高光谱图像序列中的运动弱小目标检测

高光谱图像序列中包含时域信息和光谱信息的弱小运动目标检测因其在民用和军用中的重要作用而引起了研究人员的兴趣。本文提出了一种新的空时联合异常方法来解决运动弱小目标的检测问题。该方法分别从空间域和时间域利用异常检测算法计算空间异常图和时间异常图。为了检测目标的运动一致性特征,该方法生成了运动轨迹预测图。将空间异常图、时间异常图和轨迹预测图融合后,可以很容易地从背景中检测到感兴趣的目标。该方法被应用于云杂波背景下的空中目标测试数据集。实验结果表明,该方法具有较低的虚警率和较高的检测率。     

航空发动机限寿件表面特征概率损伤容限评估

为满足航空发动机适航规章(FAR/CCAR33.70)限寿件安全性评估要求,系统总结了基于特殊材料数据库、线弹性断裂力学分析与表面特征失效概率分析的表面特征概率损伤容限评估方法.以表面孔特征为例,总结分析符合适航规章要求的孔特征概率损伤容限评估流程,描述优化的孔特征评估方法,根据咨询通告AC33.70-2中带孔特征轮盘...     

2012年3月9日中国某地球同步轨道卫星故障原因分析

利用GOES-15, SDO, SOHO卫星以及国际地磁台网的地磁活动指数数据, 对中国 某颗地 球同步轨道卫星(以GEO-X代替)在2012年3月9日02:50UTC发生的异常原因进 行了研究, 分析故障发生期间的空间天气特点, 采用文献[8]提出的SEAES-GEO空 间环境引起地球同步轨道卫星异常的专家系统对卫星故障期间的内部充电危 险系数、单粒子效应危险系数以及表面充电危险系数进行定量计算和危险等 级划分. 结果表明, 在卫星故障时刻, 其内部充电危险系数小于3, 表面充电危险 系数约为0.0011, 表面充电和内部充电不是造成GEO-X故障的原因; 受故障期间 质子事件影响, 单粒子效应危险系数持续维持在1以上, GEO-X卫星故障时刻单 粒子效应危险系数Z_SEE达到46.3, 正好处于单粒子效应危险等级的 红色阶段. 因此研究认为单粒子效应可能是造成本次卫星故障的主要原因.     

Diagnostics of equatorial and low latitude ionosphere by TEC mapping over Brazil

The total electron content (TEC) in the equatorial and low-latitude ionosphere over Brazil was monitored in two dimensions by using 2011 data from the ground-based global navigation satellite system (GNSS) receiver network operated by the Brazilian Institute for Geography and Statistics. It was possible to monitor the spatial and temporal variations in TEC over Brazil continuously during both day and night with a temporal interval of 10 min and a spatial resolution of about 400 km. The daytime equatorial ionization anomaly (EIA) and post-sunset plasma enhancement (PS-EIA) were monitored over an area corresponding to a longitudinal extension of 4000 km in South America. Considerable day-to-day variation was observed in EIA and PS-EIA. A large latitudinal and longitudinal gradient of TEC indicated a significant ionospheric range error in application of the GNSS positioning system. Large-scale plasma bubbles after sunset were also mapped over a wide range. Depletions with longitudinally separated by more than 800 km were observed. They were extended by more than 2000 km along the magnetic field lines and drifted eastward. It is expected that 2-dimensional TEC mapping can serve as a useful tool for diagnosing ionospheric weather, such as temporal and spatial variation in the equatorial plasma trough and crest, and particularly for monitoring the dynamics of plasma bubbles.     

Solar flux effects on equatorial ionization anomaly and total electron content over Brazil: Observational results versus IRI representations

The F layer critical frequency (foF2) as measured by Digisondes in the equatorial and low latitude locations in Brazil is analyzed to investigate the seasonal and solar flux controls of the intensity of the equatorial ionization anomaly (EIA) in the equinoctial month of March. The analysis also included the total electron content (TEC) as measured by a GPS receiver operated at the EIA crest location. The foF2 data set covered a period of large solar flux variation from 1996 to 2003, while the GPS TEC data was for a period in 2002–2003 when the solar flux parameter F10.7 underwent large variations, permitting in both cases an examination of the solar flux effects on these parameters. The seasonal variation pattern in TEC shows a maximum in equinoctial months and a minimum in June solstice, with similar variations for foF2. The solar flux dependence of the TEC is a maximum during equinoxes, especially for post-sunset TEC values at times when the latitudinal distribution is controlled by the equatorial evening plasma fountain processes. Significant variations with local time are found in the degree of solar flux dependence for both the TEC and EIA. The EIA intensity shows large dependence on F10.7 during post-sunset to midnight hours. These results are discussed in comparison with their corresponding IRI representations.     

解决湍流圆/平射流异常现象的数值研究

圆射流/平面射流异常现象是湍流研究领域的一个著名的难题,是验证湍流微分方程模型的试金石。本文用GAO-YONG不可压湍流控制方程对圆射流进行了数值验证,成功地解决了该难题,进一步证明了该方程对真实湍流的适定性和通用性。      

不完全数据最佳线性无偏估计方法

针对工程上存在大量不完全数据的情况,本文建立了不完全数据秩统计量的联合概率密度函数,给出不完全数据顺序统计量的均值、方差和协方差计算公式,提出不完全数据最佳线性无偏估计方法,并对正态分布、Weibull分布等位置-尺度分布进行了详细讨论。该方法能够充分开发利用试验数据中的不完全信息,从而提高不完全数据统计分析的精度。      

Study of hot flow anomalies using Cluster multi-spacecraft measurements

Hot flow anomalies (HFAs) were first discovered in the early 1980s at the bow shock of the Earth. In the 1990s these features were studied, observed and simulated very intensively and many new missions (Cluster, THEMIS, Cassini and Venus Express) focused the attention to this phenomenon again. Many basic features and the HFA formation mechanism were clarified observationally and using hybrid simulation techniques. We described previous observational, theoretical and simulation results in the research field of HFAs. We introduced HFA observations performed at the Earth, Mars, Venus and Saturn in this paper. We share different observation results of space mission to give an overview to the reader.     

Spatial distribution of TEC across India in 2005: Seasonal asymmetries and IRI prediction

Total electron content measured simultaneously at 10 locations over India during the low solar activity year 2005 is used to examine the temporal and spatial asymmetries and also to assess the predictability of the International Reference Ionosphere in respect of the observed asymmetrical distribution. The stations are distributed in latitude along 77°E and in longitude along 23°N forming a meridional and a zonal chain respectively. A longitudinal gradient positive towards east was observed in the daytime hours of equinox and summer. Equinoctial asymmetry was prevalent across India during this year. Within the crest and equator, winter anomaly has been observed. It is found that IRI 2012 (with Ne Quick option, URSI coefficients) is unable to fully capture the temporal variation and spatial gradients of the ionization density in the Indian sector during 2005. The amount of offset between the model and measurement varies with local time and location.