Propagation and Interaction Properties of Successive Coronal Mass Ejections in Relation to a Complex Type II Radio Burst
Ying D. Liu, Xiaowei Zhao, and Bei Zhu

TL;DR
This study investigates the propagation and interaction of three successive CMEs and their associated complex type II radio burst, using observations and a simple analytical model to understand their behavior from Sun to Earth.
Contribution
It introduces a free-parameterless analytical model for CME shock propagation that aligns well with observations and simulations up to 2.34 AU.
Findings
CMEs interacted and overtook each other at 0.85 AU
Shock propagation times were estimated at 14 and 6 hours
Model predictions matched observational data and MHD simulations
Abstract
We examine the propagation and interaction properties of three successive coronal mass ejections (CMEs) from 2001 November 21-22, with a focus on their connection with the behaviors of the associated long-duration complex type II radio burst. In combination with coronagraph and multi-point in situ observations, the long-duration type II burst provides key features for resolving the propagation and interaction complexities of the three CMEs. The two CMEs from November 22 interacted first and then overtook the November 21 CME at a distance of about 0.85 AU from the Sun. The time scale for the shock originally driven by the last CME to propagate through the preceding two CMEs is estimated to be about 14 and 6 hr, respectively. We present a simple analytical model without any free parameters to characterize the whole Sun-to-Earth propagation of the shock, which shows a remarkable…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
