CRESDA APPLICATION SYSTEM OF CBERS-1, RESULTS AND TYPICAL EXAMPLES OF APPLICATIONS

CRESDA Application System of CBERS-1 was established in 1999. During the operation of the system for more than two years, about 240 000 scenes of CBERS-1 Level 0 data have been archived and more than 13 000 scenes of Level 2 products have been ordered by end users from different application fields.In this paper, the typical examples of applications in crop yield estimation,calamity alleviation, resources survey and protection, environment monitoring and continuable development, and urban planning are mainly described.     

服役环境下材料S-N曲线的BP模型

目前常规条件下各种金属材料的S—N曲线已基本完备，但是考虑腐蚀环境影响的S—N曲线还很少见。本文研究了在加速腐蚀当量环境谱作用后，LY12-CZ铝舍金材料的S—N曲线随日历年限的变化规律。首先，将试件暴露于加速腐蚀环境中，进行0年、3年、8年和13年的腐蚀试验。其次进行常幅谱下的疲劳试验。试验结果表明：腐蚀环境作用后的疲劳寿命均值随日历年限的增加显著降低，而变异系数呈增长的趋势。鉴于腐蚀环境作用后的S—N曲线具有较强的非线性，本文采用反向传播网络对加速腐蚀后的疲劳试验结果进行训练，建立了日历腐蚀环境下材料S—N曲线的BP模型，仿真结果与试验结果吻合较好。     

Supernova remnants with magnetars: Clues to magnetar formation

In this paper I discuss the lack of observational evidence that magnetars are formed as rapidly rotating neutron stars. Supernova remnants containing magnetars do not show the excess of kinetic energy expected for such a formation scenario, nor is there any evidence for a relic pulsar wind nebula. However, it could be that magnetars are formed with somewhat slower rotation periods, or that not all excess rotational energy was used to boost the explosion energy, for example as a result of gravitational radiation. Another observational tests for the rapid initial period hypothesis is to look for statistical evidence that about 1% of the observed supernovae have an additional 10⁴⁰–10⁴⁴ erg/s excess energy during the first year, caused by the spin down luminosity of a magnetar.     

Journey to the Moon: Recent results,science, future robotic and human exploration

The upcoming fleet of lunar missions, and the announcement of new lunar exploration initiatives, show an exciting “Journey to the Moon”, covering recent results, science, future robotic and human exploration. We review some of the questions, findings and perspectives given in the papers included in this issue of Advances in Space Research.     

理想导电直劈的GTD解中N值的选取

本文经严密的数学推导，给出了理想导电直劈的GTD解中N值的选取方法及准确结果，为理想导电直劈散射场的最终确定提供了依据。     

SDD-1算法的研究与改进

SDD-1算法是分布式数据库查询优化的一种算法,研究SDD-1算法的过程,分析SDD-1算法的优缺点,并针对该算法的不考虑最后一点传输代价的缺点提出了改进的SDD-1算法。     

RIPv1协议路由传播问题

通过对RIPv1有类路由协议在普通网络结构中的路由传播和更新情况进行研究分析和总结,然后将总结结果应用到特殊网络结构中。调试命令观察和分析特殊结构中使用RIPv1协议的路由传播情况,通过分析特殊结构中的路由更新问题,得出结论。     

压力对有序Li1/2TiS2光学性质的影响

采用第一性原理的平面波赝势方法和局域密度近似（LDA），计算了压力对Li1/2TiS2的形成能和光学性质的影响。研究发现，Li1/2TiS2体系在压强为3GPa时形成能最小，体系最稳定，之后体系的形成能随压力的增大而单调增大；随着压力的增大，导带向高能移动而价带向低能方向移动，体系费米能级上的态密度增大，各个态密度峰值降低且数目增多；光学参量峰值的位置与介电函数虚部的峰值位置很接近，随着压力增大，均向高能方向移动（蓝移），且峰值升高。     

基于嫦娥一号高能粒子数据的地球磁层屏蔽效应研究

月球绕地球运行轨道约有1/4位于地球磁层内,因此,地球磁层是否会为月球轨道附近高能粒子提供足够的磁场屏蔽对于探索月球活动具有重要影响.嫦娥一号是中国首颗绕月人造卫星,其绕月飞行的工作轨道距离月球表面200 km.通过对嫦娥一号高能粒子探测器(HPD)的探测数据进行分析,比较了当月球位于地球磁层内外6个不同能道(能量范围4～400 MeV)时质子通量的变化,发现当月球位于地球磁层内时,这些能道的质子通量并没有发生显著减少,结果表明地球磁层不能为月球轨道附近高能粒子提供显著的磁屏蔽.