Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2916
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dc.contributor.authorRamesh, R-
dc.contributor.authorEbenezer, E-
dc.date.accessioned2008-07-29T04:38:00Z-
dc.date.available2008-07-29T04:38:00Z-
dc.date.issued2001-09-
dc.identifier.citationAstrophysical Journal, Vol. 558, No. 2, pp. L141 - L143en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2916-
dc.description.abstractWe report a transient intensity reduction/absorption burst observed at decameter wavelengths in close temporal association with an X2.0/3B flare near the disk center and the onset of a ``halo'' coronal mass ejection. The observed bandwidth of the burst was about 10 MHz. The size of the absorption region was estimated to be ~28,000 km.en
dc.format.extent272134 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/323498en
dc.subjectSun: Solar-terrestrial Relationsen
dc.subjectSun: Activityen
dc.subjectSun: Coronaen
dc.subjectSun: Flaresen
dc.subjectSun: Radio Radiationen
dc.titleDecameter Wavelength Observations of an Absorption Burst from the Sun and Its Association with an X2.0/3B Flare and the Onset of a ``Halo'' Coronal Mass Ejectionen
dc.typeArticleen
Appears in Collections:IIAP Publications

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