RADIO OBSERVATIONS OF THE QUIET SOLAR CORONA

ALISSANDRAKIS, CE

dc.contributor.author	ALISSANDRAKIS, CE	en
dc.date.accessioned	2014-03-01T01:42:15Z
dc.date.available	2014-03-01T01:42:15Z
dc.date.issued	1993	en
dc.identifier.issn	0273-1177	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/23729
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.subject.other	DECAMETER WAVELENGTHS	en
dc.subject.other	BRIGHT POINTS	en
dc.subject.other	SUN	en
dc.subject.other	RADIOHELIOGRAPH	en
dc.subject.other	HOLES	en
dc.subject.other	METER	en
dc.subject.other	SHEET	en
dc.subject.other	GHZ	en
dc.title	RADIO OBSERVATIONS OF THE QUIET SOLAR CORONA	en
heal.type	journalArticle	en
heal.language	English	en
heal.publicationDate	1993	en
heal.abstract	Observations of radio emission from the quiet solar atmosphere and the associated emission mechanisms are discussed. Long wavelength observations, with a spatial resolution of similar to 1 arc min are ideal for the study of the large scale structure of the corona, including coronal holes, arches, streamers and the base of the heliospheric current sheet. These structures are observed both beyond the limb and on the solar disk, with little line of sight integration. We also discuss diagnostics of electron temperature and density, as well as the interpretation problems arising from the inhomogeneity of the corona and refraction effects.	en
heal.publisher	PERGAMON PRESS LTD	en
heal.journalName	SOLAR CORONA	en
heal.bookName	ADVANCES IN SPACE RESEARCH	en
dc.identifier.isi	ISI:A1993BA32J00016	en
dc.identifier.volume	14	en
dc.identifier.issue	4	en
dc.identifier.spage	81	en
dc.identifier.epage	91	en