Optoacoustic laser Stark spectroscopy in the ν2 band of 14NH3

Laser Stark spectroscopy of the R(5, K) transitions in the ν₂ band of ammonia was carried out using coincidences with the 9-μm band CO₂ laser lines. We observed 22 Doppler-free resonances by using an optoacoustic detector and a Lamb-dip stabilized CO₂ laser. A simultaneous analysis of sa, aa, and ss lines yields zero-field transition frequencies with an absolute accuracy of 1 ～ 2 MHz.     

Ultra high resolution of 6.2 keV 181Ta in 2H-TaSe2

The 6.2 keV γ-rays of ¹⁸¹Ta have been used to study the hyperfine interaction of ¹⁸¹Ta in the trigonal prismatic charge density wave material 2H-TaSe₂. Using a region of interest drive and an unstrained single crystal sample, we are able to resolve the splitting between the nuclear transition $\text{±}\text{5}\text{2}\text{→ ±}\text{3}\text{2}$ and $\text{±}\text{7}\text{2}\text{→ ±}\text{5}\text{2}$. Our experimental linewidth is that of the Ta metal.     

从自旋冰到自旋液态的渡越——结构与磁性质的演化

使用固相反应法得到了Ho_2-xTb_xTi₂O₇（x=0,05,1,15,2）系列多晶样品.X射线衍射（XRD）实验与2K到300K温度区间的直流磁化率测量结果显示,随着Tb即是x的增加,体系由自旋冰Ho₂Ti₂O₇向自旋液Tb₂Ti₂O_{7关键词： 自旋冰 自旋液体 自旋阻挫 晶格结构}     

Li,N双受主共掺杂实现p型ZnO的第一性原理研究

基于密度泛函理论,采用第一性原理平面波超软赝势法,首先对六方纤锌矿结构的ZnO晶体和N,Li分别掺杂ZnO以及Li-N共掺杂ZnO晶体的几何结构分别进行了优化计算,在此基础上计算得到了未掺杂ZnO晶体和不同掺杂情况下ZnO晶体的能带结构、总体态密度、分波态密度和电荷布居数.利用计算的结果,从理论上分析了Li-N共掺杂ZnO更容易得到稳定的p型ZnO. 关键词： ZnO 电子结构 第一性原理 p型共掺杂     

发动机润滑油品质的可见-近红外光谱快速检测

研究了基于可见-近红外光谱技术的发动机润滑油品质的快速检测方法,包括粘度与含水率的预测。在获取可见-近红外光谱信息的基础上,采用广义回归神经网络分别建立了粘度与含水率的预测模型。预测集样本的确定系数分别达到了0.9818和0.9999。说明可见-近红外光谱技术能够用于发动机润滑油的含水率与粘度的预测。     

基于Matlab Simulink的物理实验——简谐振动仿真研究

以简谐振动和阻尼振动仿真为例介绍了用Simulink对物理实验进行仿真建模的方法。给出了位移、速度等振动曲线;可对振动过程中的动能、势能以及机械能进行监测。体现出Simulink仿真物理实验的优越性。     

Nearly-integrable dissipative systems and celestial mechanics

The influence of dissipative effects on classical dynamical models of Celestial Mechanics is of basic importance. We introduce the reader to the subject, giving classical examples found in the literature, like the standard map, the Hénon map, the logistic mapping. In the framework of the dissipative standard map, we investigate the existence of periodic orbits as a function of the parameters. We also provide some techniques to compute the breakdown threshold of quasi-periodic attractors. Next, we review a simple model of Celestial Mechanics, known as the spin-orbit problem which is closely linked to the dissipative standard map. In this context we present the conservative and dissipative KAM theorems to prove the existence of quasi-periodic tori and invariant attractors. We conclude by reviewing some dissipative models of Celestial Mechanics. Among the rotational dynamics we consider the Yarkovsky and YORP effects; within the three-body problem we introduce the so-called Stokes and Poynting–Robertson effects.     

High energy radiation fluences in the ISS-USLab: Ion discrimination and particle abundances

The ALTEA (Anomalous Long Term Effects on Astronauts) detector was used to characterize the radiation environment inside the USLab of the International Space Station (ISS), where it measured the abundances of ions from Be to Fe. We compare the ALTEA results with Alteino results obtained in the PIRS module of the Russian segment of the ISS, and normalize to the high energy Si abundances given by Simpson. These are the first particle spectral measurements, which include ions up to Fe, performed in the USLab. The small differences observed between those made inside the USLab and the Simpson abundances can be attributed to the transport through the spacecraft hull. However, the low abundance of Fe cannot be attributed to only this process.