Please use this identifier to cite or link to this item:
http://hdl.handle.net/2080/4406
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Rajput, Mayank | - |
dc.contributor.author | Bisoi, Susanta Kumar | - |
dc.date.accessioned | 2024-02-20T11:42:07Z | - |
dc.date.available | 2024-02-20T11:42:07Z | - |
dc.date.issued | 2024-02 | - |
dc.identifier.citation | 42nd meeting of the Astronomical Society of India (ASI), Bangalore, India, 31 Jan to 04 Feb 2024 | en_US |
dc.identifier.uri | http://hdl.handle.net/2080/4406 | - |
dc.description | Copyright belongs to proceeding publisher | en_US |
dc.description.abstract | In 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 front | en_US |
dc.subject | CMEs | en_US |
dc.subject | Type II bursts | en_US |
dc.subject | Type II emissions | en_US |
dc.title | Narrow-band Type II Emissions Associated with CMEs of Large Angular Widths: A New Characteristics for Metric Type II bursts | en_US |
dc.type | Presentation | en_US |
Appears in Collections: | Conference Papers |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2024_42ndASI_MEeting_MRajput_Narrow-band.pdf | Poster | 655.56 kB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.