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71.
Calculations are made of the resonance contribution to electron-impact excitation of H-like 13C and Li-like 23Na, 25Mg, 27Al and 29Si to the upper hyperfine levels that produce millimetre (mm) lines of likely astrophysical interest. The resonance contribution is found to be very important for these Li-like ions, considerably more important than for Li-like 57Fe considered previously. However, resonances are found to be rather unimportant for H-like 13C. The effect of radiative decay on the resonance contribution is found to be insignificant in all of the present calculations.  相似文献   
72.
Profiles of spectral lines emitted from an accretion ring around an object with strong gravitational field should be affected by Doppler shift, gravitational redshift, and deflection of light. Taking these effects into account, precise line profile of a Keplerian ring around a Kerr black hole for a distant observer is obtained by solving the kinetic equation of photons.  相似文献   
73.
An improved approach is given for deriving the physical parameters of a molecular cloud by its NH3 rotation-inversion hyperfine spectra. The optical depth τ0(1, 1) of NH3 (1,1) is obtained by considering the blending effect of the magnetic hyperfine spectral lines, the (1-1) excitation temperature Tex (1, 1) is calculated by a two level model, the effect of different collision rate and the thermalization of the (1, 1) inversion lines are discussed, the rotation temperature TR ( 2, 1) between the NH3 levels (2, 2) and (1, 1) and the column density N( 1, 1) of the NH3 (1, 1) inversion level are derived, the results of the total column density from different assumptions for the abundance ratio of ortho-NH3 and para-NH3 are also discussed.

This approach is used for the molecular cloud NGC 2023 by using the relevant observed data and its optical depth and other physical parameters are obtained.  相似文献   

74.
The authors analyzed the data collected in the Ecological Station Jiaozhou Bay from May 1991 to November 1994, including 12 seasonal investigations, to determine the characteristics, dynamic cycles and variation trends of the silicate in the bay. The results indicated that the rivers around Jiaozhou Bay provided abundant supply of silicate to the bay. The silicate concentration there depended on river flow variation. The horizontal variation of silicate concentration on the transect showed that the silicate concentration decreased with distance from shorelines. The vertical variation of it showed that silicate sank and deposited on the sea bottom by phytoplankton uptake and death, and zooplankton excretion. In this way, silicon would endlessly be transferred from terrestrial sources to the sea bottom. The silicon took up by phytoplankton and by other biogeochemical processes led to insufficient silicon supply for phytoplankton growth. In this paper, a 2D dynamic model of river flow versus silicate concentration was established by which silicate concentrations of 0.028–0.062 μmol/L in seawater was yielded by inputting certain seasonal unit river flows (m3/s), or in other words, the silicate supply rate; and when the unit river flow was set to zero, meaning no river input, the silicate concentrations were between 0.05–0.69 μmol/L in the bay. In terms of the silicate supply rate, Jiaozhou Bay was divided into three parts. The division shows a given river flow could generate several different silicon levels in corresponding regions, so as to the silicon-limitation levels to the phytoplankton in these regions. Another dynamic model of river flow versus primary production was set up by which the phytoplankton primary production of 5.21–15.55 (mgC/m2·d)/(m3/s) were obtained in our case at unit river flow values via silicate concentration or primary production conversion rate. Similarly, the values of primary production of 121.98–195.33 (mgC/m2·d) were achieved at zero unit river flow condition. A primary production conversion rate reflects the sensitivity to silicon depletion so as to different phytoplankton primary production and silicon requirements by different phytoplankton assemblages in different marine areas. In addition, the authors differentiated two equations (Eqs. 1 and 2) in the models to obtain the river flow variation that determines the silicate concentration variation, and in turn, the variation of primary production. These results proved further that nutrient silicon is a limiting factor for phytoplankton growth. This study was funded by NSFC (No. 40036010), and the Director's Fund of the Beihai Sea Monitoring Center, the State Oceanic Administration.  相似文献   
75.
76.
本文对第22太阳周(1987年1月至1992年12月)中发生过M级以上的X射线耀斑(Hα耀斑级别≥M级,并伴有X射线的耀斑)对应的395个活动区资料进行了耀斑指数的统计,得到的结果:1.22太阳周M级以上X射线耀斑级别综合指数表,2.22太阳周M级以上X射线耀斑总指数表,3.第22太阳周M级以上X射线耀斑总指数随时间的变化曲线,4.第22太阳周M级以上X射线濯斑总指数直方图,该图表明第22太阳周活动的极大年分别是1989和1991年,为第23周太阳活动预报提供了可用参数。  相似文献   
77.
太阳磁场观测研究   总被引:5,自引:0,他引:5  
简要回顾了近几年国际上太阳磁场研究的一些重要进展,包括耀斑与磁切和电流的关系,电流螺度和磁螺度,磁场拓扑性,三维磁场外推,色球磁场研究,日冕磁场研究,内网络磁元,磁流和振荡,极区磁场观测以及色球磁元观测等方面内容,同时也介绍了怀柔太阳观测站最近所取得的主要成果,自20世纪90年代以来,YOHKOH高分辨率的太阳X射线数据,SOHO的多波段大尺度观测,TRACE的高分辨太阳过渡区资料,为研究太阳磁场从内部到距离几十太阳半径处的大范围演化提供了依据,高效的空间资料结合长期的地面资料,将是正派推动太阳磁场研究的重要手段和必然趋势。  相似文献   
78.
1 INTRODUCTIONCompact Symmetric Objects (CSOs) are powerful and compact sources (overall size <1 bpc) with lobe emission on both sides of the central engine. The small size of these sourcesis almost certainly to be attributed to the youth of the sources themselves (ages < 104 yr) andnot due to a dense coallning medium (Readhead 1996). The unification scenario assumes thatCSOs evolve into compact steep spectrum (CSS) sotirces and then into Fanaroff-Riley type 11objects (Fanti 1995). …  相似文献   
79.
本矿床是我国金红石矿床重要的成因及工业类型,为具有特定化学成分的岩石在特定变质条件下形成的。本文通过对大量数据的处理,查明了化学成分与成矿的关系:高Al2O3、MgO、Fe2O3+FeO、K2O、P2O5、H2O+、MnO,低SiO2、CaO、Na2O、CO2、S等,利于钛富集;高TiO2、MgO、P2O5、S,低SiO2、CaO、K2O、Al2O3、Fe2O3/FeO,利于金红石形成;高Sc、Zr、Ni、Zn及La/Yb,低Y、Nb、Th、Cd、Ba、Be、ΣREE,利于金红石纯度提高。对研究矿床成因及寻找新的同类矿床等有重要意义  相似文献   
80.
陈刘组为新建立的岩石地层单位,代表广西早三叠世盆地滨岸相带沉积类型。层型剖面位于贵港市陈刘村附近。层型定义指位于龙潭组与板纳组之间的沉积序列,岩性为灰绿、紫红色泥岩、粉砂细砂岩夹少量火山岩及碳酸盐岩,含菊石、双壳类、牙形石等化石,厚359m。  相似文献   
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