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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3074
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dc.contributor.authorSrikant, R-
dc.contributor.authorSingh, J-
dc.date.accessioned2008-08-12T08:57:40Z-
dc.date.available2008-08-12T08:57:40Z-
dc.date.issued2000-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 265 - 268en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3074-
dc.description.abstractA gradient based algorithm which divides arbitrary images into non-overlapping surface filling tiles of opposite polarity is used to study the flux and size distributions of large scale magnetic flux concen-trations in solar and heliospheric observatory (SoHO) magnetograms. The mean absolute flux and size of the concentrations at the considered scale is found to be about 1.7 × 10/sup18/Mx and 5.2Mm for both polarities. The form of the flux distribution is characterized by a skewness of α3 = 4.9 and a kurtosis of α4, = 42.8. The fall in the distribution in the range 6.5 × 10/sup17/Mx to 5 × 10/sup18/Mx is described by an exponential fit, in agreement with a model for the sustenance of quiet region flux.en
dc.format.extent1398660 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000JApA...21..265Sen
dc.subjectSun: Granulationen
dc.subjectMagnetogramen
dc.titleTessellation of SoHO Magnetogramsen
dc.typeArticleen
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