基于粗集理论的系统评估

讨论了基于粗集理论的系统综合评估和运用粗集理论进行系统评估指标体系的选择。给出了基于粗集理论进行系统综合评估的一般步骤，研究了运用粗集基本理论进行评估指标体系建立的方法，最后的实验结果验证了本文方法的有效性。     

铝蒙皮涂装施工用的水溶性脱漆剂

本文研究的是以苯甲醇替代二氯甲烷为主溶剂的水溶性脱漆剂，它和传统的二氯甲烷型脱漆剂相比，毒性更小、对使用者的安全及身体健康元不利影响，且脱漆速度相当。通过对脱漆剂使用的研究和对比，结果证明，它对环氧类涂料、环氧锌黄底漆等都适用，尤其对于飞机蒙皮漆有良好脱漆效果。该脱漆剂具有原材料易得、对基才腐蚀性小、适用范围广、不燃烧等特点，一般常温下在30分钟内使可将漆膜溶胀。其与制工艺简单，涂覆方便、不易挥发、贮存较稳定，重涂性能好，对基村的后处理无不良影响。     

浅谈黄铜电镀生产中镀层变色问题

分析了黄铜产品的变色原因，提出了黄铜电镀生产中控制镀层变色的方法并应用于生产之中，使黄铜镀层变色问题得到有效控制。     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

Ionospheric Effects of Geomagnetic Storms in Different Longitude Sectors

This paper analyzes the state of the ionosphere during two geomagnetic storms of a different intensity evolving in different sectors of local time in different seasons. There were used the data from a network of ionospheric stations located in the opposite longitudinal sectors of 80°-150° E and 250°-310° E.This analysis has permitted us to conclude that the detected differences in the variations of the disturbances are likely to be determined by the local time difference of the geomagnetic storm development, its intensity and by the different illumination conditions of the ionosphere.      

Research on a complex CME event including Hα, LASCO, radio and MDI observations

We present our research on a fast and decelerating partial halo coronal mass ejection (CME) event detected in multi-wavelengths in the chromosphere and the corona on 14 October, 1999. The event involved a whole complex active area which spanned more than 40° of heliolongitude. It included a strong solar flare (XI/1N) and a complex eruptive filament within an active region of the entire complex. Especially, several radio sources were detected in the decimetric range prior to the CME by the Nançay Radioheliograph (NRH). A linear force-free field extrapolation of the Michelson Doppler Imager (MDI) magnetogram was performed to calculate the magnetic topology of the complex prior to the triggering of the event. The presence of a coronal null point combined with the occurrence of two distant and nearly simultaneous radio sources put strong arguments in favor of the generalized breakout model for the triggering of the eruption. The analysis of the subsequent development of the event suggests that large interconnecting loops were ejected together with the CME.     

基于SSL的数据安全传输系统的设计与实现

安全套接层协议SSL(Secure Socket Layer)是用来保障数据安全传输的协议,目前已经成为工业标准.首先简要介绍了SSL协议,设计并实现了基于SSL的数据安全传输系统,它由两部分组成:SSL客户方安全通信代理CSP(Client Secure Proxy)和服务器方安全通信网关SSG(Server Secure Gateway),二者可以在Internet上建立一个安全通道,从而能够保障敏感数据的安全传输.讨论了系统的整体结构,并详细分析了实现中的若干关键技术,主要包括握手协议的实现、密钥的协商、记录层数据的分段与填充、会话重用等.      

Great solar bursts of October 19, 22 and 23, 1989

Itapetinga measurements at 48 GHz with the multibeam technique are used to determine the relative position of solar burst centroid of emission with high spatial accuracy and time resolution. For the Great Bursts of October 19,22, 1989, with a large production of relativistic particles, and October 23, it is suggested that, at 48 GHz, the bursts might have originated in more then one source in space and time. Additionally the October 19 and 22 Ground Level Events exhibited very unusual intensity-time profiles including double component structures for the onset phase. The Bern observatory spectral radio emission data show a strong spectral flattening typical for large source inhomogeneties. The interpretation for this is that large solar flares are a superposition of a few strong bursts (separated both in space and time) in the same flaring region.     

WIND/3DP and Nancay radioheliographobservations of solar energetic electron events

Initial results of a combined study of electron events using the 3DP experiment on the WIND spacecraftand the Nançay Radioheliograph (NRH) are presented. A total of 57 electron events whose solar release time could be inferred from WIND/3DP observations occurred during NRH observing times. In 40 of them a distinct signature was detected in maps at decimetric and metric wavelengths (dm-m-λ) taken by the NRH. These events are equally distributed among two categories: (1) Electron release together with dm-m-λ bursts of a few minutes duration: these events are also accompanied by decametric-hectometric type III bursts seen by WAVES/WIND. They correspond to the well-known impulsive electron events. (2) Electron release during long duration (several tens of minutes) dm-m-λ emission: the electrons are most often released more than ten minutes after the start of the radio event. In the majority of cases the dm-m-λ radio source changes position, size, and/or intensity near the time of electron release.