绕圆头回转体通气空化流型的实验研究

为了深入了解通气空化流动现象,利用高速全流场显示技术,对绕圆头回转体通气空化流型进行实验研究。结果表明,重力效应和通气量对通气空化的多相流流型起主要作用。定义了弗洛德数和通气率两个无量纲数,将绕圆头回转体通气空化分为5种多相流流型,即透明空泡、透明气弹、透明分层、水气混合以及半透明水气混合。流动参数对流型的影响分为2个阶段,即重力起主要作用阶段和重力效应不明显阶段。在重力起主要作用阶段,通气率一定时,随着弗洛德数的增大,附着弹体的空泡倾斜程度变小,弹体上表面的断裂空泡转变为贴着弹体壁面的稳定空泡;弗洛德数一定时,随着通气率的增大弹体上表面断裂空泡的尺度不断增大。在重力效应不明显阶段,通气率一定时,随着弗洛德数的增大,雷诺数变大,流场的湍流强度增大,空泡尾流区域水气交换的程度加剧;弗洛德数一定时,随着通气率的增大,通气空化数减小,绕弹体的云雾状空泡逐渐转变为透明空泡。最后,进一步分析了重力影响下透明空泡脱落的非定常过程,以及反向射流作用下云雾状空泡交替脱落的非定常过程。     

FA表面改质剂在伺服阀压装中的应用

分析了伺服阀在精密压装中组件压装存在的工艺问题，对压装过程进行力学分析，提出了新的工艺思路，并通过利用 FA表面改质剂，改善润滑条件，解决压装中的难点。     

通用的航电系统总线接口仿真平台的设计和应用

针对当前航电系统仿真器的缺点,提出了一种通用的航电系统总线接口仿真平台的设计思想,通过建立仿真数据库,从待仿真的航电系统设备中的接口信息抽象出属性和行为,然后用数据库的方式来描述,实现了仿真软件和仿真对象的分离,从而使该仿真平台具备了通用性和灵活性。该仿真平台已经在某型机航电系统地面联试中得到了应用。     

数控系统内置式PLC的FPGA实现方法

提出了一种用FPGA实现数控系统内置式PLC的方法.通过在FPGA内部实现PLC逻辑,并提供能够编译PLC指令的编译器,实现了数控系统对通用PLC编程语言的支持.所述方法在基于ARM FPGA的数控系统上得到了实现.     

基于Petri网的建模方法在叶片制造流程重组中的应用

采用基于Petri网的流程建模方法,结合数字化条件下叶片工艺流程设计与评估的相关理论,对叶片制造流程进行重组,并绘制流程框图.利用可达树对Petri网模型进行死锁分析,从而减少流程重组的盲目性和风险.最后通过工程事例说明Petri网模型的死锁分析过程.     

大连机场一次罕见的连续四天大雾低云过程分析

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。     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

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.     

Alfvén gravity waves in viscous solar plasma: Effect of the background flow

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.     

Early analysis of precise orbit and clock offset determination for the satellites of the global BeiDou-3 system

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.