共查询到18条相似文献，搜索用时 66 毫秒
1.
利用2014年6月-2017年9月的秒级探空资料,选取四川地区5个代表性站点研究重力波在对流层（2~10 km）和平流层（18~25 km）的时空特征。选取结果表明:重力波能量在四川地区各个高度均存在明显的季节变化,冬季强,夏季弱;在对流层由于地形影响,川西和川北高原地区的能量小于其他地区。垂直波长没有明显的时空变化,在对流层和平流层分别集中分布于1.5~3 km和1.5~3.5 km;水平波长则差别较大,分别分布于0~300 km和100~700 km,平均值分别为100 km和350 km。重力波固有频率在对流层有较大的区域差异,表现为在四川西北部的高原地区固有频率平均值为3f（f为地转参数）,其他地区则仅为2.4f;平流层则没有明显的差异存在,均约为2f。四川地区重力波的垂直传播方向特征基本相同,在对流层约有50%的波动向上传播,平流层则有90%以上的波动向上传播。水平传播则存在明显的不确定性,特别是对流层;平流层水平传播方向存在明显的季节变化,表现为夏季重力波多向偏东方向传播,而其他季节则向偏西方向传播。 相似文献
2.
利用2018年6月9日—7月10日安庆、长沙、赣州、南昌、宜昌、武汉6个探空站的往返式探空观测试验数据,研究分析了重力波参数（能量密度、固有频率、波长及传播方向）,统计了试验地区6—7月的重力波特征,比较了各站之间以及上升与下降段之间重力波的差异。主要结果如下:（1）该区域重力波动能分布在0.2—1.2 J/m3,平均约为0.8 J/m3,势能分布在0.03—0.5 J/m3,平均约为0.2 J/m3。（2）垂直波长中90%样本分布在1—2.5 km,超过50%的样本分布在2—2.5 km,平均波长为1.8 km左右;水平波长分布范围40—1500 km,主要集中在200—800 km,平均600 km,重力波垂直波长与水平波长的比值很小,在平流层重力波以水平传播为主。（3）大部分站点的上升和下降段结果均存在比较明显的主要传播方向,但主要传播方向特征并不一致,以西北方向传播最多,其次是北向传播。这种往返式探空数据适用于下平流层重力波的观测与分析,下降段资料起到对重力波事件的加密观测作用。上升与下降段所获得的结果存在一定差异,但除水平传播方向外,其余参数差别较小,除能量外,其余参数在下降段结果偏大。 相似文献
3.
《高原气象》2021,40(3):590-602
大气重力波对全球大气的动力、热力结构具有重要影响,研究重力波参数气候特征是研制全球大气模式中重力波参数化的一个重要环节,通过引入重力波的影响,有利于提高大气模式的预报能力。本文利用2014-2017年太原地区(112.55°E,37.78°N)高垂直分辨率探空资料,对其对流层(2～9 km)、下平流层(17～24 km)大气重力波参数的气候特征及其之间差异特征进行研究。结果表明:(1)在1-12月,相对于对流层,下平流层的平均重力波水平波长、周期、固有相速、能量上传百分比均偏大,垂直波长均偏小,但群速在2月、5-9月偏大,其他月份偏小;(2)对流层与下平流层之间的重力波参数偏差、绝对差较大,相关性弱;(3)对流层、下平流层的重力波参数及其之间的偏差,在不同区间范围内的占有率分布特征存在明显差异;通过研究太原地区上空对流层、下平流层大气重力波参数的气候及其之间差异特征,进一步补充了中国区域的大气重力波参数气候特征,有利于研制更适合中国区域数值预报模式的重力波参数化方案。 相似文献
4.
《干旱气象》2016,(5)
针对晋西北地区2013年8月6—8日出现的一次雷阵雨天气过程,利用垂直高分辨率探空资料获取此次天气过程中大气重力波的周期、水平波长、垂直波长、波传播方向和群速等参数值,分析这些波参数值随时间的演变特征。结果表明:在此次雷阵雨生成和发展期(6—7日),由小尺度强对流天气系统引起的非地转平衡,激发出周期小、水平波长短且群速快的重力内波,其中,重力波周期、水平波长分别由1.05 h、23.36 km减小到0.22 h和5.67 km,而波群速由5.30 m·s-1增大到18.69 m·s-1,波传播方向由-93.51°转变为35.05°;当雷阵雨进入消亡期(8日),大气重新调整为准平衡状态,导致重力波周期及水平波长显著变大、且波群速明显变慢,其中,重力波周期和水平波长分别由0.22 h、5.67 km迅速增大到9.06 h和268.98 km,而波群速由18.69 m·s-1快速减小到2.60 m·s-1,波传播方向由35.05°转变为-140.10°;在整个天气过程中,重力波垂直波长变化不大。因此,是否存在周期小、水平波长短且群速快的重力波与雷阵雨的发生关系密切。 相似文献
5.
2005年4月19日19-22时,哈尔滨雷达站观测到重力波结构,本文主要利用新一代多普勒天气雷达速度场资料对本次过程的重力波结构进行分析。在本次重力波发生发展过程中,径向速度在水平方向上表现为正负速度交替分布的特征;垂直速度在水平方向上平均高度1100m以下是上升、下沉气流交替分布,垂直方向上的气流有时是与垂直方向成一定角度的;重力波波长约为5km,相速约为10m／s,周期约为8min,最大振幅约为1．3km,波动最多有8个位相。重力波的波相传播方向与波能传播方向相同,且与环境风场的方向相同。影响本次重力波发生发展的动力因子主要有700hPa的低空急流、地面到高空强烈的垂直风切变以及锋面。另外重力波对层状云降水有一定的促进作用。 相似文献
6.
重力波参数气候特征是确定全球大气模式中重力波参数化方案的一个重要环节,利用高垂直分辨率探空资料扰动场是获取重力波参数气候特征的基础数据和重要手段。目前,通常采用2～4阶曲线拟合、带通滤波方法获取高垂直分辨率探空资料扰动场,但针对不同方法之间的扰动场差异特征研究较少,本文利用2～4阶曲线拟合、带通滤波方法(0.5～5.0km)获取2014—2017年太原地区(112.55°E,37.78°N)高垂直分辨率探空资料扰动场,采用相关系数、Lomb-Scargle、不同区间范围占有率方法进行研究,结果表明:①不同方法之间的纬向风扰动场、经向风扰动场、温度扰动场均存在较明显差异,且相关性均较弱;②Lomb-Scargle分析表明,不同方法得到的平均纬向风扰动场、平均经向风扰动场、平均温度扰动场显著含有(通过90%置信检验)的垂直波长均存在明显差异;③不同方法得到的纬向风扰动场、经向风扰动场、温度扰动场显著含有的垂直波长,在不同区间范围内的占有率均存在明显差异。 相似文献
7.
殷青青任璐田文寿王涛杨景怡张健恺 《干旱气象》2022,(3):444-456
对流激发的重力波能够向中层大气输送动量和能量,准确获取重力波主要特征对于研究中层大气的动力学和热力学结构非常重要。本文利用COSMIC(constellation observing system for meteorology,ionosphere and climate)资料,结合中尺度数值预报模式WRF(weather research and forecasting),对2010年8月4日发生在华北地区上空的一次对流激发的重力波事件进行分析。结果表明:此次事件激发的重力波在平流层以中低频重力波为主,且在平流层中垂直波长、水平波长分别为9~11 km和650~800 km,约62%的动量聚集在15~25 km高度的低平流层。在对流活动发生期间,低平流层重力波势能密度一直维持较大数值,而上平流层重力波势能密度则在对流减弱后迅速减小,且伴随着下一次对流活动的出现再次迅速增大。平流层不同高度上重力波势能密度对对流活动的响应主要与对流发展高度和背景风场有关,当对流发展较浅时,其激发的重力波在低层西风中易耗散;当对流发展较深到16 km甚至更高时,其激发的重力波接近零风层,并在东风中迅速上传,使得高层重力波势能密度增加较快。 相似文献
8.
利用2019年1月1—7日AIRS观测的(80°—100°W,30°—45°N)范围内0—45 km高度的大气温度剖面数据,根据重力波的线性理论,分别采用垂直滑动窗口法、双滤波器法、单滤波器法对温度廓线数据进行处理,从中得到初始扰动剖面,再使用分离出来的对流层到平流层低层的背景温度和重力波扰动剖面计算重力波势能,最后根据提取结果比较三种方法的差异。结果表明:1) 采用垂直滑动窗口法提取的重力波势能对波长较小的波动有很好的反映,在对流层顶区域重力波势能异常偏大。2) 采用双滤波器法提取的重力波势能很好地反映各个波长的波动,更符合真实情况。3) 采用单滤波器法能够提取波长较大的重力波扰动,且扰动在对流层贡献更大;而采用双滤波器提取的重力波扰动分别在对流层顶和平流层贡献更大。 相似文献
9.
重力波参数气候特征是确定大气模式中重力波参数化方案的重要条件之一,高垂直分辨率探空资料扰动场是获取重力波参数气候特征的基础数据;目前,获取扰动场的方法较多,但基于不同方法计算的扰动场对重力波参数气候特征影响的研究较少。基于2014—2017年山西太原气象台高垂直分辨率探空资料,利用2—4阶曲线拟合方法获取下平流层（17—24 km高度）温度扰动场、纬向风扰动场和经向风扰动场,经统计发现2阶与3阶曲线拟合方法的扰动场相似程度较高;在此选取相似度较高的2阶、3阶曲线拟合方法的扰动场分别计算大气重力波参数,并对大气重力波参数间的气候差异特征进行研究。结果表明:（1）不同阶曲线拟合方法扰动场的变化振幅及随高度变化趋势存在差异,且扰动场间的相关较弱;（2）2阶、3阶曲线拟合方法扰动场得到的重力波参数大小、年内变化趋势及在不同区间范围内占有率均存在差异,且相关较弱;（3）1—12月,相对3阶曲线拟合方法的扰动场,基于2阶曲线拟合方法的扰动场得到的重力波群速、水平波长、垂直波长、周期、固有相速均较大,而重力波能量上传百分比在某些月份较大。因此,不同阶曲线拟合方法扰动场间存在差异,会导致计算得到的大气重力波参数气候特征存在差异,最终对研制大气模式中的大气重力波参数化方案产生影响。 相似文献
10.
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
11.
Summary The effects of varying horizontal and vertical grid resolution on the numerical simulation of upper-tropospheric frontal structures are examined using a, two-dimensional, dry, hydrostatic sigma-coordinate primitive equation model. These effects are illustrated with the results of 72 h model integrations in which frontogenesis is forced solely by confluence. Four different horizontal grid spacings, ranging from 100 km to 12.5 km, and four different vertical, grid resolutions, varying from 10 to 70 layers (90 mb to 13 mb), are considered.The intensity and integrity of the frontogenesis as a function of grid resolution are diagnosed in terms of time histories and spatial distributions of frontal parameters, such as the speed of the along-front jet, maxima of absolute vorticity and potential temperature gradient, and ageostrophic motions. The time histories show that, provided the vertical resolution is sufficient, increasing horizontal resolution leads to better-defined frontal structure due to the decrease in cross-frontal scale. They also indicate that for a given horizontal resolution there exists an optimal vertical resolution beyond which frontal parameters change only slightly. This optimal vertical resolution increases with increasing horizontal resolution, and apparently is related to the horizontal resolution through the slope of the frontal zone.The time histories for simulations combining low vertical resolution with high horizontal resolution exhibit substantial high-frequency variability. Cross sections show that this temporal variability appears to be manifested spatially in the form of gravity waves characterized by wavelengths on the order of 200 km and periods of 12 h, over the range of horizontal and vertical resolution that is considered. Although the source mechanism for these waves cannot be established definitively, it likely involves a grid-induced ageostrophic component of the along-front wind which disrupts thermal wind balance. This results thus demonstrates the potential risk of flawed frontal simulations, when incompatible combinations of horizontal and vertical resolution are used.With 7 Figures 相似文献
12.
Summary Seasonal variations of gravity wave characteristics are investigated using rawinsonde data observed at Pohang observatory,
Korea (36°2′N, 129°23′E) during the one-year period of 1998. Analysis is carried out for two atmospheric layers representing
the troposphere (2–9 km) and stratosphere (17–30 km). There exist clear seasonal variations in amplitudes of temperature and
wind perturbations and wave energy in the stratosphere, with their maxima in wintertime and minima in summertime. A strong
correlation is found between the wave activity and the strength of the jet stream, but there is no clear correlation between
the wave activity and the vertical gradient of static stability. The intrinsic frequency and vertical and horizontal wavelengths
of gravity waves in the stratosphere are 2f–3f, where f is the Coriolis parameter, and 2–3 km and 300–500 km, respectively. The intrinsic phase velocity directs westward in January
and northeastward in July. The vertical flux of the stratospheric zonal momentum is mostly negative except in summertime with
a maximum magnitude in January. Topography seems to be a major source of stratospheric gravity waves in wintertime. Convection
can be a source of gravity waves in summertime, but it is required to know convective sources at nearby stations, due to their
intermittency and locations relative to floating balloons. 相似文献
13.
Wavelike motions within a strong morning inversion of the planetary boundary layer were investigated experimentally using two atmospheric research aircraft: an Aerocommander 280FL and a Cessna 206. The Aerocommander aircraft, instrumented for the measurement of rapid fluctuations of temperature, water vapour density and air velocities, was flown horizontally at different levels within the inversion layer in order to document adequate data on the wave motion. An example of such motions observed on 8 June, 1974 is described and analyzed in the present paper. The aircraft records obtained within the inversion layer at about 600 m above the ground show large fluctuations of the meteorological variables with well-defined amplitudes and wavelengths.Spectra and cross-spectra of temperature, water vapour density and air velocities were computed and analyzed to determine characteristics of gravity waves according to the method described by Metcalf (1975). These spectra exhibit a sharp maximum associated with high coherences at a particular wavelength. In this narrow spectral band, phase angles ±90 ° are obtained between vertical velocity and temperature as well as between vertical and horizontal velocities. These features suggest that observed motions are horizontally propagating trapped or evanescent waves. They enable us to estimate true wavelengths (500 m), wave vector azimuths, intrinsic frequencies and phase velocities of these waves. These results appear to be mutually consistent. Furthermore, it is possible to confirm these latter with the detailed vertical profiles of the boundary layer provided by the Cessna aircraft making spiral soundings. In this regard, the vertical structure of the Brunt-Väisälä frequency confirms that the waves are everywhere evanescent except within a thin highly stable layer between the diurnal mixed layer and the overlapping inversion. Moreover, examination of the wind profiles reveals that the interfacial vertical wind shear might be a relevant parameter reducing phase velocities. Such a conclusion is also supported by the observed wave vector directions which appear to be closely parallel to the wind shear vectors at the 600-m level. Additional confirmation is found by comparing the observed wavelengths to those predicted by applying the hydrodynamical stability model of Hazel (1972) to the measured profiles. Although the wind shear clearly plays a role in wave development, local heat flux and temperature variance values show that in this case the instability is only a marginal and sporadic event embedded in nearly neutral waves. Accordingly, it is argued that the observed motions are interfacial waves at the inversion base level, the amplitude and wave vector azimuth of which are controlled by the vertical wind shear.
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Complexe Scientifique des Cézeaux BP 45 - 63170 Aubiere. 相似文献
Ondes de gravite interfaciales marginalement instables dans la couche limite planetaire
Résumé Des ondes de gravité interfaciales progressives sont étudiées à l'aide de deux avions dans la couche limite planétaire. Les spectres des vitesses et de la température fournissent les directions et vitesses de propagation. La comparaison des résultats aux profils verticaux du vent et de la température montre que ces ondes sont marginalement instables sous l'effet du cisaillement vertical du vent.
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14.
Energy- and Flux-Budget Turbulence Closure Model for Stably Stratified Flows. Part II: The Role of Internal Gravity Waves 总被引：1，自引：1，他引：0
S. S. Zilitinkevich T. Elperin N. Kleeorin V. L’vov I. Rogachevskii 《Boundary-Layer Meteorology》2009,133(2):139-164
We advance our prior energy- and flux-budget (EFB) turbulence closure model for stably stratified atmospheric flow and extend it to account for an additional vertical flux of momentum and additional productions of turbulent kinetic energy (TKE), turbulent potential energy (TPE) and turbulent flux of potential temperature due to large-scale internal gravity waves (IGW). For the stationary, homogeneous regime, the first version of the EFB model disregarding large-scale IGW yielded universal dependencies of the flux Richardson number, turbulent Prandtl number, energy ratios, and normalised vertical fluxes of momentum and heat on the gradient Richardson number, Ri. Due to the large-scale IGW, these dependencies lose their universality. The maximal value of the flux Richardson number (universal constant ≈0.2–0.25 in the no-IGW regime) becomes strongly variable. In the vertically homogeneous stratification, it increases with increasing wave energy and can even exceed 1. For heterogeneous stratification, when internal gravity waves propagate towards stronger stratification, the maximal flux Richardson number decreases with increasing wave energy, reaches zero and then becomes negative. In other words, the vertical flux of potential temperature becomes counter-gradient. Internal gravity waves also reduce the anisotropy of turbulence: in contrast to the mean wind shear, which generates only horizontal TKE, internal gravity waves generate both horizontal and vertical TKE. Internal gravity waves also increase the share of TPE in the turbulent total energy (TTE = TKE + TPE). A well-known effect of internal gravity waves is their direct contribution to the vertical transport of momentum. Depending on the direction (downward or upward), internal gravity waves either strengthen or weaken the total vertical flux of momentum. Predictions from the proposed model are consistent with available data from atmospheric and laboratory experiments, direct numerical simulations and large-eddy simulations. 相似文献
15.
一次暴风雪过程中的中尺度重力波特征及其影响 总被引：2，自引：0，他引：2
应用地面自动气象站观测资料、数字化多普勒天气雷达探测资料和WRFV2.2.1中尺度数值模拟资料,分析了中尺度重力波与基本气流的相互作用,以及重力波活动对暴雪和大风天气的重要影响。结果表明,在波导中传播的中尺度重力波能够与基本气流进行动量交换,使得对流层中上层4.5—8 km气层内的水平平均风速趋于均匀,形成斜穿整个对流层的饱和湿空气急流,即"湿急流"。在高空急流出口区激发的垂直向下传播的重力波,使基本气流的水平风速在垂直方向上出现了加速和减速的交替变化,水平风加速的气层,反射率增大;水平风减速的气层,反射率减小。随着波动下传及其随基本气流的移动,反射率回波强度沿高空风的方向(由西南向东北)出现周期性变化,回波带呈西北—东南走向,强回波中心之间为宽约40 km的弱回波区。重力波下传期间,当地面气压迅速下降时,东北风快速增长,风向有明显的改变,反射率强度开始减弱;气压脊线过后,反射率降低到最低点。地面大风中心出现在反射率回波强度周期性变化的地带,沿西南—东北方向间隔着分布。雷达探测表明,对流层低层风速在风向切变层上下边界对称相等,因此推测在重力波与切变层汇合的高度层存在垂直环流,由风切变层上下边界附近的西南气流和东北气流与受重力波影响形成的垂直方向上的上升和下沉气流共同组成。切变层上方的动量通过垂直环流的下沉支到达地面,强风中心对应着下沉气流,出现在降水回波开始减弱之际。 相似文献
16.
本文利用2012～2015年西南涡加密观测大气科学实验的剑阁、金川、九龙和名山四站探空资料,统计分析了6～7月西南涡活动期间对流层中、高层（6～12 km）的重力波过程,结果表明:青藏高原东部川西高原南部的九龙站与其余三站不同,重力波源主要来自对流层上层,波能传播方向向上,剑阁、金川和名山三站重力的波源主要来自对流层下层,波能传播方向向下。重力波过程在不同类型的西南涡活动中有明显差异,在移出型西南涡活动初期,重力波水平传播方向主要为东北向,其上传概率远大于下传概率,波动的动能和潜能较大且变化剧烈;而对应源地型西南涡,初期主要呈西北—东南向传播且重力波上传与下传概率相当,动能和潜能较小且变化相对平缓同时本次研究表明,重力波水平传播方向对西南涡的移动方向也有一定指示作用。按照发生时刻本文将重力波分为日发型重力波和夜发型重力波,在夜发型西南涡初期,重力波活动夜发（北京时20:00～08:00）的概率较大,这表明重力波的夜发性与西南涡的夜发性可能存在一定关联。 相似文献
17.
ＩｎｔｅｒｎａｌＧｒａｖｉｔｙＷａｖｅｓＧｅｎｅｒａｔｅｄｂｙａＬｏｃａｌＴｈｅｒｍａｌＳｏｕｒｃｅｉｎａｎＩｒｒｏｔａｔｉｏｎａｌＺｏｎａｌ－ＶｅｒｔｉｃａｌＰｌａｎｅ：ＮｕｍｅｒｉｃａｌＡｎａｌｙｓｉｓＺｈａｎｇＤａｉｚｈｏｕ（张代洲）（Ｃｅｎｔ... 相似文献
18.
Characteristics and sources of inertia-gravity waves revealed in the KEOP-2007 radiosonde data 总被引：1，自引：0，他引：1
Characteristics and sources of inertia-gravity waves are investigated using high-resolution radiosonde data observed at ten stations in Korea during 15 June to 15 July 2007. The wave analyses are performed in the lower stratospheric region (Z = 17–30 km). The average intrinsic frequency, vertical wavelength, and horizontal wavelength for the observed waves are 2.77f (where f is the Coriolis parameter), 2.58 km, and 620.11 km, respectively. The average eastward and westward momentum fluxes are 0.005 m2 s?2 and ?0.003 m2 s?2, respectively, and the average northward and southward momentum fluxes are 0.007 m2 s?2 and ?0.002 m2 s?2, respectively. To understand the propagation and the sources of the observed gravity waves, a three-dimensional ray-tracing model is used. The observed gravity waves are classified into two groups based on the existence of convection when and where the rays reach altitudes of 6–13 km. Sources are mostly located in the northeast and southeast of the observation stations below Z = 5 km for the convection-related cases (CONV), while those for the other cases (NCONV) are located in the northeast and southeast of the observation stations above Z = 20 km. The average intrinsic frequency and vertical wavelength of the CONV cases are somewhat larger than those of the NCONV cases. The average potential, kinetic, and total wave energies of the CONV cases are less than those of the NCONV cases. 相似文献