弹-架间隙的非线性模拟与特性分析

以大长径比低速旋转火箭为例,探讨弹-架间隙非线性特性对不同发射装置系统的动力响应的影响,当飞行器以S个定心部沿发射装置滑移时,根据弹、架横向相对位移确定其定心部处接触刚度和支承特性,模拟弹-架间隙效应。分别就刚性和柔性两种发射装置,分析了间隙量、支承刚度和转速等因素对飞行器发射中的姿态和系统动力特性的影响,算例与实际情况的相吻合证明了该方法的有效性。     

上市公司资产重组中的政府行为规范

文章通过分析上市公司重组中的行政性重组，指出政府在资产重组中的重要作用，并提出了在加入WTO后规范上市公司资产重组中政府行为的对策。     

地方政府经济行为失范的制度分析

在改革开放的过程中，地方政府对于体制改革和经济增长做出了巨大贡献，但另一方面，也存在较严重的失范现象。地方政府经济行为失范有着深刻的制度背景。理论和实践表明，要规范地方政府经济行为，就必须实现地方政府的制度创新。     

中国沪深股市中羊群行为检验

分散度检验法和横截面收益绝对差检验法是检验证券市场中羊群行为的两种方法。运用这两种方法对中国证券市场进行实证分析，结果表明：在中国的证券市场中确实存在着明显的羊群行为。     

纵列式旋翼直升机在起落架上的振动特性试验方法研究

本文基于模态分析理论和试验技术,提出了一套测定纵列式旋翼直升机在起落架上的刚体模态特性试验方法。仿真试验和工程实例验证结果表明该方法用于纵列式直升机设计的可行性。     

DYNAMIC BEHAVIOR OF A CRACKED FLEXIBLE ROTOR SUPPORTED ON JOURNAL BEARINGS

SupportedbytheNationalNaturalScienceFoundationandtheShaanxiNaturalScienceFoundationofChinaNomencIaturescd-externaldampingCP-machinedclearanceofbearingD.-externaldampingratio(=c,/(2m,eq))e.-theunbalanceeccentricityfx,f,-fluidfilmforcesk,-complexstiffnessofcrackedshaftk.-stiffnessofuncrackedshaftke,k,-stiffnessofcrackshaftin$,Vdirec-tlonsAse,As,-thelargeststiffnesschangemb,md-masslumpedatbearingandrotormid-spanS,-fiXedSommerfeldnumber(=S/n,SistheSommerfeldnumber)U-unbalanceparameter(=e./…     

Global solar magnetic field evolution inferred from geomagnetic variations

I have analyzed geomagnetic disturbance index C9, mean solar magnetic field observed at Stanford Solar Observatory for the interval January 13, 1976 – December 30, 1993. It has been established a good correspondence between high-intensity geomagnetic recurrent and solar magnetic field patterns during whole period analyzed. A surprising thing is that the behavior of the solar mean field and interplanetary medium in the latest two solar cycles is very similar. Geomagnetic activity variations actually could serve as an ecliptic monitor of solar magnetic field structure and its evolution.     

3He-Rich Solar Energetic Particle Events

³He-rich solar energetic particle (SEP) events show huge enrichments of ³He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these events: the particle energy spectra are found to be either power-law or curved in shape, with the ³He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near ∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the new insights found in the last few years.     

中国及邻近地区地磁场垂直梯度的计算与研究

根据地磁场的球谐模型,推导出地磁场各个分量垂直梯度的球谐表达式.计算出中国及邻近地区高度为0km,50km和100km处的地磁场及其垂直梯度的网点值,编绘出地磁总强度、垂直强度、水平强度和磁偏角的垂直梯度等值线图.研究了地磁场垂直梯度在地面上以及随高度的变化规律.     

Prediction tests by using “ISF” method for the geomagnetic disturbances

A so-called “ISF” prediction method for geomagnetic disturbances caused by solar wind storms blowing to the Earth is suggested. The method is based on a combined approach of solar activity, interplanetary scintillation (I) and geomagnetic disturbance observations during the period 1966–1982 together with the dynamics of solar wind storm propagation (S) and fuzzy mathematics (F). It has been used for prediction tests for 37 geomagnetic disturbance events during the descending solar activity phase 1984–1985, and was presented in 33rd COSPAR conference. Here, it has been improved by consideration of the three dimensional propagation characteristics of each event, the search for the best radio source and the influence of the southward components of interplanetary magnetic fields on the geomagnetic disturbances. It is used for prediction tests for 24 larger geomagnetic disturbance events that produced space anomalies during the period 1980–1999. The main results are: (1) for the onset time of the geomagnetic disturbance, the relative error between the observation, T_obs, and the prediction, T_pred, ΔT_pred/T_obs  10% for 45.8% of all events, 30% for 78.3% and >30% for only 21.7%; (2) for the magnetic disturbance magnitude, the relative error between the observation, ∑K_p,obs, and the prediction, ∑K_p,pred, Δ∑K_p,pred/∑K_p,obs  10% for 41.6% of all events, 30% for 79% and 45% for 100%. This shows that the prediction method described here has encouraging prospects for improving predictions of large geomagnetic disturbances in space weather events.