A4 Vertaisarvioitu artikkeli konferenssijulkaisussa
Interplanetary Radio type II and Type IV Bursts as Indicators of Propagating Solar Transients
Tekijät: Pohjolainen S., Sheshvan N.
Toimittaja: No available
Konferenssin vakiintunut nimi: URSI Atlantic Radio Science Meeting
Kustantaja: Institute of Electrical and Electronics Engineers Inc.
Julkaisuvuosi: 2018
Kokoomateoksen nimi: 2018 2nd URSI Atlantic Radio Science Meeting (AT-RASC)
Tietokannassa oleva lehden nimi: 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
Verkko-osoite: https://ieeexplore.ieee.org/document/8471416
Rinnakkaistallenteen osoite: https://arxiv.org/abs/1806.05065
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.
