一种高速低噪声信号处理电路的方案研究

文章针对中国遥感高分辨率传输型相机的发展趋势，提出了一种高速低噪声的遥感CCD相机信号处理电路的设计方案。从信号完整性理论出发，利用Cadence软件进行了仿真与验证，取得了良好的效果。     

基于特征点的地形数据存储模型

低空突防在现代战争中发挥着越来越重要的作用，而机载数字地图是现代自主式低空突防系统的一个关键子系统。突防区域内的三维地形数据是数字地图最重要的信息源，故数字地图子系统的成功构筑有赖于在机载环境下有效地存储三维地形数据。本文提出了一种基于地形特征点的三维地形存储模型，其中给出了地形特征点的提取方法及地形特征点的存储编码方式。研究表明，该存储模型可大大减小地形数据的存储空间，并有利于提高三维地形的显示速度。     

1989年3月太阳活动引起的强烈磁暴群

本文分析了1989年3月上旬一个太阳超级活动区中多次特大耀斑引起的强磁暴群.联系源耀斑的等级、位置等讨论了磁暴形态特征.随着耀斑活动区位置由东向西旋转,磁暴的形态呈现有规律的变化,充分显示了磁暴形态特征有依赖于耀斑位置的中心子午线效应和东西不对称性.     

Cyclotron masers and solar spike bursts

The theory of electron cyclotron maser emission and its application to solar spike bursts are reviewed. By analogy with the Earth's AKR, three sources of free energy are considered: a loss-cone anisotropy, a velocity-space hole, and a trapped distribution. The problem of how the radiation escapes through the second harmonic absorption layer is emphasized. Harmonic emission due to z mode coalescence may operate for some bursts, but the 2–5s delay between hard X-ray bursts and spike bursts suggests that some other mechanisms is required for most spike bursts. A model involving formation of a trapped distribution in low-density regions neighboring the flaring flux tube is considered.     

低密度小喷管流场的DSMC直接模拟

用ＤＳＭＣ方法数值模拟了低密度轴对小喷管的流场流动，获得了相应的结果，并将所得结果与用差分求解Ｎ－Ｓ方程方法获得的结果进行了对比，二者吻合较好。     

低浸渗压力制备短纤维增强铝硅合金复合材料

利用液态浸渗技术制备了氧化铝纤维增强铝基复合材料。结果表明，在低压下使液态合金浸渗纤维预制件制备铝基复合材料是可行的，在浸渗过程中，液态合金的温度对浸渗压力有较大影响。所制备的复合材料组织均匀，基体中的共晶组织可依附在纤维表面形核生长。     

酸酐固化剂对硅橡胶低密度烧蚀材料施工期的影响

通过对延长硅橡胶密度烧蚀材料体系施工期的研究，发现酸酐固化剂可以将环氧改性硅橡胶低密度烧蚀材料的施工期延长到24h以上，从而可能实现真空热压罐大面积灌注密度烧蚀材料的成型工艺。通过对固化材料进行红外分析，发现加入酸酐固化剂后并未改变硅橡胶和环氧树脂各自的反应，没有新的反应特征峰出现，说明环氧和硅橡胶之间无反应，只是物理共混，从材料拉伸断面的扫描电镜观察可以证实硅橡胶和环氧树脂以海－岛结构存在。     

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.     

Modeling of dynamic evolution of coronal loops

Parameters of expanding magnetic loops and arches and of mass flows generated by them in the corona have been computed in a 1D two-fluid approximation. Two possible trigger mechanisms of the coronal transients have been considered: (i) sudden increase of the background magnetic field strength, and (ii) heating and compression plasma inside these magnetic structures. We discuss the formation of shock waves and their dependence on dynamics and geometry of the magnetic structures.