Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4506
Title: | Coronal heating by magnetic kink waves |
Authors: | Banerjee, D Dikpati, M Choudhuri, A. R |
Keywords: | Coronal heating Magnetic kink waves Stellar astrophysics |
Issue Date: | 1998 |
Publisher: | Astronomical Society of the Pacific |
Citation: | Chan, K.L., Cheng, K.S and Singh, H.P eds., 1997 Pacific Rim conference on Stellar Astrophysics., Proceedings of ASP Conference Hongkong, PRC, 13 - 16 August, 1997., pp. 15 - 18 |
Series/Report no.: | Astronomical Society of a Pacific Conference Series; Vol. 138 |
Abstract: | 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 |
URI: | http://hdl.handle.net/2248/4506 |
ISBN: | 1-886733-58-9 |
Appears in Collections: | IIAP Publications |
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File | Description | Size | Format | |
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Coronal heating by magnetic kink waves | 383.34 kB | Adobe PDF | View/Open |
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