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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2397
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dc.contributor.authorRavindra, B-
dc.date.accessioned2008-06-03T12:12:09Z-
dc.date.available2008-06-03T12:12:09Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 297 - 298en
dc.identifier.urihttp://hdl.handle.net/2248/2397-
dc.description.abstractThe 3-D structure of quiet Sun chromospheric network magnetic field is studied by comparing the observed and computed chromospheric magnetograms. The comparison shows that the best correlation occurs at 1800 km above the photosphere at which the Fe I 8688 line forms.en
dc.format.extent70875 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..297Ren
dc.subjectSunen
dc.subjectNetworken
dc.subjectMagnetic fielden
dc.titleQuiet Sun Chromospheric Network Magnetic Fielden
dc.typeArticleen
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