运载火箭整流罩内主动降噪控制技术

运载火箭整流罩内的声振环境对有效载荷的可靠性和发射任务的成败至关重要。为改善整流罩内低频声振问题，首先从数学原理上介绍了用于主动降噪(ANC)系统的自适应滤波器和通道辨识的方法;其次针对运载火箭整流罩特定情况，建立反馈式滤波最小均方值(FxLMS)-ANC系统控制模型，并在实验室环境下搭建硬件实验平台;最后针对噪声频谱分布的不同特点开展宽带、窄带、宽带与窄带组合式ANC实验。结果表明:采取ANC控制对噪声抑制效果明显，特别是对功率谱峰值所在的频点实施窄带降噪，降噪效果更为突出。实验室环境下所得的实验结论，验证了在运载火箭整流罩内ANC的潜力。     

节流水平对气液针栓喷注单元雾化特性的影响

为了分析气液针栓喷注单元雾化特性和雾化机制，采用背光成像技术和相位多普勒（PDA）系统进行试验研究，获得了雾化模式、体积流量分布、索泰尔平均直径（SMD）分布和速度场随节流水平的变化规律。结果表明：气液针栓喷注单元雾场形态为扇形雾场，雾化模式为剪切破碎。体积流量沿径向呈单峰形分布，随着节流水平降低，雾场外缘向中心收缩。SMD沿径向呈现递增规律，雾化最好的区域分布在雾场中心和两侧。SMD随节流水平增加而增大。当动量比不变时，节流水平对SMD的分布范围影响很小。针栓头部下方的中心回流区轴向尺寸随着节流水平降低而减小。     

中弧线角度分布对跨音叶栅特性影响研究

中弧线角度分布形式对压气机叶片表面等熵马赫数分布具有重要的影响。为了对比不同压气机叶型的流动特征，采用数值模拟和平面叶栅试验相结合，对两种中弧线角度分布形式的跨音叶型在不同来流工况下的气动特性展开了详细研究。结果表明：在设计点，前加载配合均匀加载的中弧线角度分布叶型能够消除叶片吸力面的局部超音区，与前加载的中弧线角度分布叶型相比，叶片表面等熵马赫数分布更加饱满。其次，前加载配合均匀加载叶型能够推迟叶片吸力面的涡层失稳，减弱了吸力面分离涡与端壁分离涡的耦合作用，进而改善了端区的流动状况，截面平均总压损失系数降低了8.2%。最后，对非设计工况下两种中弧线角度分布的气动特性进行了分析，随着来流马赫数的降低，两种中弧线角度分布叶型的损失差异逐渐减小，均具有较优的气动性能。来流速度对叶片表面等熵马赫数、损失分布和分离面形状特征影响较小，仅影响叶片表面等熵马赫数和损失数值大小。     

Cramér-rao lower bound for pulsar rotation parameters estimation with X-ray pulsar observation data

In this paper, the Cramér-Rao Lower Bound (CRLB) for estimating the rotation parameters of pulsars using X-ray pulsar observation data is deduced, and the calculation equation is presented. In order to verify the correctness of the deduced equation, we use the X-ray pulsar observation data to estimate pulsar rotation parameters, and obtain the root mean square error (RMSE) of the estimated pulsar rotation parameters through conducting repeated experiments. The experimental results suggest that when the observation time increases, the RMSE gradually approaches the estimated CRLB, and that when the observation time is 2.4 × 10⁶ s, the error between the RMSE of pulsar frequency estimation and the CRLB stays at 10^?11 order of magnitude. This verifies that the CRLB expression deduced in this paper is the theoretical lower bound for estimating pulsar rotation parameters. The deduced CRLB in this paper helps determine the minimum variance estimator for pulsar rotation parameter estimation using X-ray pulsar data, providing a benchmark for the comparison between the minimum variance estimator and other estimators.     

GGTm-Ts: A global grid model of weighted mean temperature (Tm) based on surface temperature (Ts) with two modes

With the development of Global Navigation Satellite System (GNSS), the detection of precipitable water vapor (PWV) using the GNSS atmospheric sounding technique becomes a research interest in GNSS meteorology. In the conversion of zenith tropospheric delay (ZTD) to PWV, the weighted mean temperature (Tm) plays a crucial role. Generally, the Tm estimated by the linear regression models based on surface temperature (Ts) cannot meet the requirement for global use, and the accuracy of Tm derived from the empirical models is limited. In this study, a new Tm model, named GGTm-Ts model, was developed using the global geodetic observing system (GGOS) atmosphere Tm data and European Centre for Medium-Range Weather Forecasts (ECMWF) data from 2011 to 2015. Resting upon a global 2.5°*2° grid of coefficients of Tm-Ts linear function, the new model can provide Tm at any site in two modes, one for the case with measured Ts provided, i.e., the accurate mode, the other for the case that Ts provided by a subroutine, i.e., the normal mode. The performance of GGTm-Ts model was assessed against the Bevis formula, GPT2w and GPT2wh model using different data sources in 2016-the GGOS atmosphere and radiosonde data. The results show that the GGTm-Ts model in accurate mode achieves best performance with an improvement of 46.9 %/15.3 %, 37.8 %/19.5 % and 34.4 %/14.2 % over other three models in the GGOS atmosphere/radiosonde comparison. For the normal mode, the GGTm-Ts model outperforms the GPT2w model and achieves equivalence results with the GPT2wh model. Moreover, the impact of Tm on GNSS-PWV was analyzed to validate the performance of the GGTm-Ts model.     

负电子亲和半导体的二次电子发射

根据0.8keV≤Epomax≤5keV的负电子亲和(negative electron affinity,NEA)半导体二次电子发射(secondary electron emission,SEE)的特性，初级电子产额R，现有的次级电子产额δ的通用公式和实验数据，分别推导并实验证明了NEA金刚石的δ在0.5Epomax≤Epo≤10Epomax, GaN在2keV≤Epomax≤5keV, NEA金刚石的δ在08keV≤Epo≤3keV, GaN在08keV≤Epomax≤2keV的特殊公式;其中Epomax为δ达到最大值时的Epo, Epo为初级电子入射能。推导出了08keV≤Epomax≤5keV时NEA半导体的内部二次电子到达发射极表面后逃逸到真空中的概率B。还提出了计算08keV≤Epomax≤5keV NEA半导体1/α的方法;其中1/α为二次电子的平均逃逸深度。分析结果表明，B和1/α的理论研究有助于研究不同样品制备方法对NEA半导体中SEE的定量影响，从而生产出理想的NEA发射体，如NEA金刚石。