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Zhong-Quan Qu Shuai Wang Cheng-Lin Xu XiaoYu Zhang Ming-Guo Sun Chun-Lan Jin National Astronomical Observatories/Yunnan Astronomical Observatory Chinese Academy of Sciences Kunming zqqu@vip.km.net Graduate School of the Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2005,5(4):426-432
We analyze the spectral line broadening of those magneto-sensitive lines in solar magnetized atmospheres. The broadening at the line wings is due to the increase of the effective width of energy levels involved in Zeeman splitting, and the broadening at the line core also originated in Zeeman splitting under the condition that the Zeeman components are mixed. Therefore, the magnetoinduced or Zeeman broadening take effects on the whole line. The observed Stokes parameter data in a sunspot and outside it acquired by Solar Stokes Spectrum Telescope (S3T) are analyzed for the demonstration of this mechanism, and the Zeeman broadening rates are calculated for FeI6302.5 under some assumptions. Our result shows that the broadening is increased as the magnetic field strength becomes stronger, but the rate of increase at the line core is decreased as the field strength increases, while the rate at the wing does not show such an obvious regularity. The broadening is more effective in the line core than in the wings. 相似文献
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Fluid evolution in the Rushan lode gold deposit of Jiaodong Peninsula, eastern China 总被引：2，自引：0，他引：2
Fang-Fang Hu Hong-Rui Fan Ming-Guo Zhai Cheng-Wei Jin 《Journal of Geochemical Exploration》2006,89(1-3):161
The Rushan gold deposit in the Jiaodong Peninsula is currently the largest lode gold in China. Gold occurs mainly in pyrite- and polymetallic sulfide–quartz vein/veinlet stockworks. Fluid inclusions in the deposit are divided into three main types, namely CO2–H2O, H2O–CO2 ± CH4 and aqueous ones. Microthermometric data show that the pre-gold fluids were CO2-dominant (XCO2 up to 0.53), and the total homogenization temperatures fall in the range of 298377 °C. These fluids, modified by fluid/wallrock reactions, gradually evolved into fluids with less CO2 (XCO2 = 0.010.19) in the main ore-forming stage, and the total homogenization temperatures range from 170 to 324 °C. Hydrogen and oxygen stable isotope data suggest that ore-forming fluids were mixture of magmatic and meteoritic origin. Co-occurrence of gold and sulfides implies that gold was most likely transported in the form of gold–sulfide complexes. The wide distribution of CO2 inclusions means that the pH variation during gold transportation was controlled by CO2 buffering. 相似文献
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Ming-Guo Sun~ 《中国天文和天体物理学报》2006,6(1):87-95
A technique for obtaining a three-dimensional distribution of received pho- tons in Hα flares in the solar atmosphere is presented.It is well known that during flares hydrogen atoms in the chromosphere and photosphere are excited(even ion- ized)by the downward heating of non-thermal particles and then emit Hα photons. We trace back these Ha photons to their original layers by use of the contribution func- tion in the theory of spectral line formation,and so acquire their three-dimensional (3D)distribution.This technique is applied to the two-ribbon flare of 2002 January 20.The atmospheric models are obtained by fitting the“quasi-profiles”with the help of the generally used model atmospheres.Since the variety of the 3D images reflects the response of the atmospheric layers to the impact of energy transport,an analysis of the development of the flare is given through a comparison of the 3D images with the 2D temperature distribution. 相似文献
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Mesozoic lithosphere destruction beneath the North China Craton: evidence from major-, trace-element and Sr–Nd–Pb isotope studies of Fangcheng basalts 总被引：85，自引：1，他引：85
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江陵浅水-半深水坳陷湖盆层序地层学特征 总被引：2，自引：1，他引：2
以层序地层学理论为指导,系统研究了江陵浅水-半深水坳陷湖盆的层序地层学特征。研究表明:区域不整合界面和沉积转换界面是级层序的主要界面;层序内虽均发育低位、湖侵和高位体系域,但各体系域发育程度是不同的,致使层序的旋回性以非对称为主;层序内各体系域的沉积相构成均以河流三角洲和浅水湖泊为主,而冲积扇、扇三角洲不发育,湖泊水体基本没有发生过明显的扩张、收缩,湖平面的波动没有造成沉积相带的区域性变化,在此基础上,建立了江陵浅水-半深水坳陷湖盆特有的两种层序地层充填模式。 相似文献
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Circa 1.78 Ga mafic dyke swarms and some coeval volcanic associations constitute a Large Igneous Province in the central North China craton. The 1st generation of dykes intruded at ca. 1780 Ma and is chemically delineated into 3 groups: the LT Group is gabbroic and has low-Fe–Ti contents, acting as parental magma; the NW Group is high in Fe–Ti-contents and doleritic with an iron-enriched trend; whereas the EW Group is doleritic to andesitic and crystallized from relict siliceous liquids with a silica-enriched trend. They have an EM-I type source and record integral magmatic processes. These include contamination of lithospheric material and assimilation of crustal melts with in-situ crystallization in a magma chamber (the LT Group) and fractional crystallization in magma channels (the NW Group) and even with additional alteration (the EW Group). The 2nd generation is slightly younger (ca. 1760 Ma) and scarcely distributed. It has high-Fe–Ti contents, originated from a mixing source of DM and EM-I types. The dykes could be associated with a palaeo-plume: the 1st generation represents lower mantle melts generated from the plume head, whereas the 2nd generation records extra melts from asthenosphere entrained by the plume tail. 相似文献
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