共查询到19条相似文献，搜索用时 250 毫秒
1.
《大气科学》2015,(5)
本文基于GRAPES全球模式的短期预报误差样本,利用赤道波动正规模态研究了热带风、压场平衡特征,并根据这些特征分析了线性平衡方程(LBE)在该区域应用时存在的问题。结果表明:(1)赤道波动能成功解释热带短期预报误差样本的大部分分量,对流层中层为60%~80%,对流层顶和平流层低层为80%以上。(2)在可解释的误差方差中,赤道罗斯贝波(ER)占比仅为30%~55%,其他赤道波动的作用不可忽视。(3)在ER模态基础上引入其他赤道波动会大幅削弱原有风、压场平衡约束,重力惯性波与Kelvin波的作用最为显著。此时,对流层中层位势高度h与u风、v风间的约束接近于零,而平流层低层h–u的平衡特征由Kelvin波主导。(4)LBE主要表达了ER模态下的风、压场平衡特征,与实际情形相比高估了热带风、压场的耦合程度,进一步的改进中需削弱这一虚假平衡,使得热带风、压场分析变得更加独立。 相似文献
2.
热带风压场平衡特征及其对GRAPES系统中同化预报的影响研究Ⅱ:动力与统计混合平衡约束方案的应用 总被引：1，自引：0，他引：1
研究I的结果表明:线性平衡方程(LBE)在热带地区不适用,而进一步改进方向是削弱LBE在该区域的约束程度。本文以此为基础,在GRAPES(global/regional assimilation and prediction system)全球变分同化系统中引入动力与统计混合平衡约束方案。新方案在逐层求解LBE的基础上增加垂直方向的线性回归,回归系数随纬度和高度变化。针对背景误差协方差的分析表明,新方案可以更好的保证独立分析变量间预报误差不相关的基本要求,并大幅度减小热带地区平衡气压预报误差方差的量值和占总方差的比例。单点试验结果表明,与LBE方案相比,新方案对中、高纬影响很小,但在热带地区成功实现了风、压场分析的解耦,两者分析更为独立。并且,虽未考虑具体波动模态,但新方案给出的风、压场协相关结构与研究I的理论分析结果相近。一个月的同化循环与预报结果表明,引入新方案后,赤道外地区的同化预报效果为中性偏正,而热带地区风场的同化预报效果显著提高,LBE方案中平流层低层的风场同化预报异常被基本消除。 相似文献
3.
从六十年代发现了赤道平流层下部行星尺度波以来,对热带波的研究产生了较大的兴趣。迄今已清楚地从平流层资料中分析出两种原型赤道波——Rossby-重力混合波和Kelvin波。早期的赤道波理论模式没有提供什么线索说明,大气赤道波生成的物理机制和以某种波占优势的物理机制。然而,现在我们已有热带波能量循环的一些观测证据。Yanai和Hayashi利用互谱分析方法,指出实测的Rossby-重力混合波是与对流层顶上波能向上通量相联系的,平流层赤道波的源地在对流层内。Nitta指出,热带西太平洋上空对流层波的涡动动能主要是由涡动有效位能转换来的,后者是由对流层上部凝结潜热释放所产生的。但是, 相似文献
4.
本文从原始方程组出发,在赤道β平面上采用正交模态法,对低纬超长波进行水平结构和垂直结构分析,发现低纬超长波主要出现在对流层上层和平流层低层。其次,本文还讨论了含有低纬理想热源的原始方程模式,并通过对模式求数值解得出:低纬热源强迫是对流层上层Kelvin波的形成原因之一。 相似文献
5.
平流层爆发性增温（SSW）超前于对流层环流异常,是延长冬季寒潮低温预报时效的重要途径之一。然而强SSW事件前后地面温度响应的区域和时间存在不确定性,其中涉及的平流层—对流层耦合过程和机理也不十分清楚。本文采用1979～2021年ERA5再分析数据集,研究了2020/2021年冬季“偏心型”强SSW事件前后中高纬度地区地面温度异常的演变特征,并分析了其与等熵大气经向质量环流平流层—对流层分支的耦合演变模态的动力联系。结果表明,伴随此次强SSW事件,亚洲和北美中纬度地区的寒潮低温事件分别在绕极西风反转为东风之前和再次恢复为西风之后发生。SSW前后大气经向质量环流的平流层向极地暖支与对流层高层向极暖支、低层向赤道冷支之间呈现出三个阶段的耦合演变模态: 同位相“加强—加强”、反位相“加强—减弱”以及反位相“减弱—加强”。加强的质量环流对流层向赤道冷支是SSW前后寒潮低温事件的主要原因,而加强的向极地平流层暖支是SSW发生及其伴随的北极涛动负位相持续加强的主要原因。大气经向质量环流不同的垂直耦合模态取决于行星波槽脊在对流层顶和对流层中低层两个关键等熵面上的西倾角异常。西倾角异常表征大气波动的斜压性,主要通过影响关键等熵面以上向极地的净质量输送和其下向赤道的净质量输送进行调控。尤其在SSW发生后的极涡恢复期,对流层顶处异常偏弱的斜压性会加强对流层向极地暖支,进而加强向赤道冷支,有利于寒潮低温的发生。本次SSW事件前后大气经向质量环流三支的耦合演变模态,与历年平流层北半球环状模（NAM）负事件中极区平流层温度异常信号下传滞后的平流层—对流层耦合演变类型相一致,其在波动尺度方面也存在共同特征,即SSW事件或NAM负事件前期对流层一波加强且上传,后期对流层二波加强但较难上传。 相似文献
6.
利用1979-2007年卫星观测日平均OLR资料以及NCEP/DOE第2套再分析资料中的风场资料,采用有限区域波一频分析、合成分析等方法,分析对比对流层高、低层风场与对流场所表征的热带北半球夏季季节内振荡(BSISO)各种传播模态谱分布气候特征及其年际异常。结果表明:各要素反映的BSISO各种模态的气候特征及其年际变化存在一定差异,总体而言对流层低层风(850hPa纬向风或经向风)与对流比较一致。850hPa经向风(纬向风)所反映的纬向(经向)传播BSISO谱分布气候特征与对流情况最相似。在ENSO发展年,850hPa经向风反映的赤道东传波加强趋势与对流较为一致;850hPa纬向风、经向风反映的北传波变化趋势都与对流相似。在ENSO衰减年,850hPa纬向风(经向风)反映的赤道东传波(赤道外西传波)减弱趋势与对流较为一致;对流以及850hPa经向风、200hPa纬向风和200hPa经向风4种要素都能体现南海及周边地区北传波明显减弱这一特征。对流和850hPa纬向风所反映的北传波与印度洋偶极子模态之间关系一致。 相似文献
7.
利用欧洲中尺度天气预报中心(ECMWF)逐日的60层模式资料构建了半拉格朗日的二维θ-PVLAT坐标,在新坐标中对2003-2004年冬季北半球平流层极涡的活动过程进行诊断分析.通过对位涡距平场在新坐标下的EOF分析得到极涡扰动指数,由该指数出发对风场、温度场进行超前/滞后回归分析.得到极涡活动过程中平、对流层大气的环流输送特征.结果表明:(1)θ-PVLAT坐标有很好的物质性,它能够较好地反映出空气物质的输送特征,尤其在北半球冬季的高纬度地区它能更加真实的表达出大气环流风场、温度场的变化;(2)在极涡活动过程中平流层里存在着一对向极、向下的传播模态,不同符号的纬向风和温度异常的信号沿着这两个模态传播,而对流层中也有一向赤道的传播模态;(3)平流层中向极、向下的传播模态和对流层中向赤道的传播模态在时间上存在着一定的联系,当纬向风异常在高层传播到达极区时,低层开始向赤道传播;(4)整个极涡活动过程可以用一个非绝热加热作用和斜压波动作用共同驱动的经圈质量环流解释,这一环流造成了中低纬度地区的暖空气和极地区域的冷空气在平流层一对流层之间交换,对整层大气的热力、动力结构进行了重新组合. 相似文献
8.
热带地区,除台风外,经常发生许多热带扰动,热带波动是其中之一。过去,热带波动主要指的是东风波。近十年来,对热带波动概念有了一些改变,认为除东风波外,还包括所有在热带地区形成的波动。热带波动可能有六种来源:(1)东风波;(2)赤道波;(3)对流层上部冷涡势力向下伸展,在低空东风气流中诱生的波动;(4)由中纬度延伸或切断在低纬地区的低槽转变成的波动;(5)赤道附近东风区中风速辐合区;(6)热带低层涡旋向北伸出的倒槽。虽然热带波动包括的范围很广,但主要的是前三种。 相似文献
9.
《大气和海洋科学快报》2021,(3)
平流层准两年振荡(QBO)是赤道平流层(～100-1 hPa)变率的主要模态,可对中高纬地区的环流产生重要影响,但目前利用通用大气环流模式(GCM)对其进行准确模拟仍然是一个挑战.本文利用IAP大气环流模式(IAP-AGCM)的中高层大气模式版本(IAP-AGCML69)对QBO进行模拟,并对其动量收支情况进行分析.研究发现,QBO主要是由对流活动引起的重力波强迫(参数化)引起的,但该动量强迫被平流层赤道上升流所引起的平流过程显著削弱.模式可分辨尺度的波动强迫对赤道上空的QBO的总纬向风倾向有正贡献,在上平流层,其量值大小与参数化的重力波强迫相当.以上结果提供了对QBO形成机制以及模式模拟差异可能原因的认识. 相似文献
10.
根据1953～1991年赤道平流层纬向风资料分析,得出我国东部地区7月份主要雨带位置与赤道平流层30～50 hPa平均纬向风准两年振荡（以下简称赤道平流层QBO）有较好的关联。在西风位相条件下,我国7月主要雨带位置较偏北;在东风位相条件下,我国7月主要雨带位置易偏南。它们之间的关系主要是通过对对流层环流的影响相联系的。利用赤道平流层纬向风的变化规律并结合冬季北太平洋对流层环流特征,对我国7月主要雨带类型的预报,有一定实用意义。 相似文献
11.
Summary
The variability of the horizontal circulation in the stratosphere and troposphere of the Northern Hemisphere (NH) is compared
by using various approaches. Spatial degrees of freedom (dof) on different time scales were derived. Modes of variability were computed in geopotential height fields at the tropospheric
and stratospheric pressure levels by applying multivariate statistical approaches. Features of the spatial and temporal variability
of the winterly zonal wind were studied with the help of recurrence and persistence analyses. The geopotential height and
zonally-averaged zonal wind at the 50-, 500- and 1000-hPa level are used to investigate the behavior of the horizontal circulation
in the lower stratosphere, mid-troposphere and at the near surface level, respectively. It is illustrated that the features
of the variability of the horizontal circulation are very similar in the mid-troposphere and at the near surface level. Due
to the filtering of tropospheric disturbances by the stratospheric and upper tropospheric zonal mean flow, the variability
of the stratospheric circulation exhibits less spatial complexity than the circulation at tropospheric pressure levels. There
exist enormous differences in the number of degrees of freedom (or free variability modes) between both atmospheric layers.
Results of the analyses clearly show that the concept of a zonally symmetric AO with a simple structure in the troposphere
similar to the one in the stratosphere is not valid. It is concluded that the spatially filtered climate change signal can
be detected earlier in the stratosphere than in the mid-troposphere or at the near surface level.
Received June 28, 2000/Revised March 10, 2001 相似文献
12.
Timothy J. Dunkerton 《大气与海洋》2013,51(1):55-68
Abstract It is shown that oscillating mean flow solutions exist in the one‐dimensional Holton‐Lindzen (1972) model in the presence of a single Kelvin wave, mean flow diffusion, and an easterly zonal force per unit mass that is constant in height and time except at those points in the time‐height cross‐section where the latitudinally‐integrated mean flow is less than some prescribed easterly value. The latter forcing is intended to crudely represent the absorption of quasi‐stationary planetary Rossby waves at the tropical zero‐wind line. Our results suggest an alternative, and somewhat simpler, possible interpretation of the quasi‐biennial mean zonal wind oscillation in the equatorial lower stratosphere. 相似文献
13.
为了分析 ＥＩ Ｎｉｏ事件发生和消亡中热带太平洋纬向风应力的动力作用，建立一个类似于Ｚｅｂｉａｋ的简单热带海洋数值模式，在观测到的风应力异常的强迫下，模拟赤道太平洋地区 １９７１年１月至 １９９８年８月海表温度异常的变化。结果表明，模式对观测的Ｎｉｏ３区海表温度异常（ＳＳＴＡ）有很好的模拟能力。模拟和观测Ｎｉ区ＳＳＴＡ之间的相关系数可达 ０．９０。模式对 Ｅｌ Ｎｉｏ事件期间赤道太平洋海表温度异常随时间变化也有较好的模拟能力。为了分析Ｅｌ Ｎｉｏ期间ＳＳＴＡ的空间分布及其随时间变化的动力学机制，还对１９８６～１９８９年 ＥＮＳＯ循环期间赤道太平洋地区观测的 ＳＳＴＡ的传播特征及其形成机制进行了分析。模式较好地模拟出了观测到的赤道太平洋地区ＳＳＴＡ的传播特征，即从１９８６年底至１９８７年 ４月， ＳＳＴＡ具有向东传播的特征，从 １９８７年 ６月至 １９８８年 ２月具有向西传播的特征。动力学分析的结果表明，赤道中西太平洋地区的缔向风应力异常对 Ｅｌ Ｎｉｏ事件的发生和消亡具有重要作用。赤道中西太平洋地区的西风异常可强迫出东传的Ｋｅｌｖｉｎ波，这个东传的 Ｋｅｌｖｉｎ波对正 ＳＳＴＡ的东传起主要作用，当这个东传的 Ｋｅｌｖ 相似文献
14.
热带平流层多尺度波动分离方案的研究：多站点高分辨率无线电探空联合分析 总被引：1，自引：0，他引：1
利用太平洋地区台风过境期间6个热带气象站的高分辨率无线电探空资料,结合扩展经验正交函数（EEOF）展开,对热带下平流层行星波和重力波扰动进行了分离,给出了一种热带地区提取重力波扰动的新方案。对观测数据做EEOF展开后,选择表征行星尺度波动模态的特征向量和相应权重进行气象要素场的重建。结果显示,在不同的台风过程期间,温度、纬向风和经向风的重建扰动量显示出不同的动力学偏振关系:在准两年振荡（QBO）东风位相时与赤道开尔文波的偏振关系一致,而在准两年振荡西风位相时与混合罗斯贝-重力波（MRG）的偏振关系一致。把行星尺度波动模态从原始观测中剔除,得到新的扰动廓线,对其进行重力波垂直波数谱的谱型拟合。结果发现,与以往方法提取的重力波扰动相比,新方法所得谱型参数中特征垂直波长λ*在不同时期不同站点变化很小,稳定在1.7 km左右,且低频波数段谱斜率s的数值与理论假设1十分接近。综合其研究结果可以推测,用新方法提取的热带重力波扰动更加符合当前的理论垂直波数谱模型。 相似文献
15.
为了分析ElNio事件发生和消亡中热带太平洋纬向风应力的动力作用，建立一个类似于Zebiak的简单热带海洋数值模式，在观测到的风应力异常的强迫下，模拟赤道太平洋地区1971年1月至1998年8月海表温度异常的变化。结果表明，模式对观测的Nio3区海表温度异常(SSTA)有很好的模拟能力。模拟和观测Nio3区SSTA之间的相关系数可达0.90。模式对ElNio事件期间赤道太平洋海表温度异常随时间变化也有较好的模拟能力。为了分析ElNio期间SSTA的空间分布及其随时间变化的动力学机制，还对19861989年ENSO循环期间赤道太平洋地区观测的SSTA的传播特征及其形成机制进行了分析。模式较好地模拟出了观测到的赤道太平洋地区SSTA的传播特征，即从1986年底至1987年4月，SSTA具有向东传播的特征，从1987年6月至1988年2月具有向西传播的特征。动力学分析的结果表明，赤道中西太平洋地区的纬向风应力异常对ElNio事件的发生和消亡具有重要作用。赤道中西太平洋地区的西风异常可强迫出东传的Kelvin波，这个东传的Kelvin波对正SSTA的东传起主要作用，当这个东传的Kelvin波到达东边界，由于东边界的反射作用，在东边界产生西传的Rossby波，这个西传的Rossby波对赤道中东太平洋地区正SSTA的西传起主要作用。东传Kelvin波和反射的Rossby波对ElNio期间赤道东太平洋正SSTA二次峰值的形成具有重要作用。 相似文献
16.
The Madden–Julian oscillation (MJO) is observed to interact with moist Kelvin waves. To understand the role of this interaction, a simple scale-interaction model is built, which describes the MJO modulation of moist Kelvin waves and the feedback from moist Kelvin waves through upscale eddy heat and momentum transfer. The backward-tilted moist Kelvin waves produce eddy momentum transfer (EMT) characterized by the lower-tropospheric westerly winds and eddy heat transfer (EHT) that warms the mid-troposphere. The EHT tends to induce the lower-tropospheric easterly winds and low pressure, which is located in front of the “westerly wind burst” induced by the EMT. Adding the eddy forcing to a neutral MJO skeleton model, we show that the EHT provides an instability source for the MJO by warming up the mid-troposphere, and the EMT offers an additional instability source by enhancing the lower-tropospheric westerly winds. The eddy forcing selects eastward propagation for the unstable mode, because it generates positive/negative eddy available potential energy for the eastward/westward modes by changing their thermal and dynamical structures. The present results show that moist Kelvin waves can provide a positive feedback to the MJO only when they are located within (or near) the convective complex (center) of the MJO. The EHT and EMT feedback works positively in the front and rear part of the MJO, respectively. These theoretical results suggest the potential importance of moist Kelvin waves in sustaining the MJO and encourage further observations to document the relationship between moist Kelvin waves and the MJO. 相似文献
17.
Pauline Maury François Lott Lionel Guez Jean-Philippe Duvel 《Climate Dynamics》2013,40(9-10):2331-2344
The atmospheric variability in the equatorial regions is analysed in the Earth System Model pre-industrial simulation done at IPSL in the framework of CMIP5. We find that the model has an interannual variability of about the right amplitude and temporal scale, when compared to the El-Niño Southern Oscillation (ENSO), but that is too confined to the western Pacific. At the intra-seasonal periods, the model variability lacks of large-scale organisation, and only produces one characteristic Madden-Julian Oscillation every 10 winters typically. At shorter time-scales and in the troposphere, the model has Rossby and Kelvin Convectively Coupled Equatorial Waves (CCEWs), but underestimates the Kelvin CCEWs signal on OLR. In the model stratosphere, a composite analysis shows that the Temperature and velocities fluctuations due to the Kelvin waves are quite realistic. In the model nevertheless, the stratospheric waves are less related to the convection than in the observations, suggesting that their forcing by the midlatitudes plays a larger role. Still in the model, the Kelvin waves are not predominantly occurring during the life cycle of the tropospheric Kelvin CCEWs, a behaviour that we find to be dominant in the observations. The composite analysis is also used to illustrate how the waves modify the zonal mean-flow, and to show that the model Kelvin waves are too weak in this respect. This illustrates how a model can have a reasonable Kelvin waves signal on the velocities and temperature, but can at the same time underestimate their amplitude to modify the mean flow. We also use this very long simulation to establish that in the model, the stratospheric equatorial waves are significantly affected by ENSO, hence supporting the idea that the ENSO can have an influence on the Quasi-Biennial Oscillation. 相似文献
18.
Summary ?The fields of sea-level height anomaly (SLHA) and surface zonal wind anomaly (SZWA) have been analyzed to investigate the
typical evolution of spatial patterns during El Ni?o-Southern Oscillation (ENSO) events. Sea surface temperature (SST) changes
during ENSO events are represented as an irregular interplay of two dominant modes, low-frequency mode and biennial mode.
Cyclostationary principal component (PC) time series of the former variables are regressed onto the PC time series of the
two dominant SSTA modes to find the spatial patterns of SLHA and SZWA consistent with the two SSTA modes. The two regressed
patterns of SLHA explain a large portion of SLHA total variability. The reconstruction of SLHA using only the two components
reasonably depicts major ENSO events. Although the low-frequency component of SST variability is much larger than the biennial
component, the former does not induce strong Kelvin and Rossby waves. The biennial mode induces much stronger dynamical ocean
response than the low-frequency mode.
Further decomposition of the SLHA modes into Kelvin and Rossby components shows how these two types of equatorial waves evolve
during typical ENSO events. The propagation and reflection of these waves are clearly portrayed in the regressed patterns
leading to a better understanding of the wave mechanism in the tropical Pacific associated with ENSO. A close examination
suggests that the delayed action oscillator hypothesis is generally consistent with the analysis results reported here. Rossby
wave development in the central Pacific in the initiation stage of ENSO and the subsequent reflection of Kelvin waves at the
western boundary seems to be an important mechanism for further development of ENSO. The development of Kelvin waves forced
by the surface wind in the far-western Pacific cannot be ruled out as a possible mechanism for the growth of ENSO. While Kelvin
waves in the far-western Pacific serve as an intiation mechanism of ENSO, they also cause the termination of existing ENSO
condition in the central and eastern Pacific, thereby leading to a biennial oscillation over the tropical Pacific. The Kelvin
waves from the western Pacific erode the thermocline structure in the central Pacific preventing further devlopment of ENSO
and ultimately terminating it. It should be emphasized that this wave mechanism is clear and active only in the biennial mode.
Received August 15, 2001; revised March 6, 2002 相似文献