Seasonally steady planetary disturbances in the troposphere and stratosphere as seen in 30 years of NCEP reanalysis data

Zonal velocity and temperature daily global reanalysis data of 30 years are used to search seasonally steady planetary disturbances in the middle troposphere (400 hPa) and middle stratosphere (10 hPa). Significant wavenumber 1, 2 and 3 modes are found. Constant phase lines of zonal velocity 1 modes exhibit significant inclination angles with respect to the meridians. The winter hemisphere generally shows a more significant presence of structures. The Northern Hemisphere (NH) exhibits all over the year a larger amount of structures and more intense amplitudes than the Southern Hemisphere (SH). Middle latitudes exhibit the most significant cases and low latitudes the least significant ones. Longitudinally oriented land–sea transitions at ±$\pm$65° and −35° latitudes appear to play a significant role for the presence of steady planetary modes. The stratosphere exhibits a much simpler picture than the troposphere. Large scale structures with respectively NE–SW (NH) and NW–SE (SH) tilts in the observed temperature and zonal velocity constant phase lines recall the quasi-stationary Rossby wave trains that favor the poleward transport of angular momentum.     

End-to-End Modeling of the Solar Terrestrial System

Traditionally modeling for space science has concentrated on developing simulations for individual components of the solar terrestrial system. In reality these regions are coupled together. This coupling can be as simple as the driving of the magnetosphere – ionosphere – thermosphere system by the solar wind or as a complicated as the feedback of the ionospheric conductivity and currents on the magnetosphere. As part of the CISM project we are beginning a concentrated effort to compressively model the entire system. This approach includes chains of models. In the first chain physics based numerical models are utilized while in the second chain empirical models are coupled together. The first half of this paper discusses the numerical modeling approach by highlighting the coupling of pairs of regions within the system. In the second section we present results from empirical models which are combined to make long term forecasts of conditions in the geospace environment. It is expected that a validated and reliable forecast model for space weather can be obtained by combining the strongest elements of each chain.     

一个二次可积系统在二次保守扰动下的分支

研究了一个具有同宿轨的二次可积系统在二次保守扰动下的分支现象.此时一阶Melnikov函数恒等于零,必须考虑二阶Melnikov函数,而在一阶Melnikov函数中不起作用的扰动参数在二阶Melnikov函数中却起着非常重要的作用,因此扰动部分极为复杂.在此借助于二阶Melnikov函数的计算公式及理论分析,建立了极限环分支定理,得到了在一阶Melnikov函数恒等于零,而二阶Melnikov函数不恒等于零时,可能分支出的极限环个数最大为2的结论.     

VARIABLE STRUCTURE CONTROL OF AIRCRAFTFOR ATMOSPHERIC DISTURBANCE

ＶＡＲＩＡＢＬＥＳＴＲＵＣＴＵＲＥＣＯＮＴＲＯＬＯＦＡＩＲＣＲＡＦＴＦＯＲＡＴＭＯＳＰＨＥＲＩＣＤＩＳＴＵＲＢＡＮＣＥＺｈｕＸｉａｏｐｉｎｇ；ＺｈｏｕＺｈｏｕ（ＮａｎｊｉｎｇＵｎｉｖｅｒｓｉｔｙｏｆＡｅｒｏｎａｕｔｉｃｓａｎｄＡｓｔｒｏｎａｕｔｉｃｓ...     

高超声速钝头体边界层转捩试验

为研究高超声钝头体边界层转捩以及头部钝度对转捩的影响,在FD-14和FD-14A两座激波风洞中开展了热流、压力扰动和高速纹影显示等综合测量。试验结果表明,转捩雷诺数关于钝度雷诺数的变化显示出转捩反转的趋势。压力扰动的功率谱密度（PSD）分析结果以流向离散分布云图形式显示,边界层高速纹影图像显示了第二模态波的发展、湍流的生成和熵层对边界层结构的显著影响。大头部钝度带来的强熵梯度熵层流动对边界层压力扰动频谱特性和流动结构影响显著,在转捩反转机理中起到重要作用。此外,马赫数对转捩的影响不容忽视。     

Investigation into impact of tropical cyclones on the ionosphere using GPS sounding and NCEP/NCAR Reanalysis data

Ionospheric response to tropical cyclones (TCs) was estimated experimentally on the example of three powerful cyclones – KATRINA (23–31 August 2005), RITA (18–26 September 2005), and WILMA (15–25 October 2005). These TCs were active near the USA Atlantic coast. Investigation was based on Total Electron Content (TEC) data from the international network of two-frequency ground-based GPS receivers and the NCEP/NCAR Reanalysis data. We studied the spatial–temporal dynamics of wave TEC disturbances over two periods of ranges (02–20 min and 20–60 min). To select the ionospheric disturbances which were most likely to be associated with the cyclones, maps of TEC disturbances were compared with those of meteorological parameters.     

集主承力结构与大容量储箱支架于一体的卫星主承力筒结构研究

针对现代卫星结构的大型化、燃料储箱的大型化,提出了一种集主承力结构与大容量储箱支架一体化的卫星主承力筒结构形式,旨在降低卫星质心、提高基频;在满足储箱容积的前提下,又能满足主结构有效载荷往运载的力的传递作用.有限元数值计算表明,该结构形式能够满足卫星相关结构性能的要求,可以作为今后卫星结构设计的参考构型.     

电离层色散对DS/FH-BPSK信号解调性能影响

相位连续的DS/FH(Direct Sequence/Frequency Hopping,直接序列/跳频)扩频信号的扩频带宽比直扩信号更宽,在电离层的非线性相位以及跳频频点变化这两者的共同作用下,该信号的BPSK(Binary Phase Shift Keying,二相相移键控)解调性能明显恶化。依据随机变量概率分布的数学规律,推导得到了在背景电离层色散条件和跳频频点均匀分布前提下,某种DS/FH卫星测控信号的引导信号和长周期信号BPSK误码率的变化规律,并在特定信号参数条件下进行了误码率仿真。     

基于T96模型的极尖区位形变化特性研究

基于T96模型,定义了极尖区的位形以及相关的描述参量(例如赤道向边界磁纬的最小值,纬向宽度,子午向和晨昏向的张角,倾斜度,扁平度,中心磁地方时等),讨论了太阳风动压(P_d)、行星际磁场(IMF)及磁暴强度对极尖区位形的影响.太阳风动压和磁暴强度越大,则极尖区的赤道向边界磁纬越小,纬向宽度越大,子午向和晨昏向的张角越大,倾斜度越大,扁平度越小;南向IMF B_z越强,则极尖区的赤道向边界磁纬越小,纬向宽度越小,子午向的张角越小,晨昏向的张角越大,倾斜度越大,扁平度越大;北向IMF B_z与南向IMF B_z的情况刚好相反;极尖区的中心磁地方时受IMF B_y控制,IMF B_y为正时,极尖区向昏侧移动,而IMF B_y为负时,极尖区则向晨侧移动,并且极尖区的中心磁地方时与IMF B_y之间有着良好的线性关系.将所得结果与前人的观测结果进行了简单比较,发现利用T96模型确定的极尖区位形与观测基本一致.     

Cosmic ray anisotropy based on Yakutsk station in real time

The method has been developed to calculate galactic cosmic ray anisotropy parameters by using on-line data of the neutron monitor 24-NM-64 and muon telescope at the Yakutsk station. The preliminary analysis shows that characteristic changes in the anisotropy parameters caused by the first spherical harmonics of cosmic ray angular distribution are observed 1–2 days before the onset of the most part of large-scale geophysical disturbances on the Earth. There is reason to believe that the attraction of data of geophysical observations of other kinds will allow to develop the forecast methods for the arrival of large-scale interplanetary disturbances at the Earth.