钇对Ti-23Al-25Nb合金压缩性能的影响

采用SEM和XRD分析热处理后合金试样的显微组织及相组成,用TEM分析原始组织中钇的存在方式.结果表明,钇在原始组织中以Y2O3形式存在;钇增加O相衍射峰,提高Ti-23Al-25Nb合金压缩性能,如抗压强度、压缩率等,钇的强化作用是由于Y2O3第二相粒子强化和钇细化晶粒的晶界强化共同作用的结果.     

Partition method for improvement of piecewise linear model with full envelope covered

Since ambient conditions vary in a wide range within the full flight envelope, the existing piecewise linear model (PLM), which is based on sea-level static condition with use of corrected parameters for other points in the flight envelope, cannot meet the accuracy for replacing the nonlinear model. To obtain more accurate linear models, a method of partitioning the flight envelope over a grid of Mach number and altitude boxes was suggested. Then, a set of linear models for a given operating condition was selected by picking the nearest (Mach number, altitude) box in the flight envelope. Through the selected set of linear models, interpolating for power level based on a weighted sum of corrected rotor speeds can obtain a linear model with acceptable accuracy. Simulation results of different points within the full flight envelope showed that the maximum error between nonlinear model and the existing PLM was more than 50%, while the maximum error between nonlinear model and the improved PLM was within 8%. It is concluded that the improved PLM performs accurately, especially under the non-standard conditions. In addition, the improved PLM can satisfy the real-time requirement better than the existing PLM.      

The solar-terrestrial event of 23 February 1956

The solar flare of 23 February 1956 and the resulting geophysical disturbance ranks as one of the most remarkable solar-terrestrial events of the twentieth century. It sparked many papers and has seldom been equalled. Fifty years after the International Geophysical Year, it seems timely to review the observations of the event from today’s perspective, and to draw on the recollections of scientists who were active at the time.     

应力对DD5单晶高温合金持久过程中析出相的影响

利用扫描电镜和透射电镜研究了DD5单晶高温合金在持久性能测试过程中试样不同位置析出相的析出规律,分析了应力对析出相析出行为的影响并鉴定了两种析出相的种类。研究结果表明该合金在1 038 ℃/172 MPa条件下随着局部拉应力的增大,枝晶间和枝晶干析出相数量都明显增加;合金在871 ℃/552 MPa条件下只在枝晶间区域析出少量粒状析出相,且随拉应力的增大,析出相数量有所增加;透射电镜分析表明合金的枝晶干区域的析出相主要为μ相,枝晶间析出粒状析出相主要为M₂₃C₆碳化物相。     

降低航炮后座力的必要性及可行性

航空射击武器的后座力对其载机有诸多不利影响,因此,必须设法减小这些影响。本文就JL8飞机航炮后座力过大对飞机的不利影响进行了分析,阐述了降低航炮后座力的必要性。同时还就如何解决航炮后座力过大问题进行了研究,提出了降低JL8飞机所装23－2航炮后座力的方法。     

稀土对高纯超高强度23CoNi钢组织与性能影响的初步探索

在23CoNi钢中添加稀土可改善δ5和ψ,抗拉强度σb和冲击值aku略有提高,而对KIC和σ0.2影响较小.添加稀土后钢中形成含S和Al稀土化合物.研究表明,稀土可阻碍钢的晶粒长大,并能细化板条马氏体的板条尺寸.     

XM23胶的单轴拉伸试验及超弹性本构模型构建

文摘XM23胶广泛应用于航天光学遥感器,用于粘接光学透镜与金属结构件,可以起到减振作用。目前对XM23胶的力学性能的研究都是基于线弹性理论,但XM23胶是一种高聚合物,表现出非线性特征,无法使用线弹性材料的杨氏模量和泊松比进行准确地表征。本文首先通过XM23胶的单轴拉伸试验测试出该胶的应力应变数据,基于超弹性理论,尝试运用3种超弹性本构模型进行数据拟合。分析发现,Mooney-Rivlin 3参数本构模型最适于表征XM23胶的力学性能,其本构模型材料参数C₁₀为-0.205 9 MPa、C₀₁为0.688 8 MPa、C₁₁为0.055 7 MPa。利用此本构模型使用有限元软件模拟了该胶的单轴拉伸试验,仿真得到应力应变数据在误差范围内与试验数据一致。XM23胶的超弹性本构模型构建为XM23胶的胶接结构有限元建模提供了理论和数据支撑。     

Comparison of GPS TEC measurements with IRI-2007 TEC prediction over the Kenyan region during the descending phase of solar cycle 23

This paper presents an analysis of the Total Electron Content (TEC) derived from the International GNSS Service receiver (formerly IGS) at Malindi (2.9°S, 40.1°E), Kenya for the periods 2004–2006 during the declining phase of solar cycle 23. The diurnal, monthly and seasonal variations of the TEC are compared with TEC from the latest International Reference Ionosphere model (IRI-2007). The GPS–TEC exhibits features such as an equatorial noon time dip, semi-annual variations, Equatorial Ionization Anomaly and day-to-day variability. The lowest GPS–TEC values are observed near the June solstice and September equinox whereas largest values are observed near the March equinox and December solstice. The mean GPS–TEC values show a minimum at 03:00 UT and a peak value at about 10:00 UT. These results are compared with the TEC derived from IRI-2007 using the NeQuick option for the topside electron density (IRI–TEC). Seasonal mean hourly averages show that IRI-2007 model TEC values are too high for all the seasons. The high prediction primarily occur during daytime hours till around midnight hours local time for all the seasons, with the highest percentage deviation in TEC of more 90% seen in September equinox and lowest percentage deviation in TEC of less than 20% seen in March equinox. Unlike the GPS–TEC, the IRI–TEC does not respond to geomagnetic storms and does overestimate TEC during the recovery phase of the storm. While the modeled and observed data do correlate so well, we note that IRI-2007 model is strongly overestimating the equatorial ion fountain effect during the descending phase of solar cycle, and this could be the reason for the very high TEC estimations.     

CCAR23部飞机HIRF防护适航验证方法研究

民用飞机为获得在高强辐射场环境中的运营许可,必须按照适航当局发布的高能电磁辐射场( HIRF )防护相关适航条款进行防护设计和适航验证。当前确定航空器内部 HIRF 环境主要通过试验方法和相似性评估法,具有工作量大、测试成本高等缺点。针对仅有 A 类显示系统的 CCAR23 部飞机首次使用数据推算方法,确定飞机内部 HIRF 环境电平,用于实现整机的 HIRF 防护适航验证;提出一套适用于 CCAR23 部飞机 HIRF防护适航验证的方法,分析该方法的关键技术及可行性。本文所提出的方法已应用于 Y12F 飞机 HIRF 防护适航验证的实际工程,有效降低了整机 HIRF 防护适航验证的复杂程度,节约了整机试验所需的测试成本,提高了试验效率,为民用航空器 HIRF 防护验证提供参考。     

稀土Y对Ti-23Al-25Nb合金显微组织的影响

采用OM,XRD,XRF,SEM,EPMA,TEM等分析手段研究了稀土Y对Ti-23Al-25Nb合金显微组织的影响.结果表明:两种合金铸态显微组织均为O相;稀土Y明显细化了Ti-23Al-25Nb合金晶粒尺寸,Ti-23Al-25Nb合金的晶粒尺寸在400～600μm之间,Ti-23Al-25Nb-0.36Y合金的晶粒尺寸在40～100μm之间,细化大约6～8倍.通过Ti-23Al-25Nb-0.36Y合金背散射、各元素线分布和TEM分析发现,稀土Y在Ti-23Al-25Nb合金中以Y2O3的形式存在于晶内和晶界,根据O相形成机制和晶粒细化理论,分析了稀土Y细化O相晶粒的过程.