Two-Part Interplanetary Type II Solar Radio Bursts
Silja Pohjolainen

TL;DR
This paper analyzes two interplanetary type II solar radio burst events from 2003 and 2012, examining their characteristics, associated CMEs, and possible shock origins, with insights from multi-viewpoint observations.
Contribution
It provides a detailed comparison of two similar two-part interplanetary type II bursts, including their association with CMEs and possible shock mechanisms, using multi-viewpoint data from 2003 and 2012.
Findings
Diffuse type II burst likely caused by CME bow shock.
F-H type II burst possibly driven by separate shock fronts.
Visibility of diffuse burst varies with viewing angle.
Abstract
Two similar-looking, two-part interplanetary type II burst events from 2003 and 2012 are reported and analysed. The 2012 event was observed from three different viewing angles, enabling comparisons between the spacecraft data. In these two events, a diffuse wide-band type II radio burst was followed by a type II burst that showed emission at the fundamental and harmonic (F-H) plasma frequencies, and these emission bands were also slightly curved in their frequency-time evolution. Both events were associated with high-speed, halo-type coronal mass ejections (CMEs). In both events, the diffuse type II burst was most probably created by a bow shock at the leading front of the CME. However, for the later-appearing F-H type II burst there are at least two possible explanations. In the 2003 event there is evidence of CME interaction with a streamer, with a possible shift from a bow shock to a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics
