Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths

dc.contributor.author	Lantos, P.	en
dc.contributor.author	Alissandrakis, C. E.	en
dc.date.accessioned	2015-11-24T18:28:53Z
dc.date.available	2015-11-24T18:28:53Z
dc.identifier.issn	0273-1177	-
dc.identifier.uri	https://olympias.lib.uoi.gr/jspui/handle/123456789/16200
dc.rights	Default Licence	-
dc.title	Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths	en
heal.abstract	The Nan?ay Radioheliograph provides maps of the quiet solar corona around 160 MHz. In addition to coronal holes, localized emission sources and quiet sun, an unresolved component can be detected on the disk. The so-called coronal plateau corresponds to the K-corona dense regions observed on the limb and is thus located at the base of the interplanetary plasma sheet. Its evolution is studied from 1980 to 1986, during the declining phase of the cycle 21.	en
heal.access	campus	-
heal.fullTextAvailability	TRUE	-
heal.identifier.primary	http://dx.doi.org/10.1016/0273-1177(95)00332-9	-
heal.identifier.secondary	http://www.sciencedirect.com/science/article/pii/0273117795003329	-
heal.journalName	Advances in Space Research	en
heal.journalType	peer reviewed	-
heal.publicationDate	1995	-
heal.recordProvider	Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών	el
heal.type	journalArticle	-
heal.type.el	Άρθρο Περιοδικού	el
heal.type.en	Journal article	en

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