基于Pro/E软件的卫星三维建模方法的探讨

主要对基于Pro/E软件的卫星三维建模和高效率、高可靠性、低成本的总装设计方法等进行了初步的研究和探讨。     

论带通信道的信道容量的不确定性

依据山农的经典论证方法 ,证明山农信道容量定理仅适用于低通信道 ,不适用于带通信道。对于带通信道 ,信道容量将随信道通带的中心频率而改变。所以带通信道的信道容量具有不确定性。     

基于Web Service的B2B电子商务系统模型的研究

B2B电子商务是目前最具潜力的商务形式。但传统B2B电子商务系统的基本结构和交互接口均没有统一的标准和解决方案，带来了系统可重构性和可移植性差等缺陷。针对这种缺陷，结合Web Service技术，提出基于Web Service的B2B电子商务系统模型。该系统模型通过构建核心应用程序整合Internet和Internet范围内相对独立的Web Service，并作为供应链的一部分，能提供标准接口实现和其他应用程序如ERP，CRM和SCM等的交互，这种形式的B2B电子商务系统能很容易地进行开发和维护。最后以其中一个模块为例，给出了具体实现基于WebService的B2B电子商务系统的解决方案．     

正确认识山农信道容量定理

山农信道容量定理公式中的信道带宽恒为信源所发出的消息信号的带宽 ,是信道带宽的理论最小极限 ;它不同于现代通信工程中传输已调制信号时所需要的信道带宽。这是本文所证明的基本结论。这一结论将限制信道容量定理的普适性和实用性。     

股票投资回收期的研究

文章对股票的投资回收期及股票的标准投资回收期进行了探讨，针对不同股票的特征，提出了4种股票投资回收期的模型，从而，克服了用市盈率作为判断股票投资价值的不足，为股票投资者提供了一个投资决策方法。     

环氧改性氰酸酯树脂研究

分别采用E20和E51环氧树脂与双酚A型二氰酸酯(BADCy)共聚来改善氰酸酯树脂的力学性能.用DSC,FTIR研究了两种不同分子量的环氧改性氰酸酯体系的反应性,发现E20和E51对BADCy的固化反应均有催化作用,但E20的催化作用强于E51.断面SEM表明,经E20和E51改性的BADCy断口处存在大量的韧涡.但改性体系的热变形温度(HDT)和吸水率有所下降,当配比(质量)相同时,E51/BADCy体系比E20/BADCy体系具有更高的HDT和较小的吸水率.     

极光区电离层Hall电导率的观测及其在E层电子加热情况下的特征

本文利用欧洲的ＥＩＳＣＡＴ雷达观测资料及与这配合的地磁观测数据，用电离层参数直接计算和地面磁场反演两种方法导出了极区电离层Ｈａｌｌ电导率，特别显示出在强对流电场激发的Ｅ层等离子体不稳定波对电子加热情况下，电导率明显增高。     

Diurnal and seasonal variations in long-term changes in the E-layer critical frequency

Long-term changes in the E-layer critical frequency, foE, at three stations of the European region (Juliusruh, Slough and Rome) and also at Moscow and Wakkanai stations are analyzed by the method developed by the authors and described in detail in the previous papers. It is found that Juliusruh and Slough stations demonstrate a well-pronounced change in foE (a trend) during two previous decades. At the same time, the same features of the behavior of the aforementioned trend k(foE) are obtained. The trend is positive and negative in the morning and evening hours, respectively. Similar diurnal behavior of k(foE) is found also for Moscow station but with lower absolute values of the trends. A well-pronounced seasonal behavior of k(foE) is detected at Juliusruh and Slough: the trend is minimal and maximal in the summer period and at the end of fall—beginning of winter, respectively. The maximal amplitude in the morning hours reaches +0.04?MHz per year, whereas the minimal amplitude in evening hours is ?0.06?MHz per year. No systematic changes exceeding by the magnitude 0.01?MHz per year are found for Rome and Wakkanai stations. It is assumed that the observed trends are related to changes (trends) in the meridional wind bringing NO molecules from the auroral oval to lower latitudes.     

An attempt to study long-term variation of sporadic E layers using neural networks

Strong positive correlation between sporadic E layers and the solar activity and the long-term declining trend of Es were found in this paper. Then the feed-forward back propagation neural networks (NNs) were used to simulate the long-term variation of Es at four stations and predict foEs yearly average values. The inputs used for NNs are the yearly mean values of foEs in the daytime of the past ten years and the yearly averaged data of solar 10.7 cm radio flux (F107) of the present year, and the output is the present yearly mean value of daytime foEs. The outputs of trained NNs have high correlation with the desired values and the foEs yearly mean values predicted by NNs have good agreement with the observed data. The results indicate that NNs can make full use of the observed data to simulate the long variation rule of Es. Also, the results confirm the effect of solar activity on Es.     

Longitudinal variation of the equatorial ionosphere: Modeling and experimental results

We describe a new version of the Parameterized Regional Ionospheric Model (PARIM) which has been modified to include the longitudinal dependences. This model has been reconstructed using multidimensional Fourier series. To validate PARIM results, the South America maps of critical frequencies for the E (foE) and F (foF2) regions were compared with the values calculated by Sheffield Plasmasphere-Ionosphere Model (SUPIM) and IRI representations. PARIM presents very good results, the general characteristics of both regions, mainly the presence of the equatorial ionization anomaly, were well reproduced for equinoctial conditions of solar minimum and maximum. The values of foF2 and hmF2 recorded over Jicamarca (12°S; 77°W; dip lat. 1°N; mag. declination 0.3°) and sites of the conjugate point equatorial experiment (COPEX) campaign Boa Vista (2.8°N; 60.7°W; dip lat. 11.4°; mag. declination −13.1°), Cachimbo (9.5°S; 54.8°W; dip lat. −1.8°; mag. declination −15.5°), and Campo Grande (20.4°S; 54.6°W; dip lat. −11.1°; mag. declination −14.0°) have been used in this work. foF2 calculated by PARIM show good agreement with the observations, except during morning over Boa Vista and midnight-morning over Campo Grande. Some discrepancies were also found for the F-region peak height (hmF2) near the geomagnetic equator during times of F₃ layer occurrences. IRI has underestimated both foF2 and hmF2 over equatorial and low latitude sectors during evening-nighttimes, except for Jicamarca where foF2 values were overestimated.