注意力机制与卷积神经网络融合的军队标号识别方法     

杨云航  闵连权  侯翔  王佳伟 《测绘科学技术学报》2021,38(2):200-205,212

手绘军队标号识别是基于草图的战场态势表达的重要组成部分.针对现有的草图特征手工提取方法费时费力,以及依靠数据驱动的深度学习方法泛化能力受到训练数据多样化制约的问题,提出一种注意力机制与卷积神经网络融合的军队标号识别方法.首先构建了特征提取模型Sketch-Net,实现手绘军队标号特征的初步提取;然后引入注意力机制模块,分别捕获特征在通道和空间位置中的依赖关系,增强模型提取特征信息的有效性.结果表明,提出的方法在建立的军队标号数据集上的识别正确率达到95.75％,能有效应用于手绘军队标号的识别.  相似文献   

中高纬度大气低频模态研究进展   总被引：1，自引：0，他引：1  

张曼  许小峰  闵锦忠  高庆九 《气象科学》2015,35(6):799-806

大气低频模态是导致中高纬地区季节及气候变化的主要因素,加强低频模态动力机制的认识对于提高短期气候预测水平具有十分重要的科研意义和应用价值。由于中高纬大气低频环流本身的复杂性,关于其动力机制的研究仍然是大气动力学中重点难点问题。本文简单回顾了激发维持低频模态的前两种机制,即:外源强迫、气流的纬向非均匀性对大气低频模态的影响。从观测事实和模式结果出发,着重介绍了瞬变波与基本气流相互作用激发维持低频模态的第三种机制,且详细阐述了线性假设条件下,瞬变波与基本气流相互作用的动力机制。本文最后针对瞬变波与基本气流相互作用研究中一些尚未解决的问题进行了讨论。  相似文献   

WRF-Hybrid背景误差协方差调整在台风同化及预报中的应用研究   总被引：3，自引：1，他引：2  

沈菲菲  闵锦忠  许冬梅  王世璋 《气象科学》2015,35(2):150-159

利用雷达径向风单点试验和2006年8月超强台风"桑美"个例,首先研究了静态背景误差协方差的尺度化因子和方差在台风系统雷达资料同化中对台风路径和强度预报的影响。结果表明:在高时空分辨率的雷达资料同化中,较小的尺度化因子能显著改进对台风路径的预报;尺度化因子的影响比方差的影响更为显著。基于上述实验结果,进一步研究了WRFDA-Hybrid系统中"流依赖"控制变量的水平局地化和垂直局地化对台风预报的影响。试验结果表明:当"流依赖"的水平局地化距离与静态背景误差协方差的尺度化因子具有等效影响范围的时候,WRFDA-Hybrid能够得到比较合理的分析结果。同时针对雷达观测资料的空间分布特征,本文提出了一种新的基于雷达探测高度的垂直局地化方案,对台风的强度和路径预报均有显著的改进。  相似文献   

探测仪器特性曲线异常分析     

敬颖  闵锦忠  刘立辉  吴恒  徐爽 《气象科技》2015,43(4):601-606

探测仪器感应曲线发生变化,造成升速异常、等压面的温度、湿度错误、雷达〖CD*2〗气压高差偏大、时间〖CD*2〗高度线曲变化异常造成的规定高度上的风误差偏大,使部分资料或整份资料失真,影响探测准确性。本文主要从仪器的感应曲线变化后对各气象要素产生的影响进行分析,得出结论：不同的元件变性对气象要素产生的影响不同,气压变化的影响侧重于高差和升速,温度变化则侧重于规定等压面的温度绝对误差和规定等压面高度的偏差。采用绝对误差计算、加密气象要素计算等方法,结合图形、数据对比,可以确定感应曲线变化时间,从而及时、有效的对探测数据做出合适的处理,进一步提高探测数据的精准度。  相似文献   

Impact of Assimilating Radiances with the WRFDA ETKF/3DVAR Hybrid System on Prediction of Two Typhoons in 2012          下载免费PDF全文

XU Dongmei  HUANG Xiang-Yu  WANG Hongli  Arthur P. MIZZI  MIN Jinzhong 《Acta Meteorologica Sinica》2015,29(1):28-40

The impacts of AMSU-A and IASI (Infrared Atmospheric Sounding Interferometer) radiances assimila-tion on the prediction of typhoons Vicente and Saola (2012) are studied by using the ensemble transform ...  相似文献   

Contribution of close double white dwarfs to the Galactic gravitational wave foreground     

Jinzhong Liu  Yu Zhang  Zhanwen Han  Fenghui Zhang 《Astrophysics and Space Science》2010,329(1-2):297-303

This paper provides new detailed specifics and characteristics of the close double white dwarfs (CDWDs) LISA foreground noise floor using the newest information on the astrophysics with binary population algorithms, which were judged to satisfy the observations. We use the binary population synthesis approach of CDWDs in combination with the latest findings of synthesis models from Han (Mon. Not. R. Astron. Soc. 296:1019, 1998), here, specifically formation by the three evolutionary channels of (a) stable Roche lobe overflow plus common envelope (RLOF?+?CE), (b) CE plus CE, (c) exposed core plus CE. We collect resulting CDWDs in the frequency range of 10^?8 Hz to 10^?2 Hz and compare strength and number statistics per resolvable frequency bin to derive the properties of the noise floor and the nature of possible outliers that may become individually resolvable. We find resolvable outliers to be solely produced by CE?+?CE evolution; the other two channels contribute only to the unresolvable foreground noise. Within the CE?+?CE evolution a detailed look into the chemical buildup of the stars reveals dominantly double helium (He?+?He) WDs or carbon-oxygen CO?+?He WDs.  相似文献   

The light-weighted age and metallicity of Galactic globular clusters     

Yu Zhang  Fenghui Zhang  Zhanwen Han  Jinzhong Liu 《Astrophysics and Space Science》2010,329(1-2):255-260

Spectra synthesis is entering a new era with the availability of large and high-quality spectroscopic data and full spectrum fitting methods. Establishing the reliability whether the STARLIGHT code (a full spectrum fitting code, Cid Fernandes et al. (Mon. Not. R. Astron. Soc. 358:363, 2005)) is suitable to study the properties of various types of galaxies is vital to galaxy study. In testing this possibility, Galactic globular clusters (GCs) provide an excellent medium. Taking the 40 Galactic GCs as an example in our work, we analyze their integrated spectra from Schiavon et al. (Astrophys. J. Suppl. 160:163, 2005) and obtain their mixtures of stellar populations that best represents their composite nature. Through analyzing the distributions of stellar ages and metallicities respectively, we find that the stellar metallicity distribution is centered at a low value and the stellar age distribution is very scattered. To compare with the literature, we also calculate the light-weighted ages and metallicities of GCs, and we find that the light-weighted metallicities agree with the literature, while the light-weighted ages are lower than those of the literature. This demonstrates that STARLIGHT can be used to obtain the metallicities of GCs.  相似文献   

Present and projected degree days in China from observation,reanalysis and simulations   总被引：1，自引：0，他引：1  

Qinglong You  Klaus Fraedrich  Frank Sielmann  Jinzhong Min  Shichang Kang  Zhenming Ji  Xiuhua Zhu  Guoyu Ren 《Climate Dynamics》2014,43(5-6):1449-1462

Degree days are usually defined as the accumulated daily mean temperature varying with the base temperature, and are one of the most important indicators of climate changes. In this study, the present-day and projected changes of four degree days indices from daily mean surface air temperature output simulated by Max Planck Institute, Earth Systems Model of low resolution (MPI-ESM-LR) model are evaluated with the high resolution gridded-observation dataset and two modern reanalyses in China. During 1979–2005, the heating degree days (HDD) and the numbers of HDD (NHDD) have decreased for observation, reanalyses (ERA-Interim and NCEP/NCAR) and model simulations (historical and decadal experiments), consistent with the increasing cooling degree days (CDD) and the numbers of CDD (NCDD). These changes reflect the general warming in China during the past decades. In most cases, ERA-Interim is closer to observation than NCEP/NCAR and model simulations. There are discrepancies between observation, reanalyses and model simulations in the spatial patterns and regional means. The decadal hindcast/forecast simulation performance of MPI-ESM-LR produce warmer than the observed mean temperature in China during the entire period, and the hindcasts forecast a trend lower than the observed. Under different representative concentration pathway (RCP) emissions scenarios, HDD and NHDD show significant decreases, and CDD and NCDD consistently increase during 2006–2100 under RCP8.5, RCP4.5 and RCP2.6, especially before the mid-21 century. More pronounced changes occur under RCP8.5, which is associated with a high rate of radiative forcing. The 20th century runs reflect the sensitivity to the initial conditions, and the uncertainties in terms of the inter-ensemble are small, whereas the long-term trend is well represented with no differences among ensembles.  相似文献   

基于卷积神经网络的地铁保护区风险源识别北大核心CSCD     

闵星  黄品文  谭金祥 《测绘通报》2022,(10):162-165

城市轨道交通沿线的风险源识别是防止违规作业导致的安全事故的重要手段。为解决传统识别方法效率低、漏检率高、成本大等问题,本文基于无人机地铁保护区巡检系统,采用卷积神经网络对无人机采集的影像数据进行风险源识别。首先介绍无人机影像获取的流程,并在原始影像数据的基础上,通过数据增强的方式制作多角度、多尺度的风险源数据集;然后使用卷积神经网络建立风险源识别模型,对无人机采集影像中的风险源进行自动识别和定位。试验结果表明,多角度、多尺度风险源数据集的建立进一步提升了模型的识别准确率,且比传统方法具有效率高、成本低等优点。  相似文献   

宁南弧形构造带甘肃大沟—内蒙古乱井中上地壳电性结构          下载免费PDF全文

闵刚  程建华尹秉喜蔡学林夏时斌 《中国地质》2014,41(5):1464-1475

利用大地电磁探测方法在宁南弧形构造带内蒙古乱井—甘肃大沟段进行了中上地壳电性结构特征研究,通过二维反演获得了研究区的电性结构模型,模型清楚揭示出了该区典型的电性结构特征:(1)中上地壳电性结构整体表现为"碎块状"的构造特征,其中走廊构造带总体表现为相对低阻,北祁连碰撞造山带总体表现为相对高阻;(2)海原地震震源区的震源断裂所反映的低阻带构造样式既不像走滑断裂那样陡峭,也不像逆冲断裂那样平缓,而是兼具走滑与逆冲断裂带的双重特征;(3)研究区壳内低阻层呈现不连续分布,总体表现为南深北浅的构造样式,一般都终止于高阻地块边缘或与逆冲推覆构造的滑脱面相交汇处;(4)清水河裂褶带内发育的高阻地块可能为晚古生代或早中生代发育在元古宙基底上的古隆起,为该区燕山期构造运动提供了深部大地电磁资料证据。  相似文献