飞机选型的模糊评判

本文把模糊数学的模糊变换原理用于购买新机型的评判。给出了各评判指标的定义和隶属度:并按 Saatz 的二元对比标度确定各指标的重要度;以及模糊变换的计算方法和应用举例。     

钣金制件表面的相贯线求作方法

本文提出钣金制件表面相贯线求作的新方法。     

纵向短周期模态试飞方法和选择

对几种纵向短周期模态试飞方法及其适用性进行了初步分析。结合实际飞行经验,提出了初步判断飞机短周期特性及选择试飞方法。     

Astrophysics in 2006

The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe) and others of which there are always many, like meteors and molecules, black holes and binaries.     

The double-pulsar binary J0737–3039

A recent multibeam pulsar survey of the outer Galactic plane at Parkes has discovered the first-known double-pulsar binary, a very compact double neutron star system in which both stars are observable as radio pulsars. In this review, we briefly describe the discovery and the studies which have been enabled by the unique properties of the system. These range from the most precise confirmation yet of the theory of general relativity, with the possibility of even more new tests and the measurement of second-order post-Newtonian effects, to studies of the magnetospheres and emission properties of the two pulsars. The discovery also results in a significant increase in the expected rate of occurrence of the mergers of double neutron star systems, and hence the rate of detection of such events by the new ground-based gravitational wave detectors.     

飞机瞬时敏捷性研究

介绍了评价飞机敏捷性的衡量标准,提出瞬时敏捷性的一种估算方法,建立了这种估算方法的数学模型．最后通过估算方法对两种飞机进行了敏捷性计算和分析,得出满意的结果。     

农林飞机结构抗坠毁设计技术

农林飞机通常在3-5m的超低空进行作业飞行,在离地面3m以上的空中往往会有树木、电线杆、电线、堤坝、土堆、山丘、建筑物等障碍物,稍有不慎,就有与之撞击的可能。这样的工作条件除要求飞机具有良好的超低空飞行性能以外,还要求飞机具有一定的耐坠撞能力。本文针对农林飞机执行任务过程中可能发生的碰撞、坠毁等特点,研究了农林飞机抗坠毁设计技术、计算分析仿真技术。     

数字化机载环控地面检测系统的研究

通过采用两片PIC18F448及其外围器件实现了机载环控地面检测系统的数字化设计。通过I^2C总线实现两片单片机之间的数据传输与协调，并利用其CAN接口模块实现多套检测系统的网络化和远程控制操作。     

The Local Bubble and Interstellar Material Near the Sun

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff, has a bulk velocity of ∼19 km s⁻¹ in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet flow direction is included.