1月北大西洋东部-乌拉尔山阻塞高压频次年际尺度偶极子模态特征

基于观测和再分析资料,本文研究了近几十年来1月北大西洋东部-乌拉尔山阻塞高压频次年际变异主导模态特征及与其相联的大气背景场。结果表明,1980—2019年冬季(12月—次年2月)该地区阻塞高压频次年际变异的主导模态存在明显月际差异:12月表现为北大西洋东部-欧洲西部地区阻塞高压频次的显著同位相变化,1月为北大西洋东部-欧洲西部与乌拉尔山地区阻塞高压频次的具有显著的反位相变化即偶极子模态,2月则为北大西洋东部-乌拉尔山阻塞高压频次的显著同位相变化。进一步研究表明:1月北大西洋东部-乌拉尔山阻塞高压频次偶极子模态与同期局地纬向西风、纬向风垂直切变、经向位涡梯度等大气背景场异常偶极型变化相联系。当乌拉尔山地区关键大气背景场为负异常,而北大西洋东部-欧洲西部为正异常时,两个地区阻塞高压频次分别增加和减少,呈现偶极子模态;反之亦然。阻塞高压频次偶极子模态及相关的背景环流异常可通过调节水平温度平流、垂直运动和水汽输送等来影响1月欧亚北部气温和降水,以及它们的极端事件频次。当阻塞高压频次偶极子模态处于正位相时,乌拉尔山北部(南部)和欧洲南部增温(降温),极端暖、冷事件频次分别增加(减少)和减少(增加...     

华北近60年夏季降水年际异常与大气动力、水汽条件关系的研究

本文基于华北夏季降水数据、NCEP/NCAR再分析环流数据,采用了相关、合成和环流异常回归重构等方法,分析了东亚副热带夏季风指数、华北大气动力上升指数与华北夏季降水的关系。主要结果如下：1）东亚副热带夏季风指数、华北大气动力上升指数与华北夏季降水有很好的对应关系。当两个指数偏强时,华北夏季降水会异常偏多;两个指数偏弱,华北夏季降水异常偏少;如果两个指数强弱不一致时,华北会出现区域性降水偏多情况,但全区整体降水量基本为正常值。2）华北夏季降水异常是东亚副热带夏季风和华北大气动力上升运动协同作用的结果。在东亚副热带夏季风指数、华北大气动力上升指数偏强年,夏季500hPa层贝加尔湖槽会加深、西北太平洋副热带高压会偏北,华北处于“东高西低”的环流型控制下,西部低槽东移受阻,在华北维持较长时间的大气上升运动;850hPa层印度夏季风、东亚副热带夏季风会偏强,这时热带印度洋西风水汽输送以及东亚副热带地区偏南风水汽输送或东南风水汽输送会加强,华北水汽来源充足。这种高、低空环流配置非常有利于造成华北夏季降水异常偏多。反之,华北夏季降水会异常偏少。3）前期4—5月,东亚副热带夏季风指数、华北大气动力上升...     

高层大气密度的午夜极大值特征分析与建模

利用CHAMP (CHAllenging Minisatellite Payload)、GRACE-A (Gravity Recovery and Climate Experiment-A)、SWARM-C (The Earth''s Magnetic Field and Environment Explorers-C)等3颗极轨卫星的资料, 研究360—480km高层大气密度在低纬度区域的午夜极大值(Midnight Density Maximum, MDM)现象. MDM一般出现在23:00- 02:00 LT (Local Time)之间,峰值位置在低纬度15°以内,谷值位置在中纬度35°-45°附近,整体略偏向南半球,振幅约为平均密度的26%.随着高度增大以及太阳辐射水平的增强,MDM振幅呈减小趋势;冬至和夏至日附近的季节效应会减弱MDM振幅,在春秋分日的振幅最大.用3个主流大气模型DTM2000 (Drag Temperature Model 2000), NRLMSISE00 (US Naval Research Laboratory, Mass Spectrom-eter and Incoherent Scatter radar)和JB2008 (Jacchia- Bowman 2008 model)对MDM进行模拟,JB2008没有刻画出MDM现象;另两个模型低估了MDM效应,在360km和480km两个高度DTM2000模型的振幅仅为观测的46%和53%, NRLMSISE00模型仅为观测的33%和26%;模型没有准确刻画出MDM与高度、辐射水平和季节的关系.联合3颗卫星的资料,研究了-种基于地理纬度的6阶勒让德多项式,同时融合地方时和高度因素的经验函数,在振幅和相位上可以较好地刻画MDM特征,相关系数达到0.923,可为大气密度模型的修正提供借鉴,服务于低轨道航天器高精度轨道预报.     

热红外波段大气透过率和程辐射的估算方法

文中对M ONTRAN模型内嵌6种大气模式的主要特性差异进行分析,并以中纬度夏季大气模式为例,分析了主要参数(如水汽、臭氧以及气温等)对估算热红外波段大气透过率和程辐射的影响。论文最后对利用探空数据构造完整大气模式进行了研究。     

1980—2019年江淮地区夏季气温变化及其异常年环流特征

利用1980—2019年ERA5月平均2 m气温资料、NCEP/NCAR提供的大气环流资料以及NOAA的海表温度资料,分析了江淮地区夏季气温变化及其异常年环流特征。结果表明：江淮地区夏季气温整体呈波动上升趋势,冷暖交替出现,在2000年发生突变,空间分布上表现出整体一致性;气温变化主要受西太平洋副热带高压（简称西太副高）、东亚夏季风及西伯利亚冷空气的影响;高温年江淮地区为大范围的位势高度正距平控制,西太副高整体偏西偏强,江淮地区处于副高脊线附近,高纬度阻塞高压较强,低温年则反之;高温年赤道中东太平洋及西太平洋海温分布具有拉尼娜事件的特征,而低温年赤道中东太平洋及西太平洋海温分布具有厄尔尼诺事件的特征;赤道中东太平洋海温异常偏高年江淮地区气温整体偏低,偏低年反之。     

青海驼路沟钴(金)矿床成矿物质来源的黄铁矿氦氩硫铅同位素示踪

为查明青海驼路沟新型独立钴(金)矿床的成因和成矿物质来源,文章对矿区发育的块状、条带状和浸染状黄铁矿矿石进行了黄铁矿流体包裹体氦氩同位素和黄铁矿硫、铅同位素测试。结果表明,不同类型矿石的成矿流体氦、氩同位素组成基本一致,3He/4He介于0.10~0.31Ra(平均0.21Ra),40Ar/36Ar比值为302~569(平均373),反映钴矿化流体主要来源于在赋矿岩系中深循环的大气降水;矿石黄铁矿硫同位素值分布集中且接近于零,δ34S变化于-4.5‰~+1.5‰,集中在-1.8‰~-0.2‰,显示深部来源;矿石铅以高放射性成因为特征(206Pb/204Pb>19.279、207Pb/204Pb>15.691、208Pb/204Pb>39.627),且自地层围岩→区域早古生代火山岩→矿石依次明显增大,可能指示高放射性成因矿石铅主要是由以深循环大气降水来源为主的热液不断从围岩地层中淋取而来。     

现代尘暴和非尘暴天气大气花粉特征及其环境意义--以北京地区为例

通过2001²003年取得的尘暴和非尘暴天气大气花粉的对比研究,发现两类天气条件下大气花粉组合虽都以北京地区木本植物花粉为主,但尘暴天气样品中草本植物花粉数量有较多增加。根据尘暴活动和北京地区物候分析,推测这些草本植物花粉来自尘暴源区和路径区的表土沉积。基于上述认识,进一步对风成黄土古土壤层的花粉进行探讨,认为古土壤中草本植物花粉和木本植物花粉是同期沉积的,其木本植物花粉数量比较少可能是尘暴降尘导致草本植物花粉数增多所致。通过现代尘暴、非尘暴天气大气花粉特征的研究,对正确认识过去风成黄土和古土壤层中以草本植物花粉为主的孢粉组合特征提出了新的思路。     

Properties and stability of a meso-scale line-form disturbance

By using the 3D dynamic equations for small- and meso-scale disturbances, an investigation is performed on the heterotropic instability (including symmetric instability and traversal-type instability) of a zonal line-like disturbance moving at any angle with respect to basic flow, arriving at the following results: (1) with linear shear available, the heterotropic instability of the disturbance will occur only when flow shearing happens in the direction of the line-like disturbance movement or in the direction perpendicular to the disturbance movement, with the heterotropic instability showing the instability of the internal inertial gravity wave; (2) in the presence of second-order non-linear shear, the disturbance of the heterotropic instability includes internal inertial gravity and vortex Rossby waves. For the zonal line-form disturbance under study, the vortex Rossby wave has its source in the second-order shear of meridional basic wind speed in the flow and propagates unidirectionally with respect to the meridional basic flow. As a mesoscale heterotropic instable disturbance, the vortex Rossby wave has its origin from the second shear of the flow in the direction perpendicular to the line-form disturbance and is independent of the condition in the direction parallel to the flow; (3) for general zonal line-like disturbances, if the second-order shear happens in the meridional wind speed, i.e., the second shear of the flow in the direction perpendicular to the line-form disturbance, then the heterotropic instability of the disturbance is likely to be the instability of a mixed Rossby–internal inertial gravity wave; (4) the symmetric instability is actually the instability of the internal inertial gravity wave. The second-order shear in the flow represents an instable factor for a symmetric-type disturbance; (5) the instability of a traversal-type disturbance is the instability of the internal inertial gravity wave when the basic flow is constant or only linearly sheared. With a second or nonlinear vertical shear of the basic flow taken into account, the instability of a traversal-type disturbance may be the instability of a mixed vortex Rossby – gravity wave.     

Applications of conditional nonlinear optimal perturbation to the study of the stability and sensitivity of the Jovian atmosphere

A two-layer quasi-geostrophic model is used to study the stability and sensitivity of motions on smallscale vortices in Jupiter’s atmosphere. Conditional nonlinear optimal perturbations (CNOPs) and linear singular vectors (LSVs) are both obtained numerically and compared in this paper. The results show that CNOPs can capture the nonlinear characteristics of motions in small-scale vortices in Jupiter’s atmosphere and show great difference from LSVs under the condition that the initial constraint condition is large or the optimization time is not very short or both. Besides, in some basic states, local CNOPs are found. The pattern of LSV is more similar to local CNOP than global CNOP in some cases. The elementary application of the method of CNOP to the Jovian atmosphere helps us to explore the stability of variousscale motions of Jupiter’s atmosphere and to compare the stability of motions in Jupiter’s atmosphere and Earth’s atmosphere further.     

Implementation of the semi-Lagrangian advection scheme on a quasi-uniform overset grid on a sphere

The semi-Lagrangian advection scheme is implemented on a new quasi-uniform overset （Yin-Yang） grid on the sphere. The Yin-Yang grid is a newly developed grid system in spherical geometry with two perpendicularly-oriented latitude-longitude grid components （called Yin and Yang respectively） that overlapp each other, and this effectively avoids the coordinate singularity and the grid convergence near the poles. In this overset grid, the way of transferring data between the Yin and Yang components is the key to maintaining the accuracy and robustness in numerical solutions. A numerical interpolation for boundary data exchange, which maintains the accuracy of the original advection scheme and is computationally efficient, is given in this paper. A standard test of the solid-body advection proposed by Williamson is carried out on the Yin-Yang grid. Numerical results show that the quasi-uniform Yin-Yang grid can get around the problems near the poles, and the numerical accuracy in the original semi-Lagrangian scheme is effectively maintained in the Yin-Yang grid.