排序方式: 共有13条查询结果,搜索用时 703 毫秒
1.
Facundo L. Poblet Francisco Azpilicueta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2275-2289
The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ~27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ~27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation. 相似文献
2.
3.
随着相位噪声参数广泛的应用,其测量技术得到不断的发展,除了传统模式的相位噪声测量系统外,一些采用新技术的测量系统不断的被开发出来,包括应用互相关原理的信号源分析仪和应用高速数字信号处理的直接数字化相位噪声分析仪,它们各具优势,也将会得到广泛应用。 相似文献
4.
5.
利用不同时刻系统测量噪声具有独立同分布的特点,对脉冲响应进行相关处理,可以提高信噪比。为解决传统的基于脉冲响应的模态辨识算法的辨识精度问题,用某点脉冲响应同参考点响应之间的相关函数代替该点的脉冲响应以形成基于脉冲响应相关函数的模态辨识算法,并从理论上证明脉冲响应相关函数算法的辨识精度优于传统的脉冲响应算法。通过对一个四自由度系统模态频率和阻尼比的仿真辨识,验证了脉冲响应相关函数辨识算法的有效性。 相似文献
6.
在常规自相关粒子图像测速(PIV)系统的基础上,发展了一个采用CCD像机的互相关粒子图像测速系统。用这一新系统测量了对抗流流场的结果表明,这一技术克服了自相关粒子图像测速技术在测量具有滞止点的流场中的困难。实验说明,与自相关粒子图像测速技术相比,这一技术更快捷有效。 相似文献
7.
8.
对航天测控信号进行滤波处理,有利于改善信号品质,提高系统的测量性能。针对航天测控信号中的差分单程测距(DifferentialOne-wayRanging, DOR)信标信号等侧音信号,提出了基于非抽取小波包变换(Un-decimatedWaveletPacketTransform,UWPT)的滤波改进算法。该算法以功率平坦度为准则,判断某一节点是否需要继续分解。改进算法克服了以能量聚焦度为准则时算法误判停止分解或多重分解算法复杂、计算量大等的缺点,同时解决了阈值不易确定的问题。仿真结果表明改进算法在降低算法复杂度的同时,滤波性能相对有所提高。最后采用改进算法对仿真信号和在轨卫星数据进行处理,结果表明滤波后仿真信号差分相位估计精度提高约3倍、实测数据差分相位估计精度提高0.72倍。 相似文献
9.
10.