Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1979
Title: A dependence on solar cycle of the size of the Ca/+/ network
Authors: Singh, J
Bappu, M. K. V
Keywords: Calcium;Chromosphere;Metal Ions;Solar atmosphere;Solar Cycles;M.K.V. Bappu
Issue Date: May-1981
Publisher: Springer
Citation: Solar Physics, Vol. 71, May, pp. 161-168
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.
URI: http://hdl.handle.net/2248/1979
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1981SoPh...71..161S
Appears in Collections:M.K. Vainu Bappu ( 1960 - 1982 )

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