环境因子的分析及应用

本文通过对现行指数分布环境因子的分析，得出了两种环境条件下，产品参数随机变量之间的线性关系，进而对典型正态分布的环境因子的分析，提出了环境因子的二因子法，指出其普遍适用性，给出了应用环境因子对试验数据进行综合的一般步骤，且以实例予以说明。     

Infrared radiation from compact X-ray sources

Observations of the X-ray binaries 4U 0115+634 and A 0535+262 performed in 1981 – 1982 revealed significant IR variabilities of these sources. 4U 0115+634 was observed twice, in the state close to X-ray activity, and in the state of low activity, thus changing from K = 7^m.75 to K > 9^m. A 0535+262 shows the temporal variations ranged from tens minutes to some days. The regular variations of IR brightness are suspected with teh period close to 104 s that corresponds to the period of axial rotation of neutron star in A 0535+262. The results obtained present arguments in favour of hypothesis that IR radiation is generated near the accreting neutron star and is possibly of maser nature.     

黄道面内行星际激波相互碰撞作用过程研究—间距效应

本文用两维半MHD数值模型,模拟研究了不同间距的两扰动源所产生的激波在行星际空间黄道面内的相互碰撞过程。在内边界(18R_s),两扰动中心的间距取为24°、36°、48°、54°、72°、120°,模拟了两激波速度均为1000km/s和2000km/s两种情形。结果表明:1.速度为1000km/s的两中等激波,相距24°时,在1AU以内强烈相互作用而汇合成一新激波;相距36°时,在1AU附近发生汇合,但尚可分辨;相距48°时,在1AU以内有相互作用,但可近似认为是独立传播的;相距72°时,将独立向前传播。2.速眨为2000km/s的两强激波,相距≤48°时,将强烈汇合成一新激波;相距54°时,在1AU附近产生汇合,但尚可分辨;相距72°时,相互作用不足以汇合成新的激波;相距120°时,其传播相互独立地进行。并给出了上述情形下两激波汇合的时间和位置,详细比较了汇合激波与相同能量的单激波的等离子体特性。     

Supersoft X-ray sources

More than 100 supersoft X-ray sources (SSS) are reported in 20 external galaxies, the Magellanic Clouds (MCs) and our Galaxy. The effective temperatures of the brighter SSS are 20–100 eV. SSS with luminosities below ≈3 × 10³⁸ erg s⁻¹ are consistent with accreting white dwarfs (WDs) with steady nuclear burning or post-novae. Optical identifications exist for SSS in our Galaxy and the MCs (including orbital period determinations) and for SSS in M31 (with novae and symbiotic stars, SySs). High resolution X-ray spectra of the brightest SSS in our Galaxy and the MCs reveal the existence of spectral features due to high gravity WDs. Timing studies in X-rays (combined with the optical) of the stable nuclear burning phase in steady nuclear burning sources and in post-novae allow to constrain the mass accretion rate onto and the mass of the nuclear burning WD. The nature of a few SSS with luminosities 10³⁹ erg s⁻¹ remains unclear.     

过载状态下固体火箭发动机燃烧室内二相流动数值模拟

对过载状态下固体火箭发动机燃烧室内二相流动进行了数值研究，建立了过载状态下二维平面颗粒轨道模型，应用二阶迎风格式构造了有限体积计算框架，对有过载和无过载多种工况燃烧室内流动进行了计算，得出过载对颗粒相和气相的某些影响，结果对于发动机工作过程研究及发动机热结构设计具有一定指导意义。     

The beginning of cosmic ray astrophysics

A short history of the beginning of cosmic ray (CR) astrophysics is considered: from the hypothesis on CR origin as a result of Supernova explosions in the Metagalaxy, to a model of solar origin of CR, galactic origin based on the stochastic mechanism of charged particle acceleration in interstellar space, to extragalactic and hierarchical models of CR origin, as well as galactic CR origin taking into account radio-astronomical data. We consider also the first balloon results on the chemical contents of primary CR (especially of the contents Li, Be, B), important for any model of CR origin. Investigations of the injection problem, CR drift and diffusion acceleration by shock waves, and CR generation in Supernova remnants were also important steps in the beginning of CR astrophysics.     

轮胎参数对双轮式起落架刹车耦合振动影响研究

目前对飞机起落架低频刹车耦合振动问题的研究主要停留在考虑轮胎参数影响的起落架纵向单自由度振动特性分析，对于多自由度低频刹车耦合振动的特性研究不足。基于Simcenter 3D 动力学分析软件建立双轮支柱式起落架刚柔耦合整机滑跑刹车分析模型，研究轮胎竖向刚度和侧偏刚度对双轮支柱式起落架低频刹车纵向、横向和扭转的多自由度耦合振动的影响。结果表明：轮胎的竖向刚度对起落架横向和扭转方向上的振动影响较大，轮胎竖向刚度变化33%，横向和扭转方向上的振动变化5% 左右；轮胎的侧偏刚度对起落架低频刹车横向上的振动影响较大，轮胎侧偏刚度变化33%，横向上的振动变化15% 左右。     

新型太阳能利用装置的研究

对目前太阳能的几种常见的应用领域及相关装置进行了分析和研究,并在此基础上,结合相关理论,设计了利用太阳能的新型装置,如:太阳能房、太阳能热发电装置、聚光式太阳能电池发电装置等,这些装置将为更好地利用太阳能开辟新的途径.太阳能作为一种新兴的可再生能源有着不可限量的发展前景.     

气泡雾化喷嘴水平喷射的雾化特性研究

研究了水平喷射、端面注气方式的气泡雾化喷嘴结构及工作参数对雾化及流场特性的影响.试验全部在常温常压下进行,液体采用水,雾化气为压缩空气.用2D PDA测量了液雾的平均直径尺寸分布和速度分布.液体喷射压力变化范围200~600 kPa,气液比变化范围4%~10%左右.试验研究了端面注气方式下,注气孔孔径及数目、混合管长度、液体流动状态及工作参数对雾化特性的影响.结果表明,水平喷射的气泡喷嘴,注气孔的尺寸及数目均对雾化特性产生影响;混合段存在一最佳值范围,在此范围内,喷嘴可获得高的雾化质量;液体旋转流动对雾化特性无显著影响,但可影响两相流动中气泡的分布.     

隐身飞行器电磁散射特性分析

为对隐身飞行器的探测手段进行研究和指导隐身飞行器的研制,研究其电磁散射特性。采用外形逆向建模、理论预估和散射测量、强散射源减缩相结合的手段,对隐身飞行器的隐身性能进行预估。该方法具有精度高、速度快的优点,适合在隐身飞行器研制方案设计阶段使用。