Diffuse Interplanetary Radio Emission from a Polar Coronal Mass Ejection
Abstract
We report on the first detection of nonthermal radio emission associated with a polar coronal mass ejection. We call the radio emission as diffuse interplanetary radio emission (DIRE), which occurs in the decameter-hectometric wavelengths. The radio emission originates from the shock flanks that interact with nearby streamers.
- Publication:
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arXiv e-prints
- Pub Date:
- May 2021
- DOI:
- 10.48550/arXiv.2105.01216
- arXiv:
- arXiv:2105.01216
- Bibcode:
- 2021arXiv210501216G
- Keywords:
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- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 4 pages, 6 figures, URSI 2020 Proceedings