舰载机自动复飞决策技术研究

为保证舰载机着舰安全,下滑过程中复飞决策系统应能自动、及时进行复飞决策,发出复飞信号,实施复飞操纵。文中针对舰载机自动复飞决策技术进行了研究。主要研究了复飞决策判别准则和复飞决策技术的策略,并在Mallab／Simulink环境下建立了仿真模型,进行了仿真验证。仿真结果表明：复飞决策系统能够替代LSO,具有及时发出复飞告警、抑制着舰事故发生的能力。     

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.     

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.     

无人机(固定翼)空中飞行规律研究

对揭示和描述无人驾驶飞行器空中飞行规律的运动方程的推导过程,和运动方程中各个参数物理概念进行了详实的分析,并将无人飞行器的运动方程与有人机运动方程进行了对比研究,结果表明:无人机、导弹和有人机空中飞行遵循同一个飞行规律。     

通过GPS测量数据研究电离层电子总含量的逐日变化

提出了一种直接通过双频GPS伪距测量数据导出接收站附近垂直TEC的方法,这种方法不需要事先知道卫星和接收机电路时延的精确值,前者可在换算过程中自洽地加以修正,而接收机时钟误差则利用IRI模式的夜晚平均值作为参考来订正,这一订正存在一定的绝对误差,但不会影响逐日相对变化,却使数据处理过程大为简化.得到的垂直TEC为天顶周围60锥角内的平均值,能够相当好地反映电离层电子总含量的周日变化.一个计算实例显示了连续三天北京地区TEC的日变化情况,证实了这一方法的实用性.文中还提出一个新概念或问题,即GPS卫星仰角很小时,通常认为多径效应造成大的误差,本文的一些实例似乎表明,这种多径效应的概念应当包括电离层不规则结构的贡献.     

An investigation of the solar cycle impact on the lower thermosphere O(S) nightglow emission as observed by WINDII/UARS

The yearly variation of the integrated emission rate of the O(¹S) nightglow in the lower thermosphere is studied and the solar cycle impact is examined from the observations of the Wind Imaging Interferometer (WINDII) operated on the Upper Atmosphere Research Satellite (UARS). More than 300,000 volume emission rate profiles of the O(¹S) nightglow observed by WINDII for 40°S–40°N latitudes during November 1991–August 1997 over half of a solar cycle are utilized. These profiles are vertically integrated for the altitude range of 80–100 km and the equivalent column integrated emission rates are then zonally averaged for bins with 10° latitude and 3 month intervals. It is found that for each latitude the O(¹S) nightglow emission rate appears to increase with increasing solar F10.7 cm flux, following a linear relationship. This characterizes the solar cycle impact on the O(¹S) nightglow, while the solar influence is modulated by a seasonal variation. Based on these variations, an empirical formula is derived for predicting the three-month averages of the O(¹S) nightglow integrated emission rate. The standard error of the estimated values from the formula is smaller than 30 Rayleigh.     

地磁场与电离层异常现象及其与地震的关系

利用中国地磁台网与电离层台站资料,总结了大地震前出现的地磁低点位移、地磁日变异常及电离层f0F2(F2层临界频率)异常现象.对比研究了1997年11月8日玛尼7.5级与2001年11月14日昆仑山口西8.1级地震前磁场与电离层异常分布及特征.结果显示,两次巨大地震前磁场与电离层短临异常时空分布特征有较好的一致性,震中周围出现日变异常、拉萨台出现电离层f0F2明显异常;震前约1个月出现地磁低点位移,其突变分界线通过震中地区.      

样本量对滚动轴承振动性能变异过程评估的影响

以轴承全寿命周期内的振动时间序列为研究对象,构建最大熵泊松评估模型以研究滚动轴承振动性能的演变历程。将振动时间序列分为不同的段数,基于最大熵原理和泊松过程,计算各个振动时间序列相对本征时间序列的变异概率、性能保持可靠度及其变异速度和变异加速度等指标;分析各个性能变异指标与样本量的关系,从而选取合适的样本量;用动态平均不确定度分析性能保持可靠性评估结果的不确定性。结果表明:针对案例1和案例2,将样本量分别选取为800~1000和500~900,既可以使本征序列数据样本蕴含足够的振动信息;又可以对轴承振动性能的具体变异过程进行有效地评估。      

最差性能最优的稳健宽带Capon波束形成算法

针对常规Capon波束形成易受期望信号导向矢量失配的影响,提出了一种基于广义特征值分解的稳健宽带Capon波束形成算法。算法利用空间响应偏差约束实现宽带频率不变波束形成,同时增加期望信号导向矢量的不确定集约束,改善了算法对导向矢量偏差的稳健性,推导出自适应权矢量的两类近似闭式解。仿真结果表明,与现有的稳健宽带波束形成算法相比,算法在改善波束频响一致性的同时,提高了阵列输出信干噪比,对期望信号导向矢量的误差具有很好的稳健性。     

基于陆态网的区域电离层TEC空间变化特性分析

为研究中国陆态网区域电离层TEC在空间小尺度、高分辨率情况下的变化特性及适用精度范围,利用陆态网260个GNSS连续运行观测站数据,解算并生成2016-2017年731天陆态网区域电离层RIM格网,并进行精度验证.在同一RIM格网中,分别在经度和纬度方向上对间隔不同经纬度的TEC格网点作差分析.结果表明:陆态网区域内经度方向上TEC最大变化率和平均变化率分别为0.30TECU·（°）-1和0.11TECU·（°）-1;经度间隔1°时,TEC差值小于2TECU,且随着经度间隔的增大,其TEC差值也随之增大,并表现出一定的半年和周年变化规律;纬度方向上TEC最大变化率和平均变化率分别为1.7TECU·（°）-1和0.46TECU·（°）-1;陆态网区域内电离层TEC随纬度减小而增大,纬度间隔1°时,99.4%的TEC差值小于4TECU,且随着纬度间隔的增大,其TEC差值也随之增大,并表现出一定的半年和周年变化规律;间隔相同情况下,纬度方向上TEC的变化比经度方向上大.