KDP晶体杂质对生长及出槽应力分布的影响

KDP晶体中的杂质易导致其开裂.本文采用有限元法分析了不同属性、尺寸、形状的晶体杂质对大尺寸KDP晶体生长及出槽应力分布的影响.结果表明,不同属性的杂质对晶体生长应力和出槽应力分布具有不同程度的影响.杂质附近的生长应力与杂质的弹性模量呈正向变化;杂质附近的出槽应力与杂质和晶体的热膨胀系数之差呈正向变化;杂质的尺寸越大,形状越尖锐,杂质附近的生长应力和出槽应力均增大.     

基于近红外光谱法的多组分复杂溢油源定量建模分析

研究利用近红外光谱分析方法进行模拟复杂混合溢油源的定量分析问题。选取汽油、柴油、煤油三种轻质石油类产品,按照不同浓度比例配置成40个模拟混合溢油样本,利用傅里叶变换近红外光谱仪采集其在4 000～12 000 cm-1谱区范围内的近红外光谱;采用不同预处理方法,利用偏最小二乘算法建立混合溢油样本三组分各自的浓度定量模型。汽油、柴油和煤油的最优预处理方法均为二阶导数方法,分别在8 501.3～7 999.8 cm-1,6 102.1～4 597.8 cm-1,6 549.5～4 597.8 cm-1,7 999.8～7 498.4 cm-1和6 102.1～4 597.8 cm-1谱区范围内,预测模型的决定系数R2分别为0.998 2,0.990 2和0.993 6;RMSEP值分别为0.474 7,0.936 1和1.013 1;RPD值分别为25.126 9,10.517 3和13.072 0。实验结果表明：利用近红外光谱分析技术结合化学计量学方法能够定量确定模拟混合溢油样本中各组分的浓度,为海洋复杂溢油源的定量检测与分析提供有效手段。     

Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation

The perspective of the detectability of Galactic dark matter subhaioes on the Fermi satellite is investigated in this work.Under the assumptions that dark matter annihilation accounts for the "GeV excess" of the Galactic diffuse γ-rays discovered by EGRET and the γ-ray flux is dominated by the contribution from subhaloes of dark matter, we calculate the expected number of dark matter subhaloes that Fermi may detect.We show that Fermi may detect a few tens to several hundred subhaloes in a 1-year all-sky survey.Since EGRET observation is taken as a normalization, this prediction is independent of the particle physics property of dark matter.The uncertainties of the prediction are discussed in detail.We find that the major uncertainty comes from the mass function of subhaloes, i.e., whether the subhaloes are "point like" (high-mass rich) or "diffuse like" (low-mass rich).Other uncertainties like the background estimation and the observational errors will contribute a factor of 2-3.     

Study of energy deposition and stripper temperature for CYCIAE-100

Nowadays high intensity proton accelerators are extensively applied, and this paper gives particular emphasis on CYCIAE-100, a 100 MeV high intensity compact cyclotron being constructed at CIAE. For accelerators of this type, the study is focused on how to improve the beam intensity. As for CYCIAE-100, the charge-exchange extraction is used to get protons. So it is crucial to enhance the lifetime of the stripping foil, which is largely determined by the energy deposition on it. For this cyclotron, due to the influence of the magnetic field, the electrons will spin near the foil and lose energy each time when they cross the foil. The energy deposition refers to all the energy deposition of protons and electrons. This paper stresses the stripper study of CYCIAE-100, in which the particle distribution on the foil is simulated and the energy deposition of the protons and electrons stripped from the H- ions are calculated. The temperature distributions are then calculated as a main reference for the foil design.     

Influence of radial magnetic field on emittance in the median plane at CYCIAE-100

A 75—100 MeV H- compact cyclotron CYCIAE-100 is being constructed at China Institute of Atomic Energy (CIAE). About 200 μA proton beam will be provided by CYCIAE-100. The imperfection of magnetic fields will remarkably affect the acceleration orbit and beam envelope in CYCIAE-100. The effects to the accelerating beam by the imperfection fields, especially the field components Br on the mid-plane will be analyzed in detail with tracking code COMA. Poles misalignment that causes magnetic imperfection will be described in the paper. According to the simulation results, the tolerance of the poles machining and assembly will be illustrated in this paper.     

正方形小通道内的非牛顿流体-氮气两相流动流型的实验研究

对水力直径为2.5 mm的正方形小通道内的非牛顿流体-氮气的垂直向上两相流动流型进行了可视化实验,工质分别为:浓度0.2%的聚丙烯酰胺(PAM)和0.2%的黄原胶(XG)水溶液,表观气速0.1～100 m/s,表观液速0.01～6 m/s.观察到的典型流型有:弹状流、搅拌流、弹环状流和环状流,其中弹环状流未见于水-空气上升流动.在PAM-氮气实验中发现了一种新流型-泡状-弹状流.通过流型图对比,发现非牛顿流体的搅拌流区域较牛顿流体窄,弹状-搅拌流转变线也明显右移,非牛顿流体的黏性对流型转变的影响较大.     

Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation

The perspective of the detectability of Galactic dark matter subhaloes on the Fermi satellite is investigated in this work. Under the assumptions that dark matter annihilation accounts for the ``GeV excess' of the Galactic diffuse $\upgamma$-rays discovered by EGRET and the $\upgamma$-ray flux is dominated by the contribution from subhaloes of dark matter, we calculate the expected number of dark matter subhaloes that Fermi may detect. We show that Fermi may detect a few tens to several hundred subhaloes in a 1-year all-sky survey. Since EGRET observation is taken as a normalization, this prediction is independent of the particle physics property of dark matter. The uncertainties of the prediction are discussed in detail. We find that the major uncertainty comes from the mass function of subhaloes, i.e., whether the subhaloes are ``point like' (high-mass rich) or ``diffuse like' (low-mass rich). Other uncertainties like the background estimation and the observational errors will contribute a factor of 2—3.     

Radiation response of pseudo-MOS transistors fabricated in hardened fully-depleted SIMOX SOI wafers

The total dose radiation response of pseudo-MOS transistors fabricated in hardened and unhardened FD （fully-depleted） SIMOX （Separation by Implanted Oxygen） SOI （Silicon-on-insulator） wafers is presented. At 1 Mrad（Si） radiation dose, the threshold voltage shift of the pseudo-MOS transistor is reduced from -115.5 to -1.9 V by the hardening procedure. The centroid location of the net positive charge trapped in BOX, the hole-trap density and the hole capture fraction of BOX are also shown. The results suggest that hardened FD SIMOX SOI wafers can perform well in a radiation environment.     

ITER电流引线高温超导叠制作工艺及性能测试

ITER高温超导电流引线载流能力最大要达到68 kA,一根电流引线共需要1000多根银金基Bi-2223高温超导带并联.这些高温超导带分成90叠,每叠由12层带组成.银金基Bi-2223带价格是普通银基Bi系带的4～5倍,而目前欧洲超导公司提供的超导叠的报价几乎是其带价格加倍,所以开发超导叠的制作工艺是非常有价值的.本文详细的介绍了超导叠的真空钎焊制作工艺,并进行了77 K下超导带的接头电阻测试和77 K自场下的临界电流测试,以及模拟在实际运行温度65～5 K条件下高温超导叠的载流能力测试和接头电阻的测试.测试结果证明了此工艺的可行性.     

甲壳素类液晶高分子的研究--用CD谱研究N-邻苯二甲酰化壳聚糖溶致胆甾相的形成临界浓度

N邻苯二甲酰化壳聚糖在多种常见有机溶剂中能形成胆甾液晶相.用圆偏光二向色性谱(CD)研究了N邻苯二甲酰化壳聚糖的DMF、DMSO、DMAC和吡啶4种溶剂体系,在形成溶致胆甾液晶相前后的手性变化信息.CD谱图上观测到两类吸收,即在400nm附近较宽的吸收和330nm附近较尖锐的吸收.前者归属于胆甾相层片的超分子螺旋构象,而后者可以归属于分子链的螺旋构象.圆偏光二向色性可以作为测量胆甾液晶临界浓度的一种手段,它能捕捉到胆甾螺旋层片出现那一瞬间的浓度,以CD谱上在波长400nm左右刚出现肩峰的浓度为临界浓度,其值均比偏光显微镜法低1%,说明其灵敏度比偏光显微镜法高,且避免了偏光显微镜法的某种主观性.分别用两种方法旋转玻片进行CD测试,结果证明线性二向色性分量和双折射分量对胆甾层片螺旋的CD信号强度没有大的影响.