浅析高职英语分层次教学——长沙航空职业技术学院英语教学改革个案分析

结合高职高专院校英语教学现状,以长沙航空职业技术学院为例,提出“分层次教学”是一条高职英语教学改革的特色之路,并对高职高专院校开展分层式教学进行了探讨。     

冲压发动机用轴对称进气道设计和试验

完成了一种Ma=2.5～4.0冲压发动机用超声速轴对称混合式进气道模型的设计,通过数值模拟和风洞试验,获得了马赫数Ma=2.5,3.0,3.5,4.0,攻角α=0°,3°,6°,8°条件下的超声速轴对称混合式进气道性能。试验结果表明,随着马赫数的增加,总压恢复系数大幅度下降,亚临界稳定范围变窄,流量系数逐渐增加;随着攻角的增大,总压恢复系数和流量系数总体都呈降低趋势,在Ma≥3.0,α=6°时,进气道性能的下降小于5%,亚临界稳定范围变窄。     

Possible physical properties of the flow in the vicinity of the heliopause

An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath.     

直升机旋翼回波特性建模

给出了雷达半主动寻体制的直升机旋翼回波模型,分析了直升机旋翼回波的时频特性,以旋翼真实参数对模型进行了仿真,并研究了直升机旋翼回波在时域上的调制效应及频域分布特点。结果表明：理论模型所得结果与外场实验的导引头跟踪直升机实验数据吻合。     

加强政策支持体系建设促进中部劳动力转移

在我国劳动力市场供求形势发生变化的新时期,进一步促进农村劳动力转移,中部地区既要靠继续加快工业化、城市化进程,为农村富余劳动力转移提供更多的就业岗位,更要依赖国家宏观政策的调整与经济社会管理体制的改革,建立和完善全国统一的劳动力市场体系和相应的政策支持体系。具体包括：（1）把统筹城乡就业放到经济发展战略的核心位置,促进中部农村劳动力转移;（2）创新就业制度,建立城乡统一就业、规范有序的劳动力市场;（3）深化户籍制度和土地制度改革,为农村劳动力转移就业创造良好的制度环境;（4）推行农村四项保障制度,使农村社保制度与城市社保制度逐步对接;（5）加强农村教育和培训工作,提高农村劳动力素质;（6）积极培育农村新型社会化服务组织,促进农村服务业的发展。     

卫星天线热真空环境应变测试并行试验的可行性研究

文章论述了在KM4空间环境模拟器中同时进行两个卫星天线子阵的热真空环境应变测试试验的可行性.利用该可行性研究指导试验,试验结果满足两个子阵的试验要求,证明了这种并行试验的方法可行有效.该项试验的成功进行,为空间环境试验方法开拓了一个新的思路,可以用来进行类似的并行试验.     

倾转旋翼机旋翼/机翼气动干扰的试验研究

在模型旋翼台和风洞中,针对倾转旋翼机旋翼/机翼的两个主要干扰状态(悬停和低速前飞)进行了试验,分别测量了悬停状态不同机翼安装角和旋翼总距角、前飞状态不同机翼安装角和吹风速度等试验条件下的倾转旋翼拉力、扭矩以及机翼上下表面压力分布,并对试验结果进行了分析,得出了一些有意义的结论,为进一步研究倾转旋翼机旋翼/机翼气动干扰的特性问题做了些探索性的工作.     

Mesospheric doppler wind measurements from Aura Microwave Limb Sounder (MLS)

This paper describes a microwave limb technique for measuring Doppler wind in the Earth’s mesosphere. The research algorithm has been applied to Aura Microwave Limb Sounder (MLS) 118.75 GHz measurements where the O₂ Zeeman lines are resolved by a digital autocorrelation spectrometer. A precision of ∼17 m/s for the line-of-sight (LOS) wind is achieved at 80–92 km, which corresponds to radiometric noise during 1/6 s integration time. The LOS winds from Aura MLS are mostly in the meridional direction at low- and mid-latitudes with vertical resolution of ∼8 km. This microwave Doppler technique has potential to obtain useful winds down to ∼40 km of the Earth’s atmosphere if measurements from other MLS frequencies (near H₂O, O₃, and CO lines) are used. Initial analyses show that the MLS winds from the 118.75 GHz measurements agree well with the TIDI (Thermosphere Ionosphere Mesosphere Energetics and Dynamics Doppler Interferometer) winds for the perturbations induced by a strong quasi 2-day wave (QTDW) in January 2005. Time series of MLS winds reveal many interesting climatological and planetary wave features, including the diurnal, semidiurnal tides, and the QTDW. Interactions between the tides and the QTDW are clearly evident, indicating possible large tidal structural changes after the QTDW events dissipate.     

一种模拟整星热环境的小型单机热平衡试验

文章通过对一个典型的单机热分析和热试验的研究,提出了一种小型单机热平衡试验方法,模拟单机在整星环境下的热平衡试验,以避免只为验证其热设计而再次补做整星热平衡试验。为准确模拟单机在星内的辐射和导热过程,通过灰体间辐射热网络法和仪器安装板处单元体热平衡法,给出了等效辐射特征点和等效导热特征点的确定方法;并结合试验结果,对模型修正的合理性、局限性进行了分析,提出了在实际应用过程中应注意的问题。     

落塔微重力水平激光干涉测量方法中的干扰因素分析

落塔是获得微重力环境的重要设施,落塔微重力水平的测量对微重力科学实验的研究至关重要. 激光干涉是测量落塔微重力水平的一种新方法,这种方法的基本原理是让一个参考落体在落舱中自由下落,落舱由于受到服外空气阻力的作用将与自由落体运动略有差异,1 11. 肫内的参考落体则更接近理想的自由落体运动,这就使得落舱与参考落体之间存在着加速度差,这种加速度差便反映了落服的微重力水平,其所导致的相对运动则可通过激光干涉的方法测量出来. 本文对落塔微重力水平的激光干涉测量方法中将会遇到的一些主要干扰因素进行了分析,计算结果表明,这些干扰网素所造成的总误差约为 1.2 x 10-7g,低于微重力水平的预测值 10-4~lO-6 g,因此该方法是一种比较可行的测量方法.