Which solar EUV indices are best for reconstructing the solar EUV irradiance?

The solar EUV irradiance is of key importance for space weather. Most of the time, however, surrogate quantities such as EUV indices have to be used by lack of continuous and spectrally resolved measurements of the irradiance. The ability of such proxies to reproduce the irradiance from different solar atmospheric layers is usually investigated by comparing patterns of temporal correlations. We consider instead a statistical approach. The TIMED/SEE experiment, which has been continuously operating since February 2002, allows for the first time to compare in a statistical manner the EUV spectral irradiance to five EUV proxies: the sunspot number, the f10.7, Ca K, and Mg II indices, and the He I equivalent width.     

Relation between galactic and solar cosmic radiation at aviation altitude

Cosmic radiation bombards us at high altitude with ionizing particles; the radiation has a galactic component, which is normally dominant, and a component of solar origin. Cosmic ray particles are the primary source of ionization in the atmosphere above 1 km; below 1 km radon is a dominant source of ionization in many areas.     

一种钟控序列发生器的加速机制

提出一种钟控伪随机序列发生器的加速机制,可以使序列发生器在一个时钟周期内得到前进n步的结果,在硬件实现时使得序列发生器的工作频率提高n倍。此加速机制可应用于钟控序列发生器和序列密码发生器的密钥预置。     

自转旋翼气动特性分析及试验研究

从理论分析和试验验证两方面对自转旋翼气动特性进行了研究.采用叶素理论,以数值积分的方法建立自转旋翼气动模型,通过建模计算分析得出自转旋翼气动特性桨盘分布及与参数的关系.从原理性到实用性对试验模型和方案进行了设计.通过风洞试验,既验证了理论计算方法和结果正确可行,又发现了实践中存在的最小风速和最低预转速规律等问题.     

飞船返回舱高超声速气动特性的风洞实验分析

在返回舱再入过程中,高超声速配平升阻比是一个十分重要的参数。文章介绍球冠倒锥外形返回舱模型在φ0．5m高超声速风洞中气动力的测量结果,给出Ma=4．94、5．96、7．96,相应的Re=3×10^6、6×10^6、2×10^6（以最大横截面直径为特征长度）气流条件下,攻角从2°～-27°变化范围内返回舱的气动力特性,讨论重心位置纵移与横偏变化对配平升阻比和纵向稳定性的影响。     

The Physical Foundation of Forecasting Disturbances in the Geospace From Solar Disk Characteristics

The five main types of antisunward propagating energetic fluxes (particles and emission) may be thought of as well established to date, the effects of which lead to a particilar character of disturbance in the near-terrestrial environment (the Earth's magnetosphere, ionosphere and atmosphere). The strongest global restructuring of the magnetosphere and ionosphere is caused by fluxes of relatively dense n of 1-70 cm-3 at the Earth's orbit) Solar Wind (SW) quasi-neutral, low-energy (E ＜ 10 keV) plasma which cause magnetospheric and ionospheric storms lasting 24 hours or longer. For that reason, main attention is given to their study at the initial stage of research. The physical essence of the method of predicting disturbances in the near-terrestrial space environment, the amplitude of which can be expressed in, for example, the Kp index units, involves:(1) identifying all the most geo-effective SW streams of type, (2) determing their sources on the solar disk,and (3) quantifying the correlations between the characteristics of their solar sources with a maximum value of the Kp-index that is caused by the concerned type of SW stream. Semi-phenomenological relations have been obtained, which relate parameters of type SW stream sources to characteristics of geomagnetic storms:storm commencement, the time at which the storm intensity reaches its maximum values, the storm duration,as well as to the storm amplitude expressed in terms of geomagnetic indeces.      

Study of the Enhancement Events of Relativistic Electron at the Geosynchronous Orbit

The high flux of energetic electron on geostationary orbit can induce many kinds of malfunction of the satellite there, within which the bulk-charging is the most significant that several broadcast satellite failures were confirmed to be due to this effect. The electron flux on geostationary orbit varies in a large range even up to three orders accompanied the passage of interplanetary magnetic cloud and the following geomagnetic disturbances. Upon the investigation of electron flux enhancement events, two types of events were partitioned as recurrent events and random ones. Both of the two kinds of events relate to the interplanetary conditions such as solar wind parameters, IMF etc and their evolution characters as well. As for the recurrent events, we found that, (1) all of the events exhibits periodic recurrence about 27 days, (2) significant increase of electron flux relates to interplanetary index and characters of their distribution, (3) the electron flux also has relation to solar activity index. An artificial neural network was constructed to estimate the flux I day ahead. The random electron flux enhancement events are rare and present different distribution figures to the recurrent ones. The figure of the random events and the conditions of their occurrence is also discussed in this paper.      

导弹飞控系统可靠性仿真研究

提出了在几种主要因素影响下进行飞控系统性能和可靠性一体化分析的方法。建立了风、结构误差(包括弹体质量分布不对称、弹体不同轴、翼面安装角误差和舵面机械零位误差)、推力偏心和硬件故障等因素的扰动模型,给出了可靠性仿真的方法、实施步骤、具体算法流程和相关可靠性指标的计算公式。以某型导弹飞控系统作为案例,进行了大量仿真,分析了风等因素对该系统可靠性的影响。通过算例证明,所建立的扰动模型和可靠性分析方法是正确的。     

第2009卡林顿周太阳活动的初步分析

介绍了第 2 0 0 9卡林顿周大黑子群AR484,AR486和AR488产生的太阳活动以及这些太阳活动对地球空间环境造成的影响。依据对太阳活动的统计研究 ,简要分析了三个大黑子群活动的差异。分析结果指出 ,关注某一时期太阳活动的活动经度带以及太阳活动在某一半球的主次是解决太阳活动短期预报非常重要的思路     

卫星太阳电池阵在板展开阶段的撞击特性研究

研究了卫星太阳电池阵在板展开阶段的撞击特性,导童重要性一多体系统的动力学方程,介绍了撞击力的计算方法,计算了太阳电池阵在撞击阶段的撞击力和一些特殊节点的加速度和变化规律,计算结果表明,各点的撞击力在不同的时刻达到峰值,说明柔性板在撞击时发生了扭转,此外还发现靠近撞击处的节点的加速度在撞击瞬间比其它节点大,通过冲击波的传播引起外侧板的边界上节点的加速度不断上下振动,可以解释外侧帆板在撞击后上下、左右