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国家自然科学基金(41204120)

作品数:6 被引量:27H指数:4
相关作者:顾旭东倪彬彬周晨赵正予王豪更多>>
相关机构:武汉大学北京大学中国纺织大学更多>>
发文基金:国家自然科学基金中国博士后科学基金更多>>
相关领域:天文地球电子电信理学更多>>

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First observations of low latitude whistlers using WHU ELF/VLF receiver system被引量:17
2017年
The recently developed high-quality WHU ELF/VLF receiver system has been deployed in Suizhou, China (geomagnetic lati- tude 21.81°N, longitude 174.44°E, L=1.16) to detect low latitude extremely-low-frequency (ELF: 0.3-3 kHz) and very-low-frequency (VLF: 3-30 kHz) emissions originating from either natural or artificial sources since February 2016. Dur- ing the first-month operation of the receiver system, a total of 3039 clear whistlers have been recorded at this low latitude sta- tion with the majority (97.0%) occurring on 28 February and 1 March 2016. Observed whistlers manifest various types includ- ing single one-hop, echo train, multi-flash, and multi-path. They tend to intensify after local midnight, reach the peak around 04435 LT, and then weaken quickly. Both features of lower cutoff frequencies of most whistlers below -1.6 kHz and almost uniform dispersion for many successive multi-flash whistlers suggest that these whistlers propagate along the geomagnetic field lines in the duct mode. The computed dispersion varies between -15 s1/2 and 23 s1/2 for observed one-hop whistlers and is greater than 50 sm for three-hop echo train whistlers, indicating that the whistlers observed at the Suizhou station are low lati- tude whistlers.
CHEN YanPingNI BinBinGU XuDongZHAO ZhengYuYANG GuoBinZHOU ChenZHANG YuanNong
关键词:WHISTLERSDISPERSION
Coupling of electrons and inertial Alfven waves in the top-side ionosphere
A one dimensional kinetic model is constructed to simulate the electron acceleration by inertial Alfven waves....
Run ShiHuixin LiuA.YoshikawaBeichen ZhangBinbin Ni
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A detailed investigation of low latitude tweek atmospherics observed by the WHU ELF/VLF receiver:2.Occurrence features and associated ionospheric parameters被引量:9
2020年
As a companion paper to Zhou RX et al.(2020),this study describes application of the automatic detection and analysis module to identify all the tweek atmospherics detectible in the WHU ELF/VLF receiver data collected at Suizhou station during the period of 3 February through 29 February 2016.Detailed analysis of the identified low-latitude tweek events reveals that the occurrence rate varies considerably—from 800 to 6000 tweeks per day,and exhibits a strong diurnal and local time dependence,the peak occurring before local midnight.The diurnal variation of identified tweeks was similar to that of the lightning data obtained by the World-Wide Lightning Location Network(WWLLN)..Estimates of the propagation distance and ionospheric reflection height of tweek atmospherics suggest that the majority(~92%)of the low latitude tweeks originate from the lightning activity within a radius of 4000 km and that they are very likely to reflect from the lower ionospheric D-region at the height range of 75–85 km.At these lower ionospheric reflection altitudes,~74%of the corresponding electron densities from the tweek spectral measurements are within 24.5–27.5 cm^-3.The daily variation of estimated D-region electron densities in the considered period(February 2016)also exhibits a small overall increasing trend from early to later in the month.
Juan YiXuDong GuWen ChengXinYue TangLong ChenBinBin NiRuoXian ZhouZhengYu ZhaoQi WangLiQing Zhou
基于范阿伦卫星观测数据的等离子体层嘶声全球分布的统计分析被引量:6
2017年
等离子体层嘶声是引起辐射带电子投掷角散射进而沉降到地球大气层的重要物理机理,也被认为是导致地球内、外辐射带之间槽区形成的主因,因此研究空间等离子体层嘶声的全球分布特性具有重要科学意义.本文利用范阿伦探测双星中的A星从2012年9月到2015年5月长达33个月的高质量波动观测数据,详细计算了等离子体层嘶声的平均波幅和发生率,建立了等离子体层嘶声的全球分布数据库,并细致分析了其场强幅度随地磁活动水平、磁壳值L、地磁纬度、磁地方时的统计变化规律.结果表明,等离子体层嘶声的平均波幅与地磁活动剧烈程度具有很强的相关性,并表现出明显的昼夜不对称性.随着地磁活动的增强,日侧等离子体层嘶声的平均波幅相应增大,增强的区域集中在2.530 pT)的等离子体层嘶声的变化特性正好相反,日侧发生率增大,夜侧发生率减小.在各种地磁活动条件下,磁赤道面附近及中纬地区等离子体层嘶声都广泛存在,波动幅度位于5—30 pT范围的嘶声发生概率最大.以上统计观测结果为现有的等离子体层嘶声全球分布模型提供了合理、可靠的补充,充分说明不同场强幅度的等离子体层嘶声在2
项正谈家强倪彬彬顾旭东曹兴邹正洋周晨付松石润赵正予贺丰明郑程耀殷倩王豪
基于试验粒子模拟的电离层人工调制激发的极低频和甚低频波对磁层高能电子的散射效应被引量:2
2014年
电离层调制加热能够有效激发极低频和甚低频(ELF/VLF)波,其中向上传播进入磁层的ELF/VLF波能够与高能电子发生共振相互作用,具有人工沉降高能电子、消除辐射带等潜在实际用途.本文综合运用射线追踪和试验粒子方法模拟电离层人工激发的单频ELF/VLF波在电离层和磁层的传播,以及在外辐射带层与高能电子的共振相互作用过程,通过投掷角和能量散射系数评估人工ELF/VLF波对磁层高能电子的共振散射效应.研究表明,电离层人工ELF/VLF波传播到磁层后呈现高倾斜性,传播所能跨域的空间范围主要取决于加热的纬度位置和调制频率.在内辐射带,与~100 keV到几个MeV高能电子发生一阶共振相互作用的为>10 kHz的VLF波段;在外辐射带,为几百Hz到1 kHz的ELF波段.对于L=4.5的外辐射带,试验粒子模拟结果显示,单个粒子在人工ELF波作用下投掷角和能量(α,E)的改变具有随机性,而所有试验粒子平均化的?α2和?E2随时间呈现出近似线性的增大,说明波粒共振散射过程体现出整体性.基于试验粒子模拟得到的共振散射系数表明,幅度为10 pT的人工ELF波可在外辐射带的磁赤道局地对1 MeV电子产生较强的投掷角散射效应,进而影响高能电子的损失、沉降等动力学过程.当人工ELF/VLF波在传播过程中变得高度倾斜,不仅最基本的一阶共振十分重要,高阶共振散射也具有较大效应.这些定量分析结果表明,通过电离层加热激发人工ELF/VLF哨声波来沉降、消除辐射带高能电子具有可行性.
常珊珊倪彬彬赵正予汪枫李金星赵晶晶顾旭东周晨
甚低频接收机的开发与应用被引量:4
2018年
甚低频(VLF)信号被广泛应用于地球空间环境地基监测、全球航海通信与导航等领域。该系统在传统甚低频接收天线的基础上,进行了天线小型化的改进,通过阻抗匹配,改善了系统灵敏度。该系统包括磁环天线,低噪声模拟前端,数据采集与传输模块以及同步模块。磁环天线采用罗德施瓦茨公司生产的HZ-10型磁环天线。模拟前端分为基于差分结构的低噪放大器和巴特沃斯滤波器两部分,在带宽1~50 kHz内增益高达80 d B。数据采集和传输模块采用基于FPGA和USB 2.0总线的方法。在武汉(30.54°N,114.37°E)测得宽带甚低频波谱结果初步验证了该地基甚低频接收系统的有效性和可行性。对人工甚低频MSK调制信号进行幅度解调处理,得到其幅值的日变化曲线图。
刘卿顾旭东倪彬彬
关键词:阻抗匹配
A detailed investigation of low latitude tweek atmospherics observed by the WHU ELF/VLF receiver:Ⅰ. Automatic detection and analysis method被引量:13
2020年
As a dispersive wave mode produced by lightning strokes, tweek atmospherics provide important hints of lower ionospheric(i.e., D-region) electron density. Based on data accumulation from the WHU ELF/VLF receiver system, we develop an automatic detection module in terms of the maximum-entropy-spectral-estimation(MESE) method to identify unambiguous instances of low latitude tweeks.We justify the feasibility of our procedure through a detailed analysis of the data observed at the Suizhou Station(31.57°N, 113.32°E) on17 February 2016. A total of 3961 tweeks were registered by visual inspection;the automatic detection method captured 4342 tweeks, of which 3361 were correct ones, producing a correctness percentage of 77.4%(= 3361/4342) and a false alarm rate of 22.6%(= 981/4342).A Short-Time Fourier Transformation(STFT) was also applied to trace the power spectral profiles of identified tweeks and to evaluate the tweek propagation distance. It is found that the fitting accuracy of the frequency–time curve and the relative difference of propagation distance between the two methods through the slope and through the intercept can be used to further improve the accuracy of automatic tweek identification. We suggest that our automatic tweek detection and analysis method therefore supplies a valuable means to investigate features of low latitude tweek atmospherics and associated ionospheric parameters comprehensively.
RuoXian ZhouXuDong GuKeXin YangGuangSheng LiBinBin NiJuan YiLong ChenFuTai ZhaoZhengYu ZhaoQi WangLiQing Zhou
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