梯度热障涂层的设计

 采用电子束物理气相沉积方法 (EB PVD)制备了梯度热障涂层,其结构设计为NiCoCrAlY粘结层 /Al₂O₃ YSZ过渡层 /YSZ陶瓷层。YSZ陶瓷层的结构为柱状晶结构,Al₂O₃ YSZ梯度过渡层为梯度微孔结构。采用有限元方法对梯度热障涂层进行热应力分析,优化了Al₂O₃ YSZ梯度过渡层的组成。计算结果表明,梯度涂层的内应力显著降低,而且界面及其附近应力和应变变化较平缓。过渡层厚度的增加有利于降低涂层内应力和缓和涂层界面处的应力集中。     

供油瞬态喷油杆内燃油结焦机理及规律数值研究

为获得喷油杆通断循环供油工作模式下,供油瞬间燃油结焦速率陡增机理,本文建立起沿喷杆轴向的一维非稳态热-流-固耦合换热与燃油结焦计算模型。获得不同时刻壁温、油温与结焦速率等参数轴向分布。通过与连续供油模式下的结果进行对比,来分析供油瞬间灼热喷杆内壁对燃油热冲击的影响,以获得结焦速率陡增机理。结果表明通断供油模式下,供油瞬间会迅速形成一尖锐的油温和结焦前体浓度峰值,结焦固相表面反应被迅速激发,结焦速率陡增。在喷杆前端（x=100mm）与底部（x=260mm）附近各存在一结焦速率峰值区域。通断供油模式下,在x=100mm和x=260mm位置处,每个周期供油起始时刻结焦速率峰值分别在5000μg/cm2h和2000μg/cm2h左右,远大于连续供油下的值。但供油结束时刻,供油模式的影响大幅下降。此外通断供油下,供油瞬间热冲击对燃油结焦的影响沿喷杆轴向逐渐减小。减小喷杆供油流量,热冲击的影响有所下降,且随时间先升高后降低。提高进口油温,热冲击的影响显著减小,且随供油时间逐渐降低。     

Validation on MERSI/FY-3A precipitable water vapor product

The precipitable water vapor is one of the most active gases in the atmosphere which strongly affects the climate. China's second-generation polar orbit meteorological satellite FY-3A equipped with a Medium Resolution Spectral Imager (MERSI) is able to detect atmospheric water vapor. In this paper, water vapor data from AERONET, radiosonde and MODIS were used to validate the accuracy of the MERSI water vapor product in the different seasons and climatic regions of East Asia. The results show that the values of MERSI water vapor product are relatively lower than that of the other instruments and its accuracy is generally lower. The mean bias (MB) was ?0.8 to ?12.7?mm, the root mean square error (RMSE) was 2.2–17.0?mm, and the mean absolute percentage error (MAPE) varied from 31.8% to 44.1%. On the spatial variation, the accuracy of MERSI water vapor product in a descending order was from North China, West China, Japan -Korea, East China, to South China, while the seasonal variation of accuracy was the best for winter, followed by spring, then in autumn and the lowest in summer. It was found that the errors of MERSI water vapor product was mainly due to the low accuracy of radiation calibration of the MERSI absorption channel, along with the inaccurate look-up table of apparent reflectance and water vapor within the water vapor retrieved algorithm. In addition, the surface reflectance, the mixed pixels of image cloud, the humidity and temperature of atmospheric vertical profile and the haze were also found to have affected the accuracy of MERSI water vapor product.     

煤油液滴高压蒸发特性

采用真实流体模型描述高压下流体热物理性质的非理想性,并采用状态方程（EoS）法计算多组分高压气-液相平衡及环境气体溶解性,在此基础上建立包含亚临界和超临界两种不同机制的瞬态液滴高压蒸发模型。针对中国新一代高压补燃液氧/煤油发动机,详细研究了煤油液滴在超临界环境下的高压蒸发特性及各因素影响机理。结果表明：高压环境会显著加快液滴温升速率,但弱超临界环境下仍然为相平衡控制的亚临界蒸发状态;只有强超临界环境下才较容易发生扩散控制的超临界蒸发状态。在高压、高温环境下,忽略气相溶解性将导致液滴蒸发速率明显偏小。针对弱超临界环境,温度升高会使液滴蒸发速率单调增加;压力升高则在低温下降低蒸发速率,而在高温下加快蒸发速率。针对强超临界环境,温度升高只提升初始亚临界蒸发阶段的蒸发速率,而超临界蒸发阶段的蒸发速率与环境温度无关;压力升高则同样会提升初始亚临界蒸发阶段的蒸发速率,但会降低超临界蒸发阶段的蒸发速率,此时的总蒸发寿命随压力升高小幅下降。     

气体流场对C／C复合材料CVI致密化效果的影响

以丙烯为碳源气体,研究平板针刺预制体在不同倾斜角放置和不同进气方式条件下化学气相渗透（ CVI）工艺制备C／C复合材料的致密化效果。采用工业CT、浸泡介质法和偏光显微镜对沉积样品的密度分布、开孔孔隙率和织构分别进行表征。沉积102 h后,倾斜17°、前进气条件下试件的密度最高,达到1．45 g／cm－3。结果表明,试样由底端到顶端的密度是有小幅递增的,开孔孔隙率是逐渐减小的。4块试件热解炭的织构以光滑层为主,试样消光角的测量结果表明直立状态和倾斜17°、后进气状态热解炭织构取向度从底部到顶端有增大的趋势,这种织构的增长趋势与锥形回转体扩张段的材料设计相符合。     

沉积温度对CVD-SiC涂层显微结构的影响

介绍了采用化学气相沉积（CVD）方法在C/SiC复合材料表面制备SiC抗氧化涂层的情况.对不同工艺条件下制备出的SiC涂层,使用SEM,EDS和XRD分析了沉积层的物相和显微结构.结果表明：SiC涂层生长速度随沉积温度升高而升高,晶粒尺寸也随之增大;在较高沉积温度下,可以产生较大的沉积速度,但SiC涂层表面粗糙度将会增大.     

Assessment of precision in ionospheric electron density profiles retrieved by GPS radio occultations

The Constellation Observing System for Meteorology Ionosphere and Climate (COSMIC) is a six satellite radio occultation mission that was launched in April 2006. The close proximity of these satellites during some months after launch provides a unique opportunity to evaluate the precision of Global Positioning System (GPS) radio occultation (RO) retrievals of ionospheric electron density from nearly collocated and simultaneous observations. RO data from 30 consecutive days during July and August 2006 are divided into ten groups in terms of daytime or nighttime and latitude. In all cases, the best precision values (about 1%) are found at the F peak height and they slightly degrade upwards. For all daytime groups, it is seen that electron density profiles above about 120 km height exhibit a substantial improvement in precision. Nighttime groups are rather diverse: in particular, the precision becomes better than 10% above different levels between 120 and 200 km height. Our overall results show that up to 100–200 km (depending on each group), the uncertainty associated with the precision is in the order of the measured electron density values. Even worse, the retrieved values tend sometimes to be negative. Although we cannot rely directly on electron density values at these altitudes, the shape of the profiles could be indicative of some ionospheric features (e.g. waves and sporadic E layers). Above 200 km, the profiles of precision are qualitatively quite independent from daytime or latitude. From all the nearly collocated pairs studied, only 49 exhibited a difference between line of sight angles of both RO at the F peak height larger than 10°. After analyzing them we find no clear indications of a significant representativeness error in electron density profiles due to the spherical assumption above 120 km height. Differences in precision between setting and rising GPS RO may be attributed to the modification of the processing algorithms applied to rising cases during the initial period of the COSMIC mission.     

Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm

The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere.     

液态水相变发散冷却的实验

以液态水为冷却介质,采用高温合金粉末烧结多孔材料制造平板实验件,实验研究了具有液态水相变的发散冷却特性.用远红外热像系统记录实验平板热端表面温度分布,通过热电偶及压力传感器监控冷却腔内温度和压力变化,从而分析液态水的相变过程.实验表明:随着液态水注入率的增大,平均冷却效率不断提高;当液态水在暴露于高温主流的平板表面发生气液相变时,平均冷却效率趋于稳定且不再大幅上升;主流温度与液态水注入率决定了液态水的相变位置,并对冷却腔内压力变化产生影响.      

超临界压力下航空煤油RP-3壁面结焦特性对换热的影响

研究了超临界压力下航空煤油(RP-3)在微细管内流动过程中结焦对换热的影响规律.实验中系统压力保持为5MPa,燃油质量流量为3g/s.燃油溶解氧达到饱和,实验段进出口油温分别为127℃和450℃,实验时间为60min,并利用“称质法”获得煤油结焦量.结果表明:由于壁面结焦的差异使得换热特性沿实验段可分为3个区域:进口低温段的传热稳定区、结焦峰值处的传热恶化区和出口高温段的短期强化区.进口低温段结焦量较少,对换热的影响可以忽略;结焦峰值处由于其结焦迅速且量大致使管内传热热阻突增,传热系数下降36.1%故出现传热恶化;高温段出现短期强化是由于结焦微粒附着于管壁,增加了其粗糙度而导致近壁面处流体湍动能增大以及由于近壁面高温区域煤油裂解结焦而产生化学吸 热量,进而强化换热.随着时间的推移,结焦量不断增多,结焦热阻增加的效应抵消并超过以上两种因素的影响,因此又出现传热恶化.