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361.
362.
V.V. Hegai A.D. Legen’ka V.P. Kim K. Georgieva 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
A study of the critical frequency foF2 variations after the large earthquake (Ms = 8.1) which occurred on 29 September, 2009 in the region of Samoa Islands in the Pacific Ocean is carried out using data of the ionospheric station of Kwajalein. The epicenter of the earthquake was located at about 184 km southwest from Apia (the capital of West Samoa). It was found that wave-like perturbations of foF2 were observed for ∼3 h above the station (located approximately 3560 km northwest from the epicenter). The amplitude of the disturbance was as large as ∼20% of the average magnetic quiet day foF2 values. A comparison of the observed perturbations of foF2 with the ones detected at Stanford ionospheric station after the Alaska earthquake of 28 March 1964 (Ms = 8.4) showed a close similarity of the wave-like perturbations of foF2 in both cases. 相似文献
363.
M.V. Klimenko V.V. Klimenko I.E. Zakharenkova S.A. Pulinets B. Zhao M.N. Tsidilina 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The problems of physical explanation and possible mechanisms of the seismo-ionospheric effects formation are under discussion now. There are proposed different mechanisms of such effects, for example, large- and small-scale internal gravity waves (IGWs), atmospheric electric field, electromagnetic fields and emissions. However, the appearance of local large-scale seismo-ionospheric anomalies in Total Electron Content (TEC) is possible to explain only by two mechanisms: an atmospheric electric field and/or small-scale IGWs. In this paper, the simulation results for reproduction of the observed seismo-ionospheric great positive effects in TEC prior to strong Wenchuan earthquake are presented. The obtained results confirm the proposed mechanism of seismo-ionospheric effects formation by the penetration of the seismogenic electric field from the atmosphere into the ionosphere. It is suggested that so great TEC enhancement observed 3 days prior to Wenchuan earthquake could be explained by combined action of seismogenic vertical electric field and IGWs generated by the solar terminator. 相似文献
364.
给出用于毫米波频段精确测量介质片复介电常数的准光开放腔系统的误差分析,说明了近似理论引起的误差和被测量提取不准引起的误差。推导了相关的公式,给出了分析的数值结果和测量结果。 相似文献
365.
螺栓连接件使结构易于安装或拆卸,同时还可以承受较大的载荷,广泛应用于航空航天结构中。然而,螺栓在复杂服役环境中很容易发生松动,因此准确监测螺栓预紧力对于确保结构的可靠性和安全性具有重要意义。经过多年的发展,基于超声导波的结构健康监测方法逐渐成为螺栓连接松动监测的重要技术手段之一。对典型的螺栓预紧力导波监测方法进行了综述,包括导波能量耗散法、时间反转法、接触声学非线性法和混沌超声法等方法,介绍了这些方法的基本原理和发展现状。同时,通过实验将目前应用较多的导波能量耗散法、时间反转法进行了对比,结果表明时间反转法的监测灵敏度更高。 相似文献
366.
Chian A.C.-L. Borotto F.A. Rempel E.L. Macau E.E.N. Rosa R.R. Christiansen F. 《Space Science Reviews》2003,107(1-2):447-461
Space plasmas are dominated by waves, instabilities and turbulence. Dynamical systems approach offers powerful mathematical
and computational techniques to probe the origin and nature of space environment turbulence. Using the nonlinear dynamics
tools such as the bifurcation diagram and Poincaré maps, we study the transition from order to chaos, from weak to strong
chaos, and the destruction of a chaotic attractor. The characterization of the complex system dynamics of the space environment,
such as the Alfvén turbulence, can improve the capability of monitoring Sun-Earth connections and prediction of space weather.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
367.
368.
Distributions with excess numbers of superthermal particles are common in space environments. They are well modelled by the
isotropic kappa distribution, or, where magnetic effects are important, the kappa-Maxwellian. This paper presents a review
of some studies of electrostatic and electromagnetic waves in such plasmas, based on the associated generalized plasma dispersion
functions, Z
κ and Z
κM. In particular, the effects of low values of κ are considered, i.e. strongly accelerated distribution functions. Recently the full susceptibility tensor for oblique propagation of electromagnetic
waves in a kappa-Maxwellian magnetoplasma has been established and has been applied to the study of whistler waves. 相似文献
369.
Leon Ofman 《Space Science Reviews》2005,120(1-2):67-94
Coronal holes have been identified as source regions of the fast solar wind, and MHD wave activity has been detected in coronal
holes by remote sensing, and in situ in fast solar wind streams. I review some of the most suggestive wave observations, and
discuss the theoretical aspects of MHD wave heating and solar wind acceleration in coronal holes. I review the results of
single fluid 2.5D MHD, as well as multi-fluid 2.5D MHD models of waves in coronal holes, the heating, and the acceleration
of the solar wind be these waves. 相似文献
370.
用高分辨率的TVD格式对复杂的激波反射过程做数值模拟。激波斜壁反射计算结果与实验干涉照片、压力分布、密度分布均符合得很好。通过对运动激波绕射凸起物的数值模拟,得到非定常反射流场发展过程及复杂流场间断的清晰图谱。 相似文献