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张衡一号卫星感应式磁力仪(Search Coil Magnetometer,SCM)探测到了大量的低频电磁波动数据.本文探索从中自动识别闪电哨声波(Lightning Whistler,LW)的算法,相关结果对进一步研究空间天气闪电事件的时空变化规律具有重要研究意义.首先,以20 s的时间窗提取SCM原始波形数据,再对其做短时傅里叶变换(Short-Time Fourier Transform,STFT)得到时频图;接着,以LW在时频图中呈现明显的L形态特征为依据创建LW时频图像数据集,该数据集包括316个LW时频图,8000个非闪电哨声波的时频图;再对时频图像进行灰度化处理和尺度缩放处理以降低计算维度,同时增强闪电哨声波特征;通过设计模糊卷积核,对图像进行卷积计算以滤除大量阶跃边缘信息的影响;基于LW的形态特征设计L形态卷积核,对图像进行卷积处理以进一步增强图像中的L形态特征.最后,将增强后的L特征图输入支持向量机(Support Vector Machines,SVM)进行分类识别.大量数据处理实验结果表明:本文提出的闪电哨声波自动识别方案有效,其识别效果在精度、召回率、F1值(F1 score)和接受者操作特性曲线面积(Area Under Curve,AUC)指标上均达到94%以上. 相似文献
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地震电磁卫星的辅助数据处理是卫星数据处理分系统的一部分,它为卫星科学目标的实现提供重要的辅助信息.本文在参考法国地震电磁卫星DEMETER和探测双星的辅助数据等基础上,对我国地震电磁卫星的辅助数据进行了定义和分类;介绍了原型系统采用的JNI技术及软件架构设计;根据每类辅助数据的内容和特点,给出了各种辅助数据的处理流程,并对其处理方法分别进行了分析;最后对卫星辅助数据处理及原型系统设计进行了总结.本文所述内容和方法是我国地震电磁卫星数据处理的一个前期准备工作,将服务于利用地震电磁卫星进行地震预报. 相似文献
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等离子体波的空间分布在木星磁层高能电子动力学过程中起着重要的作用.现有大多数对木星磁层哨声波的观测仅限于|λ|≤15°的磁纬范围内,但是最新的JUNO卫星WAVES仪器提供的波动数据使得更高纬度、更广区域范围内的等离子体波动分布研究成为可能.本文通过对JUNO卫星WAVES仪器数据进行分析处理,详细研究了木星磁层哨声波的空间分布特性.观测表明,存在位于高L_J、高磁纬的木星磁层哨声波,它们广泛分布于距木星中心距离35~75个木星半径、磁纬为|λ|≤30°的空间区域.分析研究发现,WAVES仪器观测的木星磁层哨声波幅度一般为几个pT,远小于地球磁层哨声波的强度.木星磁层哨声波幅会随着L_J的增大缓慢增加,也会随着磁纬的减小趋向平缓变化.基于以上观测事实,本文利用指数幂函数分别拟合得到木星磁层哨声波幅随L_J和磁纬变化的经验模型.该模型将有助于精确理解哨声波对木星磁层高能电子动力学过程的重要影响. 相似文献
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地震孕育过程中激发的电磁波穿过大气层进入太空,引起电离层物理参量发生变化,这些扰动信号可被卫星记录下来,因此电磁卫星作为一种监测预测地震的新手段越来越受到重视.卫星记录的数据具有时空同步变化性、数据量大等特点,需要采用多种数据处理方法进行分析.本文分析了卫星观测的地震前兆电场数据服务的不同需求,对地震电离层异常分析的不同阶段所采用的数据处理方法进行了梳理和总结,指出了不同方法的适应条件和环境,对几种典型的算法给出了实例分析效果.这为利用电磁卫星进行数据分析和研究的工作者提供了参考,具有现实意义. 相似文献
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法国DEMETER(Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions)卫星是世界上第一颗专门针对地震电离层扰动监测的电磁卫星, 于2004年发射, 2010年底结束运行, 共在轨飞行6.5年, 获得3万多条整轨数据, 为地震监测及电离层物理研究提供了坚实的数据基础。 全球科学家利用这颗卫星的数据开展了大量的地震应用研究, 发表文章上百篇, 将电磁卫星的地震应用研究推向了新的阶段。 中国第一颗电磁监测试验卫星CSES(China Seismo-Electromagnetic Satellite)于2018年2月2日成功发射, 目前已完成在轨测试并交付使用, 科学数据也已正式对外发布。 如何充分发挥CSES卫星的应用效能, 将空间电磁监测向业务化运行转化, 总结和思考DEMETER卫星的技术进步、 研究成果及曾经出现过的问题, 十分重要。 因此, 本文着重介绍DEMETER卫星在地震监测应用领域的代表性研究进展, 并结合CSES卫星的设计和运转实践, 对未来空间地震电磁探测及科学研究的发展方向进行一些初步讨论。 相似文献
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中国地震电磁监测试验卫星张衡一号(ZH-1)已于2018年2月2日成功发射,正在开展卫星数据在轨测试,并对卫星数据质量进行判定.本文对ZH-1卫星2018年5月至6月夜侧的VLF频段电场功率谱数据进行了分析.通过分析位于不同L值、具有不同发射频率的多个VLF人工源上空的卫星重访轨道观测数据,发现ZH-1卫星记录的人工源信号电场变化标准差与DEMETER卫星记录电场变化标准差几乎一致,说明ZH-1卫星观测数据具有较好的稳定性.通过重访轨道均值与全波模型计算结果对比,发现两者在数值上较为接近,在形态上较为一致,说明ZH-1卫星VLF频段电场功率谱数据具有一定的可靠性.此外,研究了VLF人工源上空及共轭区的电场分布特征和电波传播规律,并与DEMETER卫星的结果进行了对比,结果表明VLF人工源产生的电磁辐射穿透电离层后以导管或者非导管的哨声波模向共轭区传播,因为传播过程中的朗道阻尼,共轭区的电场能量比辐射源顶空更小.VLF人工源位于L1.5时,电磁波传播更容易发生非导管传播,VLF人工源信号导管传播模式在共轭区的电场响应相对于共轭点会发生一定程度北向偏移. 相似文献
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本研究主要利用张衡一号电磁卫星(CSES)记录的电磁场波形数据,研发了电磁波波矢量分析工具,该工具包提供电磁波形频谱变换、奇异值分解(SVD)方法以及坡印廷能流计算功能.选取了张衡一号卫星在ULF/ELF/VLF频段观测到的哨声波、准周期辐射、电离层嘶声波等典型波动事件,开展了频谱分析和波矢量分析.通过与DEMETER卫星的对比观测研究,验证了算法的正确性,并且初步探讨了这些波动的传播特征,其结果也验证了张衡一号卫星在电磁场观测方面具有良好的性能.本研究研发的波矢量分析工具包可直接运用到张衡一号卫星的常规数据处理和科学分析应用中. 相似文献
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相对已经在轨运行的极轨卫星,搭载在静止卫星上的闪电成像仪能够提供全天候、无间断的闪电探测,是目前全球卫星闪电探测的方向.本文分析云不同特性对云顶闪电信号的影响,以及云高对静止卫星闪电定位的订正分析,将对静止卫星闪电成像仪的研发及其业务化运行提供技术支撑.研究中,通过建立云中闪电传输模型,模拟云中闪电传输.由于云粒子散射,云的体积、光学厚度和形状,以及闪电在云中发生的深度,都影响云中或云间闪电信号传输到云顶的能量衰减和持续时间,其持续时间可能超过已知静止卫星闪电成像仪假设的2 ms成像积分时间间隔,这样不能保证所有的闪电信号在一帧图像内探测到.但是,云粒子散射对云顶闪电的水平位置影响不大,闪电成像仪定位的云顶闪电可代表云中或云间的闪电位置.同时,在传统静止卫星图像定位模型的基础上,建立了闪电定位的云高订正模型.根据该模型,当云顶高度为10 km,云高所引起的闪电定位最大误差达到经向0.5379°、纬向0.2273°,超过已知静止卫星闪电成像仪假设的地面探测单元大小,有必要进行订正. 相似文献
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J. Bošková F. Jiříček E. E. Titova T. A. Yakhnina 《Studia Geophysica et Geodaetica》1990,34(3):269-277
Summary After a fractional-hop whistler, a trace of limited frequency range with somewhat higher dispersion, markedly growing when approaching the lower cutoff frequency, is frequently observed on spectrograms of broadband VLF measurements made by satellites moving in the outer ionosphere. This phenomenon, which we have called LHR spheric, has been studied on VLF measurements made by the Interkosmos-14 satellite in the height range of 500–1700 km. The results show that LHR spherics are created by the same mechanism as LHR whistlers that sometimes appear after ducted whistlers. In this event, it is a part of the electromagnetic energy radiated by a lightning flash which, on passing trough the ionosphere, has been transformed to quasi-electrostatic resonance waves. They reach the satellite in the same way as whistler-mode waves. Transformation of a part of the energy radiated by a lightning flash to electrostatic quasi-resonance waves is possible in the ionosphere due to the scattering of the original whistler wave on small-scale turbulence. 相似文献
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The correlation of whistler occurrence rate at a low latitude with thunderstorm activity at its conjugate region and with solar activity 总被引:1,自引:0,他引:1
The correlations of occurrence rate of whistlers in January during one solar cycle (1977–1987) at a low latitude station (Yamaoka, geomag. lat. 25°, L=1.26) with thunderstorm activity near its conjugate region and also with solar activity have been investigated, and it is found that the occurrence rate has no correlation with the lightning flashes near the conjugate point, while it is negatively correlated with solar activity. On the basis of these findings it is suggested that the ionospheric absorption is of major importance in the long-term variation of whistler occurrence rate, with the duct formation being of secondary effect, while the lightning activity is only a necessary condition for whistler occurrence. 相似文献
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《Journal of Atmospheric and Solar》2000,62(17-18):1719-1733
Attention is focused here on the quasilinear and nonlinear physics of cyclotron interactions between magnetospheric whistler mode waves and energetic electrons on dipolar geomagnetic flux tubes. These interactions can lead to the generation of noise-like emissions or phase-coherent discrete signals in the frequency-time domain. In the magnetosphere noise-like emissions called hiss are accompanied by a smooth electron precipitation pattern. Examples of discrete emissions are ELF/VLF chorus or VLF emissions triggered by whistlers from lightning or by radio transmitters on the ground. The rapid temporal variations of these signals are associated with fine structure of the distribution function of the radiation belt electrons, such as a transient step-like deformation or a well-organized beam, which are prepared by initial noise-like emissions or by a quasimonochromatic whistler–wave packet, respectively. These cause the properties of the electrons, which may be observed on a satellite, to evolve rapidly in time and on relatively short spatial scales. Bursts of precipitating electrons occur, and can contribute significantly to depleting the radiation belts. Recent results on improvements in the theoretical understanding of such processes and on new observations of magnetospheric electrons and whistler-mode waves are presented. 相似文献
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V. P. Sivokon’ V. V. Bogdanov G. I. Druzhin N. V. Cherneva A. V. Kubyshkin D. V. Sannikov I. V. Agranat 《Geomagnetism and Aeronomy》2014,54(6):858-864
Analysis of the experimental data obtained at Paratunka observatory (53.02° N, 158.65° E; L = 2.3) has revealed a nonstandard form of whistlers involving spectral lines that are symmetric with respect to the whistler. We have shown that this form is most likely due to the amplitude modulation of whistlers by electromagnetic pulses with a length of around 1 s and carrier frequency of around 1.1 kHz. We have suggested that these pulses could be emitted by the auroral electrojet modified by heating radiation from the HAARP facility (62.30° N, 145.30° W; L > 4.2). 相似文献
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J. Verö B. Zieger J. Szendröi M. Vellante J. Střesgtik H. Lühr A. Best A. Körmendi J. Lichtenberger T. Ménesi P. Bencze F. Märcz V. Wesztergom 《Annales Geophysicae》2000,18(8):866-873
Simultaneous whistler records of one station and geomagnetic pulsation (Pc3) records at three stations were compared. In a previous study correlation was found between occurrence and L value of propagation/excitation for the two phenomena. The recently investigated simultaneous records have shown that the correlation is better on longer time scales (days) than on shorter ones (minutes), but the L values of the propagation of whistlers/excitation of pulsations are correlated, i.e. if whistlers propagate in higher latitude ducts, pulsations have periods longer than in the case when whistlers propagate in lower latitude ducts. 相似文献