Wave-like perturbations in the ionospheric F2-layer observed after the Ms8.1 Samoa earthquake of September 29, 2009

A study of the critical frequency foF2 variations after the large earthquake (M_s = 8.1) which occurred on 29 September, 2009 in the region of Samoa Islands in the Pacific Ocean is carried out using data of the ionospheric station of Kwajalein. The epicenter of the earthquake was located at about 184 km southwest from Apia (the capital of West Samoa). It was found that wave-like perturbations of foF2 were observed for ∼3 h above the station (located approximately 3560 km northwest from the epicenter). The amplitude of the disturbance was as large as ∼20% of the average magnetic quiet day foF2 values. A comparison of the observed perturbations of foF2 with the ones detected at Stanford ionospheric station after the Alaska earthquake of 28 March 1964 (M_s = 8.4) showed a close similarity of the wave-like perturbations of foF2 in both cases.     

基于非线性阻尼的航空发动机高压转子拉杆结构装配检测方法

 为了提高航空发动机高压转子拉杆结构的装配质量,提出了基于非线性阻尼的装配检测方法。该方法运用组合阻尼模型描述拉杆结构的非线性接触特性,并通过能量方程推导出基于Hilbert-Huang变换(HHT)方法的非线性阻尼的识别公式。在拉杆结构正常装配、单个螺栓松动和2个不相邻螺栓松动的3种情况下,采用非线性阻尼识别法进行实验,将3种情况得到的实验结果进行对比,发现基于组合阻尼模型得到的非线性阻尼与装配情况具有强烈的相关性,从而验证了基于非线性阻尼的装配检测方法的有效性。     

2.4m跨声速风洞Re数模拟能力及其应用

Re数对飞行器气动特性的影响十分复杂,基于风洞试验的Re数效应预测很大程度上依赖于风洞的变Re数试验能力.综述了2.4m跨声速风洞的Re数模拟能力,并给出了某型无人机和某型战斗机在2.4m风洞的变Re数试验结果以及战斗机大迎角气动特性的Re数效应试验结果,表明了2.4m风洞的Re数模拟能力能够较好地预测Re数对飞行器气动特性的影响趋势,大迎角试验时,基于机头端部直径的试验Re数能达到超临界范围.     

突发威胁下的航迹规划问题研究

提出采用一种结合三角网格退化、变域动态规划以及航迹优化的方法来解决突发威胁下的航迹规划问题。针对无人飞行器航迹规划中应对突发威胁存在时间延迟过长问题,采用一种速度较快的退化网格方法,有效提高了重规划的速率。在动态规划中,采用一种有向变域动态规划方法,进一步缩短了路径生成的时间。仿真结果显示,该方法能有效减少时间延迟过长问题,并满足地形回避和威胁回避的要求。     

Modeling and experimental study of the 27-day variation of galactic cosmic-ray intensity for a solar wind velocity depending on heliolongitude

We develop a three-dimensional (3-D) model of the 27-day variation of galactic cosmic-ray (GCR) intensity with a spatial variation of the solar wind velocity. A consistent, divergence-free interplanetary magnetic field is derived by solving the corresponding Maxwell equations with a variable solar wind speed, which reproduces in situ observed experimental data for the time interval to be analyzed (24 August 2007–28 February 2008). We perform model calculations for the GCR intensity using the variable solar wind and the corresponding magnetic field. Results are compatible with experimental data; the correlation coefficient between our model predictions and observed 27-day GCR variation is 0.80 ± 0.05.     

Dynamics of the convection in the inner magnetosphere by observations of the diffuse aurora,SAR arc and ionospheric drift

The first results of the comparison of subauroral luminosity dynamics in 557,7 and 630,0 nm emission with simultaneous measurements of the ionospheric drift in the F2 region with a digisonde DPS-4 at the Yakutsk meridian (CGMC: 55–60N, 200°E) at Kp = 2–6 are presented. It is shown from the analysis of individual events that during the magnetospheric convection intensification after the turn of the IMF B_z – component to the south the equatorward extension of diffuse aurora takes place. At the same time the westward ionospheric drift velocity increases both in the diffuse aurora region and much equatorward of it due to the occurrence of the northward polarization electric field. We suppose that the generation of polarization field can be associated with the development of the region 2 FAC during the intensification of magnetospheric convection. The comparison of ground-based observations with measurements of the plasma drift aboard the DMSP-F15 satellite has been carried out.     

Evidence of change after 2001 in the seasonal behaviour of the mesopause region from airglow data at El Leoncito

Airglow intensities and rotational temperatures of the OH(6-2) and O₂b(0-1) bands acquired at El Leoncito (32°S, 69°W) provide good annual coverage in 1998–2002, 2006, and 2007, with between 192 and 311 nights of observation per year. These data can therefore be used to derive the seasonal variations during each of these seven years, in airglow brightness and temperatures at altitudes of 87 and 95 km. From 1998 to 2001, seasonal variations are similar enough so that they can be well represented by a mean climatology, for each parameter. On the other hand, these climatologies do not agree with what is usually observed at other sites, maybe due to the particular orographic conditions at El Leoncito. With respect to the last three fully documented years (2002, 2006, and 2007), the similarity from year to year deteriorates, and there are greater differences in the seasonal behaviour, more or less in all the parameters. The differences include, e.g., maxima occurring earlier or later than “normal”, by one or two months. All this may suggest the build-up of a new regime of intraseasonal variability, with a possible relationship to corresponding changes in wave activity.     

1989年3月太阳活动引起的电离层骚扰

本文利用我国,苏联,日本和澳大利亚等国16个电离层观测站的资料,分析了1989年3月太阳耀斑引起的大电离层骚扰特征。      

从射电天文观测中提取电离层信息的一种统计方法

本文在分析了法拉第旋转效应、多源观测效应和程差补偿误差等对可见度函数的相位的影响的基础上,确认了:当电离层不规则性尺度较基线长为大时,仅有电离层引起的可见度函数的相位与基线长成正比且具有随时间快变化的特点这一物理事实;从而提出了从米波综合孔径射电望远镜的观测数据中提取电离层信息的统计方法,并分析了该法的特点,给出了统计实例.      

Measurement Error and Correction or the Ionospheric Effect

电磁波经过电离层传播时会受到电离层折射的影响而产生延迟,星载接收机探测到的时间是信号延迟之后的到达时间．某次实验数据显示,一些波段的瞬态电测辐射信号的群时延之差可达10^5ns数量级,这在对信号源进行时差定位时是不能直接运用的．为有效消除电离层延迟的影响,将双频修正法应用于某项工程中,利用接收到的实验数据求解出电离层的TEC（电离层总电子含量）,并在此基础上对信号到达星载接收机的时间进行修正．最后,对修正结果进行了验证,给出了误差来源．