Spectrum Analysis of Wind Profiling Radar Measurements          下载免费PDF全文

RUAN Zheng  MU Ruiqi  WEI Ming  GE Runsheng 《Acta Meteorologica Sinica》2014,28(4):656-667

Unlike previous studies on wind turbulence spectrum in the planetary boundary layer, this investigation focuses on high-altitude （1-5 km） wind energy spectrum and turbulence spectrum under various weather conditions. A fast Fourier transform （FFT） is used to calculate the wind energy and turbulence spectrum density at high altitudes （1-5 km） based on wind profiling radar （WPR） measurements. The turbulence spectrum under stable weather conditions at high altitudes is expressed in powers within a frequency range of 2 × 10-5-10-3 s-1, and the slope b is between -0.82 and -1.04, indicating that the turbulence is in the transition from the energetic area to the inertial sub-range. The features of strong weather are reflected less obviously in the wind energy spectrum than in the turbulence spectrum, with peaks showing up at different heights in the latter spectrum. Cold windy weather appears over a period of 1.5 days in the turbulence spectrum. Wide-range rainstorms exhibit two or three peaks in the spectrum over a period of 15-20 h, while in severe convective weather conditions, there are two peaks at 13 and 9 h. The results indicate that spectrum analysis of wind profiling radar measurements can be used as a supplemental and helpful method for weather analysis.  相似文献   

南黄海磁性基底特征分析和综合解释     

邢涛  张训华  张向宇 《海洋与湖沼》2014,45(5):946-953

本文利用南通幅区域地质调查的重磁异常数据,在重磁异常特征分析的基础上,采用一维频谱分析法对南黄海进行磁性基底反演。结果表明:南黄海属于扬子块体向海域的延伸,具有元古代结晶基底和古生代褶皱基底的双基底结构,其磁性基底深度在2—10km之间变化,是褶皱基底与磁性层最小埋深的结合,在坳陷和隆起上表现不同。通过利用综合地质和地球物理综合方法,对南黄海区域的四大构造单元华北—狼林地块、扬子—京畿地块、华南—岭南地块、东海大陆架进行重磁异常变化特征和磁性基底特征分析,为研究区断裂等区域构造特征解释提供了依据。  相似文献   

风浪槽内风浪外频谱谱形的一些特征     

管长龙  刘珂  赵栋梁 《中国海洋大学学报(自然科学版)》2000,30(1):1-6

利用实验室风浪槽内测得的波面序列资料估计风浪外频谱。通过与实测风浪内频谱的比较,研究实测风浪外频谱的谱形特征,探讨海浪外频谱与内频谱的相似性问题。此外,还检验一种理论海浪外频谱。  相似文献   

陆丰凹陷韩江组旋回地层学分析及天文年代标尺的建立     

朱春霞  张尚锋  王雅宁  徐恩泽 《海洋地质前沿》2022,38(4):42-52

  相似文献   

泥石流高分辨率遥感影像频域特征提取方法及应用     

张悦  张锦 《测绘通报》2023,(3):111-115

在遥感影像上深入研究泥石流的相关特征条件对泥石流的分析治理具有十分重要的现实意义。本文将泥石流不同流域分区的高分辨率遥感影像从空间域转换到频率域,基于频谱分析与频域滤波,从全局和局部建立了频谱特征和泥石流流域分区特征之间的关联,并利用频域特征对泥石流高分辨率遥感影像中不同流域分区进行识别,用支持向量机进行试验验证。结果表明,对于泥石流遥感影像,除了地物光谱特性以外,充分利用频域特征可以有效地分析和识别泥石流不同的流域分区,且识别精度最高达到95%,从而对泥石流的形成过程及不同区域进行定性和定量分析,为泥石流的防治工作提供了科学依据。  相似文献   

Dynamic responses under the excitation of pulse sequences   总被引：6，自引：3，他引：3  

戴君武  Mai Tong  George C.Lee  齐霄斋  白文婷 《地震工程与工程振动(英文版)》2004,3(2):157-169

This paper studies the dynamic responses of SDOF system under pulse-dominant excitations. The purpose of the study is to prepare for scrutiny of some near-field pulse-dominant ground motions and their potential to cause structural damage. Extending the single pulse dynamics, we consider the effect of pulse sequences. This kind of excitation was particularly obvious in some of previous earthquakes such as Northridge (1994) and Chi-Chi (1995). Based on the duration,peak and rise and decay era of the main pulse as well as its relationship with the predecessor and successor pulses, we propose a classification for the pulse sequences. Consequent studies have been carried out for acceleration, velocity and displacement response spectra of the main pulse with either a predecessor or a successor pulse. The analysis also includes general response behaviors in different fundamental period segments and special aspects of response at certain points (e.g., the corresponding peak points).  相似文献   

Color-Redshift Relations and Photometric Redshift Estimations of Quasars in Large Sky Surveys     

Xue-Bing Wu  Wei Zhang  Xu Zhou Department of Astronomy  School of Physics  Peking University  Beijing  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2004,4(1):17-27

With a recently constructed composite quasar spectrum and the X2 minimization technique, we describe a general method for estimating the photometric redshifts of a large sample of quasars by deriving theoretical color-redshift relations and comparing the theoretical colors with the observed ones. We estimated the photometric redshifts from the 5-band SDSS photometric data of 18678 quasars in the first major data release of SDSS and compared them with their spectroscopic redshifts. The difference is less than 0.1 for 47% of the quasars and less than 0.2 for 68%. Based on the calculation of the theoretical color-color diagrams of stars, galaxies and quasars both on the SDSS system and on the BATC system, we expect that we would be able to select candidates of high redshift quasars more efficaciously with the latter than with the former, provided the BATC survey can detect objects with magnitudes fainter than 21.  相似文献   

Blazar天体中光学射电大爆发的频谱演化     

钱善Jie 《天文学报》1997,38(3):239-249

本文讨论Ｂｌａｚａｒ天体中光学射电大爆发频谱演化的理论模型．考虑沿喷流传播的相对论性激波所注入或加速的相对论性电子，受到康普顿、同步辐射和绝热膨胀三种损耗，并计及相对论电子能谱的高能截断．假定喷流轴线与观测者方向构成很小角度．文中给出了大爆发频谱三阶段连续演化的特性，即康普顿阶段，同步辐射阶段和绝热膨胀阶段的爆发特性．频谱演化用（Ｓｍ－ｖｍ）关系表达（见图２，图中Ｓｍ为频谱反转流量，ｖｍ为反转频率），它与一些Ｂｌａｚａｒ天体中观测到的典型形式相符合．  相似文献   

固体潮潮汐因子的特征频谱及其应用     

蒋骏  张雁滨  周翠屏 《大地测量与地球动力学》1994,(2)

本文应用非线性谱分析中的最大熵谱分析方法（ＭＥＭ）、和一般线性功率谱的分析方法，对固体潮潮汐因子的时间序列进行了综合研究，指出固体潮潮汐因子的时间序列中普遍存在明显的半月左右周期的特征频谱；将其应用于地震前兆的分析与探索，对固体潮潮汐因子特征频谱中的前兆变化特征进行了解释，得出结论：半月左右周期的频率域，是固体潮观测中前兆响应的一个重要主频域。  相似文献   

利用磁异常Zα的频谱反演二度体磁化方向     

甘西 《物探化探计算技术》1991,13(1):87-90

  相似文献