Electron density from Mg VIII emission lines

dc.contributor.author	Dwivedi B.N.
dc.date.accessioned	2025-05-24T09:58:45Z
dc.description.abstract	Mg VIII emission line intensity ratio I (430.47)/I (436.62) has been studied in detail and is found to be an excellent candidate for diagnosing the quiet Sun and the coronal holes. © 1988 Kluwer Academic Publishers.
dc.identifier.doi	https://doi.org/10.1007/BF00157488
dc.identifier.uri	http://172.23.0.11:4000/handle/123456789/23653
dc.relation.ispartofseries	Solar Physics
dc.title	Electron density from Mg VIII emission lines

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