对RLC串联电路中通频带与RLC参数关系的讨论——从一道习题引起的问题

讨论了RLC串联电路中通频带与RLC参数的关系,说明在设计一个RLC串联谐振电路时,在给定谐振频率,电感量和频带宽度时,上下边界频率不能只满足通频带宽度而任意假定,还应满足通频带与RLC这些参数之间关系的表达式.     

波音757客改货主货舱门区域改装

简要介绍了波音757-200型飞机客改货主货舱门改装的主要工作内容,以及工作中各种创新思维在关键技术难点上的应用,保证了整个主门区域改装工作的顺利完成,为今后其他类似大型改装或更高级别修理/改装积累宝贵经验。     

低平流层温度对银河系宇宙线强度变化的响应

选用芬兰中子堆监测站从lop年7月至1989年3月的宇宙线强度月平均曲线数据,和在相对应期间我国境内海拉尔等4个高空气象观测站的30hPa和100hPa等位势高度上常规气温观测月平均资料,经统计分析,取得初步结果：低平流层气温与银河系宇宙线辐射强度之间呈现负相关的特性;与银河系宇宙线辐射强度峰区和谷区相对应会在低平流层中引起幅值为2-3℃的温度变化;不同纬度观测站所得观测数据表明,上述增温幅值随纬度降低而减少。     

Stratospheric polar vortex as a possible reason for temporal variations of solar activity and galactic cosmic ray effects on the lower atmosphere circulation

Possible reasons for the temporal instability of long-term effects of solar activity (SA) and galactic cosmic ray (GCR) variations on the lower atmosphere circulation were studied. It was shown that the detected earlier ∼60-year oscillations of the amplitude and sign of SA/GCR effects on the troposphere pressure at high and middle latitudes (Veretenenko and Ogurtsov, Adv.Space Res., 2012) are closely related to the state of a cyclonic vortex forming in the polar stratosphere. The intensity of the vortex was found to reveal a roughly 60-year periodicity affecting the evolution of the large-scale atmospheric circulation and the character of SA/GCR effects. An intensification of both Arctic anticyclones and mid-latitudinal cyclones associated with an increase of GCR fluxes at minima of the 11-year solar cycles is observed in the epochs of a strong polar vortex. In the epochs of a weak polar vortex SA/GCR effects on the development of baric systems at middle and high latitudes were found to change the sign. The results obtained provide evidence that the mechanism of solar activity and cosmic ray influences on the lower atmosphere circulation involves changes in the evolution of the stratospheric polar vortex.     

武汉中层、低热层大气角谱中频雷达观测

武汉中频雷达是利用中层、低热层中电子密度不均匀体的散射来测量大气的水平风场和电子密度剖面。雷达在计算风场的过程中可得到一些该层大气中电子密度不均匀体的寿命和空间尺度等参量值。结合这些参量和大气风场值可计算得到大气的角谱。其计算方法包括全相关分析技术的谱宽法和空间相关法。前者计算的值被认为是大气角谱的上限值。应用这两种方法,利用2001年2月9日武汉中频雷达的观测数据,对武昌上空中层、低热层大气的角谱进行了计算。结果得到大气角谱随高度增加略微增加,如在68km为6°,90km达最大为11°,其平均值为9.2°。利用2001年2月4—10日86km高度上的数据,得到一个7天平均的日变化曲线,发现大气角谱值在本地夜晚最小。     

An intercomparison of meteor radar measurements at the South Pole using two different processing systems

A new meteor radar system was installed at the Amundsen–Scott station South Pole in 2001 to further the understanding of the dynamics of the Antarctic region. The antenna array consists of four yagis pointed along the 0°, 90°, 180°, and 270° meridians and five folded crossed dipoles arranged in a cross configuration and operating as an interferometer to provide position measurements for the detected radio meteors. The four yagis are time division multiplexed and used for both transmitting and receiving while the five folded crossed dipoles are only used for reception. The current arrangement of data acquisition (DAQ) systems at the South Pole allows the collection of meteors in a configuration similar to the previous meteor radar system that operated at the South Pole in the mid 1990s while also using an interferometer to accurately determine the meteor positions in the sky, which enables the determination of the vertical structure of the observed waves. This has been accomplished through the use of two DAQ and post-processing systems: COBRA (Colorado Obninsk radar) connected to the yagis and MEDAC (meteor echo detection and collection) connected to the folded crossed dipoles. With two separate DAQ systems operating in parallel we have the ability to directly compare the results and understand the inherent variability in the derived scientific results based on different system architectures and processing assumptions. The impact of operating a system without an interferometer on the amplitudes and phases of the observed wave components is considered. We find that the lack of altitude resolution of the COBRA DAQ system leads to an underestimation of the amplitude of the s = 1 component of the semidiurnal tide of ∼20% during the summer months.     

Long-period meteor radar temperature variations over Collm (51°N, 13°E) and Kazan (56°N, 49°E)

We have estimated temperatures from meteor radar measurements using the gradient method and the full width at half maximum method over Kazan (56°N 49°E) and Collm (51°N, 13°E). The time series cover the period 2016–2019. The temperature gradient model is constructed from SABER temperature observations. We demonstrate that annual mean, amplitudes and phases of the annual and semiannual oscillations of the radar temperatures are close to those of the MLS and SABER temperatures. The annual mean temperatures over Kazan and Collm differ non-significantly. The seasonal variability of the radar temperature is mostly due to the annual cycle which tends to grow with latitude. The gradient method produces temperatures which agree with the SABER temperatures better than with the MLS ones. The harmonics of the annual oscillations from periods of 73 days up to periods of about 40 days are the most significant day-to-day temperature oscillations and have zonal wavenumber zero. Their periods and phases are in good correspondence with those of the MLS and SABER ones. We also show some results which demonstrate that at 56°N the FWHM method is not as robust as the gradient method.     

民用飞机外翼与中央翼下壁板对接形式

飞机外翼与中央翼的对接结构承担着传递外翼载荷到中机身和中央翼的重任。本文首先梳理了先进民用客机的下壁板对接形式,然后给出了不同下壁板对接结构的设计要点,最后分析了典型机型下壁板对接结构的传力特性,指出下壁板结构的材料类型会影响对接结构的设计。     

Moving scanning emitter tracking by a single observer using time of interception: Observability analysis and algorithm

The target motion analysis (TMA) for a moving scanning emitter with known fixed scan rate by a single observer using the time of interception (TOI) measurements only is investigated in this paper.By transforming the TOI of multiple scan cycles into the direction difference of arrival (DDOA) model,the observability analysis for the TMA problem is performed.Some necessary conditions for uniquely identifying the scanning emitter trajectory are obtained.This paper also proposes a weighted instrumental variable (WIV) estimator for the scanning emitter TMA,which does not require any initial solution guess and is closed-form and computationally attractive.More importantly,simulations show that the proposed algorithm can provide estimation mean square error close to the Cramer-Rao lower bound (CRLB) at moderate noise levels with significantly lower estimation bias than the conventional pseudo-linear least square (PLS) estimator.     

无尾布局嵌入式舵面的大迎角纵向操纵能力研究

 针对某前掠翼翼身融合无尾布局由鸭面与尾舵组成的纵向基本控制舵面在大迎角状态操纵效率降低的问题,采用数值模拟方法研究一种机身下表面嵌入式新概念纵向操纵舵面实施大迎角纵向操纵补充的可行性。提出了嵌入式舵面的设计思想,研究了嵌入式舵面高度、偏度及其与尾舵组合时的相对位置等参数影响,提出了嵌入式舵面的设计原则、流动机理以及提供低头力矩增量的作用原理。研究结果表明:嵌入式舵面是无尾布局飞机大迎角纵向操纵的高效补充措施,单独使用,最大可提供约平衡10°迎角的低头操纵力矩,并对升阻特性影响很小;与尾舵组合使用,在研究迎角范围内(迎角α≤32°),可提供约6°迎角的低头平衡力矩增量,且对升阻性能产生有利影响。本文工作可为其他翼身融合无尾布局的气动舵面设计提供借鉴。