A dependence on solar cycle of the size of the Ca/+/ network

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1979

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DC Field	Value	Language
dc.contributor.author	Singh, J	-
dc.contributor.author	Bappu, M. K. V	-
dc.date.accessioned	2007-11-24T11:22:12Z	-
dc.date.available	2007-11-24T11:22:12Z	-
dc.date.issued	1981-05	-
dc.identifier.citation	Solar Physics, Vol. 71, May, pp. 161-168	en
dc.identifier.uri	http://hdl.handle.net/2248/1979	-
dc.description.abstract	Calcium network diameters are shown to be smaller by 5% at solar maximum than at minimum. The average cell size at minimum is 22,115 + or - 99 km. The average size at solar maximum is 20,920 + or - 112 km, though individual maxima perform differently from each other depending probably on the dispersed remnant magnetic fields. The change in size of the network is interpreted in terms of changes in the size of the supergranular convective cell.	en
dc.format.extent	640921 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981SoPh...71..161S	-
dc.subject	Calcium	en
dc.subject	Chromosphere	en
dc.subject	Metal Ions	en
dc.subject	Solar atmosphere	en
dc.subject	Solar Cycles	en
dc.subject	M.K.V. Bappu	en
dc.title	A dependence on solar cycle of the size of the Ca/+/ network	en
dc.type	Article	en
Appears in Collections:	M.K. Vainu Bappu ( 1960 - 1982 )

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