METER WAVELENGTH OBSERVATIONS OF THE QUIET SUN AND THE SLOWLY VARYING COMPONENT DURING DECLINING PHASE OF THE SOLAR-CYCLE

LANTOS, P; ALISSANDRAKIS, CE

dc.contributor.author	LANTOS, P	en
dc.contributor.author	ALISSANDRAKIS, CE	en
dc.date.accessioned	2014-03-01T01:42:12Z
dc.date.available	2014-03-01T01:42:12Z
dc.date.issued	1993	en
dc.identifier.issn	0273-1177	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/23715
dc.subject.classification	Engineering, Aerospace	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Geosciences, Multidisciplinary	en
dc.subject.classification	Meteorology & Atmospheric Sciences	en
dc.title	METER WAVELENGTH OBSERVATIONS OF THE QUIET SUN AND THE SLOWLY VARYING COMPONENT DURING DECLINING PHASE OF THE SOLAR-CYCLE	en
heal.type	journalArticle	en
heal.language	English	en
heal.publicationDate	1993	en
heal.abstract	Two dimensional maps of the Sun at 164 MHz, obtained with the Nancay Radioheliograph from April to August 1984 are presented. The quiet sun emission and the slowly varying component far from sunspots are studied. The association of local emissions with the chromospheric calcium plages is pointed out and interpreted. The altitude of the radio sources is estimated. The comparison of the location of the sources with K-corona observations confirms previous results obtained for the minimum of the cycle. The brightness temperature of the coronal plateau, which is the radio counterpart of the coronal plasma sheet, is given.	en
heal.publisher	PERGAMON PRESS LTD	en
heal.journalName	SOLAR CORONA	en
heal.bookName	ADVANCES IN SPACE RESEARCH	en
dc.identifier.isi	ISI:A1993BA32J00018	en
dc.identifier.volume	14	en
dc.identifier.issue	4	en
dc.identifier.spage	97	en
dc.identifier.epage	102	en