典型炭材料微观结构及SO2吸附机理研究

采用SEM和低温氮吸附方法研究了碳纳米管和活性炭的表面微观形貌及孔隙结构,通过固定床研究了炭材料SO₂吸附机理。研究结果表明:活性炭大孔直接暴露于表面,中孔和微孔分布于大孔内部,"聚合"是碳纳米管的重要特征;椰壳活性炭是微孔型吸附剂,煤基活性炭孔隙主要由微孔和大孔组成,碳纳米管氮吸附有明显的毛细凝聚现象,中孔和大孔是其孔隙主要组成;活性炭SO₂吸附过程受物理吸附控制,碳纳米管SO₂吸附不同于活性炭,同时受到物理吸附和化学吸附控制;孔径小于0.7 mm的微孔是炭材料SO₂吸附的主要场所。     

活性炭吸附氦气式回热器的吸附特性研究

回热式低温制冷机在空间探测和地面实验中都有重要应用,但是在液氦温区工质氦气的体积比热容高于目前几乎所有的蓄冷材料,导致回热器效率低下.直接使用活性炭吸附一部分工质氦气作为蓄冷填料是一种潜在的解决方案.基于4～J10 K温度区间内吸附量的实验数据,建立了低温动态吸附计算模型,分析了液氦温区动态吸附特性对回热器性能参数的影...     

YK-1活性炭平衡储氢特性分析

文中基于氢在椰壳活性炭YK-1上的平衡吸附数据,以探寻氢在碳基材料上适宜存储条件为目的,研究吸附氢分子间相互作用能随储存系统温度、压力、表面遮盖率的变化规律。首先,依据容积法的原理,在温度区间113K—293K、压力范围0—13MPa测试氢在YK-1椰壳活性炭上的吸附等温线。其次,应用格子理论推导通用吸附等温方程,通过等温方程的线性标绘确定氢分子在吸附表面的最大浓度,并由氢分子在活性炭典型吸附空间内受到的壁面作用势函数迭代求解氢分子受到的壁面作用势,进而获得与各吸附平衡态对应的氢分子间相互作用能。最后,根据氢分子间作用能随温度、表面遮盖率等的变化关系,分析氢分子在此活性炭上吸附的特点。     

低温吸附泵用椰壳活性炭的性能测试

活性炭的比表面积、孔径及分布是影响液氦低温吸附泵抽氢、氦性能的关键因素。为了确定制作液氦低温吸附泵的吸附剂,选取了C1、C2、C3、C4四种椰壳活性炭,用比表面积及孔径分析仪测定了其等温吸附性能,并对实验数据进行了针对性分析,获得了各活性炭的比表面积、微孔比表面积份额、不同孔径所对应的孔容等性能数据。结果表明,四种活性炭中C2最适于做为抽氢、氦的液氦低温吸附泵的吸附剂。     

氦气回收纯化系统的设计与应用

为实现激波风洞试验尾气氦气(氦含量>80%)的回收和循环利用，研制了一套氦气回收与纯化系统。该系统采用三塔真空变压吸附的技术将试验尾气中的氮气等杂质气体去除，得到纯度大于98%的氦气。系统采用开式纯化和闭式纯化相结合的工艺方式，将氦气的回收率提高到97%。系统调试结果表明，研制的氦气回收纯化系统在常温条件下实现了风洞试验尾气的回收、纯化和循环使用，有效地降低了风洞运行和维护成本，同时也节约了氦气资源。     

低温泵用椰基活性炭材料的选择和比较

为了选择用于核聚变研究领域中在氢、氦气环境下的低温吸附泵所用的吸附剂,在初步筛选基础上,比对了4种椰基活性炭材料。采用扫描电镜对材料微观结构进行了扫描,用比表面积及孔径分析仪测定了等温吸附性能,最终获得了活性炭样本的比表面积、微孔比表面积份额、不同孔径所对应的孔容等性能数据;通过对实验结果的比对分析,为筛选适用于核聚变研究环境下低温吸附泵使用的吸附剂材料,提供了重要的实验数据。     

CAEP FEL-THz低温系统氦气纯化方法研究

鉴于氦的稀缺性,中国工程物理研究院高平均功率太赫兹大型科研装置(CAEP FEL-THz)低温系统中,必须除去回收粗氦中的杂质,以实现循环再利用。文中通过对常规氦气分离方法的比较和对低温系统低纯度氦气中所含杂质成分的分析,提出了一种基于高压低温冷凝分离和吸附的氦气纯化方法,旨在将低纯度氦气的纯度提升至满足低温系统使用的要求。据此,初步设计了一套氦气纯化系统,介绍了其工艺流程和主要部件。     

活性炭对苯蒸汽吸附分离过程的实验研究

本文选用活性炭对苯蒸汽进行了动态、静态吸附性能实验,研究了苯蒸汽在不同系列活性炭上的吸附、脱附性能以及活性炭微孔结构对吸附性能的影响。结果表明:苯蒸汽在活性炭上的吸脱附性能明显与吸附剂的比表面、孔容、孔径与孔径分布直接相关。     

活性炭/沸石层状床氢气纯化穿透曲线热效应

应用变压吸附技术对氢气混合气进行分离提纯是制取高纯度氢气的有效途径。本文主要研究多组分气体在活性炭/沸石层状床中穿透曲线的热效应影响,基于多物理场仿真平台Comsol,建立了多组分气体在多孔介质中的吸附、传热与传质模型。并将模拟值与实验数据进行验证分析,探索吸附过程伴随的热效应对穿透曲线的影响机理。最后针对变压吸附氢气纯化系统运行参数研究了环境温度、吸附条件和活性炭与沸石层高度比等对穿透曲线的影响。     

非局域密度泛函理论表征活性炭孔径分布的改进算法

为提高由NLDFT计算值确定活性炭孔径分布(PSD)的精度,根据测得的77K氮在非石墨化碳黑BP460和椰壳活性炭K05上的吸附数据,比较了吸附空间及壁面结构采取不同假设对计算结果的影响。结果表明,常规将活性炭吸附空间近似为无限尺寸的石墨化碳黑表面构成的狭缝孔,并由Lorenz-Berthelot混合法则确定相互作用参数,计算值在较低压力区域和试验值之间的偏差明显;而将吸附壁面结构近似为非石墨化碳黑,并由表面粗糙度和石墨晶格分布的误差函数修正相互作用参数后,计算结果和试验值吻合良好。分析结果时发现,归一化方法和考虑周边吸附质分子作用的加权函数是影响NLDFT计算结果准确性的关键因素。     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...