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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3079
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dc.contributor.authorRamesh, K. B-
dc.contributor.authorNagabhushana, B. S-
dc.contributor.authorVarghese, B. A-
dc.date.accessioned2008-08-12T09:02:08Z-
dc.date.available2008-08-12T09:02:08Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 419 - 420en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3079-
dc.format.extent36139 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..419Ren
dc.subjectSun: Coronaen
dc.subjectEmergence of magnetic fluxen
dc.titleThe Enhanced Coronal Green Line Intensity and the Magnetic Field Gradientsen
dc.typeArticleen
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