用直接最佳法设计最大推力喷管型面

本文介绍一种用直接最佳法来设计最大推力喷管型面的方法。用一个二次多项式来模仿具有固定初始膨胀表面的喷管型面。多项式的系数随确定最大推力喷管型面的直接最佳法而改变。考虑三种直接最佳法:多维线坐标研究、最速下降法和牛顿法。提出结果,以便图解说明三种直接法的特点,证明二项式型面产生的推力基本上与用变分法确定的喷管型面所产生的推力是相同的。     

全息照相无损材料检验法

全息照相干涉测试法,是检验材料的极好方法。它可以采用双重曝光技术,或者也可采用“实时”干涉成象技术。在这两种技术的应用中,使一个不受应力的测试件立体象同一个测试件在另加应力情况下的立体象重叠起来。     

视觉模拟的新途径

视觉模拟,特别是飞机起飞和着陆的关键动作的模拟,长期以来就存在要求逼真度的问题,而且随着在低能见度的极端条件下操作的新要求而极大地增长。在实际飞机上进行训练以适应这些条件不仅困难而危险,而且训练问题还受这样情况的影响,即飞机的飞行任务必须等待既出现所希望的气候条件,同时空域又正好是可用的那种综合情况。飞机训练中人员的危险和钱财的耗费随着更复杂的兵器设备,新一代的大型喷气运输机,以及不久将来采用的超音速运输机的出现也极大地增加。模拟工业许多年来一直在为视觉问题而奋斗,同时由于大型数字计算机的应用,地面模拟器的其它方面已达到惊人的逼真性。实际结果是感觉信号模拟逼真度显著地落后于仪表飞行模拟。本文叙述模拟工业所采取的用以解决这个问题,并提供必要的训练价值的各种途径,。由于理想的系统并不存在,文中叙述了各种途径的限制,并详细地叙述了必须采取的折衷办法。这个问题的一个新途径是利用有限空中走廊模拟的基本特点,实行有限自由度飞行动作的折衷办法,提供优良的图象质量。这种方法应用电影胶片作为数据库,仔细地避免了现代电视质量较低的问题,这样做法,看来为供给训练中最关键的飞行动作部分的一切必需的感觉信号提供唯一的可能性。     

计及盘与叶片的变形时涡轮机轴临界转速的计算

高速转轴临界转速的理论研究以及涡轮机轴的实陈计算,都以下面两个假设之一作为基础的:或者以点质量来代替盘,或者将盘与固定于盘上的叶片认为是绝对刚体,而其直径惯性矩则等于静止状态下的惯性矩。 无论是第一种假设还是第二种假设,一般都不是精确的,当轴作正协调进动的转动     

VISIOMETRICS OF 2D SHOCK-PLANAR S/F/S CURTAIN INTERACTIONS: VORTEX DOUBLE LAYERS, VORTEX PROJECTILES AND DECAYING STRATIFIED TURBULENCE

INTRODUCTIONVarious geometrical configurations havebeen used to obtain an understanding of phenom-ena in accelerated inhomogeneous flows( aifs) ,e.g. Richtmyer- Meshkov ( RM) and Rayleigh-Taylor( RT) flows,where visiometrics are beingemphasized more and more by the community[1] .The classical configuration,an acceleration orimpulse directed perpendicular to a planar inter-face between fluids of different density perturbedby a small- amplitude sinusoid has attracted muchattention for evo…     

Coronal mass ejection (CME) activity of low mass M stars as an important factor for the habitability of terrestrial exoplanets. II. CME-induced ion pick up of Earth-like exoplanets in close-in habitable zones

Atmospheric erosion of CO2-rich Earth-size exoplanets due to coronal mass ejection (CME)-induced ion pick up within close-in habitable zones of active M-type dwarf stars is investigated. Since M stars are active at the X-ray and extreme ultraviolet radiation (XUV) wave-lengths over long periods of time, we have applied a thermal balance model at various XUV flux input values for simulating the thermospheric heating by photodissociation and ionization processes due to exothermic chemical reactions and cooling by the CO2 infrared radiation in the 15 microm band. Our study shows that intense XUV radiation of active M stars results in atmospheric expansion and extended exospheres. Using thermospheric neutral and ion densities calculated for various XUV fluxes, we applied a numerical test particle model for simulation of atmospheric ion pick up loss from an extended exosphere arising from its interaction with expected minimum and maximum CME plasma flows. Our results indicate that the Earth-like exoplanets that have no, or weak, magnetic moments may lose tens to hundreds of bars of atmospheric pressure, or even their whole atmospheres due to the CME-induced O ion pick up at orbital distances 相似文献   

Superlow-Frequency MHD-Eigenoscillations With a Discrete Spectrum in Parabolic Model of Magnetosphere

A new concept of the global magnetospheric resonator is suggested for fast magnetosonic waves in which the role of the resonator is played by the near part of the plasma sheet. It is shown that the magnetosonic wave is confined in this region of the magnetosphere throughout its boundaries. The representative value of the resonator's eigenfrequency estimated at f ≈ 1 mHz is in good agreement with observational data on ultraThe theory explains the ground-based localization of the oscillations observed in the midnight-morning sector of the high-latitude magnetosphere.      

A Mechanism of Solar Variability Effect on Radiative Balance of the Earth Atmosphere

Possible mechanisms of solar-climatic connections, which may be of importance as over short and long time intervals, are discussed. The variations of energetic balance of Earth's climatic system for the last fifty years are estimated. It is ascertained that the disbalance between the flux of solar energy that comes to the Earth and radiates to space is of 0.1% for the last ten years. The suggested mechanism makes it possible to explain not only the observed variation of the enthalpy of the Earth's climatic system for the period 1910-1980, but also the climate anomalies during last thousand years: the climate optimum in 12 century, and"small glacial period" in 16-17 centuries.      

巴尔迪克-径向铆接--满足最精确的铆接成形要求

巴尔迪克的铆接法可铆接以前被认为不可铆接的材料,并能得到完美的铆接面。材料沿径向滚动可防止产生扭应力,从而得到高质量的铆接面并具有很高的抗疲劳强度     

一种利用功率反演和线性约束最小方差算法的自适应天线

介绍了一种新的基于功率反演和线性约束最小方差的算法,以高度抑制GPS接收机的干扰信号。这种结构通过提调整天线阵列的权值,实时地接收并改变来自各方向的GPS信号,同时对不同方向的干扰信号有高的抑制比。对固定和移动的干扰都做了仿真,仿真表明这种结构有很深的零点,对固定干扰信号的抑制比可达到115dB,对移动干扰信号的抑制比可达到94dB。