The general class of Bianchi cosmological models with viscous fluid and particle creation in Brans-Dicke theory

This paper deals with the general class of Bianchi cosmological models with bulk viscosity and particle creation described by full causal thermodynamics in Brans-Dicke theory. We discuss three types of average scale-factor solutions for the general class of Bianchi cosmological models by using a special law for the deceler- ation parameter which is linear in time with a negative slope. The exact solutions to the corresponding field equations are obtained in quadrature form and solutions to the Einstein field equations are obtained for three different physically viable cosmologies. All the physical parameters are calculated and discussed in each model.     

Corrections to Solar Thermal Structure when a Turbulent Magnetic Field is Included

Correction of non-ideal effect due to a magnetic fluctuating tensor is derived from the ideal MHD equations. The inclusion of a magnetic turbulent field leads to modifications of the hydrostatic equilibrium equation and thermodynamical variables such as the temperature T, the adiabatic exponent γ, the adiabatic temperature gradient △↓ad and the temperature gradient △↓. In particular, the modifications in the adiabatic and radiative temperature gradients will result in a change in the Schwarzchild criterion, hence in the location of the base of the convective zone. Incorporating the modifications, we construct a modified thermodynamical equilibrium structure of the Sun.     

湍流压对中小质量恒星后期演化的影响：（Ⅰ）湍流压,物态方程及热…

本以恒星结构演化理论中常用的混合程对流理论为基础，给出了湍流压以及考虑湍流压情况下恒星内部物态方程和各热力学量的表达式。在此基础上研究了质量为２．８Ｍ和７Ｍ的恒星由主序演化到红巨星和ＡＧＢ星阶段其湍流压的大小。结果证明，在红巨星和ＡＧＢ阶段，靠近恒星表面区域内湍流压可以达到总压强的３０％。     

梅山铁矿形成物理化学条件的热力学分析

Using thermodynamic data, the authors have calculated the equilibrium constants (at high temperatures and pressures) for 47 reactions among 18 kinds of minerals present in the Meishan iron deposit, and constructed equilibrium diagrams of the mineral paragenesis.On this basis, they have discussed the physicochemical conditions of formation of the depo.sit and the relations between mineralization and wall-rock alteration.     

土地信息多级网格及其应用

多比例尺空间数据的表达与处理是GIS的一个固有问题,本文用土地信息多级网格代替多级土地数据库中的多比例尺数据库及其多比例尺表达,以解决多级土地数据库建库过程中制图综合带来的地类数据变化问题,同时也为土地数据的共享提供了方便.     

黑体辐射定律遥感教学改革设计与实践

普朗克黑体辐射定律是遥感类课程教学的重点和难点,本文以定律分析为核心,从数值模拟大气层顶太阳光谱辐照度曲线、卫星传感器光谱响应函数卷积计算、地物行星反射率计算及地表温度反演4个方面入手,对黑体辐射定律理论教学和实践教学内容进行优化设计和教学实现。实践证明,该教学改革不仅可以使学生更容易理解和掌握黑体辐射定律揭示的基本规律,而且以此为基础,能够使学生通过实践加深对地物两大特性(反射特性和热辐射特性)的理解,提高学生对遥感类课程的兴趣。     

一种计算图斑净面积的新方法

在图斑净面积计算规则下,对地类图斑和线状地物两个图层的组织结构和相互关系展开研究,提出Arc-Map空间分析计算图斑净面积方法。采用实例验证了该方法的可行性和准确性,通过对比分析可以看出,Arc-Map空间分析法具有良好的使用和推广价值。     

最新中国陆地数字高程基准模型:重力似大地水准面CNGG2011

本文回顾了近20年国内外国家局部大地水准面模型研究的概况和发展背景,采用Stokes-Helmert方法,计算了一个新的2′×2′中国重力和1985国家高程基准似大地水准面数值模型（CNGG2011）,采用了1百万余陆地重力数据和SRTM 7″.5×7″.5地形高数据,以及649个B级GPS水准点数据。CNGG2011平均精度为±0.13m,东部地区±0.07m,西部地区±0.14m。各省区局部似大地水准面平均精度为±0.06m,东部为±0.05m,西部为±0.11m。西藏精度为±0.22m。本文还讨论了重力大地水准面与GPS水准的关系,提出了今后进一步精化我国高程基准大地水准面模型的构想。