大气折射与路径弯曲延迟

电磁波信号在地球大气中的传播受到折射的影响,传播的方向发生了改变,传播的路径变为曲线,长度大于直线距离,相应的传播时间也被延长了,采用一个简化的球对称大气模型计算了光线在不同天顶距下由于路径弯曲而引起的延迟改正.     

Abundances of Jupiter's trace hydrocarbons from Voyager and Cassini

The flybys of Jupiter by the Voyager spacecraft in 1979, and over two decades later by Cassini in 2000, have provided us with unique datasets from two different epochs, allowing the investigation of seasonal change in the atmosphere. In this paper we model zonal averages of thermal infrared spectra from the two instruments, Voyager 1 IRIS and Cassini CIRS, to retrieve the vertical and meridional profiles of temperature, and the abundances of the two minor hydrocarbons, acetylene (C₂H₂) and ethane (C₂H₆). The spatial variation of these gases is controlled by both chemistry and dynamics, and therefore their observed distribution gives us an insight into both processes. We find that the two gases paint quite different pictures of seasonal change. Whilst the 2-D cross-section of C₂H₆ abundance is slightly increased and more symmetric in 2000 (northern summer solstice) compared to 1979 (northern fall equinox), the major trend of equator to pole increase remains. For C₂H₂ on the other hand, the Voyager epoch exhibits almost no latitudinal variation, whilst the Cassini era shows a marked decrease polewards in both hemispheres. At the present time, these experimental findings are in advance of interpretation, as there are no published models of 2-D Jovian seasonal chemical variation available for comparison.     

大气重力波产生大尺度赤道扩展F的理论

本文提出了大气重力波触发Ｒａｙｌｅｉｇｈ－Ｔａｙｌｏｒ不稳定性并导致大尺度赤道扩展Ｆ的理论．重力波作为外部扰动派触发等离子体扰动,这种扰动在Ｒａｙｌｅｉｇｈ－Ｔａｙｌｏｒ不稳定性的作用下继续增长,经过４００ｓ扰动幅度就能增长到５０％,经过７００ｓ后幅度趋近１００％,即为完全的等离子体泡．由于Ｅ区的影响,赤道扩展Ｆ主要出现于晚上．本文的理论阐明了重力波与Ｒａｙｌｅｉｇｈ－Ｔａｙｌｏｒ不稳定性相互作用的性质,揭示了大尺度赤道扩展Ｆ的产生机制．     

热带大气季节内振荡和ENSO的相互关系

通过观测资料的分析和数值模拟,研究了热带大气季节内振荡与ＥＮＳＯ的相互关系．一方面,在Ｅ１Ｎｉｎｏ事件发生之前,热带大气季节内振荡（尤其是在赤道中西太平洋地区）异常偏强,通过海一气相互作用它可能是Ｅ１Ｎｉｎｏ的一种重要激发机制．同时,赤道中西太平洋地区大气季节内振荡的异常加强同东亚中高纬度地区３０—６０天振荡的加强和强东亚冬季风有关．另一方面,ＥＮＳＯ对热带大气季节内振荡也有重要影响,在Ｅ１Ｎｉｎｏ期间,热带大气季节内振荡明显减弱;其结构明显趋于正压性．     

Aerosol concentrations and size distribution in the troposphere and lower stratosphere over Thumba

Rocket-borne ultraviolet photometers operating at =0.31 m have been used at Thumba (8°33N, 76°52E) to make measurements of atmospheric scattering at tropospheric and lower stratospheric altitudes. Measurements could be made of the amplitude of the scattered fluxes and the angular distribution up to an altitude of about 24 km on three rocket flights conducted as part of the 16 February 1980 solar eclipse campaign. These measurements have been used to study the size distribution as well as the number densities of aerosols in the troposphere and lower stratosphere over Thumba.     

A simultaneous interpretation,by wind speed and direction,of ambient air negative ion density in Athens,Greece

A recently developed data presentation technique, the rectangular wind frequency isopleth diagram, has been applied to examine the effect of wind speed and direction, acting simultaneously, on ambient air negative ion densities. The large negative ion concentration decreases in the majority of directions and wind speed intervals, while that of the small ions increases, as the wind speed increases. The local maxima and minima, occurring in some sectors, are properly discussed.     

Mean bulk densities of samples of dry atmospheric aerosol particles: A summary of measured data

Mean bulk densities of various samples of dry atmospheric aerosol particles sampled at different sites and during different seasons and weather situations range between 1.8 and more than 3 gm cm³.     

近地表大气环境变化对地壳形变观测的影响研究

近地表大气环境变化主要包括近地表气象因素（大气压强、温度、降雨）变化及台风、日食活动等。利用小波分析方法对2003—2013年湖北省数字化地壳形变潮汐分钟值资料进行处理后发现,近地表大气环境因素对形变观测数据具有不同频段上的特征变化影响。大气压强和温度对形变观测的响应频段主要集中在较低频段（64—128分钟）;降雨的影响主要集中在0-全日波（0—32分钟）范围内且存在高频、非潮汐成份。而台风在较高频段上有明显响应,频段分布在1—4秒和2—4分钟之间。黄梅台应变观测对2009年日食事件在128—256分钟低频段上有响应。     

乌梁素海大气重金属沉降入湖通量初步估算

重金属元素以大气颗粒物为载体,最终以沉降的方式进入湖泊水体,会引起湖泊的重金属污染.为调查大气沉降对乌梁素海重金属污染的贡献,于2013年7月1日至30日围绕乌梁素海进行大气沉降样品采集,分别测定Cu、Zn、Pb、Cd、Cr、Hg、As 7种重金属元素的含量,并在此基础上估算7月大气重金属沉降通量及入湖量.结果表明,乌梁素海重金属元素大气沉降通量大小依次为:ZnPbCuCrAsHgCd.结合社会调查情况及数据分析显示,大气微粒携带重金属借助风力迁移,较大的沉降通量出现在主风向的下风向区域,说明风向是影响乌梁素海大气重金属沉降通量的主要因素之一.排干输入与大气沉降方式下的乌梁素海重金属入湖量比较发现,大气沉降是除排干输入外湖泊的另一重要重金属污染源.Zn、Pb、Cu、Cr、As、Hg、Cd等重金属元素月入湖量分别为10.6、1.04、1.02、0.833、0.342、0.00514、0.00281t/月.通过估算底泥重金属增量来评价大气沉降对湖泊重金属的贡献表明,大气Hg、Zn、Pb、Cu、As、Cd、Cr等重金属沉降对湖泊贡献率分别为46.4%、44.7%、14.1%、12.0%、8.48%、4.75%、4.03%.