Diffuse Interplanetary Radio Emission from a Polar Coronal Mass Ejection
arXiv:2105.01216
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.
4 pages, 6 figures, URSI 2020 Proceedings