Microwave Type III Burst Group in the 1993 October 2 Flare

Microwave Type III bursts with positive frequency drifting rate were found by Stahli and Benz (1987) for first time. Type III events are especially interesting because they are well-known to be signatures of electron beams in coronal plasma, and they are effective means for diagnosting of source plasma. A microwave burst consisting of some microwave type III burst groups was registered at Beijing Astronomical Observatory with the 2545–2645–2840 MHz synchronous observing system. The distributions of frequency drifting rate, half power duration, and intensity for each impulse in the groups have been statistically analysed. From this analysis, some important parameters for the dynamic process in the flare are deduced and discussed.     

人工增雨技术研究及示范

课题在2002年严格按照与科技部签定的任务合同书顺利进行,并取得了可喜的研究成果: ■完成了夏延Ⅲ新型云物理和人工增雨飞机的改装,飞机装备有云物理综合探测系统和本课题研制的碘化银末端燃烧器,并在河南示范区冬季人工增雨(雪)科学试验中获得了一批符合科学设计的综合探测资料.     

中国古大陆及其边缘早古生代层序地层及海平面变化的基本特征

着重总结了我国古大陆及其边缘早古生代大层序（ｍｅｇａｓｅｑｕｅｎｃｅ，一级层序）和中层序（ｍｅｓｏｓｅｑｕｅｎｃｅ，二级层序），以及一级、二级海平面变化的基本特征，并与国外早古生代海平面变化进行对比．我国３大古陆（华北陆块、扬子陆块、塔里木陆块）及其边缘早古生代大层序可划分为两个（ＭＧ－１，ＭＧ－２）．中层序划分为５个（ＭＳ－１，ＭＳ－２，ＭＳ－３，ＭＳ－４，ＭＳ－５）．ＭＧ－１包括ＭＳ－１，ＭＳ－２和ＭＳ－３，时限为９４～１１２Ｍａ（寒武纪和早奥陶世），底以巨大不整合为界，顶以著名巨大沉没不整合为限，沉积了我国显生宙大部分的碳酸盐岩，赋存着丰富的油气和各种金属及非金属矿产．ＭＧ－２包括ＭＳ－４和ＭＳ－５，时限为５８～６８Ｍａ（中、晚奥陶世和志留纪），底界以巨大沉没不整合为界，为硅质碎屑－碳酸盐岩组合．海平面变化的级别划分对应于层序．中国３大古陆及其边缘早古生代海平面变化的总貌：ＭＧＳＣ－１初期普遍发生快速海进，海平面升高，尔后海平面下降，其间有多期次的小幅度海进和海退变化．ＭＧＳＣ－２则普遍海平面升高，上升幅度大于ＭＧＳＣ－１，尔后逐渐下降．     

基于理想点-可拓云模型的隧道围岩稳定性评价

为了对隧道围岩稳定性进行准确评价并解决研究过程中存在的模糊性和随机性以及评价指标不相容的问题,减少单一的主客观赋权法所带来的误差,将云模型引入可拓理论中,利用可拓理论能够实现矛盾问题向相容问题转化的特点和云模型具有处理事物双重不确定性的优势并结合理想点组合赋权法对隧道围岩进行稳定性评价研究。通过文献调研、数据统计的方式,选取具有代表性的6个指标组成隧道围岩评价指标体系,用理想点法赋予评价指标组合权重,并构建可拓云模型对隧道围岩稳定性进行综合评价。通过将此方法应用于工程实例并与其他方法对比,结果表明:基于理想点-可拓云模型的隧道围岩稳定性评价方法能够减少评价过程中存在的不确定性问题,克服单一赋权方法的不足,具有良好的适用性,可以应用于实际工程中。     

云、雨水酸度和离子浓度与其微物理参数的关系

本文1987年5-6月和1989年5-6月庐山地区的实测资料,分析了云、雨水酸度和离子浓度与其微物理量间的关系。结果表明,云、雨滴大小、含水量、谱宽等微物理量的演变直接影响着其酸度和离子浓度。     

影响生油门限深度的地质因素

本文根据三水盆地下第三系心组有机地化资料的分析,确定其生油门限深度为400米。进一步讨论了影响我国东部第三系含油气盆地成油门限值的几种地质因素。提出这些年青的盆地只要具有高地温梯度、高沉降速度、埋深大、剥蚀少就能在较短时间中形成油气。     

牛顿松弛方法的初值化与试验比较

本文采用一个有限区域数值预报模式，在平衡风和实测风初值的基础上引进和试验了牛顿松弛方法，并同单纯的平衡风初值及实测风初值作了比较，结果发现方法对初始场及总体预报结果均有明显改进。     

第23周太阳活动峰年北京天文台太阳射电观测

An introduction to the instrumonts to be used for solar radio observations in Beijing in Solar Cycle 23 is made in this paper. They are 10cm solar radio telescope which has been used for a long time,and 1.0～2.0GHz,2.6～3.8GHz and 5.2～7.6GHz spectrometers. The former two spectrometers has passed a test,showing high guality,and the 5.2～7.6GHz one will be in operation from 1999. It is believed that highl gualified data should be obtained in the next solar cycle.     

Type III burst pair

We present a special solar radio burst detected on 5 January 1994 using the multi-channel (50) spectrometer (1.0–2.0 GHz) of the Beijing Astronomical Observatory (BAO). Sadly, the whole event could not be recorded since it had a broader bandwidth than the limit range of the instrument. The important part was obtained, however. The event is composed of a normal drift type III burst on the lower frequency side and a reverse drift type III burst appearing almost simultaneously on the high side. We call the burst type III a burst pair. It is a typical characteristic of two type III bursts that they are morphologically symmetric about some frequency from 1.64 GHz to 1.78 GHz on the dynamic spectra records, which indicates that there are two different electron beams from the same acceleration region travelling simultaneously in opposite directions (upward and downward). A magnetic reconnection mode is a nice interpretation of type III burst pair since the plasma beta 0.01 is much less than 1 and the beams have velocity of about 1.07×10⁸ cm s^–1 after leaving the reconnection region if we assume that the ambient magnetic field strength is about 100 G.     

云模式中气溶胶物理过程参数化方案研究概述

介绍了大气气溶胶的浓度、气溶胶的谱形等物理性质对云的微物理过程造成的影响以及目前云模式中常用到的一些气溶胶物理过程的体积水、分档等参数化方案，并评述了这些参数化方案各自的特点。提出了在设计气溶胶物理过程参数化方案时需要注意和有待解决的几个问题，建议在设计气溶胶-云相互作用的模式时，要根据不同的研究目的选择合适的参数化方案。