渤海海面风场的一种动力诊断方法

给出一种动力诊断获取渤海海面风场的简便方法.首先建立一个简单的水平二维地面风场诊断模式,根据由微机支持的数字化仪输入的地面格点气压场,诊断出地面风场;然后利用渤海沿岸和岛屿海洋观测站(含石油平台站)实测风资料,运用简单的资料同化方法(张驰逼近方法)对诊断风场进行调整,从而得到渤海海面风场.结果表明,此方法简便有效.     

大气-海洋-海浪耦合同化模式在台风过程模拟中的应用

基于MCT耦合器,利用中尺度大气模型WRF、海洋模型FVCOM和第三代海浪模型SWAN,实现大气、海洋和海浪的三者实时耦合计算,同时采用卫星微波辐射资料AMSU-A,通过WRF大气模式的资料同化模块WRFDA,实现对风场模拟的连续同化,从而建立起大气-海洋-海浪耦合与卫星数据同化的W-F-S-A耦合同化模式。将该模型应用于2014年台风“威马逊”的数值模拟,并与其他模型进行比较。结果表明,W-F-S-A耦合同化模式对于台风路径和风速的模拟结果优于单独耦合和单独同化结果,并且可以较好地模拟上层海洋对台风的响应特征。     

深水风浪相关函数的研究

本文以风浪频谱和其相关函数的关系为基础,应用积分中值定理,给出了风浪相关函数的理论模型。进而以文氏等人的理论风浪频谱为原型,通过数值积分和待定系数法,给出了以风浪频谱的零阶矩m_0、峰频率ω_0和峰度因子P为参数的深水风浪相关函数式。最后把该式与数值计算值、实测值作了对比,证明本文所提出的深水风浪相关函数式较好地反映了各种不同成长状态的实际的相关函数。     

INFLUENCE OF THE VERTICAL SHEAR OF ENVIRONMENTAL FLOWS ON TYPHOON MOTION

Typhoon is regarded as a convergent,modified Rankine vortex.Based on the vorticity equations written attwo levels,higher and lower in the troposphere,typhoon motions are discussed in this study.The analyticalexpressions of vortex motion direction and speed have been derived for simple homogeneous basic flows at twolevels.The expressions indicate that in the easterties,vertical wind shear enhances the steering of east flow,causing the vortex moving westward faster,otherwise,in the westerlies,it reduces the steering of the west flow,causing the vortex moving eastward slower.These results explain theoretically that“cyclones in the easterliesmove to the right of,and faster than the basic flow;conversely,cyclones in the westerlies move to the left of,andslower than the basic flow.”     

基于VAP方法的多普勒雷达风场反演研究

采用VAP(Velocity Azimuth Processing)方法反演多普勒雷达风矢量场,在利用各个距离圈径向速度随方位角分布的廓线推算风向和风速的设计中,要求基数据速度资料中没有明显的脉动.介绍了在多普勒天气雷达风场反演设计中,直接将方格法的速度资料处理过程融入到方格法风场反演的过程中,利用距离方格内保持中尺度特性的特点,不改变原始资料的同时保证风场反演的正确性.     

Non-Stationary Rayleigh-Taylor Instabilities in Pulsar Wind Interaction with a Supernova Shell

The Rayleigh-Taylor instability (RTI) plays an important role in the dynamics of several astronomical objects, in particular, in the supernovae (SN) evolution. In the present paper we examine the dynamics of a shell (representing a type II SN remnant) blown-up by a wind emitted by a central pulsar. The shell is accelerated by the pulsar wind and its inner surface experiences the RTI. We develop an analytical approach by using a specific transformation into the coordinate frame co-moving with the SN ejecta. We first derive a non-stationary spherically symmetric solution describing an expansion of a gas shell under the pressure of a central source (pulsar). Then, we analyze its 3D stability with respect to a small perturbation on the inner shell surface. The dispersion relation is derived in the co-moving reference frame. The growth rate of the perturbation is found and its temporal evolution is discussed. We compare our result with the previous published studies and apply it to the Crab nebula evolution.     

Effect of offshore troughs on the South India erratic summer monsoon rainfall in June 2017

The onset and advance of southwest monsoon are accompanied by the appearance of the offshore trough along the southwest coast of India. This offshore trough escorts a deluge of rainfall to the southwest coast, and sometimes rainfall band moves eastward further into south India. These broad observations were noticed during the summer monsoon of June 2017. Meteorological agencies and media had reported a huge amount of rainfall over the southwest coast of India during the month. But, in the far interior of south India, rainfall was less. Due to the less rainfall, water resources depleted, which affected local farmers and common man of south India. The confused views of the common man on southwest coast rainfall could be due to lack of understanding related to various factors affecting rainfall over the same region. This article is an endeavor to address the preliminary understanding of the southwest coast rainfall during June 2017, with more stress on offshore troughs. The study begins with area-averaged rainfall statistics over south, southwest, and southeast India by employing satellite and rain gauge merged rainfall datasets. Area averaged analysis revealed offshore trough contributed 80 % of rainfall over the South West India, 68 % over South East India, contributing to an overall 75 % over south India in 2017. To identify offshore trough position and strength in the reanalysis and model simulations, a new method called VSV (Vertical Shear of Vorticity) method was introduced. The computed offshore troughs were categorized into Active, Normal, and Feeble based on the strength of meridional gradient of mean sea level pressure and 850 hPa horizontal winds. The contribution due to each category of the offshore trough over different sub-regions was investigated to find out the effect of the offshore trough to total rainfall. Dynamic and thermodynamic features of these categories of the offshore trough were investigated by using proxies like equivalent potential temperature and moisture flux convergence. We found that during active offshore trough an eastward propagation of rain bands persists, which was explained by using moisture flux convergence and equivalent potential temperature at different levels of the atmosphere.     

Derivation of Parametric Tropical Cyclone Models for Storm Surge Modeling

In this paper, the parametric tropical cyclone models for storm surge modeling are further developed. Instead of tangential wind speed via cyclostrophic balance and radial wind speed using a simple formulation of defection angle, the analytical expressions of tangential and radial wind speed distribution are derived from the governing momentum equations based on the general symmetric pressure distribution of Holland and Fujita. The radius of the maximum wind is estimated by tropical cyclone wind structure which is characterized by the radial extent of special wind speed. The shape parameter in the pressure model is estimated by the data of several tropical cyclones that occurred in the East China Sea. Finally, the Fred cyclone (typhoon 199417) is calculated, and comparisons of the measured and calculated air pressures and wind speed are presented.     

浮式风机一体化模拟的计算参数设置影响研究

随着海上浮式风机的大型化发展，针对漂浮式风机的一体化耦合分析越来越重要。本文利用Simo-Riflex-Aerodyn 仿真工具建立OC4-Deepcwind 漂浮式风机一体化耦合模型，分析计算时间步长、初始截断时间、弹性结构单元离散数等计算参数对模拟结果的影响，包括浮式基础运动、系缆张力、叶片受力等。结果表明：当计算时间步长为0.005 s、0.01 s、0.02 s 时，浮式风机的响应结果差别较小，而计算消耗时间相差较大，0.01 s、0.02 s 的计算时间分别是0.005 s的70%、37%。相同工况下，不同参量响应达到稳定所需时间不同，纵荡需要的时间较长，最长达200 s；不同工况下，同一参量达到稳定所需时间也不相同，切出工况需要的时间最短，较额定工况快约60 s。结构单元离散数对塔柱受力影响较小，对叶片变形影响相对明显，当叶片离散数目减小时，响应值增大12%。实际中应根据具体工况选择合理的计算时间步长、初始截断时间和弹性结构单元离散数量。     

基于Polar WRF模型的南极冰盖气温、风速和气压数值模拟北大核心CSCD

在全球变暖的背景下,南极已成为全球气候变化研究的热点,然而其区域内的观测站点稀疏且缺乏较长的时间序列,限制了人们对南极气候变化机制的分析与理解。Polar WRF作为目前最先进的极地区域气候模型之一,有力弥补了观测资料不足的缺陷,然而模式存在误差,在应用之前有必要对其定量评估。本文利用Polar WRF3.9.1对2004-2013年南极冰盖2m气温、10m风速和地表气压进行了数值模拟,并与28个气象站数据进行了对比分析,结果表明:模式对气温的模拟值在东南极沿岸偏低,在内陆偏高,在南极半岛既存在冷偏差也存在暖偏差,而对风速和气压的模拟整体呈高估。而从均方根误差和平均绝对误差的空间分布来看,模式对气温和气压的模拟结果在东南极沿岸的精度高于内陆和南极半岛,而风速则在内陆的精度要高于沿岸地区。但总体来说模拟效果较为理想,在2004-2013年间气温、风速、气压的模拟值的变化趋势与实测值的变化趋势相同。模式模拟的年平均2m气温和近地面气压在所有站点都通过了α=0.1的显著性检验,季节误差和月误差整体较小,且所有月份的相关系数都分别大于0.90与0.79。模式对10m风速的模拟精度要略低,部分沿岸站点的年平均误差超过了7.5m·s^(-1),但整体而言其在四季和各个月份的相关性均大于0.5且误差小于4.5m·s^(-1)。虽然Polar WRF作为天气模式,但在模拟长时间尺度的气候方面仍然表现较好。