Secular variations of OH nightglow emission and of the OH intensity-weighted temperature induced by gravity–wave forcing in the MLT region

Secular variations of OH airglow (8,3) band and of the intensity-weighted temperature induced by a gravity wave packet at three latitudes in the northern hemisphere in the Mesosphere/Lower Thermosphere region are investigated using a 2-D, time-dependent, fully nonlinear OH chemistry–dynamics model. A net-cycled average survives due to wave transience and dissipation. The integrated OH (8,3) volume emission rates show a 20 percent increase induced by the wave packet. The corresponding intensity-weighted temperature shows an initial increase up to 2 percent then a gradual decrease for the remainder of the simulation time by the same wave packet. These secular variations could be mistaken as long-period or short-period waves in the airglow observations. Therefore, care must be taken when analyzing the data from observations.     

考虑排放影响的飞机多学科优化设计

随着民用航空运输业的发展,飞机对气候环境的影响越来越受到重视。为了满足未来飞机设计中经济性和环保性等指标,有必要在飞机概念设计阶段综合考虑成本和排放的影响。本文使用全球平均温度变化作为衡量飞机排放对气候影响的标准,分析了飞机巡航高度和速度对于排放物的影响。进一步,通过整合气动、重量、成本和排放等学科模型,建立了飞机概念设计阶段的多学科优化框架。基于该优化框架,以机翼平面形状、飞行速度和高度等参数为优化变量,分别以排放最小和成本最低为目标,进行了单目标和多目标优化设计研究。Pareto最优前沿的优化结果显示,单位排放成本的高低会影响成本相对于排放性能的变化趋势。     

太阳微波脉冲事件的时变特性

本文利用瑞士Berne大学1988年1月-1989年12月发布的15个太阳微波脉冲事件的观测资料，分析其时间轮廓的3个主要特征：脉冲度、不对称性和半功率宽度频率响应．这些特性，可以定性地用非热电子的连续注入模，和不均匀的源模型给出较合理的解释．     

全变差正则化方法对一类热传导反问题的应用

热传导终端反问题是典型的不适定问题,应用基于全变差的正则化方法来获得它的稳定数值解,将近似解的求解范围由连续函数空间扩大到了有界变差函数空间,并将固定点迭代法用于求解非线性的Euler方程,并进行了理论分析和数值实验。结果表明:该方法与算法具有高效稳定全局收敛等优点。     

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.     

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。     

Cosmic ray measurements in High Tatra mountains: 1957–2007

Lomnický Štít (LS, situated at High Tatra mountain, 2634 m above sea level, in the direction of 49.40°N, 20.22°E; geomagnetic vertical cut-off rigidity for cosmic rays ∼4 GV) is a relevant place for cosmic ray studies. After a brief review of the LS research history we present a selection of the results based on the measurements performed by the neutron monitor located at that site. In particular, the characteristics of quasi-periodicities and the diurnal variability amplitude and phase obtained from those data are discussed.     

Climatology of global,hemispheric and regional electron content variations during the solar cycles 23 and 24

We present the results of study on the variations of ionospheric total electron content (TEC) by using global, hemispheric, and regional electron contents computed from the global ionospheric maps (GIMs) for the period from 1999 to 2020. For a low and moderate solar activity, the global and regional electron contents vary linearly with solar 10.7 cm radio flux and EUV flux. While a saturation effect in the electron content verses EUV and F10.7 is found during the high solar activity periods at all regions, the maximum effect is observed at low-latitudes followed by high and mid-latitudes region. The extent of saturation effect is more pronounced for F10.7 as compared to EUV. A wavelet transform is applied to global and hemispheric electron contents to examine the relative strength of different variations. The semi-annual variations dominate in the northern hemisphere, whereas annual variations dominate in the southern counterpart. The amplitude of annual variations in southern hemisphere is found to be higher than northern counterpart at all latitudes. This asymmetry in the amplitude of annual variation is maximum at low-latitudes, followed by mid and high-latitudes, respectively. The semi-annual variations are in-phase in both hemisphere and follow the solar cycle. The northern hemisphere depicts relatively large amplitude of semi-annual variations and exhibit the maximum effect at high-latitudes.     

基于火焰面波动机理的热释放模型理论推导及其模态分析

针对一个中心体稳定的燃烧室通过G方程的方法推导建立了火焰面波动与声波速度波动之间的耦合关系,并进而得到了燃烧热释放模型的数学函数.推导过程中考虑了燃烧膨胀效应对火焰面运动的影响,弥补了前人研究中忽略了燃烧膨胀效应的不足.该函数表明在几何结构和燃料成分等参数保持不变的情况下,湍流燃烧速度是影响热声振荡的关键参数,能够同时强烈的影响燃烧热释放模型的振幅和相位,当量比和入口空气温度等参数是通过改变湍流燃烧速度最终影响了热声振荡现象;而只有当燃烧火焰传播速度相对较大时,密度膨胀比才会对热释放幅值产生影响,并且会对热释放的相位产生影响,从而指出了各参数影响热声振荡的具体途径和相对大小.通过将推导的燃烧热释放波动模型与模态分析方法相结合,系统连续地分析了压力振幅增长率、固有频率和声压模态等重要的热声振荡特性参数随着当量比和入口空气温度的变化关系,从而得到了热声振荡稳定区间和非稳定的区间的云图.对理解和控制热声振荡现象具有重要的实际指导意义.