The gauge-generalized Gyldén–Meshcherskii Problem

The Gyldén–Meshcherskii Problem (GMP) extends the classical two-body problem of Newton and Kepler by considering time-varying gravitating masses, an important extension of the two-body problem for modeling cometary motion and cosmological phenomena. In this paper, we consider the GMP in a specialized setup, the setup of gauge theory. We show that the variational equations, modeling the effect of the mass time variation on the orbital elements, can be derived by fixing a gauge of a particular form that is different from the Lagrange gauge. Thus, the orbital elements modeling the effect of a time-varying secondary mass are non-osculating. This implies that the trajectory of a celestial body whose mass is continuously changing cannot be approximated by a series of Keplerian orbits. Finally, we provide the first-order averaged equations written in terms of non-osculating elements.     

CISA 3D Navier—Stokes程序在压气机中的鉴别和应用

用压气机叶栅试验数据、多级压气机的第4级静子计算结果和跨声速转子试验结果对CISA 3D N-S程序的计算精度进行了鉴别研究。结果表明,该程序对设计点的落后角的计算精度较高,而对损失的计算还存在一定的分散度。采用 CISA 3D N-S程序和S_2-S_1程序对一台多级压气机试验件的第3级静子进行三维造型修改设计,取得了预期的效果。     

微小卫星平台公共总线技术——CAN网络应用

对局域控制网络(CAN)协议在“清华一号”微小卫星平台上的应用作了描述。提出了微小卫星对平台公共总线的要求,介绍了CAN网络的特点,阐述了CAN协议的帧结构,并在此基础上提出了针对卫星子系统数据通讯所作的改进协议。还给出了微小卫星星载计算机子系统的CAN节点硬件设计结构和软件控制流程。     

CFM56-5B发动机性能衰退评估

发动机性能衰退通常用排气温度裕度EGTM和外界大气温度限制值OATL 来衡量。本文给出了一种CFM56-5B发动机EGTM和OATL的计算方法,可以作为发动机换发的参考。     

利用单片机控制的LD驱动系统研究

介绍了一种利用单片机控制的半导体激光（LD）驱动电源，该电源通过控制LD的工作电流和温度以及采用了可靠的保护电路，实现了LD光功率稳定、可靠、准确输出。     

物证DNA分析技术的过去与现在

使用DNA指纹鉴定技术不仅可得到可靠的否定结论,还可以得到可靠的认定结论.PCR技术极大地提高了检测生物检材的灵敏度.借助芯片技术可一次性对样品大量序列进行实时、灵敏、精确地检测和分析.从第一代分析方法应用于法庭科学开始,第二、第三代分析技术的诞生以及相继应用,使个人识别及亲子鉴定的结果愈来愈精确.     

一种通过DDC接口实现的实时并行仿真系统的研究与应用

介绍一种通过ＤＤＣ接，将ＶＡＸ机与ＹＨ－Ｆ１并行实时计算，它既发挥ＹＨ－Ｆ１的快速性，又利用ＶＡＸ机高精度优势，从而使复杂的战术导弹闭合回路实时仿真精度有很大提高。     

Transient outburst mechanisms in Supergiant Fast X-ray Transients

The recent discovery of a new class of recurrent and fast X-ray transient sources, the Supergiant Fast X-ray Transients, poses interesting questions on the possible mechanisms responsible for their transient X-ray emission. The association with blue supergiants, the spectral properties similar to those of accreting pulsars and the detection, in a few cases, of X-ray pulsations, confirm that these transients are High Mass X-ray Binaries. I review the different mechanisms proposed to explain their transient outbursts and the link to persistent wind accretors. I discuss the different models in light of the new observational results coming from an on-going monitoring campaign of four Supergiant Fast X-ray Transients with Swift.