埋入式进气道流场控制研究

针对埋入式进气道总压恢复系统数低、畸变大的特点,提出了利用扰流器对埋入式进气道进行流场控制的方案。通过吹风实验,分析了扰流器的轴向位置、长度、高度、安装角、数目等对埋入式进气道性能的影响。研究结果表明,提出的流场控制方案可以大幅度提高进气道总压恢复和降低流场畸变,总压恢复σ可提高 3.5%以上,流场畸变指数 Δσ可降低 5.4 2 %以上,使埋入式进气道的性能达到可应用的水平,为埋入式进气道流场控制提供理论和设计依据。     

飞机供电系统自动化仿真技术

飞机供电系统是现代飞机核心组成部分之一,其性能和可靠性对飞机安全至关重要,仿真方法为高品质飞机供电系统设计提供了重要手段。传统的手动仿真方法需要耗费大量人力和时间资源,且无法完全考虑系统的复杂性和不确定性,因此无法满足飞机供电系统全面分析和评估的需求。文中提出了一种将虚拟仿真和实物系统相结合的飞机供电系统自动化仿真技术,能够提高仿真效率和准确性,且可快速、高效地评估飞机供电系统的性能,发现潜在问题,指导系统的优化与改进,对提高飞机供电系统的设计、分析和优化具有重要意义。     

非轴对称静子对压气机气动性能的影响

为降低进气畸变对压气机气动性能的影响,设计了 1种压气机非轴对称静子,并对设计方案开展数值模拟研究。仿真结果表明:在最高效率工况下,非轴对称静子能减小畸变区静叶的流动分离,缩小叶尖低密流区域,提升通道的流通能力,压气机的最高效率约增加 0.46%,此外,畸变区叶片进口气流角得到改善,在 90%叶高处的峰值气流角降低 2.5°;在近失速工况下,非轴对称静子能降低畸变区静叶上半叶高的扩压因子,缩小分离范围,虽略微恶化了叶根区域流场,但压气机整体气动性能与流通能力有所提升,能够在更低的流量下工作,稳定裕度增加 31.5%。     

压力、温度组合畸变对某发动机影响的数值研究

本文给出了组合畸变的描述参数,详细地计算和分析了组合畸变对某发动机稳定性的影响,讨论和分析了在不同组合相位和畸变强度下的影响情况。计算结果表明:当压力和温度畸变相位完全重合时,压缩系统中将产生最大的稳定裕度损失;如果适当调整压力与温度的组合畸变相位,一种畸变可能削弱另一种畸变,实际上可增加稳定裕度。     

适合机动飞行的旋翼气动模型研究

为改善对旋翼空气动力他轴响应的预测,在旋翼气动模型中引入时变的尾迹弯曲参数K_R,以体现机动旋翼的尾迹畸变效应.与已有方法相比,该模型的计算结果更为接近实验数据.还建立了动态尾迹畸变模型,并分析了计入尾迹收缩效应的必要性.结果表明,为了正确计算机动飞行中的旋翼气动力,特别是操纵的他轴响应,应当在模型中采用随状态变化的尾迹弯曲参数K_R.      

Monitoring of maize lodging using multi-temporal Sentinel-1 SAR data

Lodging is a common phenomenon in maize production, which seriously affects its yield, quality, and mechanical harvesting capacity. With good penetrating power, satellite radar can monitor crop growth even under cloudy weather conditions. In this study, a method based on the change in plant height before and after lodging in maize is proposed to calculate the lodging angle and monitor the lodging degree by using dual-polarization Sentinel-1A data. The results show that the optimal sensitive polarization combinations of maize plant height before and after lodging are VH/VV and VV, respectively. The lodging angle is calculated using the plant height inversion results before and after lodging. The overall accuracy of classifying lodging grade of maize is 67%. The proposed model based on lodging angle could effectively mapped the maize lodging range on a regional scale and classify the lodging grades.     

Correction model of BDS satellite-induced code bias and its impact on precise point positioning

There are code biases on the pseudo-range observations of the Beidou Navigation Satellite System (BDS) that range in size from several decimeters to larger than one meter. These biases can be divided into two categories, which are the code biases in the pseudo-range observations of Inclined Geo-Synchronous Orbit (IGSO) satellites and Medium Earth Orbit (MEO) satellites and the code biases in the pseudo-range observations of Geosynchronous Earth Orbit (GEO) satellites. In view of the code bias of the IGSO/MEO satellites, the code bias correction model is established using the weighted least square curve fitting method. After the correction, the code biases of the IGSO and MEO satellites are clearly mitigated. A methodology of correcting GEO code bias is proposed based on the empirical mode decomposition (EMD)-wavelet transform (WT) coupled model. The accuracies of the GEO multipath combination of the B1, B2 and B3 frequencies are improved by 39.9%, 17.9%, and 29.4%, respectively. Based on the corrections above, the ten days observations of three Multi-GNSS Experiment (MGEX) stations are processed. The results indicate that the convergence time of the precise point positioning (PPP) can be improved remarkably by applying a code bias. The mean convergence time can be improved by 14.67% after the IGSO/MEO code bias correction. By applying the GEO code bias, the mean convergence time can be further improved by 17.42%.     

GOCE star tracker attitude quaternion calibration and combination

We analyse the inter-boresight angles (IBA) measured by the star trackers on board the GOCE satellite and find that they exhibit small offsets of 7–9″ with respect to the ones calculated from the rotation of the star tracker reference frames to the satellite reference frame. Further, we find small variations in the offsets with a peak-to-peak amplitude of up to 8″, which correlate with variations of the star trackers’ temperatures. Motivated by these findings, we present a method for combining the attitude quaternions measured by two or more star trackers that includes an estimation of relative attitude offsets between star trackers as a linear function of temperature. The method was used to correct and combine the star tracker attitude quaternions within the reprocessing of GOCE data performed in 2018. We demonstrate that the IBA calculated from the corrected star tracker attitude quaternions show no significant offsets with respect to the reference frame information. Finally, we show that neglecting the star tracker attitude offsets in the processing would result in perturbations in the gravity gradients that are visible at frequencies below 2?mHz and have a magnitude of up to 90?mE. The presented method avoids such perturbations to a large extent.     

Combination methods of tropospheric time series

In this article we present two methods for combination of different Global Navigation Satellite Systems (GNSS) Zenith Total Delay (ZTD) time-series for the same GNSS site, but from different producers or different processing setups. One method has been setup at ASI/CGS, the other at KNMI. Using Near Real-Time (NRT) ZTD data covering 1 year from the E-GVAP project, the performance of the two methods is inter-compared and validation is made against a combined ZTD solution from EUREF, based on post-processed ZTDs. Further, validation of the ASI combined solutions is made against independent ZTDs derived from radiosonde, Numerical Weather Prediction (NWP) model and Very Long Baseline Interferometry (VLBI) ZTD.     

威海天文台1米望远镜天体测量试验

利用威海天文台1米望远镜观测了2009年10月7日晚的疏散星团M39.观测过程中使用了I滤光片,并将CCD绕光轴旋转90°分别成像.使用最新的UCAC3星表和Platais的自行星表归算表明,该望远镜具有良好的天体测量性能,最好的单次位置测量精度达到了4～5 milli-arcsec.此外,观测资料还发现UCAC3星表具有明显的自行不准确性,证实了文献[14]的最新发现.