Chitre, S. M. ; Krishan, V. (2001) Ambipolar diffusion in the solar atmosphere Monthly Notices of the Royal Astronomical Society, 323 (2). L23-L25. ISSN 0035-8711
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Official URL: http://onlinelibrary.wiley.com/journal/10.1111/%28...
Related URL: http://dx.doi.org/10.1046/j.1365-8711.2001.04461.x
Abstract
The process of non-linear ambipolar diffusion in the region overlying the solar surface can be an effective mechanism for producing sharp magnetic structures and current sheets. These may be the sites responsible for the occurrence of connectivity of magnetic field lines, and the subsequent explosive input of energy for heating of some of the features in the atmosphere of the Sun.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to John Wiley and Sons. |
| Keywords: | Diffusion; Sun: Atmosphere; Sun: Magnetic Fields |
| ID Code: | 89038 |
| Deposited On: | 30 Mar 2012 07:03 |
| Last Modified: | 30 Mar 2012 07:03 |
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