1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2939
Full metadata record
DC FieldValueLanguage
dc.contributor.authorChitre, S. M-
dc.contributor.authorKrishan, V-
dc.date.accessioned2008-07-29T05:12:13Z-
dc.date.available2008-07-29T05:12:13Z-
dc.date.issued2001-05-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 323, No. 2, pp. L23 - L25en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2939-
dc.description.abstractThe 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.extent58656 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001MNRAS.323L..23Cen
dc.subjectDiffusionen
dc.subjectSun: Atmosphereen
dc.subjectSun: Magnetic Fieldsen
dc.titleAmbipolar diffusion in the solar atmosphereen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Chitre S. M.pdf57.28 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.