含氧杂环丁烷粘合剂的先进固体推进剂

综述了国内外氧杂环丁烷粘合剂研究的新进展。介绍了ＢＡＭＯ／ＡＭＭＯ固体推进剂的配方和性能。通过与常规推进剂的比较，分析并指出ＢＡＭＯ／ＡＭＭＯ推进剂的潜在优点。     

Prompt effects of solar wind variations on the inner magnetosphere and midlatitude ionosphere

It is well known that the solar wind can significantly affect high-latitude ionospheric dynamics. However, the effects of the solar wind on the middle- and low-latitude ionosphere are much less studied. In this paper, we report observations that large perturbations in the middle- and low-latitude ionosphere are well correlated with solar wind variations. In one event, a significant (20–30%) decrease of the midlatitude ionospheric electron density over a large latitudinal range was related to a sudden drop in the solar wind pressure and a northward turning of the interplanetary magnetic field, and the density decrease became larger at lower latitudes. In another event, periodic perturbations in the dayside equatorial ionospheric E × B drift and electrojet were closely associated with variations in the interplanetary electric field. Since the solar wind is always changing with time, it can be a very important and common source of ionospheric perturbations at middle- and low-latitudes. The relationship between solar wind variations and significant ionospheric perturbations has important applications in space weather.     

混合与扩散同时进行的环形引射系统引射性能实验研究

本文设计了“混合与扩散同时进行”的环形引射系统,并结合其驱动引射式风洞,实验探讨了该系统的参数影响规律及混合特性,结果表明,引射器系统采取“同时混合扩散”方式可达到与传统的“等截面混合后再扩散”的方式相当的性能,但新方式下则大大缩短了系统结构尺寸,因而具有重要的实用意义。实验表明“同时混合扩散”方式只宜于应用在具有周向喷流特点的系统中,同时混合扩散角应与常规扩散角相当(β=6°)。研究表明,讨论喷流马赫数Ma_j对性能的影响应与面积比A_2/A_*的变化独立开来,Mα_j变化对性能的影响不超过10％,而面积比变化对性能的影响十分显著,在面积比与膨胀比适当的配合下,可获得较高的系统效率。     

等厚度楔形杆的应力分析

本文将应力场分为基本应力场和修正应力场两个部分。基本应力场的应力σ_x用勒让德级数展开,级数的前两项系数用截面法确定;其他应力τ_(xy),σ_y由平衡方程和侧表面边界条件确定;再用余能原理确定其余各项系数。由于该级数收敛很快,故可得到封闭解并能给出该解的应用范围,为精确满足自由端的静力边界条件,又引入一个从自由端到固定端迅速衰减的修正应力场,该应力场的应力在自由端等于已知外力与基本应力解之差。其确定方法与基本应力场相同,它也有一个封闭解。将以上两应力场相加卽可得到满足全部边界条件的解。     

太阳风质子束流的演化

太阳神飞船观测表明，太阳风高速流中质子束分量相对于核分量的密度随日心距离增加而增加．提出解释这一观测现象的机理并给出二维数值模拟结果．由于阿尔芬波速随日心距离增加而减少，第二支左旋波将与更多的质子共振，把部分原来属于核分布的质子拉到束分布中来．用数值模拟方程方法求解回旋波共振导致的准线性扩散方程，数值结果与观测结果相符合．     

风挡防冰表面温度场计算

在研究国内外有关资料的基础上，采用了量纲分析的方法，建立了风挡外表面温度场的计算模型。回避了对自由流与射流相互干扰这一复杂问题的研究，同时对该计算模型进行了验证，并开发了相应的计算程序。该问题的解决，填补了国内在该领域中的空白。     

采用斜坡凹槽稳焰器强化H2超燃的数值研究

用迎风TVD格式求解三维多组分体系的全N－S方程，化学反应源项采用点隐处理，H2和空气的超燃模型用11组分、23步基地反应模型描述，得到了凹槽燃烧室不同截面组元、当量比、压力、温度等值线和速度场的分.布计算结果表明：凹槽稳焰器的回流区可提供高温自由基，有助于超燃点火；火焰在凹槽内和凹槽后斜坡的尾迹中驻定。结果对定量认识凹槽H2超燃流场、设计高效率和优化结构的一体化凹槽有着重要意义。     

壁压法在非矩形风洞中的应用

 解决大攻角洞壁干扰修正的壁压法,是利用一定数量固定位置和形状的线源和线涡来模拟风洞内模型的堵塞效应和升力效应。矩形风洞实验段边界对绕模型流动的影响,可用两个方向有限层的镜像线源和线涡来代替,并利用在风洞上下壁和侧壁上测压点处测量所得     

Experimental Aspects of Mid-Frequency Pulsations (f≈10–100 mHz) in the Southern Polar Cap

We review the results obtained in the frequency range of Pc3 (22-100 mHz) and Pc4 (7-22 mHz) pulsations at Italian Antarctic stations in the southern polar cap (“Mario Zucchelli”, at Terra Nova Bay, TNB, 80^˚.S; “Concordia”, the Italian/French base at Dome C, DMC, 89^˚.S). The absence of a midnight enhancement in the pulsation power suggests a negligible substorm influence at extreme latitudes, while the sharp noon enhancement, which appears only at TNB, is determined by the closer proximity of the station to cusp related phenomena. The relationship between the frequency of the band-limited signals and the interplanetary magnetic field strength, the cone angle influence, and the higher correlation of the Pc3 power with the solar wind speed in the morning hours suggest a global scenario in which upstream waves would be mainly responsible for the mid-frequency activity in the polar cap. However, the polarization pattern is odd with respect to the predictions for tailward propagating modes.     

翼型风洞侧壁干扰的数值模拟研究

运用Navier-Stokes数值模拟对翼型模拟试验对风洞侧壁干扰进行模拟，将简单代数湍流模型扩展用于机翼／风洞侧壁结合区流动，分析了风洞实验侧壁干扰问题的形成机理和影响翼型实验侧壁干扰的各种因素，如翼型展长、风洞侧壁边界层厚度及侧壁边界层抽吸等，对实验结果的影响，得出了一些有用的结论。计算格式空间采用中心有限体积离散，时间采用多步Runge-Kutta时间步长格式进行积分。计算结果证明了该方法的可行性和优越性。