A4 Refereed article in a conference publication
Interplanetary Radio type II and Type IV Bursts as Indicators of Propagating Solar Transients
Authors: Pohjolainen S., Sheshvan N.
Editors: No available
Conference name: URSI Atlantic Radio Science Meeting
Publisher: Institute of Electrical and Electronics Engineers Inc.
Publication year: 2018
Book title : 2018 2nd URSI Atlantic Radio Science Meeting (AT-RASC)
Journal name in source: 2018 2nd URSI Atlantic Radio Science Meeting, AT-RASC 2018
ISBN: 978-1-5386-3764-7
eISBN: 978-90-82598-73-5
DOI: https://doi.org/10.23919/URSI-AT-RASC.2018.8471416(external)
Web address : https://ieeexplore.ieee.org/document/8471416(external)
Self-archived copy’s web address: https://arxiv.org/abs/1806.05065(external)
RPID5175803. As these bursts are due to propagating shock waves, driven by coronal mass ejections, they can be followed to near-Earth distances and can be used to predict the arrival times of geo-effective disturbances. Radio type IV bursts, on the other hand, are usually due to moving magnetic structures in the low corona and trapped particles form at least part of the emission. The observed directivity of type IV emission may also be used for space weather purposes.
