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991.
992.
The influences of vegetation on intraseasonal oscillation (ISO) were examined using the Community Atmosphere Model version 3 (CAM3).Two 15-year numerical experiments were completed:the first was performed with a realistic vegetation distribution (VEG run),and the second was identical to the VEG run except without land vegetation (NOVEG run).Generally speaking,CAM3 was able to reproduce the spatial distribution of the ISO,but the ISO intensity in the simulation was much weaker than that observed in nature:the ISO has a relatively much stronger signal.A comparison of the VEG run with the NOVEG run revealed that the presence of vegetation usually produces a weak ISO.The vegetation effects on ISO intensity were significant over West Africa and South Asia,especially in the summer half-year.Vegetation also plays an important role in modulating ISO propagation.The eastward propagation of the ISO in the VEG run was clearer than that in the NOVEG run over the West African and Maritime Continent regions.The northward propagation of the ISO in the VEG run was more consistent with observation than that in the NOVEG run. 相似文献
993.
994.
A 1D model, including a time variation of eddy viscosity and mixed layer depth, is applied to study Ekman spirals. It simulates a weak velocity in the atmosphere but a jet in the upper oceanic mixed layer during daytime; and a strong velocity in the atmosphere but a weak, uniform velocity in the ocean at night. The mean spirals in both atmosphere and ocean are close to the average spirals at midday and midnight, they are not flat as suggested by previous studies but consistent with the observations of Polton et al (2013). Our results also show shorter length scale for magnitude decay than for rotation of mean velocity as observed in the ocean, which comes from the combined effects of the diurnal variation of PBL and the Coriolis force. The latter becomes more important away from the surface. In the upper oceanic mixed layer, the mean velocity mainly comes from the strong jets in the late afternoon and early evening. Near and below the depth of Ekman depth, the weak velocities change with time and cancel out each other if averaged timing is longer than the inertia period. It results in diminishing of magnitude of the mean velocity, but the amplitude of individual parcel oscillating can still be quite large near the Ekman depth. Meanwhile, the change of velocity angle from the surface is near or less than 90 degree. Hence, shorter length scale for magnitude decay than for rotation of the mean velocity is not controlled by viscosity alone. Meanwhile, the model does not need two viscosities as suggested previously.The results also show that either the diurnal variation of surface stress or eddy viscosity alone can create a diurnal oscillation of velocity in the ocean. The interactions between PBL force and the Coriolis force can create a weak instability in the atmosphere and ocean at 30° and 90°. This weak instability may explain the observed nocturnal LLJ near 30 °N on the lee of the Rocky Mountains and the intensification of mesoscale circulation simulated by Sun and Wu (1992). 相似文献
995.
热带海气相互作用对大气BSISO年际振荡的影响 总被引:2,自引:0,他引:2
利用卫星观测OLR资料以及海气耦合数值模拟试验结果,从每年波-频分析结果提取了各种传播模态的强度指数序列,分析了热带北半球夏季季节内振荡(BSISO)各种传播模态的年际变化谱特征,探讨了热带各海区海气相互作用对其影响。主要结果如下:赤道外西传波和印度洋北传波以准2 a为显著振荡周期,赤道东传波、南海北传波和西太平洋北传波则都包含准2 a和准5 a两种周期,南海北传波是5种指数中惟一以准5 a为最主要周期振荡的模态。热带印度洋、西太平洋、东太平洋各海区海气相互作用对各指数准2 a振荡、准5 a振荡既有加强作用,也有削弱作用。各海区比较而言,对赤道东传波准2 a和准5 a振荡、南海北传波准2 a和准5 a振荡起最大加强作用的是西太平洋海区海气相互作用;对赤道外西传波准2 a振荡、西太平洋北传波准2 a和准5 a振荡起最大加强作用的是印度洋海区海气相互作用。 相似文献
996.
本文着重考虑非均匀基本流的正压局地不稳定性,研究中高纬低频振荡产生的动力机制。基本流是取1980年冬、夏300 hPa的位势场。结果表明正压局地不稳定性能较好地解释中高纬大气30—60 d天振荡。这似乎表明,低频振荡是大尺度大气运动和扰动相互作用的一种固有特征,而不是外源强迫的结果。本文还讨论了适于激发季节内低频振荡的基本流场。初值问题的研究发现中高纬大气30—60 d振荡呈纬向三波模态发展,与初始扰动和基本气流的冬、夏差别无关。 相似文献
997.
分析了从1985年9月至1992年12月共115次急始型磁暴期间武昌多普勒台阵观测到的电离层暂态振荡(SIO).这种与地磁SC相伴的SIO可分成SCF(+,-),SCF(-,+),SCF(+)与SCF(-)几种类型.分析发现,伴随地磁急始在F区总是存在突发电离层暂态振荡,除非电波被吸收、穿透、被E5屏蔽,以致F区无反射回波或在反射区电离密度的高度梯度特别大,使多普勒频率很小在多普勒图上显示不出来.通常SCF(+,-)发生在白天,而SCF(-,+)发生在晚上.SIO与地磁急始有很好的对应关系. 相似文献
998.
A zonal-vertical two-dimensional equatorial model is used to study the possibility that the long period oscillation of the zonal mean flow occurring in the lower equatorial stratosphere (QBO) is caused by local thermal ac-tivities at the tropical tropopause. The model successfully reproduces QBO-like oscillations of the zonal mean flow, suggesting that the local heating or cooling at the tropical tropopause is probably the main reason of QBO’s genera-tion. The analysis of the dependence of the oscillation on the wave fencing indicates that the oscillation is not sensible to the forcing scale. The model can reproduce QBO-like oscillations with any forcing scale if the fencing period and amplitude take appropriate values, proving that the internal gravity waves generated by local thermal source take much important roles in QBO. 相似文献
999.
热带大气中的准双周(10—20天)振荡 总被引:10,自引:3,他引:10
基于欧洲中期天气预报中心(ECMWF)的资料(1981—1988),本文对全球热带大气中的10—20天(准双周)振荡进行了比较系统的研究,包括其动能的分布及演变。扰动的结构和传播特征等。资料分析充分表明,热带大气10—20天振荡是热带大气中另一重要低频系统,其动能比30—60天振荡还要大,而其结构和活动又同30—60天振荡很不一样。例如热带大气10—20天振荡主要表现为纬向波数2—4;垂直结构以正压特征更显著;主要表现为向西传播;其经向风分量与纬向风分量同等重要。因此,对热带大气10—20天振荡值得更多注 相似文献
1000.
An atmospheric general circulation model is used in a series of three experiments to simulate the intraseasonaloscillation in the tropical atmosphere.Analyses of the model daily data show that various physical variables,from sever-al different regions,exhibit fluctuations with a spectral peak between 30 and 60 days.This represents a 30—60 dayoscillation in the tropical atmosphere and possesses several features which are consistent with observations.These in-clude a horizontal structure dominated by zonal wavenumber 1 and a vertical structure which is predominantlybaroclinic.The effect of warm SST (sea surface temperature) anomalies on the 30—60 day oscillation in the tropical atmos-phere is also simulated by prescribing global SST as observed in 1983.This has the effect of weakening the oscillationwhile at the same time the vertical structure becomes less baroclinic.The importance of cumulus convection to the propagational characteristics of this oscillation is demonstrated by acomparison of results based on different parameterizations for convection.In one case,where the maximum convectionover the Pacific is simulated to be too far east,the simulated 30—60 day oscillation shows evidence of westward propa-gation.In the second case,where the convection maximum is located near the observed position in the western Pacific,there is more clearly evidence of eastward propagation.Both results suggest that the location of maximum convection in the Pacific can have an important influence on thestrength,structure and propagation of the 30—60 day oscillation. 相似文献