The First Chinese Ocean Color Satellite HY-1A

HY-1A is China's first ocean color satellite, and was launched on 15 May 2002as a piggyback satellite on the FY-1D satellite using the Long March rocket.There are two sensors on the satellite: China's Ocean Color and Temperature Scanner (COCTS), and the CCD Coastal Zone Imager (CZI). In the report,first, the properties and characteristics of HY-1A are briefly introduced; Second, the quality and availability of the data are evaluated by the mean of the Complex Signal Noise Ratio (CSNR) which is simulated theoretically; Third,the received HY-1A data are compared with SeaSTAR data to understand the accuracy of radiance measurement by the HY-1A; Finally, the remote sensing products of ocean color and temperature are mapped by HY-1A to study its application potentiality. The results show that the HY-1A has a latent capability for the application of marine environment detection, the management and protection of marine resources, and the furthering of national rights and interests.Meanwhile, some modifications are proposed for the next ocean satellite, suchas adding the case of tilt scanning, modification of the CCD element uniformity,and adding more ocean satellite receiving stations.     

蜂群无人机充电排队优化方法

针对蜂群无人机快速充电排队问题，首次提出以平均队列长度和平均等待时间作为蜂群无人机充电排队优劣的评价指标。并通过理论分析和数值计算，在多充电平台的条件下，对蜂群无人机的分布式充电和集中式充电2种充电排队方式进行了比较和分析。得出蜂群无人机在泊松到达的条件下，随着服务强度的增加，评价指标对应的曲线出现了一个交叉点。在这个交叉点前，即服务强度较弱时，集中式充电排队方式优于分布式充电排队方式。在交叉点之后，即随着服务强度的增强，分布式充电排队方式将逐渐优于集中式充电排队方式。本文为蜂群无人机高效地完成任务提供了快速充电排队解决方案。     

航线网络中基于最小费用流的航线选择问题

针对航线网络中航线选择优化问题,分析了空中交通航线网络结构和空中交通流的特点,给出了空中交通航线网络的数学描述,考虑从求解最小费用流问题的角度寻求最优航线,建立了航线网络中求解最小费用流问题的数学模型。借鉴了连续时间网络最小费用流问题中结点到达费用的概念,并结合简单算例的求解验证了航线网络中用最小费用流方法选择航线的可行性,具有良好的计算性能。     

月球探测器LP精密定轨及月球重力场模型解算

对美国1998年发射的月球探测器LP任务阶段共19个月的双程测距测速轨道跟踪数据进行了精密定轨,对定轨结果通过轨道残差及重复弧段差异进行了精度评价。利用LP正常任务阶段三个月的轨道跟踪数据进行了月球重力场模型解算,通过重力场功率谱、轨道残差和月球自由空气重力异常对解算模型进行了精度评价。结果表明精密定轨及月球重力场模型解算合理。对进一步融合嫦娥一号轨道跟踪数据和LP数据解算自主的高精度月球重力场模型具有参考意义。
　
     

嫦娥一号干涉成像光谱仪2C级图像数据质量评价

嫦娥一号干涉成像光谱仪(IIM)获取的多波段图像数据对于月表矿物成分反演具有重要意义. 从目视质量、客观参数、几何配准精度、图像质量随时间的变化情况等方面对IIM 2C级的多波段图像数据质量进行了评价. 结果显示, 其两端波段范围的图像质量较差, 不能有效识别月表单元, 中间波段图像质量较好; 自然色图像显示IIM数据存在明显的横向色调不均一性. 利用图像的客观评价指标(辐射精度、清晰度、信息量)将干涉成像光谱仪图像数据与美国Clementine UV-VIS多光谱图像数据进行对比分析, 结果表明, IIM数据清晰度好于Clementine UV-VIS, 而在方差和信息量上弱于Clementine UV-VIS. 将IIM图像数据与Clementine多光谱数据统一到相同的空间分辨率, 进行配准精度评价, 其最大控制点配准误差为0.63pixel. 此外, 还对时间跨度两个月覆盖月表同一区域的IIM图像数据从辐射精度、信息量和清晰度方面进行了评价.      

基于5W1H的教育信息查询技术研究

针对教育信息基于互联网络的快速增长以及检索日趋复杂等问题,构建了基于领域本体的四层查询体系结构,采用5W1H分析法归纳了领域本体中的概念和关系,建立了基于5W1H的领域本体概念模型,重点研究了基于Jena的领域本体持久化技术和领域本体规则推理技术,设计了基于SPARQL查询规则和基于Jena推理规则的领域信息查询算法。以教师信息为例,采用Jena开发平台和MySQL数据库,实现了教师信息领域本体查询系统的精确查询、模糊查询和语义查询等功能。     

Rotational constants of linear and/or bent Cn+1H and CnN(n = 1–6): A DFT study

The geometries, dipole moments, and rotational constants for the linear and/or bent cations, C_n+1H⁺ and C_nN⁺(n = 1–6), were studied by the B3LYP method with the modest basis sets. For C_nH⁺(n = odd; 3, 5, 7) and C_nN⁺(n = even; 2, 4, 6), the theoretical rotational constants (B_es) of closed-shell singlet C₃H⁺, C₅H⁺, C₇H⁺, CCN⁺, C₄N⁺, and C₆N⁺ were calculated to be about 11,244, 2420, 885.2, 11,970, 2439, and 880.8 MHz, respectively. By contrast, the triplets are stable than the corresponding singlets for C_nH⁺(n = odd; 2, 4, 6) and C_nN⁺(n = even; 3, 5) except CN⁺.     

O2 evolution and cyclic electron flow around photosystem I in long-term ground batch culture of Euglena gracilis

Based on the purpose of better exploring the function of green producers in the closed aquatic biological life support system, the condition of dynamic O₂ evolution and performance of cyclic electron flow around photosystem I (CEF-PSI) in long-term ground batch culture of Euglena gracilis were studied, the relationship between linear electron flow (LEF) and CEF-PSI was revealed, the function of CEF-PSI was investigated. Excellent consistency in O₂ evolution pattern was observed in cultures grown in both closed and open containers, O₂ evolution was strictly suppressed in phase 1, but the rate of it increased significantly in phase 2. CEF-PSI was proposed to be active during the whole course of cultivation, even in the declining phase 3, it still operated at the extent of 47–55%. It is suggested that the relationship between LEF and CEF-PSI is not only competition but also reciprocity. CEF-PSI was proposed to contribute to the considerable growth in phase 1; it was also suggested to play an important protective role against photosystem II (PSII) photoinhibition at the greatly enhanced level (approximately 80–95%) on the 2nd day. Our results in this research suggest that E. gracilis had very particular photosynthetic characteristics, the strict O₂ evolution suppression in the initial culture phase might be a special light acclimation behavior, and CEF-PSI could be an important mechanism involved in this kind of adaptation to the changeable light environment.     

基于L1/2范数正则化的塑性回声状态网络故障诊断模型

为了提升储备池的动态适应性能,克服回声状态网络（ESN）输出权值求解的病态不适定问题,平衡其拟合与泛化能力,提出了一种基于L_1/2范数正则化的塑性回声状态网络故障诊断模型。在储备池构建中引入BCM规则对连接权矩阵进行预训练,并在目标函数中添加L_1/2范数惩罚项以提高稀疏化效率,利用一个光滑化的L_1/2正则子克服迭代数值振荡问题,并采用半阈值迭代法对模型进行求解。将模型应用于机载电台的故障诊断问题中,仿真结果证明了模型的有效性和优越性。     

Solar particle dynamics during magnetic storms of July 23–27, 2004

It is a case study of a chain of three magnetic storms with a special attention to the particle dynamics based on CORONAS-F and SERVIS-1 low altitude satellite measurements. Solar proton penetration inside the polar cap and inner magnetosphere and dynamics at different phases of the magnetic storms was studied. We found, that solar protons were captured to the inner radiation belt at the recovery phase of the first and the second magnetic storms and additionally accelerated during the last one. No evidence of sudden commencement (SC) particle injection was found. Enhanced solar proton belt intensity with small pitch angles decreased slowly during satellite orbits for 30 days until the next magnetic storm. Then in 20–30 h we registered strong precipitation of these protons followed by the trapped proton flux dropout. Intensity decrease was more pronounced at lower altitudes and higher particle energies.