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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1756
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dc.contributor.authorVan Ballegooijen, A. A-
dc.contributor.authorHasan, S. S-
dc.date.accessioned2007-07-27T08:46:26Z-
dc.date.available2007-07-27T08:46:26Z-
dc.date.issued2003-
dc.identifier.citationAlexei A. Pevtsov and Han Uitenbroek eds., Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, ASP Conference Series, Vol. 286, held 11 - 15 March 2002 at NSO, Sunspot, New Mexico, USA. pp. 155 - 168en
dc.identifier.urihttp://hdl.handle.net/2248/1756-
dc.format.extent2027138 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseriesASP Conference Series Vol. 286en
dc.relation.urihttp://adsabs.harvard.edu/abs/2003ASPC..286..155Ven
dc.subjectPhotospheric Magnetic Fielden
dc.titlePhysics of Photospheric Magnetic Fielden
dc.typeArticleen
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