水溶液中LC4铝合金的微生物腐蚀缓蚀杀菌剂

通过电化学极化、表面分析等方法,研究了 LC4铝合金在无菌培养液和培养液加硫酸盐还原菌( sulfate-reducing bacteria,简称 SRB)的厌氧体系中加入缓蚀杀菌剂的腐蚀行为。实验结果表明 :SRB能加速LC4铝合金的腐蚀破坏,其腐蚀破坏行为属于点蚀腐蚀机理;加入缓蚀杀菌剂能够影响 SRB的生长规律,抑制 SRB和 Cl-离子对 LC4铝合金的腐蚀破坏。在所研究的 4种缓蚀杀菌剂中,BHA-2缓蚀杀菌剂具有最好的缓蚀和杀菌双重功效,且明显优于市场上广泛使用的 1 2 2 7。     

钛合金表面低氧压熔结Al-Si涂层及抗氧化能力

采用低氧压高温快速熔结技术在Ti-6Al-4V合金表面成功地制备出抗高温氧化的Al-Si熔结涂层.与Si改性渗涂层相比,这种工艺相对简单,不需要经过长时间的扩散就能形成足够厚度的Al-Si熔结涂层,省时节能,且涂层中抗氧化元素铝、硅的浓度可通过调整粉末的混合比例来进行控制.X射线检测表明涂层主要由Ti₅Si₃和TiAl₃组成.在923K空气中52h循环氧化试验结果表明:低氧压熔结Al-Si涂层在前10h的氧化过程中氧化增重较快,而在随后的氧化过程中氧化增重较为缓慢,而Si改性渗涂层在氧化过程中一直保持着较高的氧化速率.      

开关点预置三相四线SPWM逆变器研究

脉宽调制型交直交变速恒频电源采用开关点预置SPWM逆变器,该逆变器由三相桥,交流滤波器,中点形成变压器及控制、驱动电路组成。绝缘栅双极性晶体管是一种新型的电力电子器件;应用该器件为功率器件,研制了一套15kVA开关点预置SPWM逆变器。由于对电路各个部分均进行了充分分析和优化设计,实际制作的逆变器具有较小的体积、重量,并具有优越的电性能。     

MPEG-4视频DCT量化模块的FPGA实现

介绍了一种采用FPGA技术实现MPEG-4 ASP级视频DCT量化模块的设计方案。该模块包括二维DCT／IDCT、量化／反量化和帧内直流／交流(DC／AC)预测。用VHDL进行描述并通过模拟试验表明，该模块可在880个时钟周期内处理完一个宏块的数据，工作频率达到40MHZ。文章采用全硬件实现方法，提出了各模块的硬件电路结构设计，减少了电路规模。     

风云四号卫星双程测距系统精密轨道确定

针对我国新一代静止轨道卫星风云四号高精度轨道计算需求，地面跟踪系统设计了多台站双频双程测距模式。详细给出了信号传播介质改正中的电离层与对流层处理方法，并给出了风云四号卫星动力学轨道确定策略。在非变轨期间，采用动力学定轨方法。轨道确定残差分析，测量噪声均方根优于0.5 m。通过轨道重叠分析，非变轨期间精度优于20 m。动量轮卸载期间，采用估计经验力的方法，其定轨残差优于1 m。对多弧段数据处理表明文中方法满足同步卫星双程测距模式下的高精度轨道跟踪问题。     

激光选区熔化成形Ti6Al4V合金的热处理组织演变机理

激光选区熔化(SLM)Ti6Al4V成形构件需要通过热处理改善其塑性。为探究该过程中的组织特征和演变机理,研究了Ti6Al4V试样固溶时效热处理(910℃/8 h水冷,750℃/4 h炉冷)前后的微观形貌和力学性能。结果表明:沉积态的马氏体α′相尺寸具有层次结构;热处理相变时初生马氏体α′发生分解,小尺寸马氏体α′转变为β相,随后发生β→(α+β)转变,最后得到α相片层和精细(α+β)相结构均匀分布的组织;热处理后材料抗拉强度达1 055 MPa,延伸率提升至16.2%,均优于典型Ti6Al4V合金拉伸性能。采取的热处理技术对Ti6Al4V组织调控成效显著,满足后续工艺要求,可在激光选区熔化成形双相钛合金中推广应用。     

Temporal evolution of the EIA along 95°E as obtained from GNSS TEC measurements and SAMI3 model

The total electron content (TEC) derived from GNSS measurements at a trans-hemispheric meridional chain of ground stations around 95°E longitude are used to study the quiet time inter-hemispheric structure and dynamics of the equatorial ionization anomaly (EIA) during the period March 2015 to February 2016. The stations are Dibrugarh (27.5°N, 95°E, 43° dip), Kohima (25.6°N, 94.1°E, 39° dip), Aizawl (23.7°N, 92.8°E, 36° dip), Port Blair (11.63°N, 92.71°E, 9° dip) and Cocos Islands (12.2°S, 96.8°E, 43° dip). The observation shows that the northern crest of the EIA lies in the south of 23°N (Aizawl) in all seasons but recedes further south towards the equator during December solstice. The largest poleward expansion of the northern (southern) EIA is observed in the March equinox (December solstice). The equinoctial and hemispherical asymmetry of TEC is noted. The winter anomaly is observed in the northern hemisphere but not in the southern hemisphere. The highest midday TEC over any station is observed in the March equinox. The TEC in southern summer (December solstice) is significantly higher than that in the northern summer (June solstice). The observed northern EIA contracts equatorward in the postsunset period of solstice but the southern EIA persists late into the midnight in the December solstice. The asymmetry may be attributed to the different geographic location of the magnetically conjugate stations. The SAMI3 simulations broadly capture the EIA structure and the inter-hemispheric asymmetry during solstices. The difference between observations and the SAMI3 is higher in March equinox and December solstice. The higher E?×?B vertical drift in the 90–100°E sector and the large geographic-geomagnetic offset in observing stations may have contributed to the observed differences.     

Statistical characteristics of locally generated ESF during equinoctial months over Sanya

Understanding the local generation rate of equatorial spread-F (ESF) is important for forecasting ionospheric scintillation. Using the GPS ionospheric scintillation/TEC and VHF radar data during March-April and September-October from 2010 to 2014, the occurrence of ionospheric scintillation, TEC fast fluctuation, and backscatter plume were studied. Through analyzing the simultaneous occurrence of ionospheric scintillation, TEC fast fluctuation and backscatter plume, the local generation rate of ESF over Sanya was investigated. The results show that the monthly generation rate varies between 0% and 68%. A significant equinoctial asymmetry of local generation rate of ESF can be found in 2010, 2013 and 2014. The local generation rate of ESF increases from 2010 to 2014 during March-April, while it does not have similar trend during September-October. The plasma vertical drift influenced by solar activity has a significant impact on the monthly generation rate. The equinoctial asymmetry of plasma vertical drift may contribute a lot to the equinoctial asymmetry of the generation rate of ESF.