| Three—Dimensional Propagation of Magnetohydrodynamic Waves in the Solar Chromophere and Corona |
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| 引用本文： | 李波,郑惠南,等.Three—Dimensional Propagation of Magnetohydrodynamic Waves in the Solar Chromophere and Corona[J].中国物理快报,2002,19(11):1639-1642. |
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| 作者姓名： | 李波 郑惠南 |
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| 作者单位： | SchoolofEarthandSpaceSciences,UniversityofScienceandTechnologyofChina,Hefei230026 |
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| 摘 要： | We study the three-dimensional magnetohydrodynamic(MHD) wave propagation in the solar atmosphere consisting of the chromosphere and corona.Pressure enhancement and velocity shear are implemented simultaneously at the bootom of the chromophere.The global propagation of the incurred MHD waves,including fast-mode and slow-mode magnetoacoustic waves as well as Alfven wave,can be identified,Wave front positions obtained numerically with respect to specific waves fit well with those calculated with local MHD wave speeds.
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| 关 键 词： | 磁流体 太阳色球层 电晕 波传播 |
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