对流凝结加热的垂直分布与低纬大气的30～60天低频振荡

运用一个包含Wave-CISK机制的斜压半地转8层模式和本征函数展开方法，研究了三种不同的对流凝结加热廓线对低纬大气的30—60天低频振荡的影响。研究表明，不同的加热廓线分布时30～60天低频振荡具有不同的相速和周期，并且低频振荡特征相速的量级都是o(10m／s)，由Wave-CISK机制激发的低频CISK—Kelvin波和CISK—Rossby波都是稳定的。同时，还进一步揭示了不同加热廓线对低纬大气30～60天低频振荡垂直结构的影响。     

大气对热带热源低频响应的数值研究

本文设计—关于基本气流线性化的二层球面模式研究大气对不同类型赤道热源的低频响应,分析了全球大气40—50天低频振荡的结构和传播特点。结果表明:全球大气对热带热源响应特征是在热带地区表现为东西向非对称的热源东侧的Kelvin响应和西侧的Rossby响应,高低层反位相;在中高纬响应是具有低频振荡的二维Rossby波列,且具有相当正压结构。低频振荡的传播特征表明热带大气对移动性热源的响应更有利于振荡的向东传播,且该振荡可以沿波列路径向中高纬度传播,然后再折向低纬。二维Rossby波列是联系着热带和中高纬度地区低频振荡的基本动力学途径。该波列的形成取决于基本气流的分布,冬半球波列振幅较大。因此本文认为40—50天低频振荡是全球尺度的现象,它是一涉及到热带对流加热、赤道Kelvin波、亦道Rossby波、二维Rossby波列以及基本气流等动力学相互作用的过程。     

关于热带大气低频振荡的一个简单模式与数值模拟

本文首先从观测事实分析了热带大气的低频振荡现象，然后从理论上加以研究。为此，本文建立了一个包括触发热源和CISK机制的三维线性模式，用此模式讨论了热带大气低频振荡的性质、结构、传播和动力学机制。从模式的计算结果得到了周期为30d左右以大约9 m/s的速度向东传播的低频振荡现象，这种振荡为Kelvin波型的响应和向西传播的Rossby波型的响应的结合。计算还表明，这种振荡的周期与触发热源的周期关系不大，这说明了热带大气的低频振荡是大气自身的固有振荡，它是大尺度运动与对流凝结加热相互作用的结果。     

赤道以外热带大气中30—50天振荡的一个动力学研究

本文的动力学分析和模式大气的计算结果表明,在积云对流加热的反馈作用下,热带大气可以产生一种CISK-Rossby型波动。这种波与经典的热带Rossby波不同,它既可以向西也能向东移动,而且在热带大气通常的加热情况下其相速度同热带30—50天振荡的活动相一致。同时,CISK-Rossby型波动具有频散特性,其能量频散可以说明30—50天大气振荡的二维Rossby波列特征。因此可以认为,CISK-Rossby型波动是赤道以外热带大气30—50天振荡的主要激发和驱动机制。     

40—50天的纬向基流低频振荡及其失稳效应

初步的资料分析表明,大气运动的40—50天的低频振荡不仅存在于热带对流层,而且也存在于中高纬对流层及平流层.在温度及高度场的功率谱中,40—50天的振荡比双周振荡更为显著. 用球面二层模型对对流层冬季纬向振荡基流所作的稳定性分析表明,小扰动的增长随基流振荡而加强,经向温度梯度40—50天的振荡对波数3—8的波动能产生相当可观的失稳效应。对更长周期的基流振荡,增长率的频率响应出现“饱和”现象. 对平流层的分析表明,平流层定态纬向基流是动力稳定的,而纬向流的振荡分量及非纬向定态扰动则是两个可引起基态失稳的因子.     

赤道地区向西传播的40天周期低频波

本文用滤波和EOF位相合成技术对1981年7—12月份赤道地区出现的向西传播的40天周期低频波进行了分析。结果认为东太平洋地区从南半球到北半球的越赤道40天周期温度波是产生这种西传波的主要原因。这种波动主要产生于两个源地:一个是赤道150°E附近的对流层下层;另一个是110°W的赤道对流层上层。这两处产生的低频波性质不一样,前者与对流密切相关。通过计算整层积分的非绝热加热Q_1和水汽汇Q_2,结果表明Q_1加热中心在东太平洋也有越赤道传播。在150°E以西Q_2加热中心是向西北传播的,与低频波方向一致,Q_1的传播特征不明显,这说明西太平洋地区的热带对流可能有这种周期振荡。     

对流凝结加热与不稳定波

本文用综合考虑Ekman-CISK和CMM-CISK机制的柱对称模型,讨论了对流凝结加热廓线对不稳定波的影响。分析和计算结果表明,对流凝结加热廓线对不稳定波有显著影响。 通过CISK 机制对流凝结加热不仅可以产生常定不稳定波并且还可以产生一种有周期性变化的振荡型不稳定波,低层有最大的凝结加热分布更有利于振荡型不稳定波的产生。积云摩擦作用是形成最不稳定波的波长选择性的重要因素,而凝结加热廓线也对这种选择性有直接影响。不稳定波的垂直结构随加热廓线的不同而有明显的差异。 对流凝结加热廓线还直接影响能量的产生和转换。最大加热层越高,则产生最大有效扰动位能的高度就越高。更有意义的是,这时有效扰动位能向扰动动能转换的效率也愈高。因此,对流凝结加热廓线的不同可能是热带低压扰动仅部分发展为台风而另一些不能发展的重要原因之一。     

热带大气能量频散波射线的低频动力学特征

首先在非零频波条件下采用有、无辐散两类数学模型 ,讨论热带大气低频波传播动力特征 ,研究结果表明 ,非零频的波频率参数是热带大气低频振荡源能量频散波路径及其波振幅的关键影响因子 ,且热带地区低频振荡的经向传播与其伴随着的强对流云团有显著相关 ,并与热带低纬 β因子等相关。文中还进一步揭示了低纬大气低频振荡经向传播伴随的积云对流现象及向高中纬传播机理 ,描述了 WKB近似方法数学模型及其波射线方程解模态对大气低频动力特性及其水汽分布垂直结构、不稳定层结等因子的响应特征。     

青藏高原上空大气低频波的振荡及其经向传播

本文得出的初步结论是:在青藏高原所在的经度范围内,从低纬到高纬的各纬带上,大气低频波存在30—40天的周期振荡现象.500 hPa等压面上,青藏高原地区生成的气旋、反气旋切变可以向南、向北传播到低纬、高纬地区.200 hPa等压面上,中纬度地区生成的气旋、反气旋切变也可以向南、向北传播到低纬、高纬地区.对流层中层,青藏高原是大气低频波振荡源地,可能与青藏高原的热力、动力作用有关;对流层上层中纬度地区是大气低频波的振荡源地,可能是西风急流的作用. 由于大气低频波的振荡和传播与低值系统有关,与急流相联系,因而具有现实的预报意义.     

大气中的季节内振荡

本文依据最新的分析研究结果,系统地讨论了大气中的季节内(30—60天)振荡。内容包括大气季节内振荡的全球分布特征;热带大气30—60天振荡的基本特征;中高纬度大气30—60天振荡;热带和中高纬度大气30—60天振荡的相互影响;以及大气季节内振荡的动力学机制。 本文不仅对热带大气30—60天振荡提出了一些新的研究结果,特别是关于中高纬度大气30—60天振荡的讨论,以及关于热带和中高纬度大气30—60天振荡主要通过低频波列相互联系和相互影响的研究,将使我们对大气季节内振荡有比较全面的认识。     

DIAGNOSTIC STUDY FOR INTRASEASONAL OSCILLATION OF THE MIDDLE-HIGH LATITUDES IN A LOW RESOLUTION GLOBAL SPECTRAL MODEL

In this paper, five-year simulated data from a low-resolution global spectral model with triangular trunca-lion at wavenumber 10 are analyzed in order to study dynamical features and propagation characteristics ofintraseasonal oxillations over the mid-latitudes and the tropical atmosphere. The simulations show that thereis the 30-50 day periodic oscillation in the low-resolution spectral model without non-seasonal external forcing,and spatial scale of the intraseasonal oscihations is of the globe .Further analysis finds that propagation charac-ters of intraseasonal oscillations over the mid-latitudes and the tropics are different. The 30-50 day oscillationover the tropics exhibits structure of the velocity potential wave with wavenumber 1 in the latitudinal and thecharacter of the traveling wave eastward at speed of 8 longitudes/day. However, the 30-50 day oscillationsin mid-latitude atmosphere exhibit phase and amplitude oscillation of the standing planetary waves and theyare related to transform of teleconnection patterns over the mid-latitudes. The energy is not only transferredbetween the tropics and the middle-high latitudes, but also between different regions over the tropics. Based on the analysis of 5-year band pass filtered data from a 5-layer global spectral model of Jow-ordetwith truncated wavenumber l0,investigation is done of the source of intraseasonal oscillations in the extratropicalmodel atmosphere and its mechanism. Results show that (1) the convective heat transferred eastward alongthe equator serves as the source of the intraseasonal oxillation both in the tropical and the extratropical atmos--phere; (2) the velocity-potential wave of a zonal structure of wavenumber 1 gives rise to oxillation in divergentand convergent wind fields of a dipole-form as seen from the equatorial Indian Ocean to the western Pacificduring its eastward propagation, thus indicating the oscillation in the dipole-form heat soure:e/sink pattertl; (3)the tropical heat-source oscillation is responsible for the variation in phase and intensity of the extratropicalstationary wave train, and the interaction between the oscillating low-frequency inertial gravity and stationaryRossby modes that are probably mechanisms for the oscillations ip the middle-high latitudes.     

CISK-rossby wave and the 30-60 Day Oscillation in the Tropics

The 30-60 day oscillation is an important aspect of the atmospheric variance in the tropical area. A number of works have been done on this phenomenon, this article is a further one. A quasi-geostrophic linear model that consists of a two-layer free atmosphere and a well-mixed boundary layer is used to investigate the instability of intraseasonal oscillation, its propagation and vertical structures. Results show that the dynamical coupling and interaction between the barotropic and baroclinic components via boundary layer convergence / divergence are responsible for the appearance of a new kind of low-frequency wave. Such wave is very different from the traditional tropical Rossby wave. It can propagate westward and eastward. Some behaviours of it appear to resemble the observed 30-60 day oscillation mode in many aspects, such,as vertical structures, zonal and meridional propagations. Now many researchers emphasize the direct relationship between CISK-Kelvin mode and the tropical atmospheric 30-60 oscil     

Sensitivity of the Simulated Tropical Intraseasonal Oscillation to Cumulus Parameterizations

The sensitivity of the simulated tropical intraseasonal oscillation or MJO (Madden and Julian oscilla tion)to different cumulus parameterizations is studied by using an atmospheric general circulation model (GCM)-SAMIL(Spectral Atmospheric Model of IAP LASG).Results show that performance of the model in simulating the MJO alters widely when using two different cumulus parameterization schemes-the moist convective adjustment scheme(MCA)and the Zhang-McFarlane(ZM)scheme.MJO simulated by the MCA scheme was found to be more realistic than that simulated by the ZM scheme.MJO produced by the ZM scheme is too weak and shows little propagation characteristics.Weak moisture convergence at low levels simulated by the ZM scheme is not enough to maintain the structure and the eastward propagation of the oscillation.These two cumulus schemes produced different vertical structures of the heating profile.The heating profile produced by the ZM scheme is nearly uniform with height and the heating is too weak compared to that produced by the MCA,which maybe contributes greatly to the failure of simulating a reasonable MJO.Comparing the simulated MJO by these two schemes indicate that the MJO simulated by the GCM is highly sensitive to cumulus parameterizations implanted in.The diabatic heating profile plays an important role in the performance of the GCM.Three sensitivity experiments with different heating profiles are designed in which modified heating profiles peak respectively in the upper troposphere(UH), middle troposphere(MH),and lower troposphere(LH).Both the LH run and the MH run produce eastward propagating signals on the intraseasonal timescale,while it is interesting that the intraseasonal timescale signals produced by the UH run propagate westward.It indicates that a realistic intraseasonal oscillation is more prone to be excited when the maximum heating concentrates in the middle-low levels,especially in the middle levels,while westward propagating disturbances axe more prone to be produced when the maximum heating appears very high.     

Sensitivity of the Simulated Tropical Intraseasonal Oscillation to Cumulus Parameterizations

The sensitivity of the simulated tropical intraseasonal oscillation or MJO （Madden and Julian oscillation） to different cumulus parameterizations is studied by using an atmospheric general circulation model （GCM）--SAMIL （Spectral Atmospheric Model of IAP LASG）. Results show that performance of the model in simulating the MJO alters widely when using two different cumulus parameterization schemes-the moist convective adjustment scheme （MCA） and the Zhang-McFarlane （ZM） scheme. MJO simulated by the MCA scheme was found to be more realistic than that simulated by the ZM scheme. MJO produced by the ZM scheme is too weak and shows little propagation characteristics. Weak moisture convergence at low levels simulated by the ZM scheme is not enough to maintain the structure and the eastward propagation of the oscillation. These two cumulus schemes produced different vertical structures of the heating profile. The heating profile produced by the ZM scheme is nearly uniform with height and the heating is too weak compared to that produced by the MCA, which maybe contributes greatly to the failure of simulating a reasonable MJO. Comparing the simulated MJO by these two schemes indicate that the MJO simulated by the GCM is highly sensitive to cumulus parameterizations implanted in. The diabatic heating profile plays an important role in the performance of the GCM. Three sensitivity experiments with different heating profiles are designed in which modified heating profiles peak respectively in the upper troposphere （UH）, middle troposphere （MH）, and lower troposphere （LH）. Both the LH run and the MH run produce eastward propagating signals on the intraseasonal timescale, while it is interesting that the intraseasonal timescale signals produced by the UH run propagate westward. It indicates that a realistic intraseasonal oscillation is more prone to be excited when the maximum heating concentrates in the middle-low levels, especially in the middle levels, while westward propagating disturbances     

大气中40—60天低频振荡形成的数值试验

观测资料的分析表明,40—60天的低频振荡,除了在赤道附近有向东的传播外,在副热带和高纬度带还存在向西传播的现象.本文利用正压原始方程的谱模式,加以与运动(辐散)相联系的强迫(相当于加热场),模拟这类低频振荡发现有两类波存在:一类是周期约为10—20天向东传播的行星波,另一类是周期为40—60天向西传播的低频波,它是前一类行星波的波包相速度,每天5—6经度,纬向波数为1.这类低频波的出现可能是行星波与加热场非线性相互作用的结果. 这里之所以没有得到东传的40—60天的低频波,可能是由于模式格点较疏,使赤道Kelvin波不能明显激发出来.     

热带大气季节内振荡的进一步分析

利用ＥＣＭＷＦ的格点资料对热带大气季节内振荡作了进一步分析研究,表明热带大气季节内振荡既有Ｋｅｌｖｉｎ波型扰动,也有Ｒｏｓｓｂｙ波型扰动;影响热带大气季节内振荡移动的主要因素有扰动波型和积云对流活动的异常;伴随ＥｌＮｉｎｏ事件的发生,热带大气季节内振荡的动能急剧减小,而准定常扰动动能急剧增大,既反映了热带大气季节内振荡对ＥｌＮｉｎｏ的激发作用,也说明了在ＥｌＮｉｎｏ期间热带大气季节内振荡偏弱的原因。     

有蒸发-风反馈和海-气相互作用的CISK开尔文波——热带季节内振荡机制的进一步研究

将波动－CISK（积云对流加热反馈）、海－气相互作用和蒸发－风反馈都引入一个简单理论模式，研究了他们在驱动热带大气季节内振荡（ISO）中的作用。其结果表明：波动－CISK在减慢激发波的位相速度以接近观测到的热带ISO的移速过程中起主要作用；而蒸发－风反馈的主要作用是使激发波不稳定；海－气相互作用在减慢激发波的移速方面也有一定作用。因此，波动－CISK和蒸发－风反馈可认为是热带ISO的主要动力学机制。本研究还表明，由于蒸发－风反馈和海－气相互作用的影响，激发波是一种频散波，这种频散性可以更好地解释热带大气中ISO的活动特征。     

与季节内振荡-超级云团系统相关的赤道波的识别

文中重点研究与热带季节内振荡－超级云团系统相关联的赤道波的识别。考虑到赤道波的本质为截获在赤道地区的一般的气候平衡场附近的线性动力过程的固有模态,首先从原理上阐明了ＰＯＰｓ分析技术对于分离各类赤道波动的有效性,以后利用这种分析方法对日本静止气象卫星所观测到的黑体红外辐射温度资料进行了ＰＯＰｓ分析。结果表明,在热带季节内振荡－超级云团系统中,对应于４０ｄ振荡的模态基本表现为Ｋｅｌｖｉｎ波的结构;对应于１０ｄ左右的模态,亦为Ｋｅｌｖｉｎ波,而在２ｄ尺度上,则分别存在经向模态序号ｎ＝１和ｎ＝２的西进和东进惯性重力波。分析中还发现了西进的混合Ｒｏｓｓｂｙ重力波的存在。