A new stochastic model considering satellite clock interpolation errors in precise point positioning

Precise clock products are typically interpolated based on the sampling interval of the observational data when they are used for in precise point positioning. However, due to the occurrence of white noise in atomic clocks, a residual component of such noise will inevitable reside within the observations when clock errors are interpolated, and such noise will affect the resolution of the positioning results. In this paper, which is based on a twenty-one-week analysis of the atomic clock noise characteristics of numerous satellites, a new stochastic observation model that considers satellite clock interpolation errors is proposed. First, the systematic error of each satellite in the IGR clock product was extracted using a wavelet de-noising method to obtain the empirical characteristics of atomic clock noise within each clock product. Then, based on those empirical characteristics, a stochastic observation model was structured that considered the satellite clock interpolation errors. Subsequently, the IGR and IGS clock products at different time intervals were used for experimental validation. A verification using 179 stations worldwide from the IGS showed that, compared with the conventional model, the convergence times using the stochastic model proposed in this study were respectively shortened by 4.8% and 4.0% when the IGR and IGS 300-s-interval clock products were used and by 19.1% and 19.4% when the 900-s-interval clock products were used. Furthermore, the disturbances during the initial phase of the calculation were also effectively improved.     

Web服务组合处理系统的研究与实现

单个Web服务难以满足实际应用的需求,为了解决互联网应用的集成和协作问题,需要把独立的Web服务组合起来以实现复杂的业务逻辑功能.通过分析服务组合的处理机制,基于传统工作流技术,使用IBM的WSFL语言作为服务组合描述语言,设计并实现了一个面向Web服务组合语言的通用的Web服务组合处理系统.这是一个多层结构的系统,它由Web服务平台、服务组合处理引擎、JMX注册管理中心、远程管理控制台以及处理引擎配置工具五部分构成;它为WSFL语言所描述的服务组合流程提供了一个运行引擎,同时提供了一个基于JMX的管理控制台,通过它可以对正在运行的流程实例以及历史数据进行控制和管理.该系统为基于Web服务的应用集成和协作提供了一个统一的运行管理环境.     

Variations in Electron Content Ratio and Semi-thickness Ratio during LSA and MSA periods and some Cyclone Genesis Periods using COSMIC satellite observations

In this study for the first time, COSMIC satellite data have been used to deduce values of ionospheric Electron Content Ratio (ECR) and Semi-thickness Ratio (Rtb) for Low Solar Activity (LSA) (2008) and Moderate Solar Activity (MSA) (2012) periods over the Indian low-latitude (15–30°N) region with 80–95°E longitude. These two ratios provide sensitive information about bottom and topside ionosphere for different geophysical conditions. Extraction of suspected patterns and discrepancies unfold that the deviations between ECR and Rtb values during LSA period are comparatively higher than that of MSA period when the diurnal variability in these two parameters is flatter along with the diurnal-dips during pre-noon hours. The correlative relationship of ECR exhibits low association with NmF2 and anti-correlation with HmF2, whereas its correlation with Rtb is extremely high. During Cyclone Genesis Period (CGP) strong dips in ECR and Rtb values with respect to pre and post CGP occurred which helps to take decisive conclusion about the ionospheric variations to be dominant through getting relatively higher Ne concentration in the bottom side part of the ionosphere.     

基于OpenGL的飞机飞行实测数据可视化研究

为实现飞机飞行历程实测数据的可视化,并检测飞行数据是否满足飞行大纲要求,运用OpenGL (Open Graphic Library)技术,研究了飞机的三维模型建模方法、特殊场景的生成技术和三维模型的实测数据驱动;建立了飞机的三维模型和飞行场景.基于飞行实测数据驱动方式,实现了飞机飞行历程数据的多视角可视化,直观地再现...     

Microgravity gas–liquid flow through packed beds

Analysis of possible physical mechanism involved in the process of transition of bubble-to-pulse flow regime in cocurrent gas–liquid flow through a packed bed in microgravity demonstrates that the transition can be described by the key dimensionless group Suratman number and the ratio of gas to liquid Reynolds numbers. This result establishes a physical basis to the existing empirical transition equation which is also based on the same dimensionless groups. Furthermore, the concepts of driving-to-resistance force ratio and pore-level bubble flow mechanism have been utilized to explore the basis of the existing modified friction factor correlation for two-phase flow through a packed bed under microgravity.     

多孔材料下气体爆炸转扩散燃烧的特性研究

为分析多孔材料对预混气体爆炸特性参数的影响效果,采用自主搭建的爆炸实验平台,探究不同孔隙度和厚度的多孔材料对当量比为1的甲烷/空气预混气体爆炸的作用行为。实验研究表明,不同孔隙度的多孔材料对爆炸火焰和超压具有促进或抑制两种不同的影响。孔隙度较小时,爆燃火焰传播速度随着材料厚度的增大而降低,并在厚度较大时,火焰有短暂的传播延时现象。孔隙度较大时,预混火焰冲击多孔材料时发生淬熄,但随后一段时间内,由于负压抽吸作用,在已爆区域一侧的材料表面产生扩散燃烧现象,且扩散燃烧程度与材料厚度成反比关系。多孔材料的固相结构能降低压力的泄放效率,同时可吸收能量,进而提高爆炸超压的上升速率,降低超压峰值。当每英寸长度孔数δ=10的多孔材料促进火焰传播时,与当量比为1的预混气体爆炸相比,超压峰值最大可提高约2倍,造成更严重的后果。火焰冲击δ=20的多孔材料时发生淬熄,最大超压衰减可达47.17%,δ=30时最大超压衰减了24.62%。     

高温升燃烧室流动与贫油熄火过程的影响规律

为了研究高温升燃烧室在冷态和燃烧状态下的流动差异及其对贫油熄火过程的影响规律,采用粒子图像测速法（PIV） 和高速相机对2种状态下流场结构及贫油熄火过程进行测量。结果表明：主燃孔和掺混孔射流与头部旋流存在相互作用,使得燃 烧室流动处于自模化状态,其流场结构不随压损的改变而变化,但速度值随着压损的增大而提高;当量比的变化不会影响在燃烧 状态下的流场结构,但影响速度值,且燃油喷射对头部流场存在一定影响;在冷态和燃烧状态下流场结构的差异最主要体现在局 部回流区和气流速度上,燃烧状态下的轴向正速度约为冷态时的5~7倍,径向速度约为10倍;气流的流动方式对贫油熄火过程影 响显著,在局部漩涡和垂直气流作用的区域火焰首先熄灭。     

激波风洞流场密度测量的聚焦纹影技术

在激波风洞试验中发展了聚焦纹影显示技术,对流场的密度进行了定量测量。聚焦纹影显示具有对流场区域聚焦显示的特点,可获得流场某个聚焦测试区域的密度变化信息。依据聚焦纹影成像原理建立了密度计算数学模型,对试验中获得的带窗口模型流场聚焦纹影图像与试验前获得的流场图像灰度变化处理后,得到了流场聚焦区域的密度定量值。试验测量密度值与数值计算结果进行了比较,结果表明试验获得的密度值变化规律与数值模拟吻合较好,证实了利用聚焦纹影技术开展流场密度测量是可行的。     

燃烧室工作过程对冲压发动机性能潜力的影响研究

用准一维分析方法,在相同的入流条件下,假设将当量比为1的燃料热量全部添加到气流中,研究了燃烧室工作过程与性能之间的关系。结果表明,随着特征马赫数的增加,在相同飞行马赫数下,亚声速燃烧室所需扩张比逐渐减小,而双模态燃烧室所需扩张比逐渐增大;亚声速燃烧室出现所需最小扩张比和最大比冲的特征马赫数分别是1和0,双模态燃烧室在最小特征马赫数时所需扩张比最小,获得的比冲最大,且与亚声速燃烧室能获得的最大比冲相差不大,在飞行马赫数4、5、6时,差值分别为5%、4%、3%;特征马赫数在亚声速范围内变化时发动机比冲的曲线比较平缓;壁面摩擦系数的变化对燃烧室所需扩张比的影响大于对比冲的影响。直连式实验获得的等截面燃烧室极限加热量数据证明了本方法的合理性。