Type III Solar Radio Burst Source Region Splitting due to a Quasi-separatrix Layer

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Type III Solar Radio Burst Source Region Splitting due to a Quasi-separatrix Layer

We present low-frequency (80-240 MHz) radio imaging of type III solar radio bursts observed by the Murchison Widefield Array on 2015 September 21. The source region for each burst splits from one dominant component at higher frequencies into two increasingly separated components at lower frequencies...

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Bibliographic Details
Main Authors:	McCauley, P., Cairns, I., Morgan, John, Gibson, S., Harding, J., Lonsdale, C., Oberoi, D.
Format:	Journal Article
Published:	Institute of Physics Publishing 2017
Online Access:	http://hdl.handle.net/20.500.11937/59959

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