Coronal heating by magnetic kink waves

被引：0

作者：

Banerjee, D ^{[1
]}

Dikpati, M ^{[1
]}

Choudhuri, AR ^{[1
]}

机构：

[1] Armagh Observ, Armagh BT61 9DG, North Ireland

来源：

1997 PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS | 1998年 / 138卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that the magnetic kink waves generated by the motions of the photospheric footpoints of the coronal flux tubes can supply adequate energy for heating the quiet corona. We model the solar corona as two-layer isothermal atmosphere, with the lower layer having chromospheric thickness and the temperature and the upper layer having coronal temperature.

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页码：15 / 18

页数：4

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