近百年来中国的严重气候灾害

根据１８８０～１９９７年的各种气候序列,研究了１１８年中的严重气候灾害．这里严重有两重意义,首先是影响面广,其次是强度大．因此只研究了冷冬、冷夏、多台风、全国多雨、干旱及长江与黄河多雨、干旱等９种气候灾害．以大约１０年一遇为严重灾害,以３０～４０年一遇为异常灾害．给出各种灾害出现的年份,扼要地分析了各种灾害出现的规律及可能的形成原因．     

河南省近10年汛期多雨时段大尺度环流特征

利用1995~2004年气象资料,分析了河南省降水最多年份汛期降水集中时段的大尺度环流特征,结果发现:降水集中时段100hPa南亚高压120°E脊线基本维持在25~32°N之间,降水集中时段开始前南亚高压有一个东移北跳过程,降水集中期间100hPa高度场上呈现东高西低形势,有利于副高西伸和北抬;西太平洋副热带高压相对稳定,在多雨时段副高进退次数较多,且较长时间稳定在25°N左右,有利于西南暖湿气流沿副高外围进入河南省境内,为暴雨提供了充足的水汽;在降水集中时段,中纬度西风急流轴位置被北抬到40°N以北, 40°N以南基本是东风,这种中纬度地转西风持续偏弱,有利于副热带高压北跳和北跳后稳定,使雨带稳定在河南省。     

近百年东亚冬季气温及其大气环流变化型态

利用最新20世纪近百年再分析气象资料,研究近百年东亚冬季气温变化型及其相关的大气环流型态.结果表明近百年内东亚冬季气温主要有两种变化型:第一是东亚西南与东北相反气温变化型,表现在40°N以南及105°E以西地区(西南地区)气温变化与40°N以北及105°E以东地区(东北地区)变化相反;第二是40°N以南气温一致变化型.与第一种气温变化型耦合的大气模态是500hPa欧亚型遥相关、西伯利亚高压及北大西洋涛动.当欧亚型遥相关负位相,北大西洋涛动正位相及西伯利亚高压减弱时,有利于蒙古和我国105° E以东的区域增温而我国西南地区和青藏高原降温,反之亦然.第二种气温变化型耦合大气模态是500hPa西太平洋型遥相关,北太平洋涛动.当西太平洋型遥相关及北太平洋涛动处于正位相时(北太平洋北负南正),东亚40°N以南地区增温,东亚40°N以北地区降温.耦合的大气模态的型态差异,影响各阶段气温的年际变化.近一百年中,欧亚型遥相关和北大西洋涛动在1984～2010期间的型态最显著,是20世纪80年代东亚显著增暖的原因之一.研究还发现20世纪中期后东亚气温的年际变化与极地环流的变化联系紧密,表现在西伯利亚高压范围东扩并与极地环流联系,也是近百年气温趋势上升的一个原因.     

新疆百里风区强风中尺度特征分析

大尺度环流背景和天山山脉大地形共同作用形成新疆百里风区，其风力之大居全疆九大风区之首。为进一步研究百里风区强风中尺度特征及其与局地地形的关系，选取2018年5月6—8日百里风区强风天气过程，使用WRF模式进行中尺度模拟分析，形成以下结论：天山两侧气压梯度力驱动下冷空气翻越天山，经色皮山口狭管效应和过山波水跃下沉接力加速，在背风坡上空形成强风区，强风区接地形成百里风区地面大风；大风过程中，七角井盆地地形强迫引发有限振幅重力波，背风坡上空大风区之上的临界层吸收上层能量并向下传递，增大了大风区的风速，使得低空大风区的接地更加充分。低空大气稳定层结的强度与大风强度相对应。     

General polytropic spheres as gravitational lenses

We propose hydrostatic polytropic spheres governed by the Lane-Emden equation (LEE) of index $n$ as a novel set of physical models for axially averaged gravitational lenses anywhere in the Universe, alternative to the familiar singular isothermal sphere (SIS) and the Navarro–Frenk–White (NFW) profile, as such general polytropic spheres are conceptually simple, versatile in representing a series of equations of state, and able to address both the inner core and cusp features. As LEE is nonlinear, there exist several distinct classes of LEE solutions to serve as physical lens models. With a few scaling parameters, the complete problem can be readily reconstructed with full physical dimensions. A given mass density profile satisfying LEE produces lensing effects that are solely determined by a dimensionless parameter $q$ which contains geometric and kinematic information about the source-lens-observer system. The lens mapping and tangential shear or distortion profile are derived, first analytically for special cases and then asymptotically at the outskirts or near the edge of the lens. Numerical procedures for calculating full lensing profiles of a general lens are developed. Our results include the analytical “singular polytropic sphere” (SPS) profile which generalizes the SIS model and may outperform the latter in modeling dark matter halos among others. We further point out that dynamic models of general polytropic spheres in self-similar evolution can serve as several broad classes of gravitational lenses and produce time-dependent lensing effects slow or fast depending on the pertinent time scales. Astrophysical sources that can be lensed include electromagnetic wave sources in the entire frequency band, gravitational wave sources in the entire frequency band, gravitons even possibly with finite masses, neutrino sources of three different types, neutron sources, and ultra high energy cosmic rays (UHECRs) of electrically charged particles which can also interact with magnetic fields. We discuss and elabrate applications to dark matter halos, hypermassive black holes and supermassive black holes in the entire Universe including the early Universe, magnetized supermassive stars, static and dynamically evolving spherical and cylindrical lenses in contexts of astrophysics and cosmology.