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This paper presents an auto-tuning method for a proportion plus integral(PI) controller for permanent magnet synchronous motor(PMSM) drives, which is supposed to be embedded in electro-mechanical actuator(EMA) control module in aircraft. The method, based on a relay feedback with variable delay time, explores different critical points of the system frequency response.The Nyquist points of the plant can then be derived from the delay time and filter time constant.The coefficients of the PI controller can then be obtained by calculation while shifting the Nyquist point to a specific position to obtain the required phase margin. The major advantage of the autotuning method is that it can provide a series of tuning results for different system bandwidths and damping ratios, corresponding to the specification for delay time and phase margin. Simulation and experimental results for the PMSM controller verify the performance of both the current loop and the speed loop auto-tuning. 相似文献
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航空零件生产调度时,应尽量满足多目标和实时性的要求。结合某航空制造企业的实际生产情况,提出一种基于"穷尽成对比较"技术和改进匈牙利算法的动态调度方法。首先以航空零件调度时的最大完工时间、生产加工成本以及生产能耗为优化目标,构建柔性作业车间多目标动态调度数学模型;然后利用基于"穷尽成对比较"技术的权重参数调节模型对数学模型中各个目标的权重参数进行实时动态调整;最后以各个目标的加权值为总目标,采用改进匈牙利算法求得工序的最优分配结果。结果表明:与传统的动态调度方法相比,动态调度方法能够有效地提高航空企业的生产效率、减少航空企业的生产加工成本并降低对环境的污染,具有较好的综合调度性能。 相似文献
146.
本文利用常规天气图、探空图和三维中尺度模式,对大连机场2011年6月29日到7月3日出现的连续4天的大雾低云天气进行分析,发现此次大雾低云过程发生同副热带高压的位置和强度变化密不可分:副热带高压中高层的下沉逆温对大雾低云天气的低层稳定层的产生和维持起到重要作用;同时它的西进北抬和东撤南退直接导致大连机场上游天气系统三次槽线东移,进而影响本场。近地面层的水汽辐合和弱冷暖气流交汇为大雾低云天气得以维持提供良好的水汽条件。 相似文献
147.
Jia Luo Fangfang Sun Xiaohua Xu Han Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):327-336
In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed. 相似文献
148.
Mukul Kumar Wang Chi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):640-652
We study the Propagation and damping properties of Alfvén gravity waves in the presence of the vertical magnetic field in the viscous solar plasma under influence of the background flow by deriving a fourth order dispersion relation in terms of the Doppler shifted frequency. We derive the dispersion relation under WKB and Boussinesq approximation. We study the damping of Alfvén gravity waves for the wave frequencies less than and greater than the Brunt-Väisälä frequency. We find that the Brunt-Väisälä frequency divides the frequency ranges where the weakly or strongly damped oscillations occur. The background flow exhibits a strong effect on weakly damped oscillations and a weak effect on the strongly damped oscillations. We also notice that the damping of both the strong and weakly damped oscillations depend on the Brunt-Väisälä frequency and wave number. The effect of the background flow is also being governed by the Brunt-Väisälä frequency and wave number. We also study the properties of gravity wave mode after filtering the Alfvén wave mode by minimizing the magnetic field and noticed that the background flow shows a very strong effect on the gravity wave mode. 相似文献
149.
Xingyuan Yan Guanwen Huang Qin Zhang Chenchen Liu Le Wang Zhiwei Qin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1270-1279
Eight new-generation BeiDou satellites (BeiDou-3) have been launched into Medium Earth Orbit (MEO), allowing for global coverage since March 2018, and they are equipped with new hydrogen atomic clocks and updated rubidium clocks. Firstly, we analyzed the signals for the carrier-to-noise-density ratio (C/N0) and pseudorange multipath (MP) by using international GNSS (Global Navigation Satellite System) Monitoring and Assessment System (iGMAS) station data, and found that B1C has a lower C/N0, and B2a has the same level of C/N0 as the B1I and B3I signals. For pseudorange multipath, compared with the BeiDou-2 satellites, the obvious systematic variation of MP scatters related to the elevation angle is greatly improved for the BeiDou-3 and BeiDou-3e satellites signals. For the signals of the BeiDou-3 satellites, the order of the Root Mean Square (RMS) values of multipath and noise is B3I?<?B1I?<?B2a?<?B1C. Then, the comparison of the precise orbit determination and clock offset determination for the BeiDou-2, BeiDou-3, and BeiDou-3 experimental (BeiDou-3e) satellites was done by using 10 stations from iGMAS. The 3D precision of the 24?h orbit overlap is 24.55, 25.61, and 23.35?cm for the BeiDou-3, BeiDou-3e, and BeiDou-2 satellites, respectively. BeiDou-3 satellite has a comparable precision to that of the BeiDou-2 satellite. For the precision of clock offset estimation, the Standard Deviation (STD) of the BeiDou-3 MEO satellite is 0.350?ns, which is an improvement of 0.042?ns over that of the BeiDou-2 MEO satellite. The stabilities of the BeiDou-3 and BeiDou-3e onboard clocks are better than those of BeiDou-2 by factors of 2.84 and 1.61 at an averaging time of 1000 and 10,000?s, respectively. 相似文献
150.
本文采用非径向磁流管位形的假设,计算了太阳冕洞网络部分的色球-日冕过渡区的能量平衡模型。所考虑的能量流包括辐射、传导、对流和机械波加热(如阿尔芬波),计算结果表明在冕洞网络部分的过渡区中,电子温度T和密度N分别比宁静太阳中的值低60%和2倍,而其过渡区的厚度比宁静太阳中的大4倍。这种大气模型可满意地解释T≥105K范围的远紫外观测发射量度的分布。另外我们也发现在冕洞大气的过渡区中,阿尔芬波加热似乎不能忽略,尤其是在冕洞的过渡区底部,它的加热作用可能会超过热传导。在冕洞大气中,由于波动量的淀积而产生的对流能损耗也是重要的,在过渡区底部650km以上,对流能损耗逐渐超过辐射损耗。 相似文献