Ambipolar diffusion in the solar atmosphere

dc.contributor.author	Chitre, S. M
dc.contributor.author	Krishan, V
dc.date.accessioned	2008-07-29T05:12:13Z
dc.date.available	2008-07-29T05:12:13Z
dc.date.issued	2001-05
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 323, No. 2, pp. L23 - L25	en
dc.identifier.issn	0035-8711
dc.identifier.uri	http://hdl.handle.net/2248/2939
dc.description.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..	en
dc.format.extent	58656 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001MNRAS.323L..23C	en
dc.subject	Diffusion	en
dc.subject	Sun: Atmosphere	en
dc.subject	Sun: Magnetic Fields	en
dc.title	Ambipolar diffusion in the solar atmosphere	en
dc.type	Article	en