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.      

逆向卸荷式气体减压阀的静态特性分析

对影响减压阀压力调节精度的非线性因素——摩擦力和流体稳态力进行了研究与讨论,建立了逆向卸荷式气体减压阀的静态特性数学模型,其中计算结果与实验结果相吻合。分析结果表明,摩擦力和流体稳态力对减压阀的静态特性偏差有着不同程度的影响,因此在设计过程中应该考虑摩擦力、流体稳态力对减压阀静态特性的影响。     

"海洋一号"卫星的检漏技术

文章介绍了"海洋一号"卫星检漏所采用的两种方法,特别指出采用加压真空检漏方法更能真实地测得卫星的实际漏率,并可提高工作效率.     

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     

带肋变截面回转通道内沿程有效压力分布特性的实验研究

以某型航空发动机的实际涡轮叶片内部的带肋变截面180°回转通道为研究对象,以实验的方法分别研究了带90°直肋和带60°斜肋的通道内的流体流动的特性。根据研究问题的特点,定义了壁面有效压力及局部有效压力系数,并得到了其沿程分布及两种通道内有效压力系数的经验公式。实验发现,对于带90°直肋和带60°斜肋的矩形回转通道沿程有效压力的分布趋势基本一致,由于流道截面积的不规则变化,导致有效压力有沿程逆增现象。      

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     

阻力伞附加质量与阻力系数修正方法

在阻力伞试验,特别是高速滑车试验过程中,由于阻力伞系统作非匀加速的非定常运动以及前置体尾流场的影响,现有的阻力伞试验数据计算方法已经难以准确计算其阻力系数.本文针对阻力伞试验过程中的这种非定常运动和尾流干扰特性,对阻力伞系统进行了动力学分析,并对阻力伞非定常运动过程中的附加质量和尾流场特性进行了理论研究,提出了阻力伞双...     

高超声速钝锥模型及其尾迹红外辐射实验研究

介绍了利用InSb红外辐射计在弹道靶上测量底部直径为10mm、半锥角和头部半径分别为9°、2.2mm(模型A),8°、0.6mm(模型B)的两种非烧蚀钝锥模型及其尾迹的红外辐射.模型速度大于6km/s,飞行环境压力约4.8kPa,红外辐射测量波段为1~3μm、3~5μm.结果表明:非烧蚀钝锥模型头身部红外辐射远大于尾迹红外辐射,在相同飞行速度和环境压力条件下,模型A产生的红外辐射比模型B产生的红外辐射强.     

管道测压系统频率响应研究

准确测量模型表面的脉动压力对于研究建筑物表面风荷载具有重要的意义.在实验室中通常采用管道系统和传感器对物体表面压力进行测量.然而,模型表面的压力信号通过管道系统后会在幅值和相位两方面发生畸变.在管路系统中加限流器能在很大程度上改善管路系统的频率响应特性.笔者应用Tijdeman的管道频率响应理论进行了不同管子和限流器尺寸参数组合的计算,并且进行了系统的对比实验.结果表明:计算和实验结果符合良好,文中进而讨论了有关参数对管路系统频率响应特性的影响.结果对如何正确测量建筑物表面脉动压力提供了一种有效的方法.