地球同步轨道附近哨声湍流对“种子电子”的加速

本文在等离子体准线性理论下研究了地球同步轨道附近哨声湍流对亚暴“种子电子”的波-电子共振相互作用. 当发生这种共振时，“种子电子”的动量分布函数经动量扩散而随时间演化，部分低能电子数减少了，而高能尾部分的相对论电子（能量大于1MeV）数增加了，说明“种子电子”得到了哨声湍流的有效加速，且哨声湍流的能量越高，其加速效率越高. 另外，哨声湍流的频率越低（或波数越小），共振电子的能量越高（或单位质量的动量越大）；频率范围越宽，共振电子的能量范围越宽，被加速的电子数也越多. 磁层哨声湍流加速“种子电子” 大约在30h内就可以造成相对论电子数显著增加，这正好和大多数磁暴期间观测到的相对论电子通量的增长时间相当.     

Characteristics of carbonaceous particles in Beijing during winter and summer 2003

Campaigns were conducted to measure Organic Carbon (OC) and Elemental Carbon (EC) in PM2.5 during winter and summer 2003 in Beijing. Modest differences of PM2.5 and PM10 mean concentrations were observed between the winter and summer campaigns. The mean PM2.5/PM10 ratio in both seasons was around 60%, indicating PM2.5 contributed significantly to PM10. The mean concentrations of OC and EC in PM2.5 were 11.2±7.5 and 6.0±5.0μg m-3 for the winter campaign, and 9.4±2.1 and 4.3±3.0 μg m-3 for the summer campaign, respectively. Diurnal concentrations of OC and EC in PM2.5 were found high at night and low during the daytime in winter, and characterized by an obvious minimum in the summer afternoon. The mean OC/EC ratio was 1.87±0.09 for winter and Z39±0.49 for summer. The higher OC/EC ratio in summer indicates some formation of Secondary Organic Carbon (SOC). The estimated SOC was 2.8 μg m-3 for winter and 4.2μg m-3 for summer.     

鄂尔多斯盆地侏罗系低煤阶煤层气系统演化

低煤阶煤层气作为一种非常规天然气资源,具有良好的勘探开发前景。我国低煤阶煤层气资源丰富,进行低煤阶煤层气系统演化分析,对其富集成藏及开发具有重要的理论意义。鄂尔多斯盆地煤层甲烷的碳同位素δ13C₁为–33.1‰~–80.0‰,氢同位素δ_CH4为–235‰~–268‰。该盆地侏罗系煤层气藏主要有次生生物气与热成因气构成的混合型煤层气藏和热成因气藏两种类型。据构造热事件、煤层气组分及成因,结合不同阶段的煤层埋深、变质程度和生气特征等,将鄂尔多斯盆地侏罗系低煤阶煤层气系统演化划分为4个阶段:煤系浅埋–原生生物气阶段﹑煤系深埋–热成因气阶段﹑煤系抬升–吸附气逃逸散失阶段﹑煤系局部沉降–次生生物气补充阶段。其中,煤系深埋–热成因气阶段和局部沉降–次生生物气阶段是低煤阶煤层气资源的主要形成阶段。次生生物气的补充是鄂尔多斯盆地侏罗系低煤阶煤层气成功开发的重要气源。鄂尔多斯盆地侏罗系煤层气藏应属于单斜式富气成藏模式。      

弱二次切变流轴对称涡旋演变的解析研究

运用格林函数方法,给出了弱二次切变流轴对称涡旋演变的解析解.结果表明:当环境流中弱二次切变强度增加(减少)时,扰动动能的最大值增加(减小),扰动动能的变化加速(减速);而扰动涡旋的范围对扰动动能的大小与变化也存在一定的影响.     

The Global Distribution of Secondary Particulate Matter in a 3-D Lagrangian Chemistry Transport Model

A global 3-D Lagrangian chemistry-transport model STOCHEM is used to describe the tropospheric distributions of four components of the secondary atmospheric aerosol: nitrate, sulphate, ammonium and organic compounds. The model describes the detailed chemistry of the formation of the acid precursors from the oxidation of SO₂, DMS, NO_x, NH₃ and terpenes and their uptake into the aerosol. Model results are compared in some detail with the available surface observations. Comparisons are made between the global budgets and burdens found in other modelling studies. The global distributions of the total mass of secondary aerosols have been estimated for the pre-industrial, present day and 2030 emissions and large changes have been estimated in the mass fractions of the different secondary aerosol components.     

数值分析预报产品的拼合图制作系统

设计了数值分析预报产品的拼合图制作系统。该系统是在原地面传输网络上的格点资料绘图系统基础上制作的,对原系统进行了一系列改进。属于ＭＩＣＡＰＳ系统的二次开发内容之一。     

Multiple resonance in one problem of the stability of the motion of a satellite relative to the center of mass

We investigate the stability of the periodic motion of a satellite, a rigid body, relative to the center of mass in a central Newtonian gravitational field in an elliptical orbit. The orbital eccentricity is assumed to be low. In a circular orbit, this periodic motion transforms into the well-known motion called hyperboloidal precession (the symmetry axis of the satellite occupies a fixed position in the plane perpendicular to the radius vector of the center of mass relative to the attractive center and describes a hyperboloidal surface in absolute space, with the satellite rotating around the symmetry axis at a constant angular velocity). We consider the case where the parameters of the problem are close to their values at which a multiple parametric resonance takes place (the frequencies of the small oscillations of the satellite’s symmetry axis are related by several second-order resonance relations). We have found the instability and stability regions in the first (linear) approximation at low eccentricities.     

Biomass and estimated productivity of the benthic macrofauna in the New York Bight: A stressed coastal area

Waste disposal in the apex of the New York Bight has resulted in the contamination of sediments by toxic chemicals and some alteration to the community composition of the benthic macrofauna. The significance of these alterations to other communities in the area, e.g. its fishery resources, has not been clearly demonstrated. This paper presents data on an extensive survey of the macrofauna biomass, that many fish and lobster feed on, in the waste disposal impacted areas of the apex, using samples from both 1973 and 1980–1982. Variable mean production to biomass (P:B) ratios were used to estimate secondary production from the biomass of each major taxon. The macrofaunal biomass (wet wt.) of most of the apex area impacted by waste disposal was relatively high, with a mean biomass of 127 g m^?2 for 1973 and 344 g m^?2 for 1980–1982. Estimated secondary production was also high, being 201 Kcal m^?2 year^?1 in 1973 and 383 Kcal m^?2 year^?1 in 1980–1982. These values suggest there has been no inhibition of at least biomass, as the values were similar to or greater than values found in other areas of the Bight with similar bathymetric characteristics.     

Secular resonances in the asteroid belt: Theoretical perturbation approach and the problem of their location

In this paper a theoretical perturbation approach to the problem of the dynamics in secular resonance is exposed. This approach avoids any expansion of the main term of the Hamiltonian (linear term in the masses) with respect to the eccentricity or the inclination of the asteroid, in order to achieve results valid for any value of these variables. Moreover suitable action-angle variables are introduced to take properly into account the dynamics related to the motion of the argument of perihelion of the asteroid, which is relevant at high inclination. A class of secular resonances wider than that usually considered is found. An explicit computation of the location of the main secular resonances, estimating also the contribution of the quadratic term in the masses by means of classical series expansion, is reported in the last sections. The accuracy of computations obtained by series expansion is discussed in the paper.