1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3853
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.contributor.authorSatya Narayanan, A-
dc.contributor.authorEbenezer, E-
dc.date.accessioned2008-09-23T15:11:34Z-
dc.date.available2008-09-23T15:11:34Z-
dc.date.issued2003-03-
dc.identifier.citationAstronomy and Astrophysics, Vol. 400, No. 2, pp. 753 - 758en
dc.identifier.issn0004 - 6361-
dc.identifier.urihttp://hdl.handle.net/2248/3853-
dc.description.abstractWe present metric radio observations of quasi-periodic emission from the solar corona in close association with a ``halo'' CME and an ``EIT wave'' phenomenon. The radio event lasted for about 60 s. Its mean periodicity was ~8.8 s. The estimated Alfvén speed in the corona was 1034 km s-1. The derived height of the source region of the observed quasi-periodic emission, and the magnetic field at the corresponding location (for emission in the fundamental mode) were ~ 0.23 Rsun and 6.3 G, respectively. The magnetic field for harmonic emission was found to be ~ 3.1 G.en
dc.language.isoenen
dc.publisherThe European Southern Observatoryen
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:20030019en
dc.rights© The European Southern Observatory (ESO)-
dc.subjectSun: Activityen
dc.subjectSun: Coronaen
dc.subjectSun: Oscillationsen
dc.subjectSun: Radio Radiationen
dc.subjectMagnetohydrodynamics (MHD)en
dc.titleMetric observations of transient, quasi-periodic radio emission from the solar corona in association with a ``halo'' CME and an ``EIT wave'' eventen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Metric observations of transient716.47 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.