重力场中的熵产生研究

重力场中的大气处于非平衡态，其温度是空间的函数，不同的等温面之间要产生热流，从而改变熵的空间分布。本文推导出重力场中的熵产生公式，并描绘出熵产生随高度变化的近似曲线。     

对气体等温气压公式的修正

用理想气体的多方过程方程取代等温过程方程，推导出气体处于多方平衡过程时的气压公式，该公式是对气体等温气压公式的一种很好的修正．对多方指数”等于1，1．1，1．2，1．3，1．4等5种不同情况分别给出了大气压强随高度的变化曲线．此外还讨论了考虑到重力加速度随离地面高度的变化后对气压公式的修正．     

用变分方法计算天文折射

天文折射是近地大气效应,至今尚未彻底解决.该文引入重力场气体分子的玻耳兹曼分布,以及等温大气折射率与此相似的分布.用变分方法计算天文折射以     

重力场中的范德瓦耳斯气体

将地球大气近似为重力场中的范德瓦耳斯气体,在绝热过程近似下导出了大气温度、压强随高度的分布,并与理想气体近似结果进行了比较分析.     

范德瓦尔斯气体的气压公式

将大气近似为范德瓦尔斯气体,用多方过程取代等温过程,推导出范德瓦尔斯气体处于多方过程时的气压公式,该式是对理想气体恒温气压公式的一种很好的修正.     

球对称引力场中运动粒子的分布

本文将导出重力场中粒子按高度分布的精确表达式，然后将这一分布应用于大气：估算大气的总重量；导出由大气压确定高度的近似表式．     

关于Young-Laplace公式和Kelvin公式的对话

讨论了Young-Laplace公式及Kelvin公式证明和应用中的一些问题.     

楔形平板光程差公式的修正

本文具体地推导并比较了楔形平板光程差公式的几个修正式，指出了文献［l］中的修正式是不合适的．一、楔形平板光程差公式的推导在普通物理和普通物理实验的课本中，楔形平板（或尖劈薄膜）的光程差公式都近似地用平行平板的光程差公式，即中d为平板厚度，n为平板的折射率，i’为折射角，凸为相干光的光程差．在（1）式中，光程差与楔形平板的楔角的关系没有得到反映，而事实上是有关系的，文献［fi中，给出了（1）式的修正式为（2）式中的户表示平板的楔角．该书使用的示意图见图1．笔者认为用（2）式来修正是不合适的．为此，笔者的推导…     

基因算法在参数反演问题中的应用研究

提出了一种利用改进的基因算法求大气压强精确公式的参数反演方法。运用基因算法反演求出由多态方程推导大气压强公式中的大气比热比γ ,从而得到大气压强精确计算公式 ,并与文献给出的大气压强公式进行比较。结果表明 ,用基因算法所确定的大气压强公式所得计算值与实测值更加吻合 ,说明基因算法在反演问题中具有很高的应用价值。同时经数据分析得出改进基因算法比传统基因算法精度高、速度快。     

推迟势公式的导出

推迟势公式是研究电磁辐射问题的重要理论基础，因此，导出推迟势公式具有重要意义．本文在一般方法的基础上作了改进，得到两种比较简明的导出推迟势公式的方法．     

通过磁化曲线计算磁熵值

在恒定低磁场下测量磁性物质的M T 曲线,可以确定其居里点;在居里点附近测量一系列等温磁化曲线M H,根据磁化曲线并借助于磁系统的热力学关系式,通过数值计算方法得到磁性材料在施加或撤去外磁场过程中的磁熵变化值.     

高层大气风场洛伦兹光谱线型粒子辐射率探测研究

以高层大气中的极光谱线为被探测源,提出了一种高层大气(80—300km)风场洛伦兹光谱线型的粒子辐射率被动探测的新原理.采用该原理不仅可获得高层大气风场的速度、温度和压强信息,更重要的是还能同时探测到高层大气中辐射粒子体辐射率,解决了目前高层大气风场研究中只能探测高层大气风场速度、温度和压强却不能获知粒子的体辐射率的问题.给出了基于洛伦兹光谱线型的辐射源粒子体辐射率、大气风场速度、温度和压强的理论计算公式.采用计算机模拟对探测误差进行了分析,给出了体辐射率、风场速度、温度、压强的误差分布规律,为进一步丰富和完善高层大气风场探测提供了理论依据和实验基础,对航空航天、空间探测、环境保护、国家安全和国民经济建设都具有重要的科学意义和广阔的应用前景.     

随机多孔复相介质稳态温度场的多尺度数值模拟

本文就随机多孔复相介质稳态温度场,提出了多尺度分析的基本思想和具体的计算公式,它们是建立在确定性温度场的多尺度算法和Ｋａｒｈｕｎｅｎ－Ｌｏｅｖｅ展开式基础上．文中算例表明这一算法的有效性。     

Interference image spectroscopy for upper atmospheric wind field measurement

Based on the observation of natural airglow and auroral visible emission lines in the upper atmosphere as the explored source, we have surveyed the upper atmosphere wind field through interference imaging spectroscopy coupled with the Doppler effect of electrical and magnetic waves. The velocity and temperature of the upper atmospheric wind field are analyzed and studied. The survey theory and calculation formula of atmosphere wind field in all directions and multi-directions are presented when the relative velocity of the explored source to the detector and their linking line have an arbitrary angle. We also analyzed the effects of the measurement of the upper atmospheric wind field using computer simulation, and explained the reason why the auroral emission line is thought as Gaussian profile.     

Giant magnetocaloric effect in the Gd5Ge2.025Si1.925In0.05 compound

The magnetocaloric properties of the Gd 5 Ge 2.025 Si 1.925 In 0.05 compound have been studied by x-ray diffraction,magnetic and heat capacity measurements.Powder x-ray diffraction measurement shows that the compound has a dominant phase of monoclinic Gd5Ge2Si2-type structure and a small quantity of Gd 5(Ge,Si) 3-type phase at room temperature.At about 270 K,this compound shows a first order phase transition.The isothermal magnetic entropy change(△SM) is calculated from the temperature and magnetic field dependences of the magnetization and the temperature dependence of MCE in terms of adiabatic temperature change(△Tad) is calculated from the isothermal magnetic entropy change and the temperature variation in zero-field heat-capacity data.The maximum S M is 13.6 J·kg-1·K-1 and maximum △Tad is 13 K for the magnetic field change of 0-5 T.The Debye temperature(θD) of this compound is 149 K and the value of DOS at the Fermi level is 1.6 states/eV·atom from the low temperature zero-field heat-capacity data.A considerable isothermal magnetic entropy change and adiabatic temperature change under a field change of 0-5 T jointly make the Gd5Ge2.025Si1.925 In 0.05 compound an attractive candidate for a magnetic refrigerant.     

Exact explicit barometric formula for a warm isothermal Fermi gas

The exact explicit barometric formula is derived for a warm isothermal Fermi gas in a uniform potential field.     

Coherence function and mean field of plane and spherical sound waves propagating through inhomogeneous anisotropic turbulence

Inhomogeneity and anisotropy are intrinsic characteristics of daytime and nighttime atmospheric turbulence. For example, turbulent eddies are often stretched in the direction of the mean wind, and the turbulence statistics depends on the height above the ground. Recent studies have shown that the log-amplitude and phase fluctuations of plane and spherical sound waves are significantly affected by turbulence inhomogeneity and anisotropy. The present paper is devoted to studies of the mean sound field and the coherence functions of plane and spherical sound waves propagating through inhomogeneous anisotropic turbulence with temperature and velocity fluctuations. These statistical moments of a sound field are important in many practical applications, e.g., for source detection, ranging, and recognition. Formulas are derived for the mean sound field and coherence function of initially arbitrary waveform. Using the latter formula, we also obtained formulas for the coherence functions of plane and spherical sound waves. All these formulas coincide with those known in the literature for two limiting cases: homogeneous isotropic turbulence with temperature and wind velocity fluctuations, and inhomogeneous anisotropic turbulence with temperature fluctuations only. Using the formulas obtained, we have numerically shown that turbulence inhomogeneity significantly affects the coherence functions of plane and spherical sound waves.     

A general analytical method for evaluation of the thermodynamic properties of matters using virial coefficients with Morse potential at high temperature

In this paper, we established an analytical formula for the second virial coefficient (SVC) with Morse potential without using any numerical methods, and the obtained formula is applied to the calculation of the speed of sound of some matter at high temperature. This approach is based on the series expansion formula and special functions, which allows the exact evaluations of any thermodynamic properties of matter using the SVC. As an application, the obtained analytical formula is used for evaluation of the SVC with Morse potential for high‐temperature gas and the plasma region of the intermolecular interactions of neutral atom gases of B, Si, Zn, H₂, N₂, O₂, NO, CO, He, Ne, Ar, Kr , and Xe . Based on the obtained formula of SVC, the speed of sound for gases of N₂, Ar , and Zn are also determined analytically. A specific maximum temperature is chosen for every gas to ensure that there are still neutral atoms in the gas, and low temperatures are avoided due to quantum effects. The results are compared with numerical data and another analytical data from the literature. The new analytical solution is shown to be in good agreement with the compared data and is verified to supply proper thermodynamic data.     

超光谱红外卫星资料同步反演不同地表类型的大气廓线、地表温度和地表发射率

大气温度、水汽、地表温度和地表发射率是大气和地表的本征信息量。利用卫星红外资料精确反演大气温湿廓线有利于准确预报天气和研究气候变化,同时地表温度和地表发射率光谱的反演为研究植物生长与作物产量、地表水分蒸发与循环、能量平衡、地表成分及物理性质、气候变迁与全球环境提供重要参数指标。把大气和地面作为一个整体系统来考虑,建立一种能同步反演大气温度廓线、大气水汽廓线、地表温度和地表发射率的反演方法,利用超光谱红外卫星资料(atmospheric infrared sounder, AIRS),针对我国新疆地区沙漠和雪地两种典型发射率地表同步反演大气温度廓线、水汽廓线、地表温度和地表发射率。反演方法首先线性化地球-大气系统红外辐射传输方程, 提出通过经验正交函数构建大气廓线和地表发射率光谱,有效减少反演变量数,建立同步物理反演模式,然后以美国国家环境预报中心(National Centers for Environmental Prediction,NCEP)的预报结果(初始大气温度、水汽廓线以及地表参数)作为初始值,最后通过牛顿迭代得到最优化解。反演观测区域覆盖我国新疆塔克拉玛干沙漠和准噶尔盆地,分别选择位于塔克拉玛干沙漠腹地的塔中探测站(纬度38.98°, 经度83.64°)和准噶尔盆地的阜康荒漠生态系统国家野外科学观测研究站(纬度44.2°, 经度87.9° )为反演地面验证点。反演结果表明,塔克拉玛干沙漠地表温度明显高于准噶尔盆地地表温度,与实际情况相一致;根据反演的8.6和13.4 μm处的地表发射率分布情况,可以看出在8.6 μm处沙漠地表发射率明显低于雪地发射率,在6～15 μm范围内,反演的沙漠地区(塔中站)地表发射率和雪地地区(阜康站)地表发射率与美国喷气推进实验室测量的沙漠发射率光谱和雪地发射率光谱相一致。研究表明,把大气和地面作为一个整体系统来考虑,把地表发射率加入到反演中,通过比较和分析沙漠地区(塔中)和雪地地区(阜康)的大气廓线反演结果与当地气象探空值和传统反演方法反演值,改进了大气温度廓线和水汽廓线反演精度,特别是边界层温度和水汽改进尤为明显;同时分析表明在发射率光谱变化较大的沙漠地区, 大气廓线反演精度的改进比雪地要高,这是由于地表发射率光谱在沙漠、戈壁地区变化较大,而雪地的发射率光谱变化不大。用该方法针对地表发射率光谱变化较大的地区(沙漠)同步反演大气廓线、地表温度和地表发射率,可以更有效的提高大气温度廓线、水汽廓线的反演精度。该研究结果可以为数值天气预报和我国未来超光谱红外卫星应用提供服务和有力支持, 具有十分重要的意义。