天然铅及其同位素全套中子核反应数据的理论计算

用球形光学模型和核反应多步过程的半经典理论，计算了入射能量在1.0keV-20MeV的中子与^204Pb，^206Pb,^207Pb,^206Pb，和^NatPb相互作用的全套核反应数据，计算结果与评价实验数据比较，符合较好。     

一种计算中子非弹角分布的简单方法

介绍在DWBA法中应用一种数学过程简洁明了,而物理图像却很清晰的方法来计算中子非弹角分布.     

γ暴搜寻中实测角分布与角半径的关系

 考虑实测角分布和角半径的关系,在实测角分布保持一定的情况下,用MonteCarlo方法推导出1个统计意义上的最佳角半径.并通过全天区搜寻的方法去探测1个带有γ射线暴的模拟数据,进一步证实了这一结果.     

亚纯函数的公共值与幅角分布

设f(z)是下级大于2的超越亚纯函数,证明了复平面上存在一条从原点出发的射线OR,使得以OR为分角线的任意小角域内,f(z)与其导函数f’(z)至多只有一个IM公共值.     

磁场对放电阴极区中电子能量及角分布的影响

采用Ｃｏｎｔｅ Ｃａｒｌｏ模拟方法研究了磁场对直流辉光放电阻极鞘层中电子能量及角分布的影响。磁场垂直于阴极鞘层中电场的方向。电子与中性粒子的碰撞过程由自散射技术处理。计算了电子与中性粒子的非弹性碰撞次数。着重研究了电子的能量和散射角分布。结果表明，横向磁场能在一定程度上改变直流放电中电子的输运过程。磁场中电子与中性粒子的非弹性碰撞增强，这一结果与实验结果基本一致。     

树轮α-纤维素δ13C角分布及其气候含义

利用从中国天目山和庐山采集的4株树轮样，分析了树轮沿不同方位δ^13C的变化特点，讨论了角分布的成因。结果表明，树轮在不同方位上的木质α－纤维素δ^13C值不同，而且各方位上δ^13C的差异与分析期间历年平均值的年际差异在量级上大致相当。对各方位δ^13C作方差分析表明，各方位存在显性差异。说明δ^13C的角分布具有独立意义。对其中一棵柳杉树轮δ^13C角分布与气候要素的相关分析表明，不同方位的δ^13C值与年、季节和朋降水及温度相关，从而使树轮可记录住处分辨率提高、信息量增大。用树轮δ^13C的角分布重建的气候要素更能反映气候要素的实际变化情况。     

Plasma sheet stretching accompanied by field aligned energetic ion fluxes observed by the NUADU instrument aboard TC-2

The NUADU (NeUtral Atom Detector Unit) instrument aboard TC-2 recorded 4л solid angle images of charged particles (E >180 keV) spiraling around the magnetic field lines in the near-Earth plasma sheet (at ~ -7 RE, equatorial dawn-to-night side) during a geomagnetic storm (Dst =-219 nT) on August 24, 2005. Energetic ion beam events characterized by symmetrical, ring-like, solid angle distributions around ambient magnetic field lines were observed during a 34-minute traversal of the plasma sheet by the TC-2 spacecraft. Also, observations during these multiple crossings of the plasma sheet were monitored by the magnetometer experiment (FGM) aboard the same spacecraft. During each crossing, a whistler-mode chorus enhancement was observed in the anisotropic area by the TC-2 low frequency electromagnetic wave detector (LFEW/TC-2) at a frequency just above that of the local lower hybrid wave. A comparison of the ion pitch angle distribution (PAD) map with the ambient magnetic field shows that an enhancement in the field aligned energetic ion flux was accompanied by tailward stretching of the magnetic field lines in the plasma sheet. In contrast, the perpendicular ion-flux enhancement was accompanied by a signature indicating the corresponding shrinkage of the magnetic field lines in the plasma sheet. Since both parallel ion-flux and perpendicular ion-flux enhancements occurred intermittently, the data were interpreted to imply a dynamical, oscillatory process of the magnetic field line (stretching and shrinking) in the near-Earth plasma sheet, which might have acted to help establish an interaction region in this area which would support continuous aurora-substorm triggering during the ongoing magnetic storm. The whistler-mode chorus may have been produced due to ion gyro-resonance during particle pitch angle diffusion after the plasma sheet compression.     

电子与硼、碳和氮原子碰撞角分布的理论计算

用模型势方法研究和计算了电子被B、C、N原子散射的微分截面 (角分布 ) ,入射电子能量从 0 .1～ 1.0eV ,计算的角分布从 0°～ 180°.从理论研究和计算中看到 ,随入射电子能量的增加 ,电子被B、C、N原子散射的微分截面有规律性变化 .