某型战机滑跃起飞性能初步分析

根据飞行动力学理论,建立了舰载机滑跃起飞数学模型。以某型战机为例进行了数值仿真,定量分析了起飞质量、起飞迎角、甲板风、滑跑距离等因素对滑跃起飞性能的影响。结果表明:应优选起飞迎角;不同起飞质量情况下,应选择合适的滑跑距离(起飞点),并保证适当的甲板风;起落架强度应加强。     

A Possible Transfer Mechanism for the 11-Year Solar Cycle to the Lower Stratosphere

Observational evidence of the 11-year solar cycle (SC) modulation of stratosphere temperatures and winds from the ERA-40 dataset is reviewed, with emphasis on the Northern winter hemisphere. A frequency modulation of sudden warming events is noted, with warmings occurring earlier in solar minimum periods than in solar maximum periods. The observed interaction between the influence of the SC and the quasi biennial oscillation (QBO) on the frequency of sudden warmings is noted as a possible clue for understanding their mechanism of influence. A possible transfer route for the 11-year solar cycle from the equatorial stratopause region to the lowest part of the stratosphere is proposed, via an influence on sudden warming events and the associated induced meridional circulation. SC and QBO composites of zonal wind anomalies show anomalous wind distributions in the subtropical upper stratosphere in early winter. Mechanistic model experiments are reviewed that demonstrate a sensitivity of sudden warmings to small wind anomalies in this region. Various diagnostics from these experiments are shown, including EP fluxes and their divergence and also the synoptic evolution of the polar vortex, in order to understand the mechanism of the influence. Some recent GCM experiments to investigate the SC/QBO interaction are also described. They simulate reasonably well the observed SC/QBO interaction of sudden warming events and appear to support the hypothesis that tropical/subtropical upper stratospheric wind anomalies are an important influence on the timing of sudden warmings.     

Variations of the magnetic fields in large solar flares

We present preliminary results from high resolution observations obtained with the Michelson Doppler Imager (MDI) instrument on the SOHO of two large solar flares of 14 July 2000 and 24 November 2000. We show that rapid variations of the line-of-sight magnetic field occured on a time scale of a few minutes during the flare explosions. The reversibility/irreversibility of the magnetic field of both active regions is a very good tool for understanding how the magnetic energy is released in these flares. The observed sharp increase of the magnetic energy density at the time of maximum of the solar flare could involve an unknown component which deposited supplementary energy into the system. This revised version was published online in August 2006 with corrections to the Cover Date.     

Mиг－23飞机尾旋试飞体会

Ｍиг－２３飞机是一种变后掠翼战斗机，它的尾旋动态及改出尾旋的方法很复杂。根据在该机上进行的四次尾旋飞行试验，叙述其尾旋进入的方法、尾旋中的动态和改出尾旋的方法。并举出三个典型的尾旋模态实例，详细记述整个尾旋过程和进行分析，说明Ｍиг－２３飞机尾旋动态的复杂性及其表现出的特点。最后，提出了几点在判断和改出Ｍиг－２３飞机的尾旋时应注意的事项。     

飞机概念设计中的生存力效益/代价综合评估方法

 首先介绍了军用飞机在常规武器威胁下的生存力评估指标及几种提高生存力措施；其次研究了将全因素试验法应用于评价生存力提高措施对生存力评估指标的增益影响的可行性；最后基于飞机的安全性、维修性、可靠性、保障性、性能及费用等约束条件，建立了一种能应用全因素试验法在飞机概念设计中进行飞机生存力效益／代价综合评估的方法。算例初步说明了方法的有效性。     

教练机发动机设计载荷谱推导方法

系统地研究了教练机航空发动机设计载荷谱的推导方法，主要包括：（1）基准机的选取与现役发动机载荷谱的空测、统计；（2）新机发动机飞行剖面的预测；（3）新机发动机设计任务循环的编制等三大步骤。提出的方法具有一定的通用性，可以推广到其它类型的发动机设计载荷谱研究。     

What do Cosmogenic Isotopes Tell us About Past Solar Forcing of Climate?

In paleoclimate studies, cosmogenic isotopes are frequently used as proxy indicators of past variations in solar irradiance on centennial and millennial timescales. These isotopes are spallation products of galactic cosmic rays (GCRs) impacting Earth's atmosphere, which are deposited and stored in terrestrial reservoirs such as ice sheets, ocean sediments and tree trunks. On timescales shorter than the variations in the geomagnetic field, they are modulated by the heliosphere and thus they are, strictly speaking, an index of heliospheric variability rather than one of solar variability. Strong evidence of climate variations associated with the production (as opposed to the deposition) of these isotopes is emerging. This raises a vital question: do cosmic rays have a direct influence on climate or are they a good proxy indicator for another factor that does (such as the total or spectral solar irradiance)? The former possibility raises further questions about the possible growth of air ions generated by cosmic rays into cloud condensation nuclei and/or the modulation of the global thunderstorm electric circuit. The latter possibility requires new understanding about the required relationship between the heliospheric magnetic fields that scatter cosmic rays and the photospheric magnetic fields which modulate solar irradiance.     

High-Frequency Radio Signatures of Solar Eruptive Flares

Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects. This revised version was published online in August 2006 with corrections to the Cover Date.     

飞机外挂物部件气动特性的试验研究

介绍了在气动中心高速所FL-24风洞中进行的飞机外挂物部件气动特性试验研究的简要情况和典型试验结果。试验是在M=0.60～1.50、α=-4°～16°、β=0°～5°条件下,利用两台内式五分量天平,分别测量得到了某飞机干扰流场下该机左右侧机翼翼下某导弹弹翼、尾舵的气动特性。结果表明:试验获得的导弹弹翼、尾舵的气动特性变化规律合理,量值可信。试验研究的成功,提高了风洞试验能力,为飞机外挂物部件气动特性的获得提供了有效的技术途径。     

应用数字图象处理技术研究涡流场

本文描述的实验采用干冰为示踪粒子，对脱体涡系作了流动显示，并对摄取的图片进行了数字图象处理。结果清楚地提示了涡的三层结构。在主涡的诱导下，出现二次涡，而二次涡会影响脱体涡的速度分布。实验还得到了脱体涡流场的灰度分布图，并将得出的涡核直径与ＬＤＶ得到的结果进行了对比。实验结果还证明来流迎角、侧滑角及前缘后掠角会影响涡核的位置和强度。当机翼前缘后掠角增加时，脱体涡向不稳定方向发展。