Modeling of ionospheric parameter variations in East Asia during the moderate geomagnetic disturbances

The results of modeling of ionospheric disturbances observed in the East Asian region during moderate storms are presented. The numerical model for ionosphere–plasmasphere coupling developed at the ISTP SB RAS is used to interpret the data of observations at ionospheric stations located in the longitudinal sector of 90–130°E at latitudes from auroral zone to equator. There is obtained a reasonable agreement between measurements and modeling results for winter and equinox. In the summer ionosphere, at the background of high ionization by the solar EUV radiation in the quiet geomagnetic period the meridional thermospheric wind strongly impacts the electron concentration in the middle and auroral ionosphere. The consistent calculations of the thermospheric wind permit to obtain the model results which are closer to summer observations. The actual information about the space-time variations of thermosphere and magnetosphere parameters should be taken into account during storms.     

体表电位标测系统中关键技术——心电信号数据高速采集

心电信号的数据采集是体表标测系统中关键技术之一。文中提出了128通道高性能体表标测系统中心电信号数据采集的VxD算法，在Wind9x系统下利用VxD技术、锁定内存和临界资源互斥访问算法相结合，实现了心电数据高速实时采集。该软件充分利用了硬件的等待时间，具有实时性高，运行速度快占内存少的特点。该软件在VtoolsD开发平台上用VisualC＋＋开发。     

Stellar winds of massive stars in M31

We have obtained the first UV high resolution spectra of hot luminous stars in M31 with the FOS onHubble Space Telescope. The spectra, combined with optical spectroscopic and photometric observations, enable us to study their stellar winds and photospheric parameters. We derive mass-loss rates and velocity laws from the wind line profiles, with the SEI method, as well as information on abundances. The wind lines and photospheric spectra are compared with galactic stars of the same spectral type.The spectra analyzed so far indicate that the stars have mass-loss rates comparable or slightly lower than galactic stars of the same spectral type, but possibly different velocity laws in their winds. The spectra of two stars are discussed here.     

乡镇财政风险的外部因素分析及对策

乡镇财政风险影响着基层政权的正常运转与稳定，是制约地方经济发展，关系社会稳定的重大问题。近几年，随着我国农村税费改革的推进，乡镇财政潜伏的风险和隐患也日益增多。文章仅就造成乡镇财政风险的外部因素进行了分析，并提出了规范政府行为、完善财税管理体制、提高财政资源使用效率等对策建议。     

高超声速边界层转捩机理及应用的若干进展回顾

高超声速边界层转捩对飞行器的热传递、表面摩阻和流动分离等有重要影响,尤其是再入飞行器和吸气式巡航飞行器。然而,人们对边界层转捩机理中的很多问题认识还不清楚,或存在争议。本文从扰动波演化的角度回顾了高超声速边界层感受性、线性稳定性和非线性作用的国内若干研究进展,并以基于谐波共振的人工转捩技术为例示范了这些机理认识在转捩控制上的应用。扰动的产生和发展是认识边界层转捩机理的核心。通过研究扰动波来认识边界层转捩机理,开展应用创新研究对提升飞行器性能具有重要意义。     

圆锥形薄壁壳体的弹性稳定性

基于Donnell型扁壳理论,利用法分析了在均布外压作用下圆锥形薄壁壳体的弹性稳定性问题。根据外压实验观察结果和通过选取适当的位移分量表达式,文中给出了临界外压的近似表达式。数值结果表明,本文理论分析预示值与临界载荷的实验值很吻合。文中还对有关参数对临界载荷的影响进行了讨论。本文所得结果可供工程应用参考。     

公共设施投资的决策模型探讨

公共设施投资的成本与产生的社会福利如何比较，社会效益的提高有多大等等一系列基本问题为政府所关心。这一问题的解决需要通过结合公共经济学的原理与近几年出现的一些新观点做出系统的可行性分析模型加以解决。本文就是基于公共经济学的理论并结合了笔者的一些新的观点所作的常识性的探索。     

一般层合板矩形单元的几何刚度矩阵

本文简述了求解结构稳定性问题的有限元理论基础。用张量的形式指导了一般层合板矩形单元的节点力和节点位移关系方程，详细推导了一般层合板四节点矩形单元的几何刚度矩阵的公式及其显式。     

Ionospheric TEC disturbances over China during the strong geomagnetic storm in September 2017

From September 7 to 8, 2017, a G4-level strong geomagnetic storm occurred, which seriously impacted on the Earth’s ionosphere. In this work, the global ionospheric maps released by Chinese Academy of Sciences are used to investigate the ionospheric responses over China and its adjacent regions during the strong storm. The prominent TEC enhancements, which mainly associated with the neutral wind and eastward prompt penetration electric field, are observed at equatorial ionization anomaly crests during the main phase of the storm on 8 September 2017. Compared with those on 8 September, the TEC enhancements move to lower-latitude regions during the recovery phase on 9 September. A moderate storm occurred well before the start of the strong storm causes similar middle-latitude TEC enhancements on 7 September. However, the weak TEC depletion is observed at middle and low latitude on 9–10 September, which could be associated with the prevailing westward disturbance electric field or storm-time neural composition changes. In addition, the storm-time RMS and STD values of the ionospheric TEC grids over China increase significantly due to the major geomagnetic storm. The maximum of the RMS reaches 12.0 TECU, while the maximum of the STD reaches 8.3 TECU at ~04UT on 8 September.     

Identification of seismic activity sources on the subsatellite track by ionospheric plasma disturbances detected with the Sich-2 onboard probes

Using a cylindrical Langmuir probe and the authors’ proprietary two-channel pressure transducer, ionospheric plasma parameter distributions along the orbit of the Sich-2 satellite (Ukraine, 2011–2012) were measured. This paper is concerned with identifying the space–time location of ionospheric plasma disturbance sources, including the epicenters of actual earthquakes (before or during the satellite flyover) and incipient earthquakes on the subsatellite track, from the measured distributions of the electron density and temperature and the neutral particle temperature along the satellite orbit. To do this, the measured ionospheric plasma parameter distributions are connected to the coordinates on the subsatellite track.It is shown that local disturbances in the electron density and temperature and neutral particle temperature distributions in the satellite orbit in the ionosphere may serve as indicators of seismic activity on the subsatellite track. The epicenters of incipient earthquakes may be set off from other plasma parameter disturbance sources associated with seismic activity using information provided by special monitoring and survey centers that monitor the current seismic situation.