Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5861
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dc.contributor.authorBanerjee, D-
dc.contributor.authorMallik, D. C. V-
dc.contributor.authorVarghese, B. A-
dc.date.accessioned2012-08-31T16:32:24Z-
dc.date.available2012-08-31T16:32:24Z-
dc.date.issued2007-03-
dc.identifier.citationIIA Newsletter, Vol.12, No.1, March 2007, pp.1-16en
dc.identifier.urihttp://hdl.handle.net/2248/5861-
dc.descriptionOpen Accessen
dc.language.isoenen
dc.publisherIndian Institute of Astrophysicsen
dc.relation.urihttp://www.iiap.res.in/files/uploads/pdf/News-Letter-Mar-2007.pdfen
dc.rights© Indian Institute of Astrophysicsen
dc.subjectReport UN/NASA Workshop on the International Heliophysical Year 2007 and Basic Space Scienceen
dc.subjectAmbiguity in the physics of coronal loopsen
dc.subjectSolar Chromospheric Features to Ultraviolet (UV)Irradiance Variabilityen
dc.subjectVela Supernova Remnanten
dc.subjectHigh Resolution Spectroscopy Of HR3117en
dc.subjectCarbon-Enhanced Metal-Poor starsen
dc.titleIIA Newsletter, Vol.12, No.1, March 2007en
dc.typeArticleen
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