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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4049
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dc.contributor.authorNagabushana, B. S-
dc.contributor.authorGokhale, M. H-
dc.date.accessioned2008-12-12T11:23:35Z-
dc.date.available2008-12-12T11:23:35Z-
dc.date.issued1989-
dc.identifier.citationHvar Observatory Bulletin, Vol. 13, No. 1, pp. 25 - 29en
dc.identifier.issn0351-2651-
dc.identifier.urihttp://hdl.handle.net/2248/4049-
dc.descriptionOpen Access-
dc.description.abstractWe have determined statistically the horizontal gradiant of the vertical magnetic field in the neighbourhood of filaments inside and outside the active regions during a few months in 1981 and in 1984. The results show that there are meaningful upper and lower limits on the grandiant of the surrounding large scale photospheric magnetic field for the existence of a filament. These limits represent a necessary but not sufficient condition.-
dc.language.isoenen
dc.relation.urihttp://adsabs.harvard.edu/abs/1989HvaOB..13...25Nen
dc.subjectPhotospheric Field Gradienten
dc.subjectQuiescent Prominencesen
dc.titlePhotospheric field gradient in the neighbourghood of quiescent prominencesen
dc.typeArticleen
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