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951.
Planetary waves in coupling the lower and upper atmosphere 总被引:1,自引:1,他引:1
A.I. Pogoreltsev A.A. Vlasov K. Frhlich Ch. Jacobi 《Journal of Atmospheric and Solar》2007,69(17-18):2083
The purpose of the paper is to answer the question if planetary waves (PW) are capable of propagating into the thermosphere. First the simplest vertical structure equation of the classic tidal theory accounting for a realistic vertical temperature profile is considered. Analysis and simulation show that the well-known normal atmospheric modes (NM), which are trapped in the lower and middle atmosphere, exhibit a wave-like vertical structure with a large vertical wavelength in the thermosphere. Moreover, the reflection of these modes from the vertical temperature gradient in the lower thermosphere causes appearance of the wave-energy upward flux in the middle atmosphere, and in a linearized formulation this flux is constant above the source region. To investigate a possibility of the NM forcing by stratospheric vacillations and to consider the propagation of different PW up to the heights of the upper thermosphere, a set of runs with a mechanistic Middle and Upper Atmosphere Model has been performed. The results of the simulation show that quasi-stationary and longer-period PW are not able to penetrate into the thermosphere. The shorter-period NM and ultra-fast Kelvin wave propagate up to the heights of the lower thermosphere. However, above about 150 km they are strongly suppressed by dissipative processes. The role of the secondary waves (nonmigrating tides) arising from nonlinear interaction between the primary migrating tides and quasi-stationary PW is discussed. We conclude that PW are not capable of propagating directly up to the heights of the ionospheric F2 region. It is suggested that other physical processes (for instance, the electrostatic field perturbations) have to be taken into account to explain the observed PW-like structures in ionospheric parameters. 相似文献
952.
Data of neutral meridional wind obtained by the meteor radar at Esrange and data of temperature and pressure measured by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on board the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics (TIMED) spacecraft were studied with respect to a day-to-day atmospheric variability with periods ranging from 1.5 to 5 days. The detailed analysis was carried out for February 2004. Perturbations of the atmospheric parameters at the examined periods appeared mainly as eastward-propagating waves of zonal wavenumbers 1 and 2. We suggested that these waves excited by the jet instability on both flanks of the polar-night jet in the upper stratosphere and mesosphere interact nonlinearly with each other, and this interaction generates secondary waves. The radar observed both primary and secondary waves at mesospheric heights. The data analysis supports this suggestion. Under conditions of weaker instability observed in February 2003 the perturbations of atmospheric parameters of periods ranging from 1.5 to 5 days had smaller amplitudes at heights of the mesosphere than those in February 2004. It was found that the Eliassen-Palm fluxes calculated for the waves generated by the jet instability were mainly downward directed. This result suggests a possible dynamical influence of the mesospheric layers on the lower atmospheric levels. 相似文献
953.
On May 28, 1998, a moderate size earthquake of mb 5.5 occurred offshore the northwestern part of Egypt (latitude 31.45°N and
longitude 27.64°E). It was widely felt in the northern part of Egypt. Being the largest well-recorded event in the area for
which seismic data from the global digital network are available, it provides an excellent opportunity to study the tectonic
process and present day stress field occurring along the offshore Egyptian coast. The source parameters of this event are
determined using three different techniques: modeling of surface wave spectral amplitudes, regional waveform inversion, and
teleseismic body waveform inversion. The results show a high-angle reverse fault mechanism generally trending NNW–SSE. The
P-axis trends ENE–WSW consistently with the prevailed compression stress along the southeastern Hellenic arc and southwestern
part of the Cyprean arc. This unexpected mechanism is most probably related to a positive inversion of the NW trending offshore
normal faults and confirms an extension of the back thrusting effects towards the African margin. The estimated focal depth
ranges from 22 to 25 km, indicating a lower crustal origin earthquake owing to deep-seated tectonics. The source time function
indicates a single source with rise time and total rupture duration of 2 and 5 s, respectively. The seismic moment (M
o) and the moment magnitude (M
w) determined by the three techniques are 1.03 × 1017 Nm, 5.28; 1.24 × 1017 Nm, 5.33; and 1.68 × 1017 Nm, 5.42; respectively. The calculated fault radius, stress drop, and the average dislocation assuming a circular fault model
are 7.2 km, 0.63 Mpa, and 0.11 m, respectively. 相似文献
954.
Analysis of the weightiness of site effects on reinforced concrete (RC) building seismic behaviour: The Adra town example (SE Spain) 总被引:1,自引:0,他引:1
Manuel Navarro Francisco Vidal Takahisa Enomoto Francisco J. Alcalá Antonio García‐Jerez Francisco J. Sánchez Norio Abeki 《地震工程与结构动力学》2007,36(10):1363-1383
The damage distribution in Adra town (south‐eastern Spain) during the 1993 and 1994 Adra earthquakes (5.0 magnitude), that reached a maximum intensity degree of VII (European Macroseismic Scale (EMS scale)), was concentrated mainly in the south‐east zone of the town and the most relevant damage occurred in reinforced concrete (RC) buildings with four or five storeys. In order to evaluate the influence of ground condition on RC building behaviour, geological, geomorphological and geophysical surveys were carried out, and a detailed map of ground surface structure was obtained. Short‐period microtremor observations were performed in 160 sites on a 100m × 100m dimension grid and Nakamura's method was applied in order to determine a distribution map of soil predominant periods. Shorter predominant periods (0.1–0.3 s) were found in mountainous and neighbouring zones and larger periods (greater than 0.5 s) in thicker Holocene alluvial fans. A relationship T = (0.049 ± 0.001)N, where T is the natural period of swaying motion and N is the number of storeys, has been empirically obtained by using microtremor measurements at the top of 38 RC buildings (ranging from 2 to 9 storeys). 1‐D simulation of strong motion on different soil conditions and for several typical RC buildings were computed, using the acceleration record in Adra town of the 1993 earthquake. It is noteworthy that all the aforementioned results show the influence of site effects in the degree and distribution of observed building damage. Copyright © 2007 John Wiley & Sons, Ltd. 相似文献
955.
湛江港邻近海域台风浪的模拟研究 总被引:3,自引:0,他引:3
对第三代近岸海浪数值模式SWAN及包含的物理过程进行了简要介绍,利用该模式对影响南海湛江港海域的二次台风浪过程进行了模拟研究:由藤田台风风场模型同化相应时刻的台风要素、NCAR/NCEP网格点资料、单站观测资料后,提供模式所需风场;利用自嵌套的方式,提供模式波谱边界条件;两次模拟结果与实际海浪观测资料相符较好,可以为该海域台风浪的模拟预报提供较为重要的参考。 相似文献
956.
复杂地质构造波动方程数值模拟 总被引:3,自引:2,他引:3
利用全声波方程进行地震波场的数值模拟,虽然可以计算全声波波场值,但是也常常会出现层间多次波,给资料解释造成一定的困难。作者在本文中根据无反射声波方程,采用有限差分数值解法,实现了自激自收时间剖面的制作,避免了层间多次波的产生。本方法不但允许速度有纵向变化,而且允许速度有横向变化,这使得模拟复杂地质构造的地震响应成为可能。实际计算结果表明,该方法是一种行之有效的自激自收时间剖面的计算机数值模拟方法。 相似文献
957.
横向各向同性介质中的弹性波方程逆时偏移及其成像条件 总被引:1,自引:3,他引:1
作者在本文中导出了在横向各向同性介质情况下,二维弹性波逆时传播的高阶差分格式,实现了弹性波在数值空间中的逆时延拓,从snell定量出发,采用插值法求取网格空间中各点的直达波旅行时,以此作为弹性波逆时偏移的成像条件,实现多波多分量资料的逆时偏移,数值试验表明,逆时偏移能够使地表接收到的波场准确归位,提高资料处理的精度。 相似文献
958.
一种层析成像的正演和反演方法 总被引:1,自引:3,他引:1
作者在本文中提出了一种层析成像的正演和反演方法,首先对求解区作网络划分,由给定的正演速度模型在网格点上双线性插值,获得整个网格节点的速度分布,然后,对波阵面作一近似,在此基础上,用最小走时最短路径射线追踪法完成正演,反演则是通过正演的方法实现的,理论模型算例表明,本方法效果较好。 相似文献
959.
多道瞬态瑞雷波法在探测煤矿采空区中的应用 总被引:7,自引:0,他引:7
采空区探测是工程建筑和煤矿生产中亟待解决的问题。常规物探方法在对落后的“房—柱”式开采技术造成的面积较小、埋深较浅的采空区进行探测时存在漏报或误报的情况。根据采空区的地球物理特征,探讨多道瞬态瑞雷波技术的探测机理,并通过勘探实例阐述了该方法在浅层煤矿采空区探测中的实用性和有效性。 相似文献
960.