Using an adjoint model to improve an optimum interpolation-based data-assimilation system     

X.-Y. HUANG  N. GUSTAFSSON  E. R. KÄLLÉN 《地球，A辑:动力气象学与海洋学》1997,49(2):161-176

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Radiative association in Li+H revisited: the role of quasi-bound states     

O. J. Bennett  A. S. Dickinson  T. Leininger  F. X. Gadéa 《Monthly notices of the Royal Astronomical Society》2003,341(1):361-368

The role in radiative association of narrow resonances arising from quasi-bound levels is examined. For the rate coefficient the contribution from such levels is readily calculated in terms of the Einstein A -coefficient from bound rovibrational levels generated using a suitable alternative boundary condition. By locating systematically all the quasi-bound levels, an enhancement by more than an order of magnitude of the rate coefficient for Li(2s) + H(1s) association above about 600 K is obtained. The effect on the LiH abundance in the early Universe is no more than an increase of a factor of 3 for limited ranges of values of the redshift. For the Li(2p) state the effect of narrow resonances appears to have been taken into account in previous calculations.  相似文献   

Multiple bipolar structure of normal magnetic field at the magnetopause     

T Chen  Z.X LiuX.X Zhang 《Planetary and Space Science》2003,51(6):381-386

We describe how a local plasma structure can be changed by a transverse shear flow using numerical simulation to investigate the disturbance process near the magnetopause. The results show that magnetic field lines are bent by transverse shear flow disturbance near the current sheet region. There are multiple bipolar structures of the normal magnetic field in the numerical simulation. We term this new feature as K-point magnetic reconnection, realistic for discussing space observations.  相似文献   

On the influence of magnetic fields on level populations     

Z. Q. Qu  C. L. Xu  X. Y. Zhang  X. L. Yan  C. L. Jin 《Monthly notices of the Royal Astronomical Society》2006,370(4):1790-1796

The influence of magnetic fields on the energy level populations of atoms is firstly studied by analysing the Stokes profiles of Fe  i 6302.5 forming in the solar magnetized atmosphere, with the aid of a departure factor defined to evaluate the deviation from the normal Boltzmann distribution without a magnetic field. This factor is directly related to the ratio of line-source function to the continuum one. The relationship between the departure and the magnetic field reveals an effect that the magnetic field induces an exponential increase in the level population of the lower level of Fe  i 6302.5 (Landé factor   g = 2.5  ) with the field strength. This indicates that the magnetic field can cause the redistribution of populations of those levels whose Landé factors are non-zero. Therefore, this effect should be included in the calculation of the statistical equilibrium. Secondly, an experiment utilizing the Hg5461 line in the laboratory on the Earth is carried out to reveal that the exponential relation is independent of variations in temperature, and the excitation is completely magneto-induced. Finally, the exponential relation is explained by taking account of the magnetic energy in the Boltzmann distribution.  相似文献   

Muon flux at the geographical South Pole     

X. Bai  T.K. Gaisser  A. Karle  K. Rawlins  G.M. Spiczak  Todor Stanev 《Astroparticle Physics》2006,25(6):361-367

The muon flux at the South Pole was measured for five zenith angles, 0°, 15°, 35°, 82.13° and 85.15° with a scintillator muon telescope incorporating ice Cherenkov tank detectors as the absorber. We compare the measurements with other data and with calculations.  相似文献   

The Hα-cyclonic spectra of a flare loop system on 1981 April 27     

X. M. Gu  B. S. Li  Y. J. Ding  S. C. Li  Z. Li 《Solar physics》1983,87(1):155-164

The data such as the H-spectrum-spectroheliographic (SSHG) observations, the H-chromospheric observations, etc., of a flare loop prominence which occurred on the western solar limb on 1981 April 27 have been obtained at Yunnan Observatory. The distribution of the internal motions and the macroscopical motion of the flare loop prominence with time and space in the course of its eruption and ascension is derived from the comprehensive analysis of the data. The possible physical pictures and the instability of the motions of the loop are inferred and discussed.  相似文献   

RETRACTION: Numerical simulation of a wind-sand flow under different conditions of atmospheric stability     

LÜ PING  ZHIBAO DONG 《Sedimentology》2008,55(3):721-721

A theoretical model for wind‐sand flow is developed by considering the coupling between wind flow and sand particle motion, the latter subject to the Magnus effect, under different atmospheric stability conditions. Using this model, the characteristics of the wind‐sand flow are discussed in detail. The results show that the atmospheric stability and the Magnus effect both have a strong influence on wind profiles and on the trajectories of sand particles. This approach produces results with characteristics that differ from those previously reported; the latter only applying to atmospheric conditions of neutral stability. The saltating sand reaches a greater height under non‐neutral stability than under neutral stability, while the maximum horizontal distance is greater under unstable conditions and is smaller under stable conditions than under conditions of neutral stability.  相似文献   

XEPOS型偏振能量色散X射线荧光光谱仪分析蒙古铁矿石   总被引：5，自引：4，他引：1  

耿刚强  宁国东  王巧玲  丁慧  朱明达  白福全  董海成  牛素琴  王再田 《岩矿测试》2008,27(6):423-426

以熔融玻璃片和粉末压片制样,采用XEPOS型偏振能量色散X射线荧光光谱仪,建立了铁矿石中总铁、氧化钙、氧化镁、二氧化硅、三氧化二铝、硫、磷、铜等组分的快速分析方法。着重讨论硫、磷两元素测定的可行性和Lucas-Tooth、Price数学校正模型的适应性和改善方法的途径。  相似文献   

火焰发射光谱法测定氯化物型湖卤水中钾和钠   总被引：1，自引：1，他引：0  

邢谦  董迈青  谢海东 《岩矿测试》2008,27(5)

氯化物型湖卤水中一般呈现高钠低钾的分布状态,实验配制了合理的钾钠分布比例的标准系列,原水样不需特殊处理,通过逐级稀释,采用最高标准调节能量,火焰发射光谱法直接测定湖卤水中的钾和钠,在标准曲线上查得被测离子的质量,然后换算成钾和钠的含量.方法用于氯化物型湖卤水中钾和钠的测定,回收率为91%～116%,精密度(RSD,n=7)小于1%.  相似文献   

塔里木盆地塔中1井藻纹层白云岩与竹叶状白云岩成因——基于岩石学、元素与同位素地球化学的厘定   总被引：1，自引：0，他引：1  

陈永权  周新源  赵葵东  杨文静  董晨阳  朱长见 《地质学报》2008,82(6):826-834

塔里木盆地寒武系—奥陶系底部发育了大量的白云岩, 白云岩中赋存丰富的油气资源, 但是由于塔里木盆地白云岩研究基础薄弱,限制了塔里木盆地白云岩型油气藏的勘探。本文选择塔中地区塔中1井下奥陶统藻纹层白云岩与夹层竹叶状白云岩作为对象,应用岩石学与地球化学方法对其成因问题进行了研究。藻纹层白云岩与夹层竹叶状白云岩的宏观构造与微观结构指示其可能形成于高能的潮坪环境;低有序度值（0.6）与塔北地区中寒武统阿瓦塔格组潮坪同沉积白云岩(有序度值0.61)特点一致,指示该白云岩结晶速率较快;同时,高Fe、Mn含量与低U、Mo含量也与氧化环境的潮坪相一致。藻纹层白云岩与夹层竹叶状白云岩δ18O值非常集中, 变化在-7.4‰～-5.8‰;87Sr/86Sr组成变化很小,在0.709015～0.709276之间,与前人报道的晚寒武世－早奥陶世海水同位素特征一致,同时白云岩的稀土元素配分模式也与下奥陶统泥晶灰岩一致,指示了白云岩的沉积/成岩物质来源于蒸发海水;白云岩δ13C值变化从-2.5‰～+1.6‰,并有着随深度增加而升高的变化规律,可能指示了古海洋的碳同位素氧化。藻纹层白云岩与夹层竹叶状白云岩的构造特点具有原生沉积特征,同时白云岩CaO与MgO含量的正相关关系也支持该白云岩原生沉积特点。因此,塔里木盆地塔中1井钻遇的下奥陶统藻纹层白云岩与夹层竹叶状白云岩为潮坪环境下,从蒸发海水中快速沉积形成的。  相似文献