Diffuse Interplanetary Radio Emission from a Polar Coronal Mass Ejection
Solar and Stellar Astrophysics
2021-05-05 v1
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.
Cite
@article{arxiv.2105.01216,
title = {Diffuse Interplanetary Radio Emission from a Polar Coronal Mass Ejection},
author = {N. Gopalswamy and P. Makela and S. Yashiro and S. Akiyama},
journal= {arXiv preprint arXiv:2105.01216},
year = {2021}
}
Comments
4 pages, 6 figures, URSI 2020 Proceedings