Please use this identifier to cite or link to this item:
Full metadata record
DC FieldValueLanguage
dc.contributor.authorKathiravan, C-
dc.contributor.authorRamesh, R-
dc.contributor.authorSubramanian, K. R-
dc.identifier.citationThe Astrophysical Journal, Vol. 567, No. 1, pp. L93 - L95en
dc.description.abstractWe report metric radio observations and the results obtained using two-dimensional ray-tracing analysis of the solar corona close to the onset phase of the exceptionally bright prominence eruption and the associated massive coronal mass ejection (CME) of 1998 June 2. The average electron density of the observed radio enhancements at the location of the eruption was found to be ~17 times greater than the ambient medium. We also calculated their width along the line of sight, and the mean value is ~160,000 km. The radio estimate of the CME mass was about 4 times less than that of the white-light value.en
dc.format.extent89160 bytes-
dc.publisherUniversity of Chicago Pressen
dc.subjectSun: Solar-Terrestrial Relationsen
dc.subjectSun: Activityen
dc.subjectSun: Coronaen
dc.subjectSun: Prominencesen
dc.subjectSun: Radio Radiationen
dc.titleMetric Radio Observations and Ray-tracing Analysis of the Onset Phase of a Solar Eruptive Eventen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Kathiravan C.pdf87.07 kBAdobe PDFView/Open

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