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Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

Butcher, Harvey; Zucca, P; Morosan, D E; Rouillard, A P; Fallows, R; Gallagher, P T; Magdalenic, J; Klein, K-L; Mann, Gottfried; Vocks, Christian; Carley, E P; Bisi, M M

Description

Context. Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be associated with coronal mass ejections (CMEs) and reach speeds higher than the local magnetosonic speed. Radio imaging of decameter wavelengths (20–90 MHz) is now possible with the Low Frequency Array (LOFAR), opening a new radio window in which to study coronal shocks that leave the inner solar corona and enter...[Show more]

CollectionsANU Research Publications
Date published: 2018
Type: Journal article
URI: http://hdl.handle.net/1885/160464
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201732308
Access Rights: Open Access

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