthesis activity of Wolffia arrhiza as probed by chlorophyll fluorescence transients

The higher plant Wolffia arrhiza is regarded to be well suited concerning the provision of photosynthetic products in the cycle of matter of a Controlled Ecological Life Support System (CELSS) to be established in the context of extraterrestrial, human-based colonization and long-term space flight. Since UV radiation is one major extraterrestrial environmental stress for growth of any plant, effects of UV-B radiation on W. arrhiza were assessed in the present study. We found that UV-B radiation significantly inhibited photosynthetic CO₂ assimilation activity, and the contents of chlorophyll a, chlorophyll b (Chl a, Chl b) and carotenoids considerably decreased when plants were exposed to UV-B radiation for 12 h. High UV-B radiation also declined the quantum yield of primary photochemistry (φ_po), the quantum yield for electron transport (φ_Eo) and the efficiency per trapped excitation (Ψ_o) in W. arrhiza simultaneously, while the amount of active PSII reaction centers per excited cross section (RC/CS) and the total number of active reaction centers per absorption (RC/ABS) had comparative changes. These results indicate that the effects of UV-B radiation on photosynthesis of W. arrhiza is due to an inhibition of the electron transport and via inactivation of reaction centers, but the inhibition may take place at more than one site in the photosynthetic apparatus.     

一种供电特性试验设备的实现方法

随着航空电子技术的发展,实现对航空电子设备供电特性的自动化检测就变得日益重要。介绍了一种在实验室环境下实现供电特性试验自动化测试的方法。根据国内外现行的相关测试标准对机载电子设备的供电特性测试要求,以及实验室原有电源测试设备,从硬件结构和软件程序两方面进行了分析;并进行硬件改造、软件升级,设计了输出管理部件、增加了高精度可控源、更改了部分测试程序,实现了输入浪涌、输入瞬变等测试功能,从而完成机载电子设备的供电特性试验。     

SLX 1746-311 in outburst

We report on RXTE-PCA observations of SLX 1746-311 during a 100 day outburst in April 2003. We present the 3–20 keV PCA energy spectra of the source and study evolution of spectral parameters. The burst spectrum is soft with T_in 1.3 keV at the beginning of the outburst. There is a clear evidence of a hard power law component throughout the outburst. There is also an indication of a broad iron line. The source exhibits three state transitions with considerable change in the hardness ratio at low count rates. We discuss the possible scenario under which this unusual behaviour can be explained.     

Black hole spectral states and physical connections

The dramatic changes seen in the X-ray spectral and timing properties of accreting black hole candidates (BHCs) provide important clues about the accretion and jet formation processes that occur in these systems. Dividing the different source behaviors into spectral states provides a framework for studying BHCs. To date, there have been three main classification schemes with Luminosity-based, Component-based, or Transition-based criteria. The canonical, Luminosity-based criteria and physical models that are based on this concept do not provide clear explanations for several phenomena, including hysteresis of spectral states and the presence of jets. I discuss the re-definitions of states, focusing on an application of the Component-based states to more than 400 RXTE observations of the recurrent BHC 4U 1630–47. We compare the X-ray properties for the recent 2002–2004 outburst to those of an earlier (1998) outburst, during which radio jets were observed. The results suggest a connection between hysteresis of states and major jet ejections, and it is possible that both of these are related to the evolution of the inner radius of the optically thick accretion disk.