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...
| Main Authors: | , , , , , , |
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| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2017
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| Online Access: | http://hdl.handle.net/20.500.11937/59959 |