| 磁能和磁复杂性向日冕的传输 |
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| 引用本文： | 汪景琇. 磁能和磁复杂性向日冕的传输[J]. 中国天文和天体物理学报, 1995, 0(3) |
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| 作者姓名： | 汪景琇 |
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| 作者单位： | 中国科学院北京天文台 |
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| 摘 要： | 本文讨论了从太阳光球向日冕传输磁能和磁复杂性的过程。活动日冕，作为由电磁场和粒子组成的系统，其唯一的开场表面是太阳光球。光球层等离子体的运动和磁场的相互作用，是造成磁能和磁复杂性向日冕传播的主要根源；同时，光球上的耗散过程也对日冕磁能和磁复杂性的积累有不可忽视的贡献。
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| 关 键 词： | 太阳，日冕加热，耀斑 |
On the Transport of Magnetic Energy and Complexity to the Solar Corona |
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| WANG Jingxiu. On the Transport of Magnetic Energy and Complexity to the Solar Corona[J]. Chinese Journal of Astronomy and Astrophysics, 1995, 0(3) |
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| Authors: | WANG Jingxiu |
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| Abstract: | A discussion on the transport of magnetic energy and complexity to the corona is given in this paper. For an active corona, a system consisting of the electromagnetic field and particles, the only open surface is the solar photosphere. The interaction of velocity and magnetic fields on the photosphere is the primary cause of transporting the magnetic energy and complexity to the corona; meanwhile, the diffusion process at the photosphere also plays a role in the energy and complexity transportation. |
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| Keywords: | Sun coronal heating flare |
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