结构应力耦合的微悬臂阵列

微悬臂器件被广泛应用于力学显微镜和光力学研究中,实现微悬臂之间的耦合在高精密测量和量子声子网络构建方面具有重要的应用前景。不同于通过电、磁相互作用实现微纳共振器之间耦合的方法,设计并制备了通过结构应力实现耦合的微悬臂阵列。模拟和实验结果表明,这种结构应力耦合微悬臂阵列不仅可以获得较大的耦合强度和较高的力学性能,同时悬臂之间的耦合强度也容易控制。对于其它形式的微纳共振器,同样可以利用结构应力耦合这种方法来实现共振器之间耦合的阵列。     

镨铁硼低温波荡器机械结构的传热分析

对镨铁硼材料在低温和室温下的热学和力学物性进行了测量;使用实测的镨铁硼物性并结合数值模拟的方法对镨铁硼低温波荡器的传热特性进行了分析;结果表明,磁极和磁极夹持机构与磁铁间的热传导是冷却磁铁的关键因素,冷却管道宜采用双通道同向并联的方式。使用该设计通过液氮可以冷却磁铁至82K,同时能够控制由于温差带来的磁极间相位误差小于0.1度,满足镨铁硼低温波荡器设计要求。     

冲击波测试系统的动态建模及应用

若测试系统的带宽不能完全覆盖冲击波信号的有效带宽,就会存在较大的动态误差。根据冲击波测试系统的激波管动态校准实验数据,建立了冲击波测试系统动态数学模型,设计了动态校正数字滤波器。仿真结果表明,动态校正滤波器明显提高了系统动态响应的快速性,展宽了工作频带。实弹测试结果显示,校正滤波器能提高冲击波测试的精度和可靠性。该方法能有效消除动态误差,提高测试数据的准确性。     

农药丁吡吗啉与腐殖酸作用机理探讨

探讨农药丁吡吗啉与腐殖酸的作用机理, 可进一步了解农药在土壤中腐殖酸催化下降解的行为过程。将市售腐殖酸进行逐级分离,获得黄腐酸、棕腐酸和黑腐酸的固态或溶液状态,而后分别与农药丁吡吗啉进行作用,利用红外,荧光两种分析方法对其作用机理进行了解释。结果表明,三组分与丁吡吗啉之间广泛存在范德华力、次级键等弱作用力。黄腐酸与丁吡吗啉之间存在氢键和电荷转移吸附等作用力,棕腐酸与丁吡吗啉存在电荷转移吸附等作用力,黑腐酸与丁吡吗啉之间的作用力最弱,即依照黄腐酸、棕腐酸、黑腐酸三组分平均分子量依次递增的顺序,与农药丁吡吗啉之间的作用力依次降低。     

Measurement of Gamma-Rays from 11ΛB and 12ΛC

From the ^12 C（π^＋,K^＋）^12 AC reaction the γ -rays of 261.6±0.24 ke V（7/2^＋ →5/2^＋）and 1481.7±0.7 ke V（1/2^＋ →5/2^＋） of ^11 A B,and 2667.3±2.8 keV（1^- 2 → 2^- 1）of ^12 A C hypernuclei have been identified using a large germanium detector array Hyperball2 at K6 beam line of KEK. The observed energies of the transitions 1481.7keV and 261.6 keV are significantly different from the values predicted by the shell model using the △ and SN parameters determined from the ^7 △ Li data.     

Measurement and analysis of fission rates in a spherical mockup of uranium and polyethylene

Measurements of the reaction rate distribution were carried out using two kinds of Plate Micro Fission Chamber （PMFC）. The first is a depleted uranium chamber and the second an enriched uranium chamber. The material in the depleted uranium chamber is strictly the same as the material in the uranium assembly. With the equation solution to conduct the isotope contribution correction, the fission rate of 238U and 235U were obtained from the fission rate of depleted uranium and enriched uranium. Then, the fission count of 238U and 235U in an individual uranium shell was obtained. In this work, MCNP5 and continuous energy cross sections ENDF/BV.0 were used for the analysis of fission rate distribution and fission count. The calculated results were compared with the experimental ones. The calculation of fission rate of DU and EU were found to agree with the measured ones within 10% except at the positions in polyethylene region and the two positions near the outer surface. Because the fission chamber was not considered in the calculation of the fission counts of 238U and 235U, the calculated results did not agree well with the experimental ones.     

145Er的β延发质子衰变性质研究

通过92Mo(58Ni, 2p3n)熔合蒸发反应生成了非常缺中子核145Er。利用氦喷嘴带传输系统把研究目标核传输到低本底测量站, 进行了质子 γ符合测量, 得到了不受同量异位素干扰的145Er的β延发质子谱。经过仔细分析与延发质子符合的γ谱, 发现了145Er的11/2-同核异能态具有β延发质子衰变性质。经拟合退激144Dy不同激发态γ跃迁的衰变曲线, 得出145Er的1/2+基态和11/2-同核异能态的半衰期分别为(1.6±0.6)和(0.6±0.1) s。最后, 简单介绍了中重质量区缺中子新核素的合成及衰变研究计划。The neutron deficient isotope 145Er was produced via the fusion evaporation reaction 92Mo(58Ni, 2p3n). The reaction products were transported to a low background counting area using a He jet tape transport system, and proton γ coincidence measurements were carried out. Based on the analysis of γ transitions in coincidence with β delayed protons, the β delayed proton decay of an νh11/2 isomer in 145Er was proposed. By fitting the decay curves of the γ transitions depopulating the low lying states in 144Dy, the half lives of the ground state and the νh11/2 isomeric state in 145Er were deduced to be (1.6±0.6) and (0.6±0.1) s, respectively. An experimental plan to synthesize new β delayed proton precursors in the medium heavy mass region has been presented.     

太阳的光辉

 人类处在天地之间，每日目睹昼夜更替，每年经历寒暑变迁。"日居月诸，照临下土"。人类在阳光下生活、生存，与生具备的亘古不变的好奇心，也一直激励人们关心周围的自然现象，"日月安属?列星何陈?"几千年来，人类历经世代更迭，观念更新，从以地球为中心的地心说到以太阳为中心的日心说，直至1609年伽利略开始使用望远镜观测太阳黑子，人类对太阳逐渐有了正确的科学了解。到国际天文学联合会（IAU）成立的1919年为止，人们已经发现了太阳光谱中的大量谱线（Fraunhofer，1814）；发现了太阳黑子的蝴蝶图分布及其11年活动周期（Schwabe，1843）；发现了剧烈的太阳耀斑活动（Carrington，1859）；通过日食期间的太阳光谱观测，发现了一种新元素：氦（Secchi，1868），次年又发现了一条与众不同的谱线，它与当时所有已知元素的谱线都不吻合，以为是发现了另一种新元素；此外，还发现了太阳黑子具有强磁场（Hale，1908），这是人类首次在地球以外的天体上发现磁场。这些工作为太阳物理以及天体物理的发展奠定了重要基础。     

Epidemic spreading on random surfer networks with infected avoidance strategy

In this paper, we study epidemic spreading on random surfer networks with infected avoidance(IA) strategy. In particular, we consider that susceptible individuals' moving direction angles are affected by the current location information received from infected individuals through a directed information network. The model is mainly analyzed by discrete-time numerical simulations. The results indicate that the IA strategy can restrain epidemic spreading effectively. However,when long-distance jumps of individuals exist, the IA strategy's effectiveness on restraining epidemic spreading is heavily reduced. Finally, it is found that the influence of the noises from information transferring process on epidemic spreading is indistinctive.     

CF2燃料组件主要堆内辐照性能

结合辐照考验方案,评价了CF2先导燃料组件的机械性能及燃料棒的热力性能,结果表明各项性能均满足准则要求。结合辐照后池边检查结果,对CF2燃料组件的主要堆内辐照性能进行了研究,包括燃料组件及燃料棒生长和弯曲、定位格架生长等各项燃耗相关性能。结果表明,在燃耗达到44500 MWd/tU的情况下CF2燃料组件主要辐照性能均达到了预期水平,满足反应堆的使用要求。CF2燃料组件后续可批量应用于华龙一号。