GDJ人卫目视观测数据采集和处理系统的研制

本文介绍了ＧＤＪ跟踪打印经纬仪在人造卫星的观测中如何应用计算机对多圈卫星的目视观测资料进行实时采集、处理等工作过程的原理和方法。     

山东威海太阳物理国际研讨会(2002年8月5～12日,威海)

以国家自然科学基金委员会“九五”重点项目“太阳射电爆发频谱及其物理机制”、国家重点基础研究发展规划项目“太阳剧烈活动与空间灾害天气”子课题“太阳高能粒子的起源与输出”等研究为背     

Ellerman Bombs,Type Ⅱ White—light Flares and Magnetic Reconnection in the Solar Lower Atmosphere

Ellerman bombs and type Ⅱ white-light flares share many common features despite the large energy gap between them.Both are considered to result from local heation in the solar lower atmosphere.This paper presents numerical simulations of magnetic reconnection occurring in such a deep atmosphere,with the aim to account for the common features of the two phenomena.Our numerical results manifest the following two typical characteristics of the assumed reconnection process:(1)magnetic reconnection saturates in-600-900s,which is just the lifetime of the two phenomens;(2)ionization in the upper chromosphere consumes quite a large part of the energy released through reconnection,making the heation effect most significant in the lower chromosphere.The applicationof the reconnection model to the two phenomena is discussed in detail.     

现代天文选址中的视宁度（Ⅱ）

在文献」１「４ 基础上，根据近年文选址实践中提出的问题，先进一步讨论了大气相干直径和时间的的物理和意义，然后强调了自由大气湍流的天文成像效应及选址中进行研究和测量的重要性。最后对差分像运动方法测量视宁度的定标和系统误差等问题作了分析。     

CSAO和VS NIIFITRI等高仪国际合作观测精度的初步分析

初步分析了ＰＨＡ Ｉ在伊尔库茨克近１４个月中观测的８２２组星的精度。ＰＨＡ Ｉ创造了它历史上最多的观测星组数和最高的观测精度。１９９６年在俄罗斯地球自转参数系统中获取１５％的权重，约为该系统平均仪器权重的３倍多。