层合双曲率厚壳的状态方程及其半解析法

采用正交曲线坐标导出了角铺设层合双曲率厚壳的状态方程及其半解析法。该方法在α－β曲面内采用通常的有限元离散,而沿壳厚（ｒ）方向采用状态空间法给出解析解,从而计入了剪切效应的影响,且通过状态转移矩阵的建立,保证了层界面之间层间位移和应力的连续,减少了计算中未知量数目。     

高负荷跨音速复合气冷涡轮叶片的设计与计算

本文提出了一套跨音速复合式气冷涡轮叶片内冷气流量分配、温增、内外换热系数和温度场的计算方法 ,对设计的“冲击 -对流 -气膜”多种冷却方案进行了计算。与实测值比较 ,验证了本计算方法的可靠性和精确度 ,择优选取了四套叶片内冷结构 ,精心地进行了结构设计     

导流板对25°倾角Ahmed类车体尾流与气动阻力的影响

在雷诺数8．7×10^5的条件下,运用眼镜蛇探针、压力扫描阀和表面油膜流动可视化技术对倾角为25°的Ahmed类车体尾流与尾部压力分布进行了研究。对比了模型尾部斜面上边缘和两侧不同宽度导流板对模型尾流与气动阻力的影响规律。实验发现模型尾流中存在一对对称的拖曳涡,其在尾流中心线附近形成强烈的下扫流。拖曳涡强度与模型尾部压力分布和气动阻力有直接关系,较强的拖曳涡对应的模型尾部负压以及气动阻力均较大。斜面两侧导流板宽度为1％模型长度时,不仅无减阻效果,反而会使气动阻力增加约3．0％。当导流板宽度增加为2％和3％模型长度时,能够明显削弱斜面上的分离泡,对应的减阻效果分别为3．5％和7．2％。斜面上边缘导流板可有效地抑制分离流在斜面上的再附,并消除斜面上的分离泡,其抑制拖曳涡强度和降低气动阻力的效果明显优于同等宽度的斜面两侧导流板。上边缘导流板宽度为模型长度的1％,2％和3％时,减阻率分别可达9．3％,10．7％和10．9％。     

基于非结构动网格的非定常激波装配法

从ALE方程出发,通过修正体积的新思路构建离散几何守恒律,基于非结构动网格的信息传递方法得到网格重构以后新网格的流场参数,采用一阶格式捕捉法得到的流场确定装配法的初始激波位置,成功地把激波装配法应用到非定常流动的模拟。模拟超声速飞行环境下整流罩分离的非定常流固耦合过程,在马赫数6条件下装配法和捕捉法的计算结果完全一致,随着马赫数增加,二阶精度格式的捕捉法需要进行调整限制器参数、时间步长等人工干预,但是装配法直到马赫数20计算过程没有出现异常。该基于非结构动网格技术的激波装配方法,与传统的激波装配方法相比,能够用于复杂外形产生的非规则形状激波和非定常流动产生的运动激波,解决二阶精度有限体积法用于高马赫数飞行条件下多体分离过程的流动模拟时遇到的稳定性问题。     

双排叉排孔气膜冷却特性研究 (二) 绝热有效温比

本文介绍双排叉排孔气膜冷却绝热有效温比η的测量结果和数值计算。根据η沿主流和横向的变化, 特别是在近孔区的分布规律分析了前后排孔二次射流的不同流动特点。数值计算采用求解椭圆方程的三维差分程序, 吹风比M等于0.6。      

低信噪比情况下识别模态参数的时域平均方法

 <正> 1.引官 模态参数识别方法在应用中需要解决的一个重要问题是观测噪声的干扰问题。为了有效地抑制观测噪声的影响,各种时域参数识别方法普遍引入了估计方法,以ITDM为代表的利用脉冲响应包括对脉冲激励的响应和脉冲响应函数)识别模态参数的识别方法还引入了噪声模态     

非系统RS码的删／错译码算法

研究了非系统RS码的删/错译码算法。详细阐明了删/错译码原理,推导了各步的计算公式。该算法特别适用于干扰严重的组合信道中级连RS码的译码。     

BDS-3 PPP模糊度固定实现及精度评估

精密单点定位(PPP)模糊度固定(AR)能够显著提升精密定位的收敛速度和精度。通过在BDS-2和BDS-3之间添加系统间偏差的方法实现BDS-3的模糊度固定,并基于全球MGEX测站静态、仿动态数据和车载实验数据全面评估了BDS-3模糊度固定的效果。结果表明,相对于浮点解,BDS-3 PPP模糊度固定能够显著提升PPP的精度,在东北天3个方向上静态解算精度提升依次为37.4%、26.2%和20.1%;仿动态解算精度提升依次为38.3%、27.2%和11.1%;车载动态实验BDS-3模糊度固定精度在三维方向上综合提升为40.4%。此外,模糊度固定后,以浮点解稳定后的两倍定位精度为基准,在东北天方向上,静态定位时间提升程度依次为63.5%、64.0%和40.3%;仿动态定位时间提升程度依次为58.7%、56.8%和25.4%;车载实验在三维方向的收敛时间为30.0 min。以上结果证明了所提方法的有效性及BDS-3模糊度固定的性能提升。     

Analysis of the brightness temperature features of the lunar surface using 37 GHz channel data from the Chang'E-2 microwave radiometer

Compared with other remote observations, brightness temperatures (T_B) derived from microwave emission measurements provide a unique means to characterize the physical properties of the lunar surface. Using Chang’E-2 microwave radiometer data, we produced 12 global T_B images of the lunar surface during a diurnal cycle with different local times separated by approximately 2?h. There are two types of remarkable T_B units on the lunar surface, the “hot regions” occurring during the lunar day in the lunar Maria regions and the “microwave cold spots” occurring during the nighttime typically related to young craters. Compared with their surroundings, the hot regions are much warmer during the lunar day and slightly colder at night, while the microwave cold spots are much colder during the lunar night and slightly warmer in the daytime. Moreover, the T_B heating and cooling rates of these two units are larger than others at the same average latitude where they are located during the lunar day, especially after sunrise and before sunset. The hot regions have a good agreement with the mare regions with high TiO₂ abundance. Besides, brightness temperatures in the lunar Maria correlate closely with their TiO₂ abundance. For most microwave cold spots, they agree with the young craters, and their brightness temperature distributions have a significant negative correlation with the lunar surface nighttime temperature and rock abundance.     

Inter-satellite calibration of FengYun 3 medium energy electron fluxes with POES electron measurements

We perform an L-shell dependent inter-satellite calibration of FengYun 3 medium energy electron measurements with POES measurements based on rough orbital conjunctions within 5?min?×?0.1?L?×?0.5 MLT. By comparing electron flux data between the U.S. Polar Orbiting Environmental Satellites (POES) and Chinese sun-synchronous satellites including FY-3B and FY-3C for a whole year of 2014, we attempt to remove less reliable data and evaluate systematic uncertainties associated with the FY-3B and FY-3C datasets, expecting to quantify the inter-satellite calibration factors for the 150–350?keV energy channel at L?=?2–7. Compared to the POES data, the FY-3B and FY-3C data generally exhibit a similar trend of electron flux variations but more or less underestimate them within a factor of 5 for the medium electron energy 150–350?keV channel. Good consistency in the flux conjunctions after the inter-calibration procedures gives us certain confidence to generalize our method to calibrate electron flux measurements from various satellite instruments.