Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/4406
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dc.contributor.authorRajput, Mayank-
dc.contributor.authorBisoi, Susanta Kumar-
dc.date.accessioned2024-02-20T11:42:07Z-
dc.date.available2024-02-20T11:42:07Z-
dc.date.issued2024-02-
dc.identifier.citation42nd meeting of the Astronomical Society of India (ASI), Bangalore, India, 31 Jan to 04 Feb 2024en_US
dc.identifier.urihttp://hdl.handle.net/2080/4406-
dc.descriptionCopyright belongs to proceeding publisheren_US
dc.description.abstractIn this study, We correlated frequency bandwidth of 12 Type II bursts to the angular width of the associated CMEs and obtained an anticorrelation coefficient of ~ 60 % suggesting that the CMEs with large angular widths could produce narrow-band Type II emissions, in stark contrast to the recent report[1], that they produce broad-band Type II emissions. We further deduced the height of the Type II bursts (rType II ) at the onset time of the burst was < CME height (rCME), suggesting that the Type II emissions could be produced in the flank region of the shock rather than in the shock fronten_US
dc.subjectCMEsen_US
dc.subjectType II burstsen_US
dc.subjectType II emissionsen_US
dc.titleNarrow-band Type II Emissions Associated with CMEs of Large Angular Widths: A New Characteristics for Metric Type II burstsen_US
dc.typePresentationen_US
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