Sm2-xCexCuO4的物性研究

制备了Sm2-xCexCuO4的多晶样品.X-射线粉末衍射结果表明,该系列样品为K2NiF4214结构,当0.090.17时,为T'相.电阻率测量在0.15,0.17,0.19样品上观测到超导转变.最高Tc对应于x=0.17为13.6K,均远低于(Pr0.8La1.2)1.85Ce1.2CuO4 的超导转变温度(30K).这是由于该系列样品在远高于超导转变温度时就存在更强的载流子局域化效应.磁化率测量结果表明x=0.17的样品为体超导.该体系样品的Tc低、抗磁信号小与载流子的强局域化效应有关.热电势测量结果表明,在最佳超导组份附近斜率改变符号,欠掺杂区域载流子为电子型,过掺杂区域载流子为空穴型.     

基于软集合参数约简的一种启发式算法

在比较和分析了原有软集合参数约简文献的基础上,本文总结出了一些参数约简的结论,并结合参数约简的思想,提出了一种参数约简的启发式算法.同时,本文给出了该启发式算法的具体算法过程及算例,并对该算法的相关理论进行了证明.最后,将该算法的约简结果与其它两种算法进行对比分析,表明本文算法的高效性和优越性.     

空间低能离子探测器的紫外响应测试

在空间离子探测过程中,太阳紫外光也会进入探测器产生光污染信号。为了考察它对离子探测的影响,搭建了一套模拟太阳紫外光污染的地面测试系统,并对自主研制的空间低能离子探测器原理样机进行了紫外响应测试。实验结果表明:沿水平方向进入分析器的紫外光响应可以忽略,而以一定倾斜角进入分析器的紫外光响应计数率约为102~ 103 s−1。根据测试结果,估算出探测器对太阳紫外光的抑制率约为10−8,分析了紫外光污染对探测空间低能离子如质子和 粒子的影响。对于质子,由于其通量大,紫外光的影响不大。而对于通量较小的 粒子,紫外光的影响较大,需要进一步采取有效措施进行抑制。此外,本测试系统可以推广到其它空间粒子探测器的太阳紫外光污染的地面模拟测试。In the detection of space ions, solar ultraviolet (UV) can also enter the detector and generate a noise to the signal of ions. A testing system on the ground is built to test the UV response of detector. Experiments on a home-made principle prototype of space low-energy ion detector are carried out by using this system. The results show that the response of detector to the UV entering the electrostatic analyzer along the horizontal direction can be negligible and counts of the response to the UV along a bias direction are about 102 ~103 s−1. According to the measured results, the UV suppression ratio is estimated to be about 10−8 and the inuence of solar UV on the detection of space low-energy ions such as proton and alpha particle has been analyzed. For proton, the inuence is insigni cant due to its high ux. But for the low ux alpha particle, the inuence of solar UV is noticeable and further rejection is needed. In addition, this system can also be applied to test the UV response of other space particle detectors.