dc.contributor.author | Bappu, M. K. V | |
dc.contributor.author | Sivaraman, K. R | |
dc.date.accessioned | 2006-06-13T11:47:37Z | |
dc.date.available | 2006-06-13T11:47:37Z | |
dc.date.issued | 1966 | |
dc.identifier.citation | IQSY, New Delhi | en |
dc.identifier.uri | http://hdl.handle.net/2248/1000 | |
dc.description.abstract | Auto-correlation measures of the coarse Ca+ network made on selected spectroheliograms obtained during the solar minimum period of 1964 and 1965 are described. The full width at half maximum of the normalised A.C. curve gives a mean value of (31.37 ± 0.4) x 10/sup3/ km for the size of the network. The relationship between these network cells and those of the supergranulation are discussed. | |
dc.format.extent | 207171 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en | en |
dc.subject | Solar chromosphere | en |
dc.subject | Sun spot | en |
dc.title | Size of the Ca+ Coarse Network in the Solar Chromosphere at Sunspot Minimum | en |
dc.type | Article | en |