基于全极化SAR影像的舰船目标检测算法研究

介绍了基于星载极化SAR影像的舰船目标检测的处理流程,针对基于不同杂波模型的CFAR检测法和基于相干信息的2L-IHP检测法,分析实现了瑞利分布、Gauss分布、韦布尔分布、对数正态分布,四种常用杂波分布模型的CA-CFAR检测法,通过实验检测海面舰船目标,发现这四种杂波模型针对不同海况有着不同的适应性,其检测效果也大不相同。而2L-IHP检测法不依赖于海杂波模型,通过子孔径相干提高目标和背景之间的对比度,实验结果表明,该方法能大幅提高海面舰船目标的检测概率。     

实时精密单点定位中的数据预处理研究

提出了适用于实时环境的一套数据预处理方案,包括钟跳修复、联合使用Geometry-Free和Melbourne-Wübbena组合进行周跳探测。通过丰富的实验算例,说明了对观测值进行钟跳修复的必要性;证明了联合使用GF与MW组合能够准确有效地探测出实际数据中存在的以及手工模拟加入的周跳。     

一次对流降水过程增雨催化时机的模拟分析和雷达识别

为加深对对流云增雨催化机制的理解,避免催化指标的随意性,通过三维积云数值模拟和雷达加密探测资料分析相结合的方法,对发生在湖北省西北部多山地区的一次对流降水过程进行了增雨催化时机的分析和识别.首先运用三维积云模式,通过催化模拟敏感试验,得出对流云增雨催化存在时间窗,最佳的催化时机应该为对流云发展的早期,催化后关键是增加雨和冰晶冻结后碰并霰增长这一冰相微物理过程的产量.根据模式分析结果,结合雷达观测资料分析,发现对流回波在生成及发展上表现出一些规律性,可以作为通过雷达观测识别增雨催化的时机和潜力区域的指标.     

气候变暖条件下水文循环变化检测与归因研究的几点认识

气候变化检测与归因的实践指南(GPGP)综合了4种检测归因方法,它囊括了目前研究这一因果链采用的不同途径。自1990年政府间气候变化专门委员会(IPCC)第一次评估报告以来,气候变化的检测与归因从气温升高和其他系统或变量变化趋势的研究开始,经历了从全球、半球、海洋与陆地、七大洲乃至区域尺度的细化进程。人为气候变化的指纹检测与归因方法已普遍用于全球大尺度水文循环要素——纬度带平均降水、强降水、径流、比湿、水汽含量等时空型态变化的研究,个别地也应用到流域尺度,如以冰雪融水补给为主的河流的天然流量、积雪和最低温度变化的研究。对于以降水为主,且受人类活动干扰较大的流域,观测的水文循环要素变化的检测与归因,大多数聚焦于观测的气候要素及非气候变量对其的影响,而不回答变化是自然的还是人为强迫引起的。这种方法要求高质量长系列的观测数据、先进的统计检验技术以及物理基础好的水文模型。对于水文循环要素对气候变化敏感的流域,若观测数据满足要求,则采用正规的检测与归因方法或最优指纹法识别外强迫及驱动因子的影响研究,将具有重要科学意义和发展前景。     

基于贝叶斯网络分类的遥感影像变化检测

遥感成像过程中,地面、大气等诸多要素的不确定性和波段之间的相关性等原因影响了分类精度,导致变化检测的不准确性。为了提高分类精度往往需要引入先验知识。贝叶斯网络是一种新的数据表达和推理模型,对数据没有严格的正态分布前提要求,通过动态地调整先验概率密度,能有效提高分类精度。以北京通州地区1996-05-29和2001-05-19两个时相的陆地卫星Landsat TM遥感影像为例,介绍了基于贝叶斯网络的分类算法,并在此基础上实现了两个时相遥感影像的变化检测。实验结果表明:基于贝叶斯网络分类算法的后分类比较变化检测方法是遥感影像变化检测的一种新的有效方法。     

多特征差分核支持向量机模型的湿地变化检测

文章通过对不同特征空间、不同时相信息和不同类别引入多核函数组合和类别加权方式,构建了基于多特征差分核的加权支持向量机变化检测模型,能够获得平衡样本大小、综合多特征空间的变化检测结果.以上海崇明岛东端地区为例,利用4期ETM+/TM影像数据,基于构建的SVM变化检测模型,最终得到研究区湿地资源的空间变化格局,结果表明检测模型能够有效、准确地提取多种湿地变化类别的空间分布信息;并从景观水平上对检测结果进行格局分析,为湿地保护和管理提供科学参考.     

The sensitivity of the next generation of lunar Cherenkov observations to UHE neutrinos and cosmic rays

We present simulation results for the detection of ultra-high energy (UHE) cosmic ray (CR) and neutrino interactions in the Moon by radio-telescopes. We simulate the expected radio signal at Earth from such interactions, expanding on previous work to include interactions in the sub-regolith layer for single dish and multiple telescope systems. For previous experiments at Parkes, Goldstone (GLUE), and Kalyazin we recalculate the sensitivity to an isotropic flux of UHE neutrinos. We find the published sensitivity for the GLUE experiment to be too high (too optimistic) by an order of magnitude, and consequently the GLUE limit to be too low by an order of magnitude. Our predicted sensitivity for future experiments using the Australia Telescope Compact Array (ATCA) and the Australian SKA Pathfinder (ASKAP) indicate these instruments will be able to detect the more optimistic UHE neutrino flux predictions, while the square kilometre array (SKA) will also be sensitive to all bar one prediction of a diffuse ‘cosmogenic’, or ‘GZK’, neutrino flux.Outstanding theoretical uncertainties at both high-frequency and low-frequency limits currently prevent a reliable estimate of the sensitivity of the lunar Cherenkov technique for UHE cosmic ray (CR) astronomy. Here, we place limits on the effects of large-scale surface roughness on UHE CR detection, and find that when near-surface ‘formation-zone’ effects are ignored, the proposed SKA low-frequency aperture array could detect CR events above 56 EeV at a rate between 15 and 40 times that of the current Pierre Auger Observatory. Should further work indicate that formation-zone effects have little impact on UHE CR sensitivity, observations of the Moon with the SKA would allow directional analysis of UHE cosmic rays, and investigation of correlations with putative cosmic ray source populations, to be conducted with very high statistics.     

高效液相色谱-紫外光谱分析氢醌-双(β-羟乙基)醚

建立了高效液相色谱-紫外光谱法测定聚氨酯扩链剂氢醌-双(β-羟乙基)醚(HQEE)工业品中HQEE主含量和对苯二酚残留的方法。在氰基柱上,以甲醇-水-1%乙酸溶液(体积比10∶50∶40)为流动相,流速1.0 mL/min时,HQEE、对苯二酚及其他相关杂质得到良好分离,紫外光谱285 nm检测。方法简便、快捷,结果准确可靠,在工业生产中可有效地指导HQEE合成过程的质量控制。     

General seismic wave and phase detection software driven by deep learning

We developed an automatic seismic wave and phase detection software based on PhaseNet, an efficient and highly generalized deep learning neural network for P- and S-wave phase picking. The software organically combines multiple modules including application terminal interface, docker container, data visualization, SSH protocol data transmission and other auxiliary modules. Characterized by a series of technologically powerful functions, the software is highly convenient for all users. To obtain the P- and S-wave picks, one only needs to prepare three-component seismic data as input and customize some parameters in the interface. In particular, the software can automatically identify complex waveforms (i.e. continuous or truncated waves) and support multiple types of input data such as SAC, MSEED, NumPy array, etc. A test on the dataset of the Wenchuan aftershocks shows the generalization ability and detection accuracy of the software. The software is expected to increase the efficiency and subjectivity in the manual processing of large amounts of seismic data, thereby providing convenience to regional network monitoring staffs and researchers in the study of Earth's interior.     

Fault detection by reflected surface waves based on ambient noise interferometry

Detecting subsurface fault structure is important for evaluating potential earthquake risks associated with active faults. In this study, we propose a new method to detect faults using reflected surface waves observed in ambient noise cross correlation functions. Ambient noise tomography using direct surface waves obtained from ambient noise interferometry has been widely used to characterize active fault zones. In cases where a strong velocity contrast exists across the fault interface, fault-reflected surface waves are expected. We test this idea using a linear array deployed in the Suqian segment of Tanlu fault zone in Eastern China. The fault-reflected surface waves can be clearly seen in the cross-correlation functions of the ambient noise data, and the spatial position of the fault on the surface is close to the stations where the reflected signals first appear. Potentially reflected surface waves could also be used to infer the dip angle, fault zone thickness and the degree of velocity contrast across the fault by comparing synthetic and observed waveforms.