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Observations of near-simultaneous split-band solar type-II radio bursts at low frequencies

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dc.contributor.author Hariharan, K
dc.contributor.author Ramesh, R
dc.contributor.author Kathiravan, C
dc.date.accessioned 2020-11-17T13:54:21Z
dc.date.available 2020-11-17T13:54:21Z
dc.date.issued 2015-09
dc.identifier.citation Solar Physics, Vol. 290, No. 9, pp. 2479-2489 en_US
dc.identifier.issn 1573-093X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7083
dc.description Restricted Access © Springer The original publication is available at springerlink.com http://dx.doi.org/10.1007/s11207-015-0761-5 en_US
dc.description.abstract We report ground-based radio spectral and polarimeter observations of two successive split-band Type-II bursts that occurred on 20 February 2014 at low frequencies (<100 MHz) in association with a solar coronal mass ejection (CME). The temporal interval between the onset of the two bursts was very small, ≈ one minute. Both of the bursts exhibited fundamental–harmonic structure. The coronal magnetic-field strength [B] in the upstream region of the associated magnetohydrodynamic (MHD) shock, estimated from the split-band observations, is in the range B≈1.3--1.1 G over the radial distance [r] interval r≈1.49--1.58 R⊙ for the first Type-II burst, and B≈1.3--1.0 G over r≈1.49--1.64 R⊙ for the second Type-II burst. Based on the results obtained, we show that the first and the second Type-II bursts in the present case were likely due to MHD shocks generated by the near-simultaneous interaction of two different regions of the aforementioned CME with a preceding CME and a pre-existing coronal streamer. en_US
dc.language.iso en en_US
dc.publisher Springer en_US
dc.subject Sun en_US
dc.subject Flares en_US
dc.subject Coronal mass ejections en_US
dc.subject Shock waves en_US
dc.subject Radio bursts en_US
dc.subject Type II en_US
dc.subject Coronal magnetic-field en_US
dc.title Observations of near-simultaneous split-band solar type-II radio bursts at low frequencies en_US
dc.type Article en_US


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