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太阳米波和分米波的射电观测是对太阳爆发过程中耀斑和日冕物质抛射现象研究的重要观测手段。米波和分米波的太阳射电暴以相干等离子体辐射为主导，表现出在时域和频域的多样性和复杂性。其中II 型射电暴是激波在日冕中运动引起电磁波辐射的结果。在II 型射电暴方面，首先对米波II 型射电暴的激波起源问题和米波II 型射电暴与行星际II 型射电暴的关系问题进行了讨论；其次，结合Lin-Forbes 太阳爆发理论模...
Sc III Spectral Properties of Astrophysical Interest
Oscillator strengths lifetimes coupled-cluster method
2011/10/18
Transition properties such as oscillator strengths, transition rates, branching ratios and lifetimes of many low-lying states in the doubly ionized scandium (Sc III) are reported. A relativistic metho...
Galactic Planetary Nebulae with Wolf-Rayet Nuclei III. Kinematical Analysis of a Large Sample of Nebulae
Galactic Planetary Nebulae inematical Analysis Wolf-Rayet Nuclei III
2009/6/30
Galactic Planetary Nebulae with Wolf-Rayet Nuclei III. Kinematical Analysis of a Large Sample of Nebulae。